{{data.name}}
{{data.totalSize | filesize}}
{{resourceService?.frmelmnts?.lbl?.downloading}} {{data.totalSize | filesize}}
{{resourceService?.frmelmnts?.lbl?.uploading}}
{{resourceService?.frmelmnts?.lbl?.uploadPaused}}
{{resourceService?.frmelmnts?.btn?.resuming}}
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{{resourceService?.frmelmnts?.btn?.completed}}
{{resourceService?.frmelmnts?.desktop?.lbl?.completing}}
{{resourceService?.frmelmnts?.lbl?.downloadFailed}}
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{{resourceService?.frmelmnts?.lbl?.cancelDownload}}


This feature offers advanced search and analysis capabilities on top of the ABAP Development Tools
Attention: Most of the features are only available if the necessary ABAP Coding is available in the ABAP Project you are working
on. For detailed installing instructions look here: abap-search-tools (GitHub).


We're going to put a new web page on the internet.
Example: Gargoyles fan page.
Example: To infinity and Beyond.
There are two steps: we set up an example page, then you add your own content.
Let's go!
Choose the 'Free' option and click 'Continue'
You will have to check your email to get the code for the next page.
One the page after that, click 'Go to the dashboard >>' to skip Neocities' tutorial. (We want you to do our tutorial instead!)
This is the dashboard, which shows all the files in your website.
You can hold your mouse over a file and you will see 'edit' or 'delete' or both.
Edit your index page by moving your mouse over the index.html file and clicking the 'Edit' link that appears.
This opens a tab where you can change your page.
Tab 2: Click on the 'View' button on this page.
This opens a new tab where you check how your page looks.
Right now, your page will be a white page with some instructions on it. You can ignore those instructions. We are going to delete them in a moment.
Now you have two tabs that you will use: One to look at your site, and one to edit your site.
Copy the link to your page, and paste it into our team chat on the girl code slack.
Copy the link like this... (this is the link from the tab where you view the page, not the one where you edit.)
In Slack, join your class channel. A channel is like a chatroom and they are listed on the left-hand side.
Paste your link into your class channel.
Now it's in the Slack, so your team can see what you're working on. It's really important to be comfortable sharing your work, even when it's not finished!
Go to the tab for editing (it says Dashboard > index.html)
Delete all the code until the dark grey area is empty. That's right, delete it all!
Then copy and paste this in instead:
<!DOCTYPE html>

Welcome to my page

This is a paragraph.

Click 'save' at the top right to save.
Now switch to the tab that shows your website. Refresh the page and you should see your changes appear.
It should look like this.
Congratulations! You have made a beautiful website! Well, kind of.
Maybe you want to change it a little…
Continue on to part two!


{% load static from staticfiles %}
The Experiment Factory
{{ experiment_load | safe }} {{run | safe}}
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about me
coding
design
skills
leejaehun
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coding
introducing the coding
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creatively
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creative
my bring genuine ideas
and bold concepts to life.


client.common
— Twisted Async Modbus Client¶
API Documentation¶
Modbus Client Common¶
This is a common client mixin that can be used by both the synchronous and asynchronous clients to simplify the interface.
-
class
pymodbus.client.common.
ModbusClientMixin
[source]¶ This is a modbus client mixin that provides additional factory methods for all the current modbus methods. This can be used instead of the normal pattern of:
# instead of this client = ModbusClient(...) request = ReadCoilsRequest(1,10) response = client.execute(request) # now like this client = ModbusClient(...) response = client.read_coils(1, 10)
-
read_coils
(address, count=1, **kwargs)[source]¶ Parameters: - address – The starting address to read from
- count – The number of coils to read
- unit – The slave unit this request is targeting
Returns: A deferred response handle
-
read_discrete_inputs
(address, count=1, **kwargs)[source]¶ Parameters: - address – The starting address to read from
- count – The number of discretes to read
- unit – The slave unit this request is targeting
Returns: A deferred response handle
-
write_coil
(address, value, **kwargs)[source]¶ Parameters: - address – The starting address to write to
- value – The value to write to the specified address
- unit – The slave unit this request is targeting
Returns: A deferred response handle
-
write_coils
(address, values, **kwargs)[source]¶ Parameters: - address – The starting address to write to
- values – The values to write to the specified address
- unit – The slave unit this request is targeting
Returns: A deferred response handle
-
write_register
(address, value, **kwargs)[source]¶ Parameters: - address – The starting address to write to
- value – The value to write to the specified address
- unit – The slave unit this request is targeting
Returns: A deferred response handle
-
write_registers
(address, values, **kwargs)[source]¶ Parameters: - address – The starting address to write to
- values – The values to write to the specified address
- unit – The slave unit this request is targeting
Returns: A deferred response handle
-
read_holding_registers
(address, count=1, **kwargs)[source]¶ Parameters: - address – The starting address to read from
- count – The number of registers to read
- unit – The slave unit this request is targeting
Returns: A deferred response handle
-
read_input_registers
(address, count=1, **kwargs)[source]¶ Parameters: - address – The starting address to read from
- count – The number of registers to read
- unit – The slave unit this request is targeting
Returns: A deferred response handle
-
readwrite_registers
(*args, **kwargs)[source]¶ Parameters: - read_address – The address to start reading from
- read_count – The number of registers to read from address
- write_address – The address to start writing to
- write_registers – The registers to write to the specified address
- unit – The slave unit this request is targeting
Returns: A deferred response handle
-
mask_write_register
(*args, **kwargs)[source]¶ Parameters: - address – The address of the register to write
- and_mask – The and bitmask to apply to the register address
- or_mask – The or bitmask to apply to the register address
- unit – The slave unit this request is targeting
Returns: A deferred response handle
-


Textman
Upload a picture and have the text extracted from it.
Select a file
{% if label %}
{{label}}
{% endif %}


#2693
16th cross, 31st main
Sector 1, HSR Layout, Bangalore 560102
P: (963) 254- 8615
Reach us
contact@vgulp.com


Highlight: Data scientist with good mathematical background
Mathematical/Statistical Skills: 3+ years of experience
Derivation: Advance calculus of differential equations, stochastic calculus and real analysis
Modeling: Machine learning, time series analysis, sampling, ANOVA analysis, A/B testing, linear algebra, model/feature selection
Hands on experience: applying several ML/statistical algorithms to real world problems: Gradient Boosted Trees, Random Forest, Clustering, GLM, Markov, Game Theory and Simulation Models.
Programming Skills: 3+ years of experience
Programming: R (inclusive of Rshiny), Python, PySpark, SQL, VBA and basic Java
Data visualization: R, Python and Tableau
Data engineering: Hadoop and AWS, experience with building end-to-end machine platform using python and Spark (and Hive)


ZDRAS-TVUY-TE
Opens new tab
This is a bold link
This is a placeholder link, goes no where, for now
how to... make a 'sammich'
- become hungry
- lay 2 pieces of bread on a plate
- smear the bread with peanut butter, one side for each piece of bread
- add a layer of jelly
- bring the sammich bread pieces together
- eat
5 Favorite Musicians/Bands
- Nas
- Jay-Z
- Kendrick
- The Beatles
- The Notorious BIG
Class Action Animals
| animal class |
animal name |
| mammalia |
panthera leo |
| mammalia |
Loxodonta africana |
| chondrichthyes |
Carcharodon carcharias |
| aves |
buteo jamaicensis |
in closing...


Autodue is a native Android application that allows a user to create a to-do list where tasks have a due-date, priority, and expected duration. By using their device's calendar, Autodue is able to automatically find an empty time slots and create events for the tasks based on their priority and due date.
Autodue was created in a team of 5 for a Software Engineering course at UC San Diego. Throughout the process we worked closely with another group acting as our client. After determining their needs through user interviews, we used Agile development methods in order to deliver incremental updates and receive user feedback in short, one-week iterations.
Our initial user interviews were quite open-ended, with more general questions about daily problems that our users faced. During our discussion, issues about user productivity were brought up several times. Another user also talked about he struggled with completing tasks due to his busy schedule.
Our group decided that a way to tackle the problem would be to create a to-do list that sorts itself based on priority. When we went to our client group with this solution, the suggested we integrate it with the user's Google calendar. This gave us the baseline functionality for our application.
Our team had no previous experience with Android development, so we all went through the Android development tutorials and worked overtime to deliver a working, native Android app prototype. In our first week, we were only able to deliver an application that linked to the user's calendar and another separate application that allowed a user to create a task. Our client group was unable to give us any useful feedback for the first week due to this.
One for the main issues for the first week was the lack of version control. After our initial failure, I created a shared repository on GitHub for our group to use. While my team was familiar with using git on their own, a few members had no previous experience using it in a team setting. In order to ensure a smooth development process, I taught them how to properly create a new branch and then merge it back into master.
After dealing with these initial problems, my team created basic mockups for our app. We did this initially working on a whiteboard, and then translating higher-fidelity wireframes. The general idea we had was to have a task list and a calendar view.
We also attempted to incorporate some elements of Google's material design. To do this, we added a floating action button on the task list page for adding tasks and used a side drawer for navigation.
With our general design set, we were able to focus on specific functionality. My first task was to implement our to-do list. After researching the Android documentation and looking through several deprecated elements, I settled on the RecyclerView. The initial implementation was simple, and each item had only it's name, priority, and due date. Based on user feedback we added the amount of time left before the due date, the duration, and color coded each task based on priority.
After we had the main functionality for adding events to the user's calendar, our clients recommended that we add a way to set certain hours off-limits to the application. This way, Autodue wouldn't add events at times the user was typically asleep. Implementing this functionality was another of my responsibilities. I implemented it by allowing the user to set an interval of time where events could not be added.
Here's an example of the full flow for adding a task to the to-do list and then generating the event in your Google Calendar.


