Hello world!
Are you learning CSS?
Note: For [attribute|=value] to work in IE8 and earlier, a DOCTYPE must be declared.
Note: The value has to be a whole word, either alone, like class="top", or followed by a hyphen( - ), like class="top-text"!
Hello world!
Are you learning CSS?
The first div element. [attribute$="value"]
The second div element.
The third div element.
This is some text in a paragraph.

The first div element asd. [attribute*="value"]
The second div eleasdment.
The third div element.
This is some teasdxt in a paragraph.


Select Measurement Unit
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In the 2016 Washington state elections, there will be a ballot initiative proposed by Carbon Washington asking voters if they want to implement a revenue-neutral carbon tax policy in the state. How are you going to make this decision? The goal of this visualization is to help you make an informed choice by providing information about the estimated financial impacts of such a policy on households around the state.
With the drop-down selector, you can change which variable is encoded on the map, histogram, and bubble chart. For these variables, "average" means electricity is calculated assuming electricity is provided by an average utility in the region in terms of carbon impact. Similarly, "best" and "worst" assume the utility with the best carbon impact and the worst carbon impact, respectively.
With the brush filters, you can change which types of households are included in the data that is displayed on the map and histogram. Also, by clicking a region on the map, only households in that region are included in the histogram.
The coloring of the map shows the relative financial impacts on the selected variable, with red coloring the regions for which the average household is impacted more negatively and blue coloring the regions for which the average household is impacted more positively. For more detail beyond the average household, look to the histogram, which shows the distribution of impacts for the selected variable. For even more detail, the bubble chart breaks the data down further.
| Household financial impact variable: |
Income filter ($): | Number of dependents filter: | Number of bedrooms filter: | Number of vehicles filter: |
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{% avocado load field "variants.variant.chr" as chromosome %} {% avocado load field "variants.variant.pos" as position %}


CAMBRIDGE, Mass. — One night late in 1979, an itinerant young physicist named Alan Guth, with a new son and a year’s appointment at Stanford, stayed up late with his notebook and equations, venturing far beyond the world of known physics.
He was trying to understand why there was no trace of some exotic particles that should have been created in the Big Bang. Instead he discovered what might have made the universe bang to begin with. A potential hitch in the presumed course of cosmic evolution could have infused space itself with a special energy that exerted a repulsive force, causing the universe to swell faster than the speed of light for a prodigiously violent instant.
If true, the rapid engorgement would solve paradoxes like why the heavens look uniform from pole to pole and not like a jagged, warped mess. The enormous ballooning would iron out all the wrinkles and irregularities. Those particles were not missing, but would be diluted beyond detection, like spit in the ocean.
“SPECTACULAR REALIZATION,” Dr. Guth wrote across the top of the page and drew a double box around it.
On Monday, Dr. Guth’s starship came in. Radio astronomers reported that they had seen the beginning of the Big Bang, and that his hypothesis, known undramatically as inflation, looked right.
Reaching back across 13.8 billion years to the first sliver of cosmic time with telescopes at the South Pole, a team of astronomers led by John M. Kovac of the Harvard-Smithsonian Center for Astrophysics detected ripples in the fabric of space-time — so-called gravitational waves — the signature of a universe being wrenched violently apart when it was roughly a trillionth of a trillionth of a trillionth of a second old. They are the long-sought smoking-gun evidence of inflation, proof, Dr. Kovac and his colleagues say, that Dr. Guth was correct.
You have 3 free articles remaining. Subscribe to The TimesInflation has been the workhorse of cosmology for 35 years, though many, including Dr. Guth, wondered whether it could ever be proved.
If corroborated, Dr. Kovac’s work will stand as a landmark in science comparable to the recent discovery of dark energy pushing the universe apart, or of the Big Bang itself. It would open vast realms of time and space and energy to science and speculation.
Confirming inflation would mean that the universe we see, extending 14 billion light-years in space with its hundreds of billions of galaxies, is only an infinitesimal patch in a larger cosmos whose extent, architecture and fate are unknowable. Moreover, beyond our own universe there might be an endless number of other universes bubbling into frothy eternity, like a pot of pasta water boiling over.
‘As Big as It Gets’In our own universe, it would serve as a window into the forces operating at energies forever beyond the reach of particle accelerators on Earth and yield new insights into gravity itself. Dr. Kovac’s ripples would be the first direct observation of gravitational waves, which, according to Einstein’s theory of general relativity, should ruffle space-time.
Marc Kamionkowski of Johns Hopkins University, an early-universe expert who was not part of the team, said, “This is huge, as big as it gets.”
He continued, “This is a signal from the very earliest universe, sending a telegram encoded in gravitational waves.”
The ripples manifested themselves as faint spiral patterns in a bath of microwave radiation that permeates space and preserves a picture of the universe when it was 380,000 years old and as hot as the surface of the sun.
Dr. Kovac and his collaborators, working in an experiment known as Bicep, for Background Imaging of Cosmic Extragalactic Polarization, reported their results in a scientific briefing at the Center for Astrophysics here on Monday and in a set of papers submitted to The Astrophysical Journal.
The Theory of Inflation
Astronomers have found evidence to support the theory of inflation, which explains how the universe expanded so uniformly and so quickly in the instant after the Big Bang 13.8 billion years ago.
The Universe is just under 14 billion years old. From our position in the Milky Way galaxy, we can observe a sphere that is now about 92 billion light-years across. But there's a mystery. Wherever we look, the universe has an even temperature.
Not Enough Time The universe is not old enough for light to have traveled the vast distance from one side of the universe to the other, and there has not been enough time for scattered patches of hot and cold to mix into an even temperature.
Distance Coffee At a smaller scale, imagine using a telescope to look a mile in one direction. You see a coffee cup, and from the amount of steam, you can estimate its temperature and how much it has cooled.
Coffee Everywhere Now turn around and look a mile in the other direction. You see a similar coffee cup, at exactly the same temperature. Coincidence? Maybe. But if you see a similar cup in every direction, you might want to look for another explanation.
Still not enough time There has not been enough time to carry coffee cups from place to place before they get cold. But if all the coffee cups were somehow filled from a single coffee pot, all at the same time, that might explain their even temperature.
Inflation solves this problem. The theory proposes that, less than a trillionth of a second after the Big Bang, the universe expanded faster than the speed of light. Tiny ripples in the violently expanding energy field eventually grew into the large-scale structures of the universe.
Fluctuation Astronomers have now detected evidence of these ancient fluctuations in swirls of polarized light in the cosmic background radiation, which is energy left over from the early universe. These are gravitational waves predicted by Einstein.
Expansion Returning to our coffee, imagine a single, central pot expanding faster than light and cooling to an even temperature as it expands. That is something like inflation. And the structure of the universe mirrors the froth and foam of the original pot.
By LARRY BUCHANAN and JONATHAN CORUM
Dr. Kovac said the chance that the results were a fluke was only one in 10 million.
Dr. Guth, now 67, pronounced himself “bowled over,” saying he had not expected such a definite confirmation in his lifetime. “With nature, you have to be lucky,” he said. “Apparently we have been lucky.”
The results are the closely guarded distillation of three years’ worth of observations and analysis. Eschewing email for fear of a leak, Dr. Kovac personally delivered drafts of his work to a select few, meeting with Dr. Guth, who is now a professor at Massachusetts Institute of Technology (as is his son, Larry, who was sleeping that night in 1979), in his office last week.
“It was a very special moment, and one we took very seriously as scientists,” said Dr. Kovac, who chose his words as carefully as he tended his radio telescopes.
Andrei Linde of Stanford, a prolific theorist who first described the most popular variant of inflation, known as chaotic inflation, in 1983, was about to go on vacation in the Caribbean last week when Chao-Lin Kuo, a Stanford colleague and a member of Dr. Kovac’s team, knocked on his door with a bottle of Champagne to tell him the news.
Confused, Dr. Linde called out to his wife, asking if she had ordered anything.
“And then I told him that in the beginning we thought that this was a delivery but we did not think that we ordered anything, but I simply forgot that actually I did order it, 30 years ago,” Dr. Linde wrote in an email.
Calling from Bonaire, the Dutch Caribbean island, Dr. Linde said he was still hyperventilating. “Having news like this is the best way of spoiling a vacation,” he said.
By last weekend, as social media was buzzing with rumors that inflation had been seen and news spread, astrophysicists responded with a mixture of jubilation and caution.
Max Tegmark, a cosmologist at M.I.T., wrote in an email, “I think that if this stays true, it will go down as one of the greatest discoveries in the history of science.”
John E. Carlstrom of the University of Chicago, Dr. Kovac’s mentor and head of a competing project called the South Pole Telescope, pronounced himself deeply impressed. “I think the results are beautiful and very convincing,” he said.
Paul J. Steinhardt of Princeton, author of a competitor to inflation that posits the clash of a pair of universes as the cause of genesis, said that if true, the Bicep result would eliminate his model, but he expressed reservations about inflation.
Lawrence M. Krauss of Arizona State and others also emphasized the need for confirmation, noting that the new results exceeded earlier estimates based on temperature maps of the cosmic background by the European Space Agency’s Planck satellite and other assumptions about the universe.
“So we will need to wait and see before we jump up and down,” Dr. Krauss said.
Corroboration might not be long in coming. The Planck spacecraft will report its own findings this year. At least a dozen other teams are trying similar measurements from balloons, mountaintops and space.
Spirals in the SkyGravity waves are the latest and deepest secret yet pried out of the cosmic microwaves, which were discovered accidentally by Arno Penzias and Robert Wilson at Bell Labs 50 years ago. They won the Nobel Prize.
Dr. Kovac has spent his career trying to read the secrets of these waves. He is one of four leaders of Bicep, which has operated a series of increasingly sensitive radio telescopes at the South Pole, where the thin, dry air creates ideal observing conditions. The others are Clement Pryke of the University of Minnesota, Jamie Bock of the California Institute of Technology and Dr. Kuo of Stanford.
“The South Pole is the closest you can get to space and still be on the ground,” Dr. Kovac said. He has been there 23 times, he said, wintering over in 1994. “I’ve been hooked ever since,” he said.
In 2002, he was part of a team that discovered that the microwave radiation was polarized, meaning the light waves had a slight preference to vibrate in one direction rather than another.
This was a step toward the ultimate goal of detecting the gravitational waves from inflation. Such waves, squeezing space in one direction and stretching it in another as they go by, would twist the direction of polarization of the microwaves, theorists said. As a result, maps of the polarization in the sky should have little arrows going in spirals.
Detecting those spirals required measuring infinitesimally small differences in the temperature of the microwaves. The group’s telescope, Bicep2, is basically a giant superconducting thermometer.
“We had no expectations what we would see,” Dr. Kovac said.
The strength of the signal surprised the researchers, and they spent a year burning up time on a Harvard supercomputer, making sure they had things right and worrying that competitors might beat them to the breakthrough.
A Special TimeThe data traced the onset of inflation to a time that physicists like Dr. Guth, staying up late in his Palo Alto house 35 years ago, suspected was a special break point in the evolution of the universe.
Physicists recognize four forces at work in the world today: gravity, electromagnetism, and strong and weak nuclear forces. But they have long suspected that those are simply different manifestations of a single unified force that ruled the universe in its earliest, hottest moments.
As the universe cooled, according to this theory, there was a fall from grace, like some old folk mythology of gods or brothers falling out with each other. The laws of physics evolved, with one force after another splitting away.
That was where Dr. Guth came in.
Under some circumstances, a glass of water can stay liquid as the temperature falls below 32 degrees, until it is disturbed, at which point it will rapidly freeze, releasing latent heat.
Similarly, the universe could “supercool” and stay in a unified state too long. In that case, space itself would become imbued with a mysterious latent energy.
Inserted into Einstein’s equations, the latent energy would act as a kind of antigravity, and the universe would blow itself up. Since it was space itself supplying the repulsive force, the more space was created, the harder it pushed apart.
What would become our observable universe mushroomed in size at least a trillion trillionfold — from a submicroscopic speck of primordial energy to the size of a grapefruit — in less than a cosmic eye-blink.
Almost as quickly, this pulse would subside, relaxing into ordinary particles and radiation. All of normal cosmic history was still ahead, resulting in today’s observable universe, a patch of sky and stars billions of light-years across. “It’s often said that there is no such thing as a free lunch,” Dr. Guth likes to say, “but the universe might be the ultimate free lunch.”
Make that free lunches. Most of the hundred or so models resulting from Dr. Guth’s original vision suggest that inflation, once started, is eternal. Even as our own universe settled down to a comfortable homey expansion, the rest of the cosmos will continue blowing up, spinning off other bubbles endlessly, a concept known as the multiverse.
So the future of the cosmos is perhaps bright and fecund, but do not bother asking about going any deeper into the past.
We might never know what happened before inflation, at the very beginning, because inflation erases everything that came before it. All the chaos and randomness of the primordial moment are swept away, forever out of our view.
“If you trace your cosmic roots,” said Abraham Loeb, a Harvard- Smithsonian astronomer who was not part of the team, “you wind up at inflation.”