|
BTK Python wrapper
0.3dev.0
Python bindings for the Biomechanical ToolKit library (BTK)
|
Container of analog channels representing an inertial measurement unit (IMU). More...
Public Member Functions | |
| def | Clone |
| def | GetAccelerometerX |
| def | GetAccelerometerY |
| def | GetAccelerometerZ |
| def | GetCalMatrix |
| def | GetChannel |
| def | GetChannelNumber |
| def | GetChannels |
| def | GetDescription |
| def | GetFrameNumber |
| def | GetFrequency |
| def | GetGyroscopeX |
| def | GetGyroscopeY |
| def | GetGyroscopeZ |
| def | GetLabel |
| def | GetTimestamp |
| def | GetType |
| def | Rotate |
| def | SetCalMatrix |
| def | SetChannel |
| def | SetChannels |
| def | SetDescription |
| def | SetFrameNumber |
| def | SetFrequency |
| def | SetLabel |
| def | Update |
Container of analog channels representing an inertial measurement unit (IMU).
Container of analog channels representing an inertial measurement unit (IMU). This class proposes to store any number of analog channels but the 6 first channels could be used for 3 accelerometers and 3 gyroscopes as some convenient methods are proposed in this way (see SetChannels(), GetAccelerometerX(), GetAccelerometerY(), GetAccelerometerZ(), GetGyroscopeX(), GetGyroscopeY(), GetGyroscopeZ()). The storage of the channel is done using an ID and not an array index. You can then use the same ID for some kind of sensor even if other are missing (i.e. IMU with accelerometers disabled or configured with 1 acc, and 2 gyros., etc.). Note: This class is still experimental and could be modified in a new release.
| def btk.btkIMU.Clone | ( | self | ) |
Clone(self) -> btkIMU
| def btk.btkIMU.GetAccelerometerX | ( | self | ) |
GetAccelerometerX(self) -> btkAnalog Convenient method to return the analog channel with the ID 0 (which should correspond to an accelerometer measuring data on the X axis of the IMU).
| def btk.btkIMU.GetAccelerometerY | ( | self | ) |
GetAccelerometerY(self) -> btkAnalog Convenient method to return the analog channel with the ID 1 (which should correspond to an accelerometer measuring data on the Y axis of the IMU).
| def btk.btkIMU.GetAccelerometerZ | ( | self | ) |
GetAccelerometerZ(self) -> btkAnalog Convenient method to return the analog channel with the ID 2 (which should correspond to an accelerometer measuring data on the Z axis of the IMU).
| def btk.btkIMU.GetCalMatrix | ( | self | ) |
GetCalMatrix(self) -> array (NumPy)
| def btk.btkIMU.GetChannel | ( | self, | args | ) |
GetChannel(self, id) -> btkAnalog GetChannel(self, arg2) -> btkAnalog Returns the analog channel with the given ID or label. If there is no analog channel with the given ID, then an exception is thrown.
| def btk.btkIMU.GetChannelNumber | ( | self | ) |
GetChannelNumber(self) -> int Returns the number of analog channels associated to this IMU.
| def btk.btkIMU.GetChannels | ( | self | ) |
GetChannels(self) -> btkAnalogCollection Returns the analog channels of the IMU in a collection. The analog channels are pushed in the collection by using their ID.
| def btk.btkIMU.GetDescription | ( | self | ) |
GetDescription(self) -> std::string const &
| def btk.btkIMU.GetFrameNumber | ( | self | ) |
GetFrameNumber(self) -> int Returns the number of frames set in this IMU.
| def btk.btkIMU.GetFrequency | ( | self | ) |
GetFrequency(self) -> double Returns the frequency set to the IMU. (by default it is 0 Hz).
| def btk.btkIMU.GetGyroscopeX | ( | self | ) |
GetGyroscopeX(self) -> btkAnalog Convenient method to return the analog channel with the ID 3 (which should correspond to a gyroscope measuring data on the X axis of the IMU).
| def btk.btkIMU.GetGyroscopeY | ( | self | ) |
GetGyroscopeY(self) -> btkAnalog Convenient method to return the analog channel with the ID 4 (which should correspond to a gyroscope measuring data on the Y axis of the IMU).
| def btk.btkIMU.GetGyroscopeZ | ( | self | ) |
GetGyroscopeZ(self) -> btkAnalog Convenient method to return the analog channel with the ID 5 (which should correspond to a gyroscope measuring data on the Z axis of the IMU).
| def btk.btkIMU.GetLabel | ( | self | ) |
GetLabel(self) -> std::string const &
| def btk.btkIMU.GetTimestamp | ( | self | ) |
GetTimestamp(self) -> unsigned long Returns the timestamp of the object.
| def btk.btkIMU.GetType | ( | self | ) |
GetType(self) -> int Returns the type of the IMU.
| def btk.btkIMU.Rotate | ( | self, | args | ) |
Rotate(self, arg2) Convenient method to rotate the analog channels with the IDs 0-5. This method handles the case where some of these analog channels are missing.
| def btk.btkIMU.SetCalMatrix | ( | self, | args | ) |
SetCalMatrix(self, array)
| def btk.btkIMU.SetChannel | ( | self, | args | ) |
SetChannel(self, id, btkAnalog) Sets an analog channel to the given ID. If an analog channel is already set to this ID, then it is replaced.
| def btk.btkIMU.SetChannels | ( | self, | args | ) |
SetChannels(self, btkAnalog, btkAnalog, btkAnalog, btkAnalog, btkAnalog, btkAnalog) Sets the 6 first channels of the IMUs with the analog channels @a accX, @a accY, @a accZ, @a gyroX, @a gyroY, @a gyroZ.
| def btk.btkIMU.SetDescription | ( | self, | args | ) |
SetDescription(self, arg2)
| def btk.btkIMU.SetFrameNumber | ( | self, | args | ) |
SetFrameNumber(self, fn) Set the number of frames for the IMU and modify also the number of frames for the channels.
| def btk.btkIMU.SetFrequency | ( | self, | args | ) |
SetFrequency(self, f) Sets the acquisition sample rate associated to the IMU.
| def btk.btkIMU.SetLabel | ( | self, | args | ) |
SetLabel(self, arg2)
| def btk.btkIMU.Update | ( | self | ) |
Update(self) Updates the ProcessObject associated with this DataObject.


Package io.ebean.event
Interface BeanPersistRequest<T>
-
public interface BeanPersistRequest<T>
Holds the information available for a bean persist (insert, update or delete).This is made available for the BeanPersistControllers.
-
-
Method Summary
All Methods Instance Methods Abstract Methods Modifier and Type Method Description T
getBean()
Returns the bean being inserted updated or deleted.boolean[]
getDirtyProperties()
Flags set for dirty properties (used by ElasticSearch integration).EbeanServer
getEbeanServer()
Return the server processing the request.Set<String>
getLoadedProperties()
For an update or delete of a partially populated bean this is the set of loaded properties and otherwise returns null.Transaction
getTransaction()
Return the Transaction associated with this request.Set<String>
getUpdatedProperties()
For an update this is the set of properties that where updated.Map<String,ValuePair>
getUpdatedValues()
Returns a map of the properties that have changed and their new and old values.boolean
hasDirtyProperty(Set<String> propertyNames)
Return true for an update request if at least one of dirty properties is contained in the given set of property names.
-
-
-
Method Detail
-
getEbeanServer
EbeanServer getEbeanServer()
Return the server processing the request.
-
getTransaction
Transaction getTransaction()
Return the Transaction associated with this request.
-
getLoadedProperties
Set<String> getLoadedProperties()
For an update or delete of a partially populated bean this is the set of loaded properties and otherwise returns null.
-
getUpdatedProperties
Set<String> getUpdatedProperties()
For an update this is the set of properties that where updated.Note that hasDirtyProperty() is a more efficient check than this method and should be preferred if it satisfies the requirement.
-
getDirtyProperties
boolean[] getDirtyProperties()
Flags set for dirty properties (used by ElasticSearch integration).
-
hasDirtyProperty
boolean hasDirtyProperty(Set<String> propertyNames)
Return true for an update request if at least one of dirty properties is contained in the given set of property names.This method will produce less GC compared with getUpdatedProperties() and should be preferred if it satisfies the requirement.
Note that this method is used by the default ChangeLogFilter mechanism for when the
@ChangeLog
updatesThatInclude attribute has been specified.- Parameters:
propertyNames
- a set of property names which we are checking to see if at least one of them is dirty.
-
getUpdatedValues
Map<String,ValuePair> getUpdatedValues()
Returns a map of the properties that have changed and their new and old values.
-
-


The Quantifying Uncertainty project develops code, examples and documentation for the Generalized Metropolis-Hastings (GMH) algorithm proposed in (Calderhead, 2014). It forms part of the Oxford/UCL/Microsoft Research 2020 Science project. GMH implements a class of parallelized Monte-Carlo Markov Chains methods (MCMC) that can be used to estimate model parameters of complex physical and biological processes. Details of the GMH algorithm can be found in the scientific publications listed in the References.
The GMH MCMC library is written in Julia, a language designed for fast and flexible mathematical and technical computing. It combines aspects of R, MATLAB and Python and can be easily parallelized to take advantage of multi-processor machines and clusters. It has an active developer community making it available on Windows, Linux and Mac, and via cloud computing services such as JuliaBox or Amazon Web Services (AWS).
There are 2 different, potentially overlapping, situations in which to use the GMH library:
The GMH code and documentation resides on GitHub in GeneralizedMetropolisHastings.jl. Example models, scripts and notebooks to help users develop their own MCMC simulations are included in GMHExamples.jl.
The remainder of this documentation outlines how to setup GMH on different platforms. It explains how to sign up for AWS (Section 2), how to use GMH on AWS (Section 3), on JuliaBox (Section 4) or on your local machine (Section 5), how to prepare AWS to run GMH on a cluster of machines (Section 6) and how to publish your own AMIs to accompany the publication of scientific articles that use the GMH repository (Section 7).
| Acronym | Full Name | Description |
|---|---|---|
| AMI | Amazon Machine Image | A pre-configured software image of a virtual server |
| AWS | Amazon Web Services | Amazon's cloud computing services |
| EC2 | Elastic Cloud Computing | AWS service to run virtual servers |
| IAM | Identity and Access Management | AWS service to create users |
| GMH | Generalized Metropolis Hastings | Parallel Metropolis-Hastings from (Calderhead, 2014) |
| MCMC | Monte-Carlo Markov Chain | Class of algorithms to sample from unknown probability distributions |
This step requires a credit card to set up an account and a phone number to receive a security callback. By using Amazon's "Free Tier", it is possible to avoid being billed, but a credit card is still required. Follow the instructions in the AWS documentation:
http://docs.aws.amazon.com/AWSEC2/latest/UserGuide/get-set-up-for-amazon-ec2.html
You should complete the following steps:
When setting up a Security Group, specify the following inbound rules:
| Service | Port | Source | Access |
|---|---|---|---|
| SSH | 22 | <IP_ADDRESS>/0 | SSH command-line access |
| Custom TCP Rule | 8998 | <IP_ADDRESS>/0 | Access to IJulia server |
| Custom TCP Rule | 49152 - 65535 | <IP_ADDRESS>/32 | Localhost ports for IJulia server |
The “<IP_ADDRESS>/0” in the “Source” field means that incoming connections from any IP address are allowed. You can make the security group more secure by only allowing incoming connections from known IP addresses (e.g., "My IP" in the EC2 security group control panel). This means, however, that every time you change your local IP address you will have to update the Security Group. As long as you are careful in implementing the security steps outlined in Section 3, the above settings should be fine.
The entire process of setting up an AWS account is likely to take between 1 and 2 hours, depending on your familiarity with AWS. These steps need to be completed only once.
This step typically needs to be performed only once - especially upon first signing up for AWS or if you cannot find the published AMIs listed in Section 3. Amazon regions (data centers) are independent of each other. In order to find the GMH AMIs, you need to be logged into the correct region. At this moment, the only region in which the GMH AMIs are published is Ireland. You can check and change the region in the top right corner of the AWS and EC2 dashboards, between your IAM username and “Support”.
| AMI Name | Description | Relevant Publication |
|---|---|---|
| GMH-JULIA0.4-PHOTO | Code to run GMHPhotoReceptor | (Calderhead,2014) |
Once logged into the AWS dashboard, go to the EC2 console. Select Instances in the left-hand menu, and click the Launch button at the top of the panel. Select Community AMIs from the left-hand menu and in the search box that appears, copy-paste one of the published AMI names from Table 3. Click the Select button to launch the AMI.
Troubleshooting: if the AMI does not appear in the list, then check the AWS region.
Here you select the physical hardware on which to run. Whereas the t2.micro is free to use under Amazon's free tier scheme, it is recommended that you select one of the larger machines (e.g., the t2.medium or higher) as the system needs sufficient memory to operate (>1GB).
When selected, click Next: Configure Instance Details.
From the "Subnet" drop-down list, select a subnet that corresponds to a particular availability zone, which is important if you will also attach an existing EBS-backed volume to contain your data (this is optional - see Step 3.3 below). Make a note of which availability zone you select (currently eu-west-1a, 1b or 1c). Choose Next: Add Storage at the bottom of the page.
Optional: you are welcome - if required - to add an additional drive to contain your private data and code. This can either be done on this page and/or at a later stage, in which case see Add an EBS volume.) Click Next: Tag Instance.
Optional: add descriptive tags for your instance. Then click Next: Configure Security Group.
Select the radio button Select an existing security group and select both the default VPC security group and the security group for Jupyter/IJulia access that you made in Step 2.1. Click Next: Review and Launch.
It is safe to ignore the warning that the Security Group is open to the world (if the security steps outlined in Step 3.4 are adhered to). Click Launch at the bottom of the page. A pop-up window comes up. If you previously made a Key Pair, select Choose an existing key pair. Otherwise select Create a new key pair and make sure to download the private SSH key to a safe location on your local machine.
Click Launch Instances. On the next window, Launch Status, click View Instances, which takes you to the Instances page. Once the Instance State becomes green and says running, you can connect via SSH.
The username for this machine is ubuntu. There is no password, but verification occurs with the SSH Key Pair you created previously.
Instructions on how to connect to the instance via SSH can be found here:
http://docs.aws.amazon.com/AWSEC2/latest/UserGuide/ec2-connect-to-instance-linux.html
If you are using Windows and PuTTy, follow these instructions to transform your local key: http://docs.aws.amazon.com/AWSEC2/latest/UserGuide/get-set-up-for-amazon-ec2.html#create-a-key-pair
Troubleshooting: if you cannot connect, then it may be because of the Security Group settings you launched the machine with. Check that they correspond to the ones in Table 2. If you opted to not allow access from all IP addresses (i.e., did not select <IP_ADDRESS>/0 in Table 2), then make sure that the IP address in the Security Group is the same as the IP address of your local machine (visit http://myipaddress.com to find out).
Optional: you can add additional storage to hold your data and experiments by following these instructions:
http://docs.aws.amazon.com/AWSEC2/latest/UserGuide/ec2-add-volume-to-instance.html
When connected to the instance via SSH, mount the new volume in the home folder rather than in the location suggested in the AWS user guide, for example:
sudo mount /dev/xvdf ~/data
If you create an EBS volume, limit the size to a few GB as the Free Tier only comes with 30GB of free storage for all volumes combined.
This step configures the Jupyter Notebook Server for access via a browser such as Chrome or Firefox.
Important: During the running of the configuration script, you will be asked for a password to login via a browser into the Jupyter Notebook Server. Ensure to select a secure password, consisting preferably of 3 unconnected words, e.g., "apple-spring-saxophone". If the password you select is not secure, then your AWS server is vulnerable to attack as the Notebook server allows any system command to be executed via a web browser.
Execute the configuration script:
GMHConfigure/gmh-server/config.sh
As part of the configuration, the script will ask you to enter a password, and create a self-signed SSL certificate to encrypt the communication to the server. It will ask for some information. You may press enter to accept all default values.
On the SSH command line, you can start the Notebook server:
jupyter notebook &
The ampersand means that the notebook server is placed in the background. Once you see that the server is running on Port 8998, you can logout of the SSH session, and the server will continue to run in the background until the instance is stopped.
The Jupyter server prints status messages to the console. You can redirect this output to a log file:
jupyter notebook > ~/.jupyter/jupyter_output.log 2>&1 &
To connect to the Notebook server via your browser, get the public IP address of your running instance from the EC2 console (the “Instances” page) and type it in the address bar of your web browser. Make sure to use https to connect (rather than plain http).
https://xxx.xxx.xxx.xxx:8998
The browser will complain that the connection is not private because the identity of the self-signed SSL certificate could not be checked. You can safely ignore these warnings.
You are now at the notebook server login page. Type the password you created above.
Under the Files tab in the notebook server, you will see repositories with example experiments in IJUlia Notebooks. Notebooks contain both code and documentation, so please refer to these notebooks for further information.
You can start individual notebooks by navigating to one of the folders containing a notebook, and double-clicking it. You can also start a command-line terminal by selecting “New/Terminal” from the right-hand side of the screen. For further information on the notebook server interface, see the Jupyter documentation.
When finished, there are multiple levels of halting/terminating the Notebook server and AWS machine:
Go to https://juliabox.org and sign in with your Google credentials.
At the top of the JuliaBox window, select Terminal. The currently preferred version of Julia to run the GMH module is v0.4.
Start a Julia session in the terminal window by executing:
juser@juliabox:~$ julia
If this is the first time you are using the GMH module in your JuliaBox, you will need to install the required packages by executing at the Julia command prompt:
julia> Pkg.add("GeneralizedMetropolisHastings")
Run a package update to ensure the latest versions are installed:
julia> Pkg.update()
You can now test if GMH installed correctly and is compatible with this particular JuliaBox installation by running the GMH tests:
julia> Pkg.test("GeneralizedMetropolisHastings")
Sync repositories with examples from GitHub to your JuliaBox home folder. At the top of the JuliaBox window, select Sync. Add the following to the “Git Repositories”.
Paste the above https URLs into the “Git Clone URL”. Accept “master” as branch, "GMHExamples.jl" (or "GMHPhotoReceptor.jl") as location, and press "+" to add the repository. This will now download the package to the specified location.
Please refer to the documentation of the GMHExamples.jl and GMHPhotoReceptor.jl repositories for details on how to use them.
Add the path to the GMHPhotoReceptor.jl
module file to ~/.juliarc.jl
by executing the following command in the terminal window.
juser@juliabox:~$ echo 'push!(LOAD_PATH,"/home/juser/GMHExamples.jl")' > .juliarc.jl
juser@juliabox:~$ echo 'push!(LOAD_PATH,"/home/juser/GMHPhotoReceptor.jl")' > .juliarc.jl
The command creates the file if it does not yet exist. You can check that it was correctly added by executing cat ~/.juliarc.jl
in the terminal window.
Install Julia from http://julialang.org/downloads/. You can also install a development environment. On Windows, Juno is recommended.
Start Julia and follow the instructions from Step 4.3 to install and test the Generalized Metropolis-Hastings packages.
Install the GMHExamples.jl and GMHPhotoReceptor.jl repositories from GitHub in a local folder. Instructions on how to install from GitHub can be found on GitHub.
Please refer to the documentation of the GMHExamples.jl and GMHPhotoReceptor.jl repositories on how to use them.
Add the following line to the ~/.juliarc.jl
file, inserting the correct path to the GMHPhotoReceptor.jl
folder.
push!(LOAD_PATH,"/path/to/GMHExamples.jl")
push!(LOAD_PATH,"/path/to/GMHPhotoReceptor.jl")
.juliarc.jl
should reside in your home folder, which is system dependent. On Windows, this is usually C:\users\<your name>
.
The master server in the cluster needs to be configured with AWS Access Keys. Please follow the steps outlined in "To create, modify, or delete a user's access keys" in:
Make sure to download the AWS Access Key ID and Secret Access Key to your local machine and store them in a secure location. Typically, this step needs to be executed only once.
Note: if you see in your security credentials that you have an AWS Access Key ID, but did not create this yourself, did not download the Secret Access Key, or lost the Secret Access Key, you will have to create a new one as outlined in the documentation above. In that case, you can also delete the existing AWS Access Key as you will not be able to use it.
Follow the steps in Section 3 to set up your own Jupyter/IJulia Notebook server. Connect to this machine using SSH, as explained in Step 3.2.
This machine will be the only one in your cluster which can be accessed from outside AWS, which is determined by the security group specified in Step 2.1.
To configure SSH access to the additional worker machines in the cluster, run the following script:
GMHConfigure/gmh-cluster/config.sh
The script asks for your AWS Access Keys and region. The default region is currently eu-west-1.
The script creates a Key Pair for password-less login over SSH, saves the private key to a secure location on the master server, and adds the public key to your AWS console. The name of the key is julia-cluster-access-xxx.xxx.xxx.xxx with xxx standing for the private IP address of the cluster.
Return to the Instances tab in the AWS console, click Launch Instance and launch 1 or more Worker instances in a similar manner to the Launch Instance procedure outlined in Step 3.1. Launch the same AMI as your master server using the My AMIs section, specifying the desired number of instances in option 3. Configure Instance, and ensure to launch it into the same subnet (Step 3.1.3). For the security group (Setp 3.1.6), this time only select the default VPC security group.
When selecting the key pair (Step 3.1.7), select the julia-cluster-access-xxx.xxx.xxx.xxx Key Pair you created in the previous step.
Go to the instances page, select the launching instance, and in the Description tab in the bottom half of the page, note down the Private IPs.
You should test that passwordless SSH access to this worker is set up correctly by executing in your existing SSH terminal session.
ssh<EMAIL_ADDRESS>where xxx.xxx.xxx.xxx is the private IP address you obtained from the AWS console.
If you have followed all steps, this command should log into the slave machine. This step also results in the SSH key being added to the list of known hosts and is required before automatic SSH login can work inside Julia.
Type exit to log out from your internal SSH session and return to the original SSH session.
To test that you can now launch Julia worker processes on the additional worker machines in the cluster, open a Julia REPL (by typing julia
) and execute the following:
julia> machvec = [("ubuntu@xxx.xxx.xxx.xxx",:auto),("ubuntu@xxx.xxx.xxx.xxx",:auto)]
Where xxx.xxx.xxx.xxx are the private IP addresses you obtained in Step 6.4.
As shown above, you can add multiple (IP address,:auto) pairs to the vector, separated by commas. The :auto
symbol ensures that each worker machine launches as many processes as it has cores.
Launch additional workers on the remote machine by executing the following command:
julia> addprocs(machvec,topology=:master_slave)
The function call will return a list of the new process IDs.
You can run the tests of the GeneralizedMetropolisHastings package in such a way that it will utilize these additional workers:
julia> cd(Pkg.dir("GeneralizedMetropolisHastings"))
julia> include("test/runtests.jl")
If you have more than 1 worker running, in the last printout of the tests you will notice a line that says that the test ran with more than 1 remote segment:
RemoteSegments with 4 segments and 13 proposals per segment.
For a cluster with 1 master process and 4 worker processes.
Close all remote workers by executing:
julia> rmprocs(workers())
Close the julia session by typing exit()
.
You can now launch the Jupyter/IJulia server as explained in Step 3.4 and Step 3.5. You are now ready to run Julia scripts and notebooks on the cluster.
Starting from a fresh Ubuntu Server 14.04LTS or similar, follow the instructions to launch and connect to an AMI over SSH.
In the SSH terminal, execute the following commands to install the Git repository software:
sudo apt-get update
sudo apt-get -y install git
Install the configuration scripts from the GMHConfigure repository:
git clone https://github.com/QuantifyingUncertainty/GMHConfigure
GMHConfigure/gmh-ami/config.sh
The script will install Julia, the GeneralizedMetropolisHastings code, the example repositories and all required packages.
It will also run the tests of the GeneralizedMetropolisHastings package in Julia. These tests should normally pass, but the installation is allowed to continue in case they fail.
The last line printed by the script will indicate whether the installation process was successful.
To remove all private keys, command-line history and other settings from the AMI prepared using the steps from Section 7.1, run the script:
GMHConfigure/gmh-ami/prepare-for-publication.sh
After this script has been executed, you will not be able to log in again to the same instance. Logout from the instance, stop the instance from the EC2 console, and follow these steps to create the AMI:
http://docs.aws.amazon.com/AWSEC2/latest/UserGuide/creating-an-ami-ebs.html#how-to-create-ebs-ami
Further security guidelines can be found in: https://aws.amazon.com/articles/0155828273219400
Here are general guidelines to share a public AMI:
http://docs.aws.amazon.com/AWSEC2/latest/UserGuide/sharing-amis.html
If you have made changes to the GMHConfigure repository, you can submit them to the GMHConfigure repository. If you do not have write permissions to the repository, fork, submit and submit a pull request, as explained in the GitHub documentation. If you do have write permissions, you can submit your changes via the following commands:
git commit -a
Check if the remote branch is set correctly by executing git remote -v
. If not, add it with the following command:
git remote add origin https://github.com/QuantifyingUncertainty/GMHConfigure
Push the changes to the remote repository:
git push
You will be asked for your GitHub username and password.
Calderhead B. (2014), A general construction for parallelizing Metropolis-Hastings algorithms, PNAS, Vol: 111, Pages: 17408-17413