 Using Blade style syntax, you can easily setup tasks for deployment, Artisan commands, and more. Currently, Envoy only supports the Mac and Linux operating systems. However, Windows support is achievable using WSL2.
Installation
First, install Envoy into your project using the Composer package manager:
composer require laravel/envoy --dev
Once Envoy has been installed, the Envoy binary will be available in your application's vendor/bin
directory:
php vendor/bin/envoy
Writing Tasks
Defining Tasks
Tasks are the basic building block of Envoy. Tasks define the shell commands that should execute on your remote servers when the task is invoked. For example, you might define a task that executes the php artisan queue:restart
command on all of your application's queue worker servers.
All of your Envoy tasks should be defined in an Envoy.blade.php
file at the root of your application. Here's an example to get you started:
@servers(['web' =><EMAIL_ADDRESS>'workers' =><EMAIL_ADDRESS>@task('restart-queues', ['on' => 'workers'])
cd /home/user/example.com
php artisan queue:restart
@endtask
As you can see, an array of @servers
is defined at the top of the file, allowing you to reference these servers via the on
option of your task declarations. The @servers
declaration should always be placed on a single line. Within your @task
declarations, you should place the shell commands that should execute on your servers when the task is invoked.
Local Tasks
You can force a script to run on your local computer by specifying the server's IP address as <IP_ADDRESS>
:
@servers(['localhost' => '<IP_ADDRESS>'])
Importing Envoy Tasks
Using the @import
directive, you may import other Envoy files so their stories and tasks are added to yours. After the files have been imported, you may execute the tasks they contain as if they were defined in your own Envoy file:
@import('vendor/package/Envoy.blade.php')
Multiple Servers
Envoy allows you to easily run a task across multiple servers. First, add additional servers to your @servers
declaration. Each server should be assigned a unique name. Once you have defined your additional servers you may list each of the servers in the task's on
array:
@servers(['web-1' => '<IP_ADDRESS>', 'web-2' => '<IP_ADDRESS>'])
@task('deploy', ['on' => ['web-1', 'web-2']])
cd /home/user/example.com
git pull origin {{ $branch }}
php artisan migrate --force
@endtask
Parallel Execution
By default, tasks will be executed on each server serially. In other words, a task will finish running on the first server before proceeding to execute on the second server. If you would like to run a task across multiple servers in parallel, add the parallel
option to your task declaration:
@servers(['web-1' => '<IP_ADDRESS>', 'web-2' => '<IP_ADDRESS>'])
@task('deploy', ['on' => ['web-1', 'web-2'], 'parallel' => true])
cd /home/user/example.com
git pull origin {{ $branch }}
php artisan migrate --force
@endtask
Setup
Sometimes, you may need to execute arbitrary PHP code before running your Envoy tasks. You may use the @setup
directive to define a block of PHP code that should execute before your tasks:
@setup
$now = new DateTime;
@endsetup
If you need to require other PHP files before your task is executed, you may use the @include
directive at the top of your Envoy.blade.php
file:
@include('vendor/autoload.php')
@task('restart-queues')
# ...
@endtask
Variables
If needed, you may pass arguments to Envoy tasks by specifying them on the command line when invoking Envoy:
php vendor/bin/envoy run deploy --branch=master
You may access the options within your tasks using Blade's "echo" syntax. You may also define Blade if
statements and loops within your tasks. For example, let's verify the presence of the $branch
variable before executing the git pull
command:
@servers(['web' =><EMAIL_ADDRESS>@task('deploy', ['on' => 'web'])
cd /home/user/example.com
@if ($branch)
git pull origin {{ $branch }}
@endif
php artisan migrate --force
@endtask
Stories
Stories group a set of tasks under a single, convenient name. For instance, a deploy
story may run the update-code
and install-dependencies
tasks by listing the task names within its definition:
@servers(['web' =><EMAIL_ADDRESS>@story('deploy')
update-code
install-dependencies
@endstory
@task('update-code')
cd /home/user/example.com
git pull origin master
@endtask
@task('install-dependencies')
cd /home/user/example.com
composer install
@endtask
Once the story has been written, you may invoke it in the same way you would invoke a task:
php vendor/bin/envoy run deploy
Completion Hooks
When tasks and stories finish, a number of hooks are executed. The hook types supported by Envoy are @after
, @error
, @success
, and @finished
. All of the code in these hooks is interpreted as PHP and executed locally, not on the remote servers that your tasks interact with.
You may define as many of each of these hooks as you like. They will be executed in the order that they appear in your Envoy script.
@after
After each task execution, all of the @after
hooks registered in your Envoy script will execute. The @after
hooks receive the name of the task that was executed:
@after
if ($task === 'deploy') {
// ...
}
@endafter
@error
After every task failure (exits with a status code greater than 0
), all of the @error
hooks registered in your Envoy script will execute. The @error
hooks receive the name of the task that was executed:
@error
if ($task === 'deploy') {
// ...
}
@enderror
@success
If all tasks have executed without errors, all of the @success
hooks registered in your Envoy script will execute:
@success
// ...
@endsuccess
@finished
After all tasks have been executed (regardless of exit status), all of the @finished
hooks will be executed. The @finished
hooks receive the status code of the completed task, which may be null
or an integer
greater than or equal to 0
:
@finished
if ($exitCode > 0) {
// There were errors in one of the tasks...
}
@endfinished
Running Tasks
To run a task or story that is defined in your application's Envoy.blade.php
file, execute Envoy's run
command, passing the name of the task or story you would like to execute. Envoy will execute the task and display the output from your remote servers as the task is running:
php vendor/bin/envoy run deploy
Confirming Task Execution
If you would like to be prompted for confirmation before running a given task on your servers, you should add the confirm
directive to your task declaration. This option is particularly useful for destructive operations:
@task('deploy', ['on' => 'web', 'confirm' => true])
cd /home/user/example.com
git pull origin {{ $branch }}
php artisan migrate
@endtask
Notifications
Slack
Envoy supports sending notifications to Slack after each task is executed. The @slack
directive accepts a Slack hook URL and a channel / user name. You may retrieve your webhook URL by creating an "Incoming WebHooks" integration in your Slack control panel.
You should pass the entire webhook URL as the first argument given to the @slack
directive. The second argument given to the @slack
directive should be a channel name (#channel
) or a user name (@user
):
@finished
@slack('webhook-url', '#bots')
@endfinished
By default, Envoy notifications will send a message to the notification channel describing the task that was executed. However, you may overwrite this message with your own custom message by passing a third argument to the @slack
directive:
@finished
@slack('webhook-url', '#bots', 'Hello, Slack.')
@endfinished
Discord
Envoy also supports sending notifications to Discord after each task is executed. The @discord
directive accepts a Discord hook URL and a message. You may retrieve your webhook URL by creating a "Webhook" in your Server Settings and choosing which channel the webhook should post to. You should pass the entire Webhook URL into the @discord
directive:
@finished
@discord('discord-webhook-url')
@endfinished
Telegram
Envoy also supports sending notifications to Telegram after each task is executed. The @telegram
directive accepts a Telegram Bot ID and a Chat ID. You may retrieve your Bot ID by creating a new bot using BotFather. You can retrieve a valid Chat ID using @username_to_id_bot. You should pass the entire Bot ID and Chat ID into the @telegram
directive:
@finished
@telegram('bot-id','chat-id')
@endfinished