---
layout: default
title: Scrum Sprint Schedule
---
Feb 5 to 9th
- Setup Eclipse Workspaces
- Training
- APP Developement (Hands On)
Sprint #1
Feb 5 to Feb 16
- Install CPM
- Fiori Decoupled NW
- HANA XSA
- CI Components (Continuous Delivery)
Sprint Logistics
Week of Feb 26 Meeting
- Overview of Sprint Logistics
- Agile Tools and How to Use Them
- Process Flow
- Issue Management
- Roadblocks, Iceblock, Scope/InOut
Sprint #2
Mar 5 to 16
- Process: Opportunity to Project Estimate
- CRM Integration
- Analysis Office Workbook Models
- Project Team Roles
- Workflow Approvals for Project Estimate
- Workflow Handoff from CRM to CPM and CPM to CPQ
- Alerts, Actions to Support Process
- Details of Sprint 2
Sprint #3
Mar 19 to 30
- Validate final process flow for Oppoertunity to Estimate
- Develop use cases for all business unit scenarios
- Review design specification for opportunity to estimate and finalize
- Release 1 of web apps
- Refine and finalize app requirements for opportunity to estimate (CPM Only)
Sprint #4
Apr 2 to 13
- Process: Project Templates, Customer Acceptance and Project Setup
- Project Structures
- Sale Products
- Project Types
- Templates of Tasks Per Product
- Sales Order
- Customer Acceptance
- Auto Create of Project Structures
- Details to Sprint
Sprint #5
Apr 16 to 27
- Process: Issue Management and Risk Management
- Issues Management Apps
- Risk Management Apps
- Workflow to Process Issues, Risks Change Orders
- Alerts, Actions to Support Process
Sprint #6
Apr 30 to May 11
- Process: Change Orders
- Change Orders
- Workflow to Process Change Orders
- Alerts, Actions to Support Process
Sprint #7
May 14 to 25
- Process: Project Billing, Revenue, Revenue Recognition
- Time and Materials
- Fixed Price with Milestone Billing
- Periodic Billing
- Delivery Related Billing
- Booking of Revenue
- Revenue Recognition
Sprint #8
May 28 to June 8
- Process: Misc Supporting Processes
- Forecasting, ETC, Earned Value, POC
- Project Procurement
- Material Components
- Reporting and Dashboards
Sprint #9
June 11 to June 22
- Process: Multi-Resource Scheduling
- Scheduling
- Integration between projects and field service
- Resource planning
- Reporting and Dashboards


All About Me!
Hello! I am Kavish!I am in 7th grade!I am 12 years old. One of the hobbies I enjoy is playing with Robots.


| Class and Description |
|---|
| ISearchMonitor
|
| Class and Description |
|---|
| IMonitorContradiction
An interface to monitor contradiction in search loop
|
| IMonitorSolution
An interface to monitor solution instruction in the search loop
|
| ISearchMonitor
|
| Class and Description |
|---|
| IMonitorContradiction
An interface to monitor contradiction in search loop
|
| IMonitorInitialize
An interface to monitor the initialization action of the search loop
|
| IMonitorOpenNode
An interface to monitor open node action in the search loop
|
| IMonitorSolution
An interface to monitor solution instruction in the search loop
|
| IMonitorUpBranch
An interface to monitor up branch actions in the search loop
|
| ISearchMonitor
|
| Class and Description |
|---|
| ISearchMonitor
|
| SearchMonitorList
|
| Class and Description |
|---|
| IMonitorInterruption
An interface to monitor interruption of the search loop
|
| IMonitorRestart
An interface to monitor restart instruction in the search loop
|
| IMonitorSolution
An interface to monitor solution instruction in the search loop
|
| ISearchMonitor
|
| Class and Description |
|---|
| IMonitorInitPropagation
An interface to monitor the initial propagation of the search loop
|
| IMonitorUpBranch
An interface to monitor up branch actions in the search loop
|
| ISearchMonitor
|
| Class and Description |
|---|
| IMonitorClose
An interface to monitor close operation of the search loop
|
| IMonitorContradiction
An interface to monitor contradiction in search loop
|
| IMonitorDownBranch
An interface to monitor down branch actions in the search loop
|
| IMonitorInitialize
An interface to monitor the initialization action of the search loop
|
| IMonitorInitPropagation
An interface to monitor the initial propagation of the search loop
|
| IMonitorInterruption
An interface to monitor interruption of the search loop
|
| IMonitorOpenNode
An interface to monitor open node action in the search loop
|
| IMonitorRestart
An interface to monitor restart instruction in the search loop
|
| IMonitorSolution
An interface to monitor solution instruction in the search loop
|
| IMonitorUpBranch
An interface to monitor up branch actions in the search loop
|
| ISearchMonitor
|
| SearchMonitorFactory
|
| Class and Description |
|---|
| IMonitorClose
An interface to monitor close operation of the search loop
|
| IMonitorContradiction
An interface to monitor contradiction in search loop
|
| IMonitorDownBranch
An interface to monitor down branch actions in the search loop
|
| IMonitorInitialize
An interface to monitor the initialization action of the search loop
|
| IMonitorInitPropagation
An interface to monitor the initial propagation of the search loop
|
| IMonitorOpenNode
An interface to monitor open node action in the search loop
|
| IMonitorRestart
An interface to monitor restart instruction in the search loop
|
| IMonitorSolution
An interface to monitor solution instruction in the search loop
|
| IMonitorUpBranch
An interface to monitor up branch actions in the search loop
|
| ISearchMonitor
|
| Class and Description |
|---|
| IMonitorSolution
An interface to monitor solution instruction in the search loop
|
| Class and Description |
|---|
| IMonitorContradiction
An interface to monitor contradiction in search loop
|
| IMonitorDownBranch
An interface to monitor down branch actions in the search loop
|
| IMonitorRestart
An interface to monitor restart instruction in the search loop
|
| ISearchMonitor
|
| Class and Description |
|---|
| IMonitorContradiction
An interface to monitor contradiction in search loop
|
| IMonitorRestart
An interface to monitor restart instruction in the search loop
|
| IMonitorSolution
An interface to monitor solution instruction in the search loop
|
| ISearchMonitor
|
| Class and Description |
|---|
| IMonitorClose
An interface to monitor close operation of the search loop
|
| IMonitorInitPropagation
An interface to monitor the initial propagation of the search loop
|
| ISearchMonitor
|
Copyright © 2015. All rights reserved.


{{define "cmd.html"}} {{with .pdoc}}
The go get command cannot install this command because of the following issues:


Class SpatialMap<T>
Designed as an more efficient data structure for recording objects on a map. The simple version: if you're about to use a List to store a bunch of objects in your map, consider using this or MultiSpatialMap instead!
Implements
Inherited Members
Namespace: GoRogue
Assembly: GoRogue.dll
Syntax
public class SpatialMap<T> : AdvancedSpatialMap<T>, ISpatialMap<T>, IReadOnlySpatialMap<T>, IEnumerable<ISpatialTuple<T>>, IEnumerable where T : class, IHasID
Type Parameters
| Name | Description |
|---|---|
| T | The type of object that will be contained by this SpatialMap. Must implement IHasID and be a reference-type. |
Remarks
Typical roguelikes will use a 2D array (or 1D array accessed as a 2D array), for terrain, and lists of objects for things like entities, items, etc. This is simple but ultimately not efficient; for example, in that implementation, determining if there is an object at a location takes an amount of time proportional to the number of objects in this list. However, the other simple option is to use an array with size equal to the size of the map (as many do for terrain) for all object lists. This is even less ideal, as in that case, the time to iterate over all objects becomes proportional to the size of the map (since one has to do that for rendering, ouch!), which is typically much larger than the number of objects in a list. This is the problem SpatialMap is designed to solve. It provides fast, near-constant-time operations for getting the object at a location, adding entities, removing entities, and will allow you to iterate through all objects in the SpatialMap in time proportional to the number of objects in it (the best possible). Effectively, it is a more efficient list for objects that have a position associated with them. This implementation can only allow one item at a given location at a time -- for an implementation that allows multiple items, see MultiSpatialMap. The objects stored in a SpatialMap must implement the IHasID (see that interface's documentation for an easy implementation example). This is used internally to keep track of the objects, since uints are easily (efficiently) hashable.
Constructors
| Improve this Doc View SourceSpatialMap(Int32)
Constructor. Creates an empty SpatialMap.
Declaration
public SpatialMap(int initialCapacity = 32)
Parameters
| Type | Name | Description |
|---|---|---|
| System.Int32 | initialCapacity | The initial maximum number of elements the SpatialMap can hold before it has to internally resize data structures. Defaults to 32. |


Alan Bersten Posts ‘Proud’ Message For Hannah Brown On Day Of ‘DWTS’ Finale
November 25, 2019
Alan Bersten Posts ‘Proud’ Message For Hannah Brown On Day Of ‘DWTS’ Finale
Alan Bersten shared a sweet new message for his Dancing With The Stars partner, Hannah Brown, on Instagram today. Today is notably the day of the finale, as the pair will hit the dance floor with hopes of winning the coveted Mirrorball Trophy.
The photo that pro-dancer Alan chose showed the duo posing on the ground. Hannah wore a white sports bra and tight navy leggings, while her neon yellow sneakers popped in the shot. Alan wore a black t-shirt with a low, relaxed neckline and navy blue pants. He opted for black Adidas sneakers. The former Bachelorette star was seen smiling with her lips closed, as she slung her left arm over Alan’s shoulders. Alan smiled too, with his lips closed, as she rested his left arm on his knees. He wore a couple of bracelets, which gleamed in the light.
Hannah also wore her hair in a half-up, half-down hairstyle. It was hard to see if she wore any makeup. But considering that she may have been getting ready to practice, or just wrapped up practice when the shot was taken, it’s likely she kept things minimal.
The photo was taken in a room at night, as the duo were illuminated while sitting on the wooden floor. Behind them was darkness, however, and windows that lit up with orange light.
Fans had plenty of nice messages for the pair in the comments section.
“So proud of you guys. You both truly deserve the MBT so much,” raved a follower.
“Huge fan – you got this Hannah – pretend it’s a crown you want – which you do!!!!” exclaimed an admirer, referring to her pageant days.
Loading...

“Next photo can be of you guys winning the mirror ball trophy or maybe kissing plz lol,” expressed a fourth Instagram user.
The pair have been dealing with a large number of rumors about a potential romantic relationship. Both have denied the claims again and again, but it’s clearly not stopping the fans from hoping.
And in addition, Alan posted another photo of him and Hannah several days ago, as the reality TV star showed off her figure in a form-fitting blue dress. They were seen posing indoors at what looked like a banquet hall. Hannah’s dress featured a sweetheart neckline and 3/4-length sleeves, along with a skirt that reached her knees. She smiled widely while Alan posed alongside her.


Mnangagwa meets British Ambassador
by Staff ReporterBritish Ambassador to Zimbabwe, Melanie Robinson is this Wednesday paying a courtesy call on President Emmerson Mnangagwa at his Munhumutapa Offices in Harare.
Also present are envoys, Harriet Matthews, the Director for Africa in the Foreign and Commonwealth office and Debbie Palmer, the Director for West and Southern Africa in the UK Department for International Development. The envoys are currently in a closed-door meeting.
The meeting is held when Zimbabwe is trying to mend relations with the international community, particularly the West whose relations with Zimbabwe turned sour two decades ago over alleged human rights violations committed during the fast track land reform programme.
More: ZBC News


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{% comment %} Trade Agreement (TA) Text Template for trade scenario TWUK_TA_NoRoO: For countries with a UK trade agreement, or EPA (Economic Partnership Agreement) - but without continuing GSP (Generalised Scheme of Preferences) access, and for which TWUK does not have the Rules of Origin data. {% endcomment %}
The UK has a trade agreement with {{ country_name }}.
Where applicable, tariff preferences are available. If the conditions for preferential access are not met, the Most Favoured Nation (MFN) rate applies.


| << Wëap | Table of Contents | Legal Status >> |
Appendix I - Combat Ratings
Your combat rating is based on the number of kills you have made, which is the sum of the strengths of all the ships you have destroyed, adjusted to a baseline where shïp ID 128 represents 1 unit. The scale is as follows:
Kills: Rating: 0 No Ability 1 Little Ability 200 Fair Ability 400 Average Ability 800 Good Ability 1600 Competent 3200 Very Competent 6400 Worthy of Note 12,800 Dangerous 25,600 Deadly 51,200 Frightening The text strings listed above are given only by way of illustration, since they can be changed by editing STR# 138.
| << Wëap | Table of Contents | Legal Status >> |
(©) 2000-2002 by Matt Burch and Ambrosia Software, Inc.