Chapter 11 Lab 11: Mixed Factorial ANOVA
No amount of experimentation can ever prove me right; a single experiment can prove me wrong —Albert Einstein
11.1 Do you remember things better when you take pictures of them?
People take pictures of things all the time on their phones. Barasch et al. (2017) asked whether taking pictures of things had consequences for later memory of those experiences.
11.1.1 Study description
In Experiment 1, participants visited a museum exhibit. Half of the participants were allowed to take photographs (with camera, at least 10 pictures) and the other half were not (no camera). They freely looked at anything in the exhibit, and were allowed to take pictures of anything they wanted (if they were in the camera condition). Additionally, while visiting the exhibit, participants listened to audio guides about the things the were looking at.
After participants were done with the exhibit the returned to the sign-in desk. At this point they were given two memory tests for the things they saw and heard in the exhibit. They were given a visual recognition test containing pictures of objects, and were asked to identify which objects they remembered seeing. They were also given an auditory recognition test containing statements that could have been on the audio guide, and they had to identify which ones they had heard before.
This is a 2x2 mixed design. IV 1 was a between-subjects manipulation involving picture-taking (camera vs. no camera). IV2 was a within-subject manipulation of memory test (visual vs. audio). The dependent measure was performance on the memory test.
An overarching question was whether or not participants would have better visual memory for exhibit objects when they took pictures, compared to when they didn’t. Additionally, taking pictures or not, may have no influence on memory for the statements in the audio guide.
11.2 Lab Skills Learned
- Conducting a 2x2 mixed design ANOVA
11.3 Important Stuff
- citation: Barasch, A., Diehl, K., Silverman, J., & Zauberman, G. (2017). Photographic memory: The effects of volitional photo taking on memory for visual and auditory aspects of an experience. Psychological science, 28(8), 1056-1066.
- Link to .pdf of article
- Data in .csv format
11.4 JAMOVI
In this lab, we will use jamovi to conduct and graph a Mixed-Factorial Analysis of Variance (ANOVA)
11.4.1 Experiment Background
People take pictures of things all the time on their phones. Barasch et al. (2017) asked whether taking pictures of things had consequences for later memory of those experiences.
In this experiment participants visited a museum exhibit. Half the participants were able to use a camera to document their visit, while the other half were not, all while listening to an audio tour of the exhibit. At the end of the visit, everyone was given two memory tests (visual and audio) for the content they saw and heard, respectively.
This is a 2x2 Mixed-Factorial design. The individuals in the photo group are different than the individuals in the no photo group (this is our between-subjects variable–it is called condition
), while the memory test_type
(audio and visual) is our within-subjects variable since everyone took both types of tests.
11.4.2 Conduct a Mixed-Factorial Analysis of Variance (ANOVA)
Open the data file linked here. It is called “study1_data_photo.sav”. Scroll through the file. Find the variable named condition
. This variable tells you if the row in question corresponds to a person who was or was not able to use a camera. Now, find the variables apercent
and vpercent
. These variables refer to the percentage score received by everyone on the audio and visual memory tests, respectively.
Notice that every row in the data file only has ONE “condition” label. That is, you were either in the camera or no camera condition. BUT, everyone in the file has scores for BOTH tests, audio and visual. This is the way your data must be structed in jamovi in order to perform a mixed-factorial ANOVA. To conduct a mixed-design ANOVA with post-hoc tests in jamovi, follow these steps, and you will see the rght side of the screen update with the chosen analyses and statistics:
Let’s look at our output tables. Based on its values, we can tell that:
There is a significant main effect of test type, F(1, 295)=108.59, p<.05. Overall, memory test scores were higher for the audio test than the video test.
There is a significant ineraction effect between test type and condition, F(1, 295)=13.79, p<.05. People taking photos did worse on the audio test than people without photos, however, on the visual test, people taking photos did better than those who did not take photos.
There is no significant main effect of condition, F(1, 295)=2.26, p=NS.
11.4.3 Practice Problems
- Using the same data file we used for this lab’s tutorial, run a Mixed-Factorial ANOVA using test type (audio and visual) and Gender (Male, Female). Use an alpha level of .05. Report your results in standard statistical reporting format.


Optional wrapper for cache keys to provide support for custom affinity mapping. The value returned by Affinity will be used for key-to-node affinity.
More...
| Apache.Ignite.Core.Cache.Affinity.AffinityKey.AffinityKey |
( |
object |
key | ) |
|
| Apache.Ignite.Core.Cache.Affinity.AffinityKey.AffinityKey |
( |
object |
key, |
|
|
object |
affinity |
|
) |
| |
- Parameters
-
| key | The key. |
| affinity | The affinity key. |
| bool Apache.Ignite.Core.Cache.Affinity.AffinityKey.Equals |
( |
AffinityKey |
other | ) |
|
- Parameters
-
| other | An object to compare with this object. |
- Returns
- true if the current object is equal to the other parameter; otherwise, false.
| override bool Apache.Ignite.Core.Cache.Affinity.AffinityKey.Equals |
( |
object |
obj | ) |
|
- Parameters
-
| obj | The object to compare with this instance. |
- Returns
true
if the specified object is equal to this instance; otherwise, false
.
| override int Apache.Ignite.Core.Cache.Affinity.AffinityKey.GetHashCode |
( |
| ) |
|
- Returns
- A hash code for this instance, suitable for use in hashing algorithms and data structures like a hash table.
- Parameters
-
| left | The left. |
| right | The right. |
- Returns
- The result of the operator.
- Parameters
-
| left | The left. |
| right | The right. |
- Returns
- The result of the operator.
| override string Apache.Ignite.Core.Cache.Affinity.AffinityKey.ToString |
( |
| ) |
|
- Returns
- A string that represents this instance.
| void Apache.Ignite.Core.Cache.Affinity.AffinityKey.WriteBinary |
( |
IBinaryWriter |
writer | ) |
|
| object Apache.Ignite.Core.Cache.Affinity.AffinityKey.Affinity |
|
get |
| object Apache.Ignite.Core.Cache.Affinity.AffinityKey.Key |
|
get |


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{{> components/head }} {{> components/nav }}the right lube is a platform for thoughts by Maz Murray and Hava Carvajal,
plus anyone else who wants to join in!
contact us at<EMAIL_ADDRESS>{{config.details.bubbletwo}}


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A static import statement was introduced in Java 5. With static import statements, you can omit the class name when using static members.
package net.java_school.examples; import static java.lang.Math.*; public class StaticImportTest { public static void main(String[] args) { System.out.println(sqrt(4));//You can omit Math. } }
2.0
import java.util. *;
In the above import statement, * means all types in the java.util package.
import static java.lang.Math. *;
In the above import statement, * means all static members of the Math class.
If you only want the sqrt() method of the Math class, modify the import statement as follows:
import static java.lang.Math.sqrt;


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WITNESS LIST Insurance Committee February 23, 1999-2:00P overview on OPIC On: Bordelon, Rod (Office of Public Insurance Counsel) overview on TDI On: Montemayor, Jose (Texas Department of Insurance) overview on TIPA On: Jobe, Clark (Texas Insurance Purchasing Alliance)


Inside, the inn was every bit as busy as the sounds coming from it had indicated and more. The party from Emond’s Field followed Master Fitch through the back door, soon weaving around and between a constant stream of men and women in long aprons, platters of food and trays of drink held high. The bearers murmured quick apologies when they got in anyone’s way, but they never slowed by a step. One of the men took hurried orders from Master Fitch and disappeared at a run.
“The inn is near full, I’m afraid,” the innkeeper told Moiraine. “Almost to the rafters. Every inn in the town is the same. With the winter we just had . . . well, as soon as it cleared enough for them to get down out of the mountains we were inundated—yes, that’s the word—inundated by men from the mines and smelters, all telling the most horrible tales. Wolves, and worse. The kind of tales men tell when they’ve been cooped up all winter. I can’t think there’s anyone left up there at all, we have that many here. But never fear. Things may be a little crowded, but I’ll do my best by you and Master Andra. And your friends, too, of course.” He glanced curiously once or twice at Rand and the others; except for Thom their clothes named them country folk, and Thom’s gleeman’s cloak made him a strange traveling companion as well for “Mistress Alys” and “Master Andra”. “I will do my best, you may rest assured.”
Rand stared at the bustle around them and tried to avoid being stepped on, though none of the help really seemed to be in any danger of that. He kept thinking of how Master al’Vere and his wife tended the Winespring Inn with sometimes a little assistance from their daughters.


By MICHAEL D. SHEAR
President Obama’s self-assured State of the Union address reflected his sense of being liberated and emboldened, White House aides said.


The "Guide Me" mode walks you through benchmarks for various methods of loading data in RIAs. This includes descriptions of each method and explanations for the results. The "Navigator" mode allows you to run the benchmarks on your own. To continue in "Guide Me" mode click the next button above, or select the benchmark from the dropdown.
Note: You can see the output of the last benchmark by selecting the "Output" panel on the right. To see all the timings that go into the running averages displayed by the charts, select the "Data" tab on the right.


{% autoescape true %}
Home
Admin
Import
Name
Min Players
Max Players
Min Time
Max Time
Rating
BGG ID
Save
Delete
{% endautoescape %}


I was recently working on a project that used WCF web services extensively. Everything was ready for deployment, I deployed to the remote host, and voila – nothing works (nothing WCF related). After a LOT of frustration, I managed to make it work. I found two areas which were causing the problem:
1. The .svc extension was NOT setup right at our host. You can set this in the web.config webhandlers section for IIS 7, but not for IIS 6.0. I had IIS 7, but decided to bug my host to set up the extension on the server ;)
2. I had multiple host headers; i.e. my site worked for both http://mysite.com and http://www.mysite.com. To resolve this issue, you can either disable all but one if your host permits. Otherwise, you need to use a factory. Here’s an example of such a factory:
using System; using System.Collections.Generic; using System.Linq; using System.Web; using System.ServiceModel; using System.ServiceModel.Activation; namespace Shipping.WebService { public class MultipleIISBindingSupportServiceHostFactory : ServiceHostFactory { protected override ServiceHost CreateServiceHost(Type serviceType, Uri[] baseAddresses) { Uri[] requiredAddress = GetAppropriateBase(baseAddresses); return base.CreateServiceHost(serviceType, requiredAddress); } Uri[] GetAppropriateBase(Uri[] baseAddresses) { List<Uri> retAddress = new List<Uri>(); retAddress.Add(baseAddresses[0]); return retAddress.ToArray(); } } }
Granted, it can be way more efficient and you can do nifty tricks with the url to support both http:// and http://www, but I can happy to have just one for my webservice.
Next, you need to set the factory in the markup of the ,svc file. You can do it like this:
<%@ ServiceHost Language="C#" Debug="false" Factory="Shipping.WebService.MultipleIISBindingSupportServiceHostFactory" Service="Shipping.WebService.ClientService" CodeBehind="ClientService.svc.cs" %>
Hope that helps.


Donec elementum mi vitae enim fermentum lobortis. In hac habitasse platea dictumst. Ut pellentesque, orci sed mattis consequat, libero ante lacinia arcu, ac porta lacus urna in lorem. Praesent consectetur tristique augue, eget elementum diam suscipit id.
Interdum et malesuada fames ac ante ipsum primis in faucibus. Nam condimentum laoreet sagittis. Duis quis ullamcorper leo. Suspendisse potenti.
Template comes with five color themes (Blue, Orange, Green, Red and Grey). All you need to do is to use relevant CSS file.
There is no color scheme that matches your branding? No problem. You can easily compile your own by changing one variable - thanks to LESS!
This template is build taking the advantage of LESS. It makes easier to build your own color schemes.
We are also using lesshat mixins which makes development even more easier. Please check http://lesshat.com for more information
It looks great on desktops, laptops, tablets and smartphones - mPurpose template was built to shine on all devices :)
You can be sure that all the components are responsive.
Template comes with 247 flag icons representing most countries in the world


Pink Taco founder and Lindsay Lohan's ex Harry Morton dies aged 38
The founder of Pink Taco has died after being found unresponsive at home, TMZ reports.
Harry Morton, who previously dated Lindsay Lohan, is understood to have been found by a relative yesterday.
The businessman was the son of Hard Rock Cafe co-founder Peter Morton.
An autopsy is pending, and foul play is not said to be suspected.
Mr Morton was pronounced dead at the scene in Beverly Hills after he was found by a relative.
As well as dating Ms Lohan in the 2000s, he was also since linked to Demi Moore, Britney Spears and Paris Hilton.
He founded LA-based Pink Taco in 1999 aged just 18.
In 2008, he also bought Hollywood nightclub the Viper Room.
Mr Morton survived by both of his parents, Peter Morton and Paulene Stone.
A Pink Taco spokesman said: ‘We are saddened by the passing of Harry Morton, the founder and former owner of Pink Taco.
Advertisement Advertisement
‘Harry was a visionary and restaurateur ahead of his time, and his contributions, both professionally to our brand and personally to those he worked with, were numerous.
‘Our thoughts and condolences are with his family and friends during this difficult time.’
Got a story for Metro.co.uk?
Get in touch with our news team by emailing us at<EMAIL_ADDRESS>For more stories like this, check our news page.


{% assign first_two_services = include.events | slice:0, 2 %} {% assign remaining_services = include.events | slice:2, 100 %} {{ event.name }} 2019 {%- for event in include.events -%} {{ event.date }} {{ event.time }} {{ event.title }} {{ event.description }} {%- endfor -%} More Events Fewer Events


D3 is a JavaScript library which can use data to manipulate HTML and SVG. This makes it a powerful tool for building data visualisations.
D3 does not provide a standard set of charting options 'out of the box'. Instead it provides lower-level functions for data transformation, physics, and HTML or SVG manipulation.
Although D3 has a somewhat steep learning curve this can be attributed to its specialised purpose which is quite unlike any other JavaScript libraries. With some basic familiarity it is a greatly expressive and efficient library to work with.
This is a simple demo to see D3 in action. Here we draw a simple bar chart with HTML elements.
Inspect this chart with your browser's developer tools.
You will see that the #chart1
element contains a separate <div>
for each of the eight random values in the data set and their heights are determined by those values.
Also see the documented source code in source/chart1.js
An issue which you might have noticed in Chart 1 is that the chart height relates directly to the largest data value.
For example in
source/chart1.js
, changeconst max = 1000;
.
You will see that the chart is rendered much taller because the values are much larger numbers.This leads us into Chart 2 which introduces scales.
A simple HTML bar chart with scaling of the bar heights.
Here we use d3.scaleLinear
determine the bar heights.
No matter what the largest value is, its bar will have a height of 100 pixels.
D3 also provides other scale types such as time, and logarithmic. See the D3 scale documentation for details.
See the documented source code in source/chart2.js
Scales are one of the most frequently used features of D3.
In essence a scale accepts a number within an expected 'domain' (between a minimum and maximum) and returns a number within an expected 'range'.
For example, a scale with a domain of
[-100, 100]
and a range of[0, 1]
would return values like below:
Input value Return value -100 0 0 0.5 100 1
A simple line chart which plots values over time. This renders an inline SVG and draws a path from the data. SVG graphics are used because they offer much more visual features than plain HTML elements.
A linear scale is used here to scale the X axis to the chart height and a time scale is used to scale Y axis to the chart width.
The path drawn with a straight lines between points but it is also possible to specify other curve functions. See the D3 curves documentation for details.
See the documented source code in source/chart3.js
A heatmap which plots values over time.
D3 provides an extensive set of interpolations functions for blending between to values.
Here we use d3.interpolateRgb
to determine which colour each tile should be based on its value.
See the D3 interpolate documentation for details.
See the documented source code in source/chart4.js


Domains are computers/devices that share difference types of data. These domains can be administered and accessed with a common set of rules.
There are often many confusing terms that sound similar that are also used interchangeably including Domains, Domain Names, URLs and Web addresses, but what are all of these? Simply put, a domain name is your web address, and your web address is a URL. We use these domains as a type of address to identify where your webpage lives.
An example of a domain would be www.google.com or www.github.com. These URL's point to a certain web address which is stored in a server. This is more practical than remembering the long numerical IP address for your website.
Learn more about domainsICANN Stands for the Internet Corporation for Assigned Names and Numbers. They are the nonprofit org that coordinates the maintenance and upkeep of many crucial databases. They are the group that performs the technical maintenance to ensure the networks stable and secure operation
They are the group that performs the technical maintenance to ensure the networks stable and secure operation and are vital to keeping our networks and systems healthy.
They were founded more than 2 decades ago and have been very involved with developing policies on the internalization of the DNS system. The image above is their logo which you may have seen before!
Read more about ICANN


Mysore
Facts about Mysore:
- The sprawling city of Mysore is a delight to explore thanks to its eclectic mix of fine old colonial architecture; regal Indian palaces; and lush, well-manicured gardens.
- While those inclined towards shopping will enjoy spending time in the city's famous silk and sandalwood bazaars, the main attraction is magnificent Mysore Palace.
- Completely rebuilt in 1897 after a devastating fire, this beautiful three-storied palace features highlights such as its elegant square towers and domes; the many ornate ceilings and pillars in Durbar Hall; and the splendid Marriage Pavilion, with its glazed floor tiles, stunning stained glass, artworks, and displays of jewelry (it's also where, on special occasions, the exquisite Golden Throne is exhibited).
Excursion:
- For a real treat, be sure to catch one of the splendid light displays held each Sunday and during holidays, when the palace is illuminated by more than 90,000 lights. A fun way to explore the palace's massive grounds and gardens is as part of a cycle tour, available free once inside.


Objects being serialized over a REST endpoint may contain references to other objects. It is frequently required to
serialize the referenced objects as well. This sample uses two classed named
Company
and
Project
with a one-to-many
association from the former to the later.
To see a sample object graph represented as JSON make a regular HTTP GET request to
/graph.json
on this server.


Id: 21
Name: Aqua Morty
Status: unknown
Species: Humanoid
Type: Fish-Person
Gender: Male
OriginName: unknown
OriginUrl:
LocationName: Citadel of Ricks
LocationUrl: https://rickandmortyapi.com/api/location/3
Image: https://rickandmortyapi.com/api/character/avatar/21.jpeg
Episode: ['https://rickandmortyapi.com/api/episode/10', 'https://rickandmortyapi.com/api/episode/22']
Url: https://rickandmortyapi.com/api/character/21
Created: 2017-11-04T22:39:48.055Z


@(acceptanceForm: Form[Acceptance]) @import helper._ @main("What ya want to do?") { @form(action = routes.Application.accept()) {
Maybe it's Thursday, maybe Friday..


"ADRAMYTTIUM "a city of Asia Minor on the coast of Mysia, which in early times was called AEolis. The ship in which Paul embarked at Caesarea belonged to this city (Acts 27:2). He was conveyed in it only to Myra, in Lycia, whence he sailed in an Alexandrian ship to Italy. It was a rare thing for a ship to sail from any port of Palestine direct for Italy. It still bears the name Adramyti, and is a place of some traffic.
"ADRAMYTTIUM "a city of Asia Minor on the coast of Mysia, which in early times was called AEolis. The ship in which Paul embarked at Caesarea belonged to this city (Acts 27:2). He was conveyed in it only to Myra, in Lycia, whence he sailed in an Alexandrian ship to Italy. It was a rare thing for a ship to sail from any port of Palestine direct for Italy. It still bears the name Adramyti, and is a place of some traffic.


How to fix iPhone 11 overheating issues
by Svetlana MilWhen it comes to smartphones in general, there is an issue many people complain about – overheating. There is a wide range of things to try on your own, and if you own iPhone 11 you landed on the right page. In this article, we are going to share a guide and show you how to fix iPhone 11 overheating issues.
What you need to keep in mind is that the way you use your device has a huge impact on its battery life and the temperature. So, before we list the solutions, here are a few quick tips:
- Avoid using your phone when it is charging
- Avoid direct sunlight
- If you love playing games, pause after an hour. Gaming apps are very demanding, and every demanding app affects the battery and the temperature.
- If you are using a case or a cover for your iPhone, remove it.
- Turn off Bluetooth, Wi-Fi, and GPS when not in use.
- Whenever you notice that your device is getting hot, leave it to cool off. Using it when it is already hot can cause damage.
See also: How to fix iPhone 11 Wi-Fi issues
How to fix iPhone 11 overheating issues
Solution 1: Restart your iPhone
As we already suggested, when you notice your iPhone is getting hot, you should let it cool off first. Once it is back to normal, restart it. A restart will close the processes and apps that run in the background. Also, it will refresh the memory of the phone.
Solution 2: All about apps
Smartphones would not be fun without apps, right? So, everything goes around apps. The first thing you should do is see how the apps behave. You can do that by viewing Battery usage information. Go to Settings > Battery > Background Activity. There, you can see how the apps behave in the background and how they affect battery life. Usually, the apps that affect battery life the most are the ones that can cause overheating as well. You may turn off Background activity for the apps you want.
 This is a pretty simple thing to do but you may find it effective.
Solution 4: Update the apps
As we mentioned before, it is all about apps. So, now you know the background activity, you have removed the apps you don’t use, it is the time to update the ones you have. Open the App Store and choose the option to update all.
Solution 5: Update the software
People often forget how important software updates are. When you think about an update, you are usually focused on new features. But, software updates are more than new features. Every new version includes security patches, and most importantly, bug fixes. Here is what you need to do:
- Go to Settings
- Tap General
- Tap Software update.
If there is a new version, tap Download and Install.
Solution 6: Reset all settings
To reset all settings on your device, follow the steps:
- Go to Settings > General > Reset
- Tap Reset all settings
- Enter your passcode
- Tap Reset all settings to confirm.
Solution 7: Erase all content and settings
A factory reset is another thing for you to try, but first, create a backup because the settings will go to factory defaults and data will be erased. When you complete this, do the following:
- Navigate to Settings
- Tap General
- Tap Reset
- Choose Erase all content and settings option
- Enter your passcode
- Tap Erase iPhone to confirm.
When all of it is done, follow the steps to set up your iPhone 11 as a new device.
If you still experiencing overheating, contact Apple.