Search on Developer's repositories and
their details
Details included are: Repos,projects,followers & following
search


Source IP
Destination IP
Network
Specify an IP and CIDR mask.
Source Port
Destination Port
Protocol
TCP
UDP
ICMP
Leave blank for none. (Default)
Protocol Number
Limit PCAP to a protocol number.
Before Absolute Time
Specify a time in UTC RFC3339, like
2017-04-30T13:26:43Z
. Use this
or
the time range.
After Absolute Time
Specify a time in UTC RFC3339, like
2017-04-30T13:26:43Z
. Use this
or
the time range.
Before Time Range
Specify an integer with
m
(minutes) or
h
(hours).
After Time Range
Specify an integer with
m
(minutes) or
h
(hours).
I solemnly swear I am up to no good.
Submit


#include "_doctype.html"
| x |
| x | #define NDATE(x)x |
| #define NCOLE |
Stuff "gets moved here" from the news page, so some of the links on this page are more likely than others not to work anymore. I still think this page may be of value and I just want you to be aware of this fact. Use the search field to find working pages with similar info.
#include "_footer.html"


{% include sidebars/sections/recent_posts.html %} {% include sidebars/sections/github.html %} {% include custom/sidebars/sections/twitter_multi.html %}


Please enter society name
Enter the established date
Please enter owner name
Please enter owner contact number
Please select block manager
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Please enter Secretary Name
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Please select logo image
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Enter Merchant Salt
Uncroped image will not save.


|
xpcc
|
Common data structures (list, queue etc.) More...
Classes | |
| class | xpcc::BoundedDeque< T, N > |
| Double ended queue. More... | |
| class | xpcc::DoublyLinkedList< T, Allocator > |
| doubly-linked list More... | |
| class | xpcc::DynamicArray< T, Allocator > |
| Dynamic Arrays. More... | |
| class | xpcc::LinkedList< T, Allocator > |
| Singly-linked list. More... | |
| class | xpcc::Pair< T1, T2 > |
| Pair<FirstType, SecondType> is a heterogeneous pair. More... | |
| class | xpcc::Queue< T, Container > |
| FIFO queue. More... | |
| class | xpcc::BoundedQueue< T, N, Container > |
| Bounded queue. More... | |
| class | xpcc::SmartPointer |
| Container which destroys itself when the last copy is destroyed. More... | |
| class | xpcc::Stack< T, Container > |
| LIFO stack. More... | |
| class | xpcc::BoundedStack< T, N, Container > |
| Bounded stack. More... | |
Functions | |
| xpcc::IOStream & | xpcc::operator<< (xpcc::IOStream &s, const xpcc::SmartPointer &sPtr) |
A container is a holder object that stores a collection other objects (its elements). They are implemented as class templates, which allows a great flexibility in the types supported as elements.
Many containers have several member functions in common, and share functionalities. The decision of which type of container to use for a specific need does not generally depend only on the functionality offered by the container, but also on the efficiency of some of its members (complexity). This is especially true for sequence containers, which offer different trade-offs in complexity between inserting/removing elements and accessing them.
xpcc::Stack and xpcc::Queue are implemented as container adaptors. Container adaptors are not full container classes, but classes that provide a specific interface relying on an object of one of the container classes (such as xpcc::BoundedDeque or xpcc::LinkedList) to handle the elements. The underlying container is encapsulated in such a way that its elements are accessed by the members of the container class independently of the underlying container class used.
Sequence containers:
Container adaptors:
Other:
Two special containers worth mentioning hide in atomic section:
The first is a simple, interrupt-save queue (but only for the AVRs). Whenever you need an to exchange data between a interrupt routine and the normal program consider using this queue.
The atomic container wraps objects and provides atomic access to them. This comes in handy when simple objects are accessed by an interrupt and the main program. The container provides secure access without much work in this case.
All implementation share a common set of function. Not every container implement every one of it, only a subset which is sufficient for the container.


add "Id" to every td element and label them with chess notations!
in order to allow drag and drop of piece (fonts!)
Rules :
1. pawns can move horizontally (left and right, too). Pawns Queen only from one end of the board to the other
2. A White player can move any white piece during his turn.
3. when a king dies, all pieces in his "kingdom" becomes immobile but remains on the board until the other same color king is mated.
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Please make sure that you have enabled pop-ups on your browser! To delete/edit a single item, click on it!


Use this section to specify what IntelliJ IDEA should use when you run tests, build, or run tasks in the selected linked project.


List of all members.
Detailed Description
downloader. Uses multiple SingleFileDownloader's for size checking before & downloading.
Member Function Documentation
Returns destination path which aFilename should be downloaded to. Doesn't check does aFilename exist in _filenames array.
| + (id) downloaderWithFiles: |
|
(NSArray *) |
files |
| withSourcePath: |
|
(NSString *) |
aSourcePath |
|
|
| |
Creates FilesDownloader with given source path & filenames.
- Parameters:
-
| files | Array of NSStrings of filenames. Each string is subPath that will be added to aSourcePath to determine full URL for single file. I.e. "foo/bar/file.txt" |
| aSourcePath | - path to download from (shared part for all files) I.e. "http://foo.com/files/" |
| - (id) initWithFiles: |
|
(NSArray *) |
files |
| withSourcePath: |
|
(NSString *) |
aSourcePath |
|
|
| |
Inits FilesDownloader with given source path & filenames.
- Parameters:
-
| files | Array of NSStrings of filenames. Each string is subPath that will be added to aSourcePath to determine full URL for single file. I.e. "foo/bar/file.txt" |
| aSourcePath | - path to download from (shared part for all files) I.e. "http://foo.com/files/" |
Returns total bytes count downloaded.
Returns total size for all content in bytes.
Returns download progress completion in percents.
Property Documentation
Delegate for download status callbacks.
The documentation for this class was generated from the following file:


DISNEY'S THE KID A film review by Steve Rhodes Copyright 2000 Steve Rhodes RATING (0 TO ****): ***
In DISNEY'S THE KID, Russ Duritz (Bruce Willis) is a control freak who doesn't abide any troubles in his life. With an assistant, Janet, played in full scene-stealing mode by Lily Tomlin, who is ready to try to turn the power off on Atlanta if need be, Russ never lets problems get near him. He also keeps love, in the form of a warm and beautiful girlfriend, Amy (Emily Mortimer), at arm's length.
One day into his rigid world comes a pair of hallucinations. The first involves a guy in a shiny red biplane who keeps swooping about. The other, and the more troubling, is an 8-year-old named Rusty (Spencer Breslin), who starts hanging around Russ's lavish home.
A very uptight image consultant, Russ surrounds himself with material possessions from $2,000 suits to sleek sports cars. He's a cynical human being who thinks he can manipulate opinion at will -- after all that's what he does for a living and he's the best at it.
His past is an embarrassment to him and something which he never thinks about. When his dad asks for personal help in packing, he sends a check to hire movers instead.
Russ's carefully orchestrated life is torn apart when he learns that Rusty is himself at age 8. Although Russ is supremely proud of his conspicuous accomplishments, Rusty isn't so pleased to learn how his life has turned out. "No dog!" Rusty wails. "No dog! I grow up to be guy with no dog!" Rusty is also disappointed to learn that he isn't married and doesn't fly jets as he planned. "I'm a loser!" Rusty concludes.
Russ, on the other hand, remembers what a pudgy, clumsy, whimpering child he was and is not pleased either. When he tries to teach himself (as a kid) a thing or two, the results are hilarious, albeit not particularly successful.
The chemistry between the two actors is delightful. Physically they look like such an odd pairing that their relationship will never work, but it does beautifully. The kid holds his own against a famous star and gives as much as he gets. You can see the mutual respect in their eyes.
The script by Audrey Wells (THE TRUTH ABOUT CATS AND DOGS) is funny without ever being insulting or patronizing. Avoiding slapstick almost entirely, the script is remarkably intelligent and sharp.
The story, which is at once sweet and serious, turns into a journey of exploration for Russ, and it's a trip that he has avoided all of his life. "When I look at him, I see awful memories," Russ tells Amy about Rusty. "Memories that I've spent my life trying to forget." The kid is obviously there for a purpose. But what exactly? The poor kid, on the other hand, just wants to get home and out of all this time traveling.
The conclusion wraps things up well and without ever trying to become FREQUENCY 2. DISNEY'S THE KID is a unique little movie with a big heart. You'll laugh, you might even cry, and your heart will be touched -- something that probably isn't the least bit obvious from the saccharine and sort of silly trailers for the picture. A satisfying movie, it is wonderful family entertainment as well, although very young viewers may get very fidgety as the ones did at our screening. But for the older kids and the adults, the movie has a lot to offer.
DISNEY'S THE KID runs 1:41. It is rated PG for mild language and has nothing to offend any one of any age.
My son Jeffrey, age 11, was there with several of his classmates of the same age. He found the film funny, cute and really sweet and gave it a full ****. Johanna, who also gave it ****, was bursting with positive adjectives, ranging from fantastic to hilarious. Maxim thought it was funny and gave it ***.
Email<EMAIL_ADDRESS>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