Tours will leave from the meeting place at the scheduled time. If you will be late for the tour, please contact Tokyo Handsome Boys as soon as possible through the site's contact form. When you have arrived at the meeting point, one of the tour guides will come to pick you up and take you to the current tour spot. If you miss the tour completely, unfortunately, we cannot offer you a refund.
If you are unable to participate in a tour, you must cancel by 3 days before the tour (so if the tour is on 5/24, for example, you must cancel by 5/21). If you cancel within 2 days before the tour, there is a 50% cancellation fee, so half of the tour cost will be refunded. If you cancel on the day of the tour, there will be a 100% cancellation fee. If you are unable to attend a tour and don't want to cancel, you are free to send a substitute to go on the tour in your place. There is no deadline for assigning a substitute, but please let us know sometime before the tour. Please note that we may not be able to accomodate that person's allergies and tastes if we are informed of them within 24 hours of the tour.
We will begin booking a custom tour as soon as the reservation comes in. As such, we must be strict about cancellation. Because it will take us at least five days to plan the tour, we must charge a 100% cancellation fee for all cancellations within five days before the tour (so if the tour is on 5/24, for example, you must cancel by 5/19). In addition, if you wish to change a destination for the custom tour, you must do so by three days prior to the tour. Because Custom Tours are charged on a group basis, we are still able to carry out the tour even with a decreased number of participants; however, if a member cannot attend, feel free to send a substitute in your place without an additional fee. However, we cannot guarantee that we can change a destination to accommodate that person's allergies and tastes if we are informed within three days of the tour.
The director and staff of Tokyo Handsome Boys, are released from, and specifically disclaim, all responsibilities for injuries or illness incurred traveling to and from tours, during tours, or resulting from food prepared at any restaurant included in the tour or otherwise eaten together with Tokyo Handsome Boys members. Tour fees do NOT INCLUDE food & beverage not specifically mentioned in the program description, or the cost of local transportation when not specifically mentioned. Participants in all programs are responsible for making arrangements for, and making payment for, their airfare, lodgings, and transportation to/from/within Japan. Participants are also responsible for obtaining and paying for any travel/trip/health insurance coverage they would like to have.
All content on this website is ©2017 Tokyo Handsome Boys. Copying and use of any and all materials without permission is prohibited.


{% trans
irc_channel="https://client02.chat.mibbit.com/?server=irc.mozilla.org&channel=%23sumo",
reddit="http://reddit.com/r/firefox",
twitter="https://twitter.com/firefox" %}
This site will have limited functionality while we undergo maintenance to
improve your experience. If an article doesn't solve your issue and you want
to ask a question, we have our support community waiting to help you at @firefox on
Twitter, /r/firefox on Reddit, or live on our IRC channel #sumo.
{% endtrans %}


Lisense
Licenses sometimes have little sense. Too often they're difficult to read, incredibly long and full of legal traps.
Lisense is a simple web app that aims to improve the world of licenses.
Paste a license below:
More? Search for Terms of Service / EULA / License.
by: @nbartlomiej


This is an attractive seaside town just east of Cap Frehel, 8nm west of St Malo. It now provides one of the few all tide ports in this area. There an attractive path has been built along the base of the cliffs, into the town.
Position 48° 38'12"N , 02º 14'48"W (marina)
St Cast Marina ©St Cast Marina
The building of a breakwater joining several rocky islets to the existing breakwater, has allowed an all tide marina to be created here.
The bay in front of the town still provides an anchorage, but unless of shoal draft, it is quite a distance from the shore and rather exposed.
The access channel to the marina runs parallel to the extended breakwater. On rounding the head of the breakwater the port entrance is situated between the Bec Rond Rock (+5 metres) and the La Feuillade Rock. To the East, a pontoon for fishing boats and three pontoons for large pleasure craft run perpendicular to the quay where the port is dredged to a depth of 2.25m below chart datum. To the West, five pontoons, with a depth of 1.25m below chart datum, run parallel to the Vallets shore platform.
A Cardinal South perch marker marks the southern extremity of the breakwater separating the marina from the swinging moorings to the west, and which is submerged at high water.
In the marina, mooring officers (English speaking) available 7/7 from 08:00 to 21:00 during the season to greet incoming boats and guide them to their berths.
Last updated July 2016.


Welcome to the Express Playground!
Use this interactive code editor to learn all the basic parts of an Express app.
As you type, the images on the right side will change depending on your code. You can also hover over text within the editor to learn more about it.
We will compare an Express app to running a restaurant. If you want more background, check out this guide called "Express.js Explained by Eating at a Restaurant"
const express = require('express');
const app = express();
app.use('/table', function(req, res, next){
let shirt = req.shirt;
let shoes = req.shoes;
if(shirt && shoes){
next();
}
});
app.get('/table/:amount', function(req,res){
let party = req.params.amount;
res.send('We are searching for your table for ' +party+'!');
});
app.listen(8080, function(){
console.log('We are open for business!');
});
Please fix errors!
The Manager/ Express
"Hi, my name is app."
"I make the rules."
Seating Rules/ Middleware
1. Must have shirt
2. Must have shoes
Seating Guests/ GET route
"I need to find a table for (amount)"
Restaurant Address/ Port
"We are open for business at 8080!"


#include "xtfile.h"
#include "xfs.h"
#include "xep_hal.h"
#include "xtmemory.h"
#include "xtsemaphore.h"
#include "task_monitor.h"
#include <FreeRTOS.h>
#include <task.h>
#include <string.h>
Functions | |
| static bool | xtfile_lock (void) |
| static void | xtfile_unlock (void) |
| static uint32_t | xtfile_create_instance (void **handle, uint32_t type, uint32_t identifier) |
| static uint32_t | xtfile_free_instance (void *handle) |
| static bool | xtfile_is_open (uint32_t type, uint32_t identifier) |
| static uint32_t | xtfile_close_all_files (void) |
| uint32_t | xtfile_init (XepDispatch_t *dispatch, uint32_t address, uint32_t size) |
| Initialize the file system. More... | |
| uint32_t | xtfile_uninit (void) |
| Uninitialize the file system. More... | |
| uint32_t | xtfile_format (uint32_t format_key) |
| Formats the file system. More... | |
| uint32_t | xtfile_get_largest_free_size (uint32_t *size) |
| Gets the largest free section of space in the file system. More... | |
| uint32_t | xtfile_get_size (uint32_t type, uint32_t identifier, uint32_t *size) |
| Gets the size of the file with the specified type and identifier. More... | |
| uint32_t | xtfile_find_all_files (uint32_t *type, uint32_t *identifier, uint32_t max_count, uint32_t *count) |
| Finds all files and stores the type and identifier of each file in the given buffers. More... | |
| uint32_t | xtfile_search_for_files_of_type (uint32_t type, uint32_t *identifier, uint32_t max_count, uint32_t *count) |
| Searches for and returns a list of identifiers for all files of the specified type. More... | |
| uint32_t | xtfile_create_and_open_empty (void **handle, uint32_t type, uint32_t identifier, uint32_t size) |
| Creates and opens a new file with given type and identifiers with an empty content of given size. More... | |
| uint32_t | xtfile_create_and_open (void **handle, uint32_t type, uint32_t identifier, void *data, uint32_t size) |
| Creates and opens a new file with given type and identifiers with the contents provided in the data buffer of given size. More... | |
| uint32_t | xtfile_delete (uint32_t type, uint32_t identifier) |
| Deletes the file with the specified type and identifier. More... | |
| uint32_t | xtfile_get_handle (void **handle, uint32_t type, uint32_t identifier) |
| uint32_t | xtfile_open (void **handle, uint32_t type, uint32_t identifier) |
| Opens an existing file with given type and identifier. More... | |
| uint32_t | xtfile_get_buffer (void *handle, void **data, uint32_t *size) |
| Gets the pointer and size of the content of the file. More... | |
| uint32_t | xtfile_clear (void *handle) |
| Clears the entire file contents. More... | |
| uint32_t | xtfile_write (void *handle, void *data, uint32_t offset, uint32_t size) |
| Writes data to file. More... | |
| uint32_t | xtfile_close (void *handle) |
| Closes an open file. More... | |
Variables | |
| void * | xtfile_lock_object = NULL |
| FileInstance_t | file_instance [XTFILE_MAX_OPEN_FILES] |
| uint32_t xtfile_clear | ( | void * | handle | ) |
Clears the entire file contents.
Must be done prior to writing.
| handle | Handle of open file |
| uint32_t xtfile_close | ( | void * | handle | ) |
Closes an open file.
| handle | Handle of open file to close |
|
static |
| uint32_t xtfile_create_and_open | ( | void ** | handle, |
| uint32_t | type, | ||
| uint32_t | identifier, | ||
| void * | data, | ||
| uint32_t | size | ||
| ) |
Creates and opens a new file with given type and identifiers with the contents provided in the data buffer of given size.
| handle | Pointer to handle for opened file |
| type | Type of file |
| identifier | Identifier of file |
| data | Buffer holding the data to write to the new file |
| size | Size of the new file |
| uint32_t xtfile_create_and_open_empty | ( | void ** | handle, |
| uint32_t | type, | ||
| uint32_t | identifier, | ||
| uint32_t | size | ||
| ) |
Creates and opens a new file with given type and identifiers with an empty content of given size.
| handle | Pointer to handle for opened file |
| type | Type of file |
| identifier | Identifier of file |
| size | Size of the new file |
|
static |
| uint32_t xtfile_delete | ( | uint32_t | type, |
| uint32_t | identifier | ||
| ) |
Deletes the file with the specified type and identifier.
| type | Type of file |
| identifier | Identifier of file |
| uint32_t xtfile_find_all_files | ( | uint32_t * | type, |
| uint32_t * | identifier, | ||
| uint32_t | max_count, | ||
| uint32_t * | count | ||
| ) |
Finds all files and stores the type and identifier of each file in the given buffers.
| type | Pointer to list for types |
| identifier | Pointer to list for identifiers |
| max_count | Max number of list |
| count | Pointer to variable to hold count of files |
| uint32_t xtfile_format | ( | uint32_t | format_key | ) |
Formats the file system.
|
static |
| uint32_t xtfile_get_buffer | ( | void * | handle, |
| void ** | data, | ||
| uint32_t * | size | ||
| ) |
Gets the pointer and size of the content of the file.
The content of the buffer is located in flash and can not be modified directly, but this can be done by using xtfile_clear and xtfile_write commands. The size of the file can not be changed, and must be done by deleting and creating a new file.
| handle | Handle of open file |
| data | Pointer to flash location |
| size | Pointer to variable to hold size of file |
| uint32_t xtfile_get_handle | ( | void ** | handle, |
| uint32_t | type, | ||
| uint32_t | identifier | ||
| ) |
| handle | Pointer to handle for opened file |
| type | Type of file to get handle for |
| identifier | Identifier of file to get handle for |
| uint32_t xtfile_get_largest_free_size | ( | uint32_t * | size | ) |
Gets the largest free section of space in the file system.
This is the largest file that can be created without deleting files or defragmenting.
| size | Pointer to variable to hold size |
| uint32_t xtfile_get_size | ( | uint32_t | type, |
| uint32_t | identifier, | ||
| uint32_t * | size | ||
| ) |
Gets the size of the file with the specified type and identifier.
| type | Type of file |
| identifier | Identifier of file |
| size | Pointer to variable to hold size |
| uint32_t xtfile_init | ( | XepDispatch_t * | dispatch, |
| uint32_t | address, | ||
| uint32_t | size | ||
| ) |
Initialize the file system.
| dispatch | Pointer to the dispatcher |
| address | Address of application storage |
| size | Size of application storage |
|
static |
|
static |
| uint32_t xtfile_open | ( | void ** | handle, |
| uint32_t | type, | ||
| uint32_t | identifier | ||
| ) |
Opens an existing file with given type and identifier.
| handle | Pointer to handle for opened file |
| type | Type of file |
| identifier | Identifier of file |
| uint32_t xtfile_search_for_files_of_type | ( | uint32_t | type, |
| uint32_t * | identifier, | ||
| uint32_t | max_count, | ||
| uint32_t * | count | ||
| ) |
Searches for and returns a list of identifiers for all files of the specified type.
| type | Type of file to search for |
| identifier | Pointer to list for identifiers |
| max_count | Max number of identifiers for list |
| count | Pointer to variable to hold count of files |
| uint32_t xtfile_uninit | ( | void | ) |
Uninitialize the file system.
|
static |
| uint32_t xtfile_write | ( | void * | handle, |
| void * | data, | ||
| uint32_t | offset, | ||
| uint32_t | size | ||
| ) |
Writes data to file.
Make sure file contents is cleared before writing.
| handle | Handle of open file |
| data | Pointer to data to write |
| offset | Offset from file start |
| size | Size to write |
| FileInstance_t file_instance[XTFILE_MAX_OPEN_FILES] |
| void* xtfile_lock_object = NULL |


servREC
(service in module tri
)
Specific I/O services for REC mode tables
This service also contains many of the common functions with servTBL
directly accessed by the
support routines via the servREC.
prefix.
Refer to Record Storage for a description of the record modes and to servCRUD for the API common functions.
Used internally for the retrieval and update methods to maintain the cache of Data Objects when they are organized as chunks. See Records Storage to understand 'chunks'.
oTP – {Object} –
The Table.props
where the object array is store.
objs – {Object[]} –
The array of Data Objects to store.
chunk – {number} –
The chunk index relative to 0.
Used internally. The oCol
type is assumed to be 'property'. The user is prompted to
name a unique property within the oCol
properties array. When validated a key of the returned user value is created
of null value. Used to create key/value pairs within a column of type 'property'.
The validation cycle is used later to validate the value of a key/value pair.
oTP – {Object} –
The Table.props
values where the column array is stored
oCol – {Object} –
The dynamic Col object
Used internally. Returns the Col object whose col
property
matches the sCol
parameter. Null is returned if not found.
oTP – {Object} –
The Table.props
values where the column array is stored
sCol – {string} –
The column name to find
{Object}
– oCol The dynamic Col object if found or null if not found.
Gets the current editor for the current selected Data Object. In actuality this is the $scope pointer for the Edit Controller.
{Object}
– The standard or replacement Edit Controller used to edit the current Data Object.
Used internally. Returns the model name for a given column.
oCol – {Object} –
The dynamic Col object
{string}
– A 'ng-model=...' suitable for insertion into an HTML input element.
Used internally. For each Col object whose type property matches the sType col
property the
related select
method is called. The accumulated results are returned.
scope – {Object} –
The scope to use
schema – {Object} –
The related sub-schema to use.
sType – {string} –
The type to match against
{Object[]}
– The accumulated return values of the Col object select
method
Used internally. Returns the array of Data Object rows within oObj
that belong to oSchema.base
.
Refer to the Deps.js source code as an example. Used to allow editing of an array of Data Object objects
belonging to a single Data Object object.
scope – {Object} –
The scope to use
oObj – {Object} –
The Data Object containing the rows.
oSchema – {Object} –
The related sub-schema to use.
{Object[]}
– The rows within oObj
of property oSchema.base
Used internally. For each Col object whose type property matches the sType col
property the
related select
method is called. The accumulated results are returned.
scope – {Object} –
The scope to use
oTP – {Object} –
The Table.props
values where the column array is stored
sType – {string} –
The type to match against
{Object[]}
– The accumulated return values of the Col object select
method
Sets the current editor for the current selected Data Object.
ctrl – {Object} –
The standard or replacement Edit Controller used to edit the current Data Object.
Used internally to insert a record into the Data Object cache. If the oaa
is null a new Data Object is inserted.
When bInter
is true
the saveRecords function is not invoked.
Used when several objects must be updated (such as a cheque renumbering pass) before persisting. Not supported in chunked mode.
See Record Storage to understand 'chunks'.
oTP – {Object} –
The Table.props
cache where the object array is stored.
obj – {Object} –
The Data Object to insert.
oaa – {Object} –
The Object Access Address. A string or number determining the insert point. See Record Storage for a description of oaa
.
bInter – {Boolean} –
When true
the update is intermediate with more to follow. Therefore do not update invoke the saveRecords function.
Used when several objects must be updated (such as a cheque renumbering pass) before persisting.
Returns whether the service type combines the individual JSON objects into an array for storage and retrieval.
{Boolean}
– Always returns true
.
Used internally. Returns the referenced value in Col oneOf
related table based on the setting of
the Data Object column.
oObj – {Object} –
The Data Object
oCol – {Object} –
The dynamic Col object
oCol is assumed to have the oneOf
property which points to another Table
{string}
– The mapped value
Used internally to cause updates to show correctly on the display by resetting the cache and mapped objects as well as a hidden input field that display screens can create dependencies against.
sig – {string} –
Caller id to aid diagnostics in the log file
oTP – {Object} –
The current Table.props
where the cache is stored.
Used internally to refresh the Data Objects cache from the server.
oTP – {Object} –
The Table.props
cache where the object array is stored.
Used internally. The oCol
type is assumed to be 'property'. After confirming with the user through a prompt
the property within the oCol
properties array of key sKey
is removed.
The validation cycle is used later to validate the requirements of having a key/value pair for sKey
.
oTP – {Object} –
The Table.props
values where the column array is stored
oCol – {Object} –
The dynamic Col object
sKey – {string} –
The name of the property key value.
Used internally to persist reords to the localStorage cache and the data storage on the server.
oTP – {Object} –
The Table.props
cache where the object array is stored.
oRecs – {Object} –
The Data Object array to insert.
sRecName – {string} –
The record name used as the third component of the object key.
sLSName – {string} –
The localStorage name. Null means there is no localStorage copy such as for User records.
bRfsh – {Boolean} –
When true
the update is intermediate with more to follow. Therefore do not update invoke the saveRecords function.
Used when several objects must be updated (such as a cheque renumbering pass) before persisting.
Sets the servREC
oCRUD
pointer to crud so the servREC
has access to the common routines. Required to prevent circular definitions.
crud – {Object} –
Pointer to servCRUD
.
Used internally for the retrieval and update methods to maintain the cache of Data Objects.
oTP – {Object} –
The Table.props
where the object array is stored.
objs – {Object[]} –
The array of Data Objects to store.
Used internally. If present the oCol
showList value is returned. Otherwise true
is returned.
oCol – {Object} –
The dynamic Col object
{Boolean}
– true
is returned if the column should be shown in 'list' mode.


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Here's a timeline of COVID-19 in Alberta
- March 5: Alberta identifies its first presumptive COVID-19 case, a Calgary woman returning from a California cruise.
- March 11: The World Health Organization declares COVID-19 a pandemic, while Alberta begins to recommend against out-of-country travel. The following day, Alberta bans gatherings of more than 250 people.
- March 15: Calgary is among Alberta cities to declare a state of local emergency, closing most non-essential businesses and services. Alberta cancels all school classes and declares a provincial public health state of emergency the following day.
- March 19: Alberta records its first COVID-19 death, an Edmonton man in his 60s. The province’s case count rises to 146, the majority of which originated through out-of-country travel.
- March 31: A third resident of the McKenzie Towne Continuing Care Centre dies of COVID-19. An outbreak at the facility would go on to claim the lives of 19 residents.
- April 6: Alberta chief medical officer of health Dr. Deena Hinshaw recommends the use of non-medical face masks when physical distancing is difficult. Modelling suggests a mid-May peak for COVID-19 in Alberta, with around 800,000 total cases in the province. Twenty-four Albertans have died of the virus, with almost 1,350 infections.
- April 20: The Cargill meat-packing plant in High River temporarily closes down amid a COVID-19 outbreak. The outbreak would become the largest in Alberta, linked to more than 1,500 case and three deaths. Meanwhile, the JBS meat-processing plant in Brooks would record more than 650 cases.
- April 23: The Calgary Stampede cancels its 2020 event, the first time the show didn’t go on since it became an annual tradition in 1923, as Hinshaw restricts gatherings of more than 15 people. The 319 new cases reported stands as Alberta’s highest single-day tally. There are 3,720 total cases in the province, with 68 deaths.
- May 3: Alberta records fewer than 100 cases of COVID-19 for the first time since mid-April, signalling the end of the province’s first wave of the virus.
- May 13: Alberta enters Stage 1 of its COVID-19 relaunch, letting businesses like restaurants and retailers reopen, but Calgary and Brooks are singled out of the relaunch due to ongoing meat-plant outbreaks. Both municipalities are allowed to join in the relaunch May 25.
To learn more from here Alberta's Six Months Covid timeline