The problem of the existence of life beyond Earth is investigated, drawing from recent research in astronomy and other fields. For non-science majors. Prerequisite: ASTRO 001, ASTRO 005, or ASTRO 010
ASTRO 140 provides 3 credits at the undergraduate level and satisfies part of the University's General Education Natural Sciences (GN) requirement for a baccalaureate degree. The course is designed for non-science majors who have had a semester or more of science; it is not intended as the students’ first university-level science course. Many students have taken a general astronomy class (ASTRO 1, 5, 6, 7, or 10) but also students with classes in Earth sciences, biology, or chemistry are probably also adequately prepared. Please contact the instructor to discuss your background if you do not have the formal prerequisites.
There are no face-to-face classes for this World Campus course; it is on-line only. The class follows the University academic calendar. There is no Final Exam but there are assignments that must be completed by exam week. The curriculum is divided into 15 weeks with five themes (listed below).
An Introduction to Astrobiology, 3rd Edition, edited by David A. Rothery, Iain Gilmour & Mark A. Sephton (Cambridge University Press, 2018, ISBN 978-1-108-43083-8, paperback). It is important that students have this book, as we will read much of it during 12 of the 15 weeks of the course. The 3rd edition has the latest discoveries for Solar System and exoplanet discoveries. It can be purchased or rented from MBS Direct or other book vendor like Barnes & Noble and Amazon.com. MBS Direct (working with PSU World Campus) promises rapid delivery even to locations outside of the USA and can be contacted by phone at 1-800-325-3252.
The course content, class discussions, quizzes, and the gradebook are all integrated in Penn State’s Canvas course management system. Students need to be registered for the course and have an Penn State ACCESS account to log into the course Web site.
The possible existence of life beyond Earth is one of the most fundamental questions relating human beings to the physical Universe around us. While considerations of extraterrestrial life were in the domains of philosophy and science fiction in the past, today we have considerable scientific knowledge that can be applied to the question. Advances in modern astronomy have dramatically improved our understanding of our cosmic surroundings: most importantly we now know (in the past decade) that most stars we see at night have their own planetary systems, and some of appear to be habitable. Several fields -- geology, biochemistry, paleontology (fossils), evolutionary biology -- give insight (though not a complete understanding) on how life arose on Earth, and robotic spacecraft are actively searching for life elsewhere in our Solar System.
The results from studies on Earth, the Solar System, and exoplanets across the Galaxy together indicate that the conditions for life are widespread in the Universe; extraterrestrial life has not been found yet, but does not seem implausible. Interstellar space travel between habitable planets, by humans or other advanced beings, is exceedingly difficult but not physically impossible. The course is thus rooted in modern science, but is connected to the long-standing philosophical question: Are we alone in the Universe? In the past, this question is often embedded in science fiction (such as movies about aliens) and discussion about whether aliens have visited Earth. Today, astronomical studies are leading the way in answering parts of the question with a strong scientific foundation. But there is no evidence yet for life outside of Earth.
Part of the course resembles a traditional classroom learning environment: We have lectures by the instructor (online rather than in person except for introductory videos), read chapters of our textbook, and take quizzes to evaluate that we have learned the material. But the course also has more interactive assignments: students participate in focused discussion forums; take part in a huge citizen science research effort to find exoplanets; and engage in science writing. The result is a multifaceted learning experience encouraging students to engage in active learning processes. At Penn State, students are expected to devote around 9 hours-per-week to a 3-credit course during the 15-week semester. It is not a trivial commitment. Student responsibilities are distributed throughout the semester and the course cannot be completed in a rush.
Having no face-to-face classes in a World Campus class has the disadvantage that we never meet as a learning community, much like all university classes during last year's Covid-19 pandemic. But distance learning also has advantages. Students need not reside or travel to the Penn State campus; they can live anywhere in the world. Students do not have to attend Astro 140 classes at specific times; all interactions are asynchronous. This is very convenient for individuals with other important responsibilities. But the independence provided by World Campus does mean that students must be disciplined in devoting time to the course continuously during the semester. Duties include: studying course material (on-line lectures, linked on-line material, textbook reading), taking timed quizzes (which must be taken in the Canvas Web environment within specified 4-day intervals), writing short research papers (with specified deadlines), participating in interactive discussions, and engaging in an on-line Citizen Science activity. Details of the student responsibilities appear below under Graded Activities.
The course is divided into five themes that are, in turn, divided into several topics. The course is designed as a 15-week course with a new Web page environment for each week. Readings from our textbook, An Introduction to Astrobiology (abbreviated AIA) associated with each week are listed. Note that Thanksgiving Holiday takes place between Weeks 13 and 14.
Theme I: Astronomical context for life (Weeks 1-2)
Theme II: Life on Earth (Weeks 3 - 4)
Life elsewhere in the Solar System (Weeks 5-7)
Theme IV: Planetary Systems in the Galaxy (Weeks 8 - 11)
Theme V: Life Around Other Stars (Weeks 12 - 15)
40% Quizzes After each Theme, students will take a quiz on recent material covered in the class, associated reading and online material. The quizzes have combinations of multiple choice, short answer and short essay questions. Students may have access to notes, the textbook, and the Web, but study prior to the quiz is necessary because of the time constraint. Each quiz will be taken in Penn State's Canvas Web environment in a single sitting anytime over a 4-day period starting early-Friday and ending end-of-Monday. Dates are: Quiz #1, Quiz #2, Quiz #3, Quiz #4, Quiz #5. For each student, the lowest scoring quiz is dropped and each remaining quizzes is worth 10% of the course grade.
30% Papers Students will submit two original papers using topics and resources provided by the instructor. The goals are: (1) investigating a narrow scientific issue in some detail; (2) assimilating diverse information into a coherent narrative; and (3) training in the art of scientific writing. The papers review scientific findings and present them in a formal style. Papers have 3 pages single-spaced of text supplemented by references and figures. The student learns how to write high-quality scientific documents from background material benefiting from individual interaction with the instructor on Paper #1. The student then writes Paper #2 on their own. There are three deadlines: preliminary draft of Paper 1 (outline + 2 paragraphs, 3% of grade), final version of Paper 1 (12%), and delivery of Paper 2 (15%). More details about science writing, paper requirements, and sample topics will be given in the course content website.
20% Discussion Throughout the course, we will hold informal discussions on through the Canvas Discussion environment. The instructor will start with a question, often accompanied with on-line material. Students then participate with with commentary and interaction based on scientific fact and reasoning. Points are earned by number and quality of contributions with a maximum of 20% of the course grade.
10% Project During Weeks 8-10, we will engage in the Zooniverse Citizens Science' activity Planet Hunters TESS based on NASA’s Transiting Exoplanet Survey Satellite launched in 2018. After Web-guided training, each student will examine a different subset of TESS’s star ‘light curves’, looking for the characteristics repeated dips in brightness that occur when an exoplanet passes in front of the star. Students will submit a document of their effort and analysis, and the class’s collective contribution will be discussed.