basically works
is whitespace agnostic
supports multiple staves with a newline
adds a space at the end if the last word is a newline (so that the newline immediately indicates that it has occurred, by taking up space in the display)
Macros
converts clef macros correctly
Comments
supports inline comments
still supports codes with curlies, despite those being comment chars, and can even include them inside of comments as long as they aren't the first or last characters of a whitespace-separated word
Unrecognized and Unicode literal codes
includes a space after unrecognized codes so that when you have multiple in a row you can distinguish them
d o n ' t k n o w w h a t i ' m d o i n g
well, this is really a regression test, but: it doesn't mysteriously throw away the first unrecognized code
f n o r d
spaces unrecognized codes away from recognized codes even when Smart Stave is off
u n r e c
Smart Position
the most recently used position is automatically applied if none is specified
don't manifest until they are needed (only apply to glyphs with ligatures to be vertically shifted by them)
persists until a new position is used (is 'sticky')
does not actually put the middle position on the stave; there is no zero position glyph in SMuFL, so we temporarily use a code point from the Sagittal range, but it has no actual effect so it shouldn't be emitted
works for the positions supplement
Smart Clef
assume treble clef even if no clef has been provided
change depending on the clef
clefs are smart and they stick until you change them (you can change from one to the other)
a new clef resets the position to middle staff
Smart Advance
advances by the width computed for each glyph from the Bravura font lgln
advances by the width computed for each glyph from the Bravura font trcl
advances by the width computed for each glyph from the Bravura font ntdbwh
advances by the width computed for each glyph from the Bravura font ntwh
advances by the width computed for each glyph from the Bravura font nt2up
advances by the width computed for each glyph from the Bravura font ntup
advances by the width computed for each glyph from the Bravura font nt8up
advances by the width computed for each glyph from the Bravura font nt16up
advances by the width computed for each glyph from the Bravura font nthfdn
advances by the width computed for each glyph from the Bravura font ntqrdn
advances by the width computed for each glyph from the Bravura font nt8dn
advances by the width computed for each glyph from the Bravura font nt16dn
does not repeatedly advance if multiple smart advance codes are provided (besides adding the default 2 spacing, in preparation for if you were to provide an actual next glyph)
if more than one unicode has occurred since the previous advance, uses the width of the unicode with the max width
resets the advance amount after each application
can have the spacing adjusted from the default of 2
supports manual advance amounts
supports positioning the next glyph with its right edge against the right edge of the current line with the advance-to-end code
the advance-to-end code also works for the double barline
the advance-to-end code behaves like a normal smart advance when smart staff is not on (so that if the user deletes the ston code from their sentence, things look basically the same, just without the staff)
the advance-to-end code works for glyphs with widths between 1 and 8
the advance-to-end code works for glyphs with widths of exactly 8
the advance-to-end code works for glyphs with widths between 8 and 16
the advance-to-end code works for glyphs with widths of exactly 16
the advance-to-end code works for glyphs with widths between 16 and 24
the advance-to-end code works for glyphs with widths of exactly 24
you can continue the same line after using an advance-to-end code, and it will include the proper spacing for the character which used to be up against the exact right edge of the line
the advance-to-end code is canceled by a line newline
the advance-to-end code can be adjusted with manual advance
the advance-to-end code can be adjusted with manual advance, when the manual advance amount is greater than the difference between the width of the glyph and the remaining stave
allows codes which end in digits or other advance codes to be immediately followed by the semicolon without a space
x e n
Smart Stave
automatically adds stave lines as needed, if smart stave has been asked for
does not add additional lines as needed, if only a manual stave has been asked for
can be turned off and on, and upon turning it off, it advances you to the end of the stave it has already laid down
provides leger lines automatically for notes and noteheads beyond ±5 staff positions
only puts leger lines on every other position (the ones that would have been lines)
provides multiple leger lines if the note is very beyond the staff
turns off leger lines when smart stave is off
provides leger lines of the smallest size which is wider than the glyph they are for lglnnr
provides leger lines of the smallest size which is wider than the glyph they are for lgln
provides leger lines of the smallest size which is wider than the glyph they are for lglnwd
provides leger lines of the smallest size which is wider than the glyph they are for beyond lglnwd
makes exceptions for upward notes with flags, ignoring the width the flags contribute nt8up
makes exceptions for upward notes with flags, ignoring the width the flags contribute nt16up
makes exceptions for upward notes with flags, ignoring the width the flags contribute nt32up
makes exceptions for upward notes with flags, ignoring the width the flags contribute nt64up
makes exceptions for upward notes with flags, ignoring the width the flags contribute nt128up
makes exceptions for upward notes with flags, ignoring the width the flags contribute nt256up
makes exceptions for upward notes with flags, ignoring the width the flags contribute nt512up
makes exceptions for upward notes with flags, ignoring the width the flags contribute nt1024up
should not display anything when you've only entered 'ston'
should not display anything when you've only entered 'ston' and an example of the type of staff you want to automate
can be configured to automate different types of staves, by providing one stave of that kind
manual stave of the same type as the automated type has no effect (including if it's the default type)
when smart stave is on, and a code is unrecognized, it first finishes the smart stave, and then for that final space (the one for separating it from other unrecognized codes, but nice to have regardless) it turns smart stave back on, to ensure the next code appears on top of stave
n t h n t h
when smart stave is off, and a code is unrecognized, it behaves otherwise the same, with the same amount of spacing that is, but just no stave
n t h n t h
the stof command is a noop when Smart Stave is not on


Below is the ITS DataHub metrics dashboard. The metrics dashboard provides statistics on user activity on the ITS DataHub, data.transportation.gov (DTG), and the National Transportaion Library (NTL). Statistics include data and page views, data downloads, programmatic data access, and GitHub Repository views.
Table of Contents:


[§551E‑17] Principles of law and equity. Unless displaced by a provision of this chapter, the principles of law and equity shall supplement this chapter. [L 2014, c 22, pt of §1]


Italian flood warnings spread beyond Venice to Pisa and Florence
by Alice TideyAfter a wave of rainstorms recently hit Italy, there are fears other major cities could soon join Venice in being several feet underwater.
In Pisa, in north-western Italy, 170 paratroopers were deployed on Sunday to bolster the city's flood defences after the Arno river which flows through the city rose dramatically.
Fears of flooding had receded in Florence on Sunday evening. The Arno, which also goes through the historical city, had risen by 4.8 metres because of the rain but remained under the critical level of 5.5 metres.
Aerial footage shared earlier in the day by the police showed the river's level perilously close to the medieval Ponte Vecchio's deck.
"The situation is under control and monitored continuously," Mayor Dario Nardella wrote on Facebook, thanking first responders for carrying out 47 interventions throughout the municipality.
He noted however that the wider Tuscany region remains under amber warning until early afternoon on Tuesday.
In the Emilia Romagna region, which is still under yellow warning for rain and thunderstorms, bridges have been closed; hundreds of people have been evacuated and the railway between Bologna and Porto Maggiore has been cut.
Some 10,000 people also remain without electricity in Modena while an elderly couple had to be airlifted out by firefighters after the Idice river flooded Bologna.
Meanwhile in Venice the state of emergency continues as the UNESCO city was flooded on Sunday by a record third exceptional tide in one week.
The floodwater reached 1.5 meters as strong storms and winds battered the region again.
The perilous deluges have already caused millions of euros worth of damage prompting the government to release €20 million in funds to tackle the devastation.


| Vehicle |
You flight or you drive. |
|
|
| Runway Usage |
Determine which runway pair get used most. Left first, right last. Must supply as many values as number of alligned runways. |
[0.75, 0.25]: Left gets used more than right. |
|
| Taxi Hold |
How long a plane hold a taxi position before entering the runway |
[60, 300]: Between 60 and 360 seconds. |
|
| Take-off Hold |
How long a plane hold takeoff position on the runway before actually taking off |
[10, 60]: Between 10 and 70 seconds. |
|
| Arrival delay |
How long ahead / late a plane arrives accoring to its scheduled time. |
[-20, 50]: Between 20 minutes in advance and 30 minutes late. |
|
| Departure (additionnal) delay |
How long ahead / late a plane leaves accoring to its scheduled time. |
[-10, 30]: Between 15 minutes in advance and 30 minutes late. If the planed arrived late, its delay is ADDED to this extra delay. |
|
| AODB preannouce |
How long ahead a scheduled flight is announced. |
360 minutes. |
|
| AODB planned flight time announcement. |
Time when Planned flight arrival/departure time is announced. |
[40, 20]: Planned arrival/departure time is announced between 40±20 minutes before actual arrival/departure time. |
|
| AODB planned flight time announcement. |
Time ADDED to the above planned flight time announcement. This randomness represent "delays" added by external computers to provide the information. |
600: Up to 600 seconds are added to above time. |
|
| Passenger / Cargo Flight Ratio |
Ratio |
0.2: 20 percents of flights are PASSENGER (PAX) flights. The other 1 - 0.2 = 0.8 = 80% flights are CARGO flights. |
|
| Jitter |
Omnidirectional "noise" added to GPS coordinates, in meter. |
10: Meters. GPS coordinates are sent with that amount of uncertainty added to them, in all, random direction. |
|
| Time between flights |
Time, in minutes, between flights. |
[0,15]: There are always between 0 and 15 minutes between flights. |
|
| Minimum time between flights |
If random selected time is lower than this, this is the time between 2 flights, never less. |
2.5: There are always at least 2.5 minutes between flights. |
|
| Turnaround time |
Time of turnaround for planes that arrive and then leave. |
[70,120]: Turnaround takes between 70 and 120 minutes to complete. |
|
|
Parameter for TRUCKS |
|
|
| Loading time |
Time of unload and load a truck. |
[35,75]: Unloading and re-loading a truck takes between 35 and 75 minutes to complete. |
|
| Time between trucks arriving at dock. |
Time, in minutes, between arrival of trucks at dock. |
[2,25]: There are always between 2 and 25 minutes between two trucks arriving at a dock. |
|


DON JUAN DEMARCO A film review by Christopher Null Copyright 1995 Christopher Null
Don Juan, the world's greatest lover is ... Johnny Depp? I can believe it, after seeing DON JUAN DEMARCO, a new film by first-time director Jeremy Leven. With excellent flare, Leven brings us this beguiling tale of a young man who may or may not be the legendary seducer of over one thousand women.
When a distraught Don Juan is about to commit suicide because of the loss of his (most recent) love, psychiatrist Jack Mickler (Marlon Brando) is brought in to bring him back to reality. This proves to be a major undertaking, as Mickler slowly begins to realize that the "delusional" Don Juan may actually be who he says he is. As his last case before retirement, Mickler is given ten days to determine whether or not to institutionalize Don Juan, and there, the journey into the man's past begins.
What the doctor finds is a perfect blend of comedy and romance, a serious questioning of our perceptions of reality, and a serious analysis of our beliefs about love. Depp's convincing portrayal of the great lover keeps us constantly guessing as to his true identity, and Brando pulls off his role as a comic foil perfectly. Faye Dunaway has a few good scenes as Brando's wife, with whom he rediscovers their cooled passion as a result of his conversations with Don Juan.
This romantic fable is the type of story that is generally labeled as "cute," but its exquisite performances and comic sensibility prevent the film from taking itself too seriously and becoming a trite sitcom. Instead, the film manages to be touching and convincing. Despite the highly contrived plot and the silly ending, DON JUAN DEMARCO is a memorable update of an ancient tale.
RATING: ****
|* Unquestionably awful | |** Sub-par on many levels | |*** Average quality, hits and misses | |**** Good, memorable film | |***** Perfection |
The review above was posted to the
rec.arts.movies.reviews newsgroup (de.rec.film.kritiken for German reviews).
The Internet Movie Database accepts no responsibility for the contents of the
review and has no editorial control. Unless stated otherwise, the copyright
belongs to the author.
Please direct comments/criticisms of the review to relevant newsgroups.
Broken URLs inthe reviews are the responsibility of the author.
The formatting of the review is likely to differ from the original due
to ASCII to HTML conversion.
Related links: index of all rec.arts.movies.reviews reviews


A Awesome Product
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find him
Worried family issue desperate Facebook appeal to find missing Fife man George Brownlie
by Kirsty FeerickA WORRIED family have issued a desperate Facebook appeal to find a missing Fife man.
George Brownlie vanished from the Townhill area leaving his loved ones distraught.
One concerned family member took to social media in frantic bid to find him, which has been shared over a thousand times.
They begged the public to keep an eye out for George as his disappearance is very out of character.
She said: "He is from the Townhill area and this is very out of character from him.
"He is usually seen in the Townhill area regularly near the library, the park, cost cutters and so on.
"Urging all people to please and I beg please keep an eye out for him as we are all worried sick.
"He sometimes goes out walking in the area but has not been seen in a few days now.
"Can people please share this and if anyone sees him or thinks they have seen him get in Contact with myself or Dunfermline police station right away.
"I pray your safe and are found soon uncle George all my love."
A spokesperson for Police Scotland said: "We can confirm George Brownlie is a missing person."


I am a 3rd year Coe thapar student from patna. I Live my life care Free!!!
He analysed it to find sentiment and also made this website.


4.5 is building on top of 4.2 success and includes:
- Multiple search improvements with more relevant results
- Updates to latest stable versions of underlying Node.js components
- Multiple bug fixes
- Over 100 Additional Code Examples
- Code Examples linked to Guidelines
- Over 100 Additional How Tos
- Merged Articles
- General sweep for outdated content
4.2 is a major rewrite of TEAM Mentor under new architecture. This includes:
- Simplified, modern, easy to use interface and intuitive design
- Focus on making it easy to find answers to security questions
- Improved search and filter capability. It algorithmically presents the most relevant articles and allows to further narrow down results with robust filtering
- Improved ability to browse content. Users can now browse by subject matter, technology, article type and other keywords. Progressively narrowing down results with selected filters
- Main User UI fully written in Node JS.
- Main User UI support for all browsers. Including legacy and mobile browsers.
- Underlying use of a NoSQL database
- Robust integration current editor and admin interfaces
- Integration with Piwik for statistical information
- Content had been re-classified into subject matter areas for easy browsing through the taxonomy
- Article filters appropriately changed to making more intuitive to find relevant information
- Major clean-up of articles. Removal of articles with too little information
- Moved away from multiple library structure. All of the content is now in one well-organized library.
- New AWS content
MINIMUM REQUIREMENTS
Note the change in minimum requirements specified here:
Server Side Requirements
Please note that it may be possible to run TEAM Mentor with less RAM and Storage. However performance does degrade under load and minimal configuration listed above is recommended for production environments. Also note, when connecting to TEAM Mentor on local machine (connecting to "localhost") SSL certificate is not required. Self-signed certificate may be used for test environments.
Client Side Requirements
The main client side version code named Flare requires:
There is a fallback version code named Jade. Jade supports all available browsers, including IE8 and Lynx.
TM 3.6 Back-end (used for Administration and Editing) supports the following browsers


gtk-update-icon-cache - Icon theme caching utility
gtk-update-icon-cache [--force] [--ignore-theme-index] [--index-only | --include-image-data] [--source NAME] [--quiet] [--validate] PATH
gtk-update-icon-cache creates mmapable cache files for icon themes.
It expects to be given the PATH to a icon theme directory containing an index.theme, e.g. /usr/share/icons/hicolor, and writes a icon-theme.cache containing cached information about the icons in the directory tree below the given directory.
GTK+ can use the cache files created by gtk-update-icon-cache to avoid a lot of system call and disk seek overhead when the application starts. Since the format of the cache files allows them to be mmaped shared between multiple applications, the overall memory consumption is reduced as well.
--force, -f
Overwrite an existing cache file even if it appears to be uptodate.
--ignore-theme-index, -t
Don*(Aqt check for the existence of index.theme in the icon theme directory. Without this option, gtk-update-icon-cache refuses to create an icon cache in a directory which does not appear to be the toplevel directory of an icon theme.
--index-only, -i
Don*(Aqt include image data in the cache.
--include-image-data
Include image data in the cache.
--source, -c
Output a C header file declaring a constant NAME with the contents of the icon cache.
--quiet, -q
Turn off verbose output.
--validate, -v
Validate existing icon cache.


In addition to supporting digital audio with minimum latency, Jack also has support for MIDI data.
 The original version of Jack considered digital audio only, but it was later extended to transport MIDI data between MIDI clients.
Jack does not talk directly to hardware. This is the job of device drivers such as ALSA. For digital audio, you create a hardware endpoint by starting Jack with device output as in
jackd -dalsa
For MIDI, ALSA supplies a MIDI sequencer. This does not play the MIDI, just sends the MIDI events at the right time to a backend. This was discussed in ALSA MIDI. For example, TiMidity can be run as the backend by
timidity -iA -B2,8 -Os -EFreverb=0
while FluidSynth can be run as
fluidsynth --server --audio-driver=alsa -C0 -R1 -l /usr/share/soundfonts/FluidR3_GM.sf2
You will probably find that a TiMidity server is already running.
Philipp Überbacher explains the options for using Jack MIDI with (or without) ALSA MIDI:
-Xraw
then the ALSA MIDI sequencer is ignored
and Jack MIDI output is sent only to hardware MIDI devices
-Xseq
then each ALSA MIDI port is made
visible as a Jack sequencer port
a2jmidid
will make the ALSA MIDI sequencer ports visible
to Jack.
The difference between the last two can be seen graphically using qjackctl
.
Using a2jmidid
the MIDI clients show under a a2j
dropdown
and have meaningful names:
Using the -Xseq
option, the same MIDI clients show with names given by Jack
which are not so useful:
The application jack-keyboard
is a piano keyboard.
This can play MIDI events by holding down "keys" with the mouse
or by using the keyboard.
It looks like
It will show in qjackctl
as both an output port and (probably less usefully) as an input port.
How can you check it is working okay? It's not too hard:
pasuspender cat
.
Restart it at the end of the Jack session by ctl-D to cat
jackd -dalsa
qjackctl
.
a2jmidid
to map ALSA ports into Jack ports.
Under the MIDI tab of qjackctl
you may now see TiMidity or other synthesizer as an input port
aseqdump
from the command line.
This can show the events at an ALSA sequencer port in the terminal window.
This will now show in qjackctl
as an input port.
jack-piano
output port to an aseqdump
input port as in
aseqdump
130:0 Note on 0, note 73, velocity 32
130:0 Note off 0, note 73, velocity 32
130:0 Note on 0, note 82, velocity 32
130:0 Note off 0, note 82, velocity 32
130:0 Note on 0, note 86, velocity 32
130:0 Note off 0, note 86, velocity 32
130:0 Note on 0, note 73, velocity 127
130:0 Note off 0, note 73, velocity 127
130:0 Note on 0, note 73, velocity 127
130:0 Note off 0, note 73, velocity 127
130:0 Note on 0, note 70, velocity 127
130:0 Note off 0, note 70, velocity 127
Another useful application is jack-smf-player
from
Simple JACK MIDI player and recorder
by Edward Tomasz Napierała.
This will play a MIDI file to a Jack MIDI input client.
With one of the Jack-ALSA links by aj2midid
or jackd -dalsa -Xseq
,
TiMidity will probably show up as a Jack MIDI input, and we know it is a synthesizer to
play MIDI events. Unfortunately, I have not yet succeeded in getting it to play anything:
connecting the keyboard or file player to it results in obstinate silence.
The same things happens if I run FluidSynth as a backend server to alsaseq
:
no sound.
The solution I have found so far is to start another TiMidity server with Jack as output (-Oj) using
timidity -iA -B2,8 -Oj -EFverb=0
Then using qjackctl it shows up under the Audio tab with two output ports.
I can connect these to the System playback ports as in
It also shows up under the MID tab (here as midi_playback 28-31) and I can connect
jack-keyboard
or other MIDI producer such as
jack-smf-player
as in
Then I can send Jack MIDI to the TiMidity Jack MIDI inputs which send audio out on the TiMidity Jack Audio output ports which is then played by the Jack Audio system playback ports.
FluidSynth can also be run in the same way by setting its audio driver to Jack
fluidsynth --server --audio-driver=jack /home/httpd/html/LinuxSound/MIDI/User/TimGM6mb.sf2
and connecting MIDI output ports to FluidSynth input ports and FluidSynth audio output ports to the
system playback ports.


Demonstrates the Grow effect on images, also uses the setup & finish callback function to set the z-index style property:


DSN_fe¶
-
class
MonitorControl.FrontEnds.DSN.
DSN_fe
(name, inputs=None, output_names=None)¶ Bases:
MonitorControl.FrontEnds.FrontEnd
Class for DSN front ends with no M&C functions
Methods Summary
Tsys_vacuum
([beam, pol, mode, elevation])System temperature without an atmosphere
The downlink bands allocated to Space Research (Space to Earth) are.
rx_noise_temp
([pol, mode, elevation])Noise temperature measured at the feed
Methods Documentation
-
Tsys_vacuum
(beam=1, pol='R', mode='X', elevation=90)¶ System temperature without an atmosphere
This ignores attenuation through the atmosphere. Attenuation by the atmosphere is about 0.8% at S-band and between 0.8 and 1.3% at X-band. It also ignore ground pickup
:param beam : beam number, only significant for K-band :type beam : int
:param pol : polarization, “R” or “L” :type pol : str
:param mode : “X” or “SX”, only significant for X-band :type mode : str
-
get_frequencies
()¶ The downlink bands allocated to Space Research (Space to Earth) are:
S X K Ka near Earth: 2200-2290 8450-8500 25500-27000 deep space: 2290-2300 8400-8450 31800-32300
References
http://deepspace.jpl.nasa.gov/dsndocs/810-005/201/201B.pdf
The actual bandpasses are given in the code.
-
rx_noise_temp
(pol='R', mode='X', elevation=90)¶ Noise temperature measured at the feed
From Appendix A of 810-005 module 101
:param pol : either ‘R’ (DSN standard) or ‘L’ :type pol : int
:param mode : either ‘X’ or ‘SX’ for dual (diplexer in) :type mode : str
:param elevation : angle in deg from horizon to zenith :type elevation : float
-