WITNESS LIST
Public Health Committee
March 6, 2013 - 8:00 AM
Against:
Wilson, Stacy (Texas Hospital Association)
On:
Lovelace, Joe (Texas Council of Community Centers)
Registering, but not testifying:
For:
Sprinkle, Gk (Texas ambulance association)
For:
Draker, Sheryl (Self)
Herndonqq, Patrick (Self; Community Medicine)
Sokol, Marian (Self; Parents of children with fasd)
Against:
Carter, Kimberly (Self; Texas Medical Association)
On:
Ingalsbe, Sylvia (Texas Office for Prevention of Developmental Disabilities)
Rodriguez, Gerardo (Texas Office for Prevention of Developmental Disabilities)
Registering, but not testifying:
For:
Crockett, Sarah (Self; Texas Association for Infant Mental Health)
Garcia, Eileen (Texans Care for Children)
LeBleu, Stephanie (Texas CASA)
Snider, Stewart (League of Women Voters of Texas)
Switzer, Gyl (Mental health america oqf texas)
Against:
Sjoberg, Elizabeth (Texas Hospital Association)
On:
Cooper, Sam (Texas department of State Health Services)
Sharkis, Janet (Texas Office for Prevention of Developmental Disabilities)
For:
Bone, Jennifer (Self; Texas Academy of General Dentistry)
Peppard DDS, Mark (Self; Tx Dental Assoc)
On:
Jones, Lisa (Texas State Board of Dental Examiners)
1
WITNESS LIST
Registering, but not testifying:
For:
Gibson, Stephanie (Texas Dental Hygienists Association)
Rudd, Tyler (Texas Academy of Pediatric Dentistry)
On:
Parker, Glenn (Texas State Board of Dental Examiners)
For:
Andolino, Debbie (Self)
Barillas, Ph.D., Katherine (One Voice Texas)
Dorsett, Vivian (Self; Foster Care Alumni of America-Texas Chapter)
Foster, Mike (Self; Tacpa)
Hamilton, Cathy (Casa)
Henderson, Javier (Self)
Lavallo, Richard (Disability rights texas)
Obaseki, Min. Tyrone (Self)
Provost, Tressa (Self)
Sharp, Kristopher (Self)
Sparks, Andrea (Texas CASA)
Spiller, Lee (Citizens Commission on Human Rights)
Wagner, Laquinton (Self)
On:
Amberboy, Tina (Supreme Court of Texas Children's Commission)
Kromrei, Elizabeth "Liz" (Department of Family and Protective Services)
Streusand, William (Self)
Woomer, Eric (Federation of Texas Psychiatry)
Registering, but not testifying:
For:
Breeding, John (Self)
Crockett, Sarah (Texas Association for Infant Mental Health)
Garcia, Eileen (Texans Care for Children)
Haskin, Becky (CASA)
Hastings, Paul (Self; Texas Home School Coalition)
Merfish, Brett (Texas appleseed)
Milam, Susan (National Association of Social Workers/Texas Chapter)
Moore, Jim (Self; Cchr)
Sheely, Jessica (Texas CASA)
On:
Fazio, Heather (Self; Texans for Accountable Government)
Harper, Michelle (HHSC)
Raymond, Kerry (Department of State Health Services)
Rogers, James "Jim" (Department of Family and Protective Services)
2
WITNESS LIST
On:
Vasquez, Andy (HHSC)
For:
Herman, Guy (Self; Presiding Judge of the Statutory Probate Courts of Texas)
On:
Powdrill, Bill (Audubon behavioral Healthcare)
Registering, but not testifying:
On:
Raymond, Kerry (Department of State Health Services)
For:
Hench, Marina (Texas Association for Home Care and Hospice)
Against:
Gonzales, David (Texas Association of Health Plans)
On:
Littlefield, Lindsay (Legislative Budget Board)
McDade, Gwen (HHSC OIG)
Registering, but not testifying:
On:
Foster, Mike (Self; Texas assoc of child placing agencies)
Sparks, Joy (HHSC's OIG)
Villarreal, Rudy (HHSC)
Wilson, Douglas (HHSC)
For:
Buckingham, James (Self)
Friese, Jan (Texas counseling association)
Powdrill, Bill (Self; Audubon behavioral healthcare)
Rushing, Susan (Self; Burke center)
Registering, but not testifying:
For:
Kenderdine, Marshall (Texas Pediatric Society)
Woomer, Eric (Federation of Texas Psychiatry)
On:
Spinks, Darrel (TX State Board of Examiners of Psychologists)
3
WITNESS LIST
For:
German, Tony (Texas Ambulatory Surgery Center Society)
On:
Elerian, Nagla (Texas Department of State Health Services)
Levine, Ken (Sunset Commission)
Registering, but not testifying:
For:
Kolodzey, Patricia (Texas Medical Association)
Against:
Dewitt, Cathy (Texas association of business)
On:
Dewitt, Cathy (Teas association of business)
Raimer, Ben (Texas institute for health care quality and efficiency board of directors, presiding
officer)
4


Creating and Managing Services
Services provide stable endpoints for Pods based on a set of labels.
In this chapter you will create the monolith
service and "expose" the secure-monolith
Pod externally. You will learn how to:
-
Create a service
-
Use label selectors to expose a limited set of Pods externally
Tutorial: Create a Service
Explore the monolith service configuration file in manifests/app/services/monolith.yaml
Notice:
-
The service type (
None
,ClusterIP
,NodePort
orLoadBalancer
) -
Pod selector to identify all pods targeted by the service
-
ports configuration:
-
targetPort
to define which container port(s) your service targets -
port
to define on which port your service is exposed inside the cluster -
nodePort
(optional), to explicitely specify on which port to expose your service outside of the cluster.
-
Then create the monolith service using kubectl:
kubectl apply -f manifests/app/services/monolith.yaml
Specifically on Google Cloud Platform, you need to allow incoming traffic to your cluster node’s port.
Use the gcloud compute firewall-rules
command to allow traffic to the monolith
service:
gcloud compute firewall-rules create allow-monolith-nodeport --allow=tcp:31000
Exercise: Interact with the Monolith Service Remotely
Hints
On GCP, Kubernetes cluster nodes are standard Google Compute Engine VM instances managed by GKE.
With service of type NodePort, you should be able to connect to your monolith throught the service node port, which is defined to 31000
in our yaml.
List the GCP VMs which compose the GKE cluster to get their public IP addresses
gcloud compute instances list
Output:
NAME ZONE MACHINE_TYPE INTERNAL_IP EXTERNAL_IP STATUS
gke-istio-workshop-default-pool-e37360ba-369z europe-west1-b n1-standard-1 <IP_ADDRESS> <IP_ADDRESS> RUNNING
gke-istio-workshop-default-pool-e37360ba-3hz4 europe-west1-b n1-standard-1 <IP_ADDRESS> <IP_ADDRESS> RUNNING
gke-istio-workshop-default-pool-e37360ba-8345 europe-west1-b n1-standard-1 <IP_ADDRESS> <IP_ADDRESS> RUNNING
Then use any of the External IP
to connect to the NodePort
curl -k https://<EXTERNAL_IP>:31000
Exercise: Explore the monolith Service
Tutorial: Add Labels to Pods
Currently the monolith
service does not have any endpoints. One way to troubleshoot an issue like this is to use the kubectl get pods
command with a label query.
kubectl get pods -l "app=monolith"
kubectl get pods -l "app=monolith,secure=enabled"
Notice this last query does not print any results
Use the kubectl label
command to add the missing secure=enabled
label to the secure-monolith
Pod.
kubectl label pods secure-monolith 'secure=enabled'
View the list of endpoints on the monolith
service:
kubectl describe services monolith
Tutorial: Remove Labels from Pods
In this exercise you will observe what happens when a required label is removed from a Pod.
Use the kubectl label
command to remove the secure
label from the secure-monolith
Pod.
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Genesis 8:12
And he stayed yet other seven days; and sent forth the dove; which returned not again unto him any more.


Chile
Daniela Tejada is a graduate of Public Administration and currently a Masters Candidate in Political Science at the University of Chile. She is the Research Coordinator at Fundación Ciudadano Inteligente, which includes data gathering and analysis, use of social research methodologies, and organizing the research team.
Chile ranked #29 in the 2014 Open Data Index / Other stories from Americas
This version is translated from the original Spanish version.
Open Data and Open Government policies have had a breakthrough the last years in Chile. The process began in 2002, but gained strength with the enactment of Access to Public Information law in 2008 and with the Citizen Participation in Public Administration law in 2011. That year was also created the Modernization and Digital Government area and the first version of Open Data portal of Government (datos.gob.cl), together with the entry of Chile to the Open Government Partnership (OGP). Year 2012 was followed by an Open Government Presidential Instruction urging the public bodies to publish datasets on the Open Government portal, as well as to encourage the strengthening of mechanisms for citizen participation. Finally, this year was formulated and presented the new OGP action plan for years 2014-2016, while the government continues enlarging modernization, digital government, open government and public innovation strategies.
However, modernization policies and openness are not measured in the number of laws enacted or government efforts to release public information, but the value they actually generate. In that sense, the exercise proposed by the Global Open Data Index, makes sense and relevance to deliver a first approximation with respect to the levels of progress and effectiveness of our governments in strengthening their opening strategies, as well as analyze comparatively the national progress in relation to regional and global environment.
The process that we lived in Chile during the development of the Index was generally quite simple. Most datasets are centralized in the web of government data, followed by the corresponding website of the different Ministries in each of the topics. The main difference in this respect is that the Digital Government Unit does care to deliver the documents in an non-proprietary format (CSV) while the Ministries tend to release the documents with paid licences (XLS).
In this regard, we note that countries above Chile as well as those with the same score in the ranking, are nations with extensive development of Government and Open Data policies, hence is valuable to share that closeness and progress with them. However, we know that the exercise conducted by the index is only a small sample of all areas and datasets that we should measure, so the challenge is to continue advancing in the release of more and better information, as well as analyse usage that is effectively being given to it and the value generated for citizenship, or well, what information that people need is still not delivered by the State. That is essentially the work that must be considered on, since the goal obviously is not Open Data itself, but generating public value through them.


Provides data set and function for exploration of Multiple Indicator Cluster Survey (MICS) 2014 Household Listing questionnaire data for Punjab, Pakistan (<http://www.mics.unicef.org/surveys>).
| Version: | 0.1.0 |
| Depends: | R (≥ 3.1) |
| Imports: | data.table, stats |
| Published: | 2017-09-07 |
| Author: | Muhammad Yaseen [aut, cre], Muhammad Usman [ctb] |
| Maintainer: | Muhammad Yaseen <myaseen208 at gmail.com> |
| License: | GPL-2 |
| URL: | https://github.com/MYaseen208/PakPMICS2014HL |
| NeedsCompilation: | no |
| Materials: | README NEWS |
| CRAN checks: | PakPMICS2014HL results |
| Reference manual: | PakPMICS2014HL.pdf |
| Package source: | PakPMICS2014HL_0.1.0.tar.gz |
| Windows binaries: | r-devel: PakPMICS2014HL_0.1.0.zip, r-release: PakPMICS2014HL_0.1.0.zip, r-oldrel: PakPMICS2014HL_0.1.0.zip |
| OS X binaries: | r-release: PakPMICS2014HL_0.1.0.tgz, r-oldrel: PakPMICS2014HL_0.1.0.tgz |
Please use the canonical form https://CRAN.R-project.org/package=PakPMICS2014HL to link to this page.


The RW-X model Hanging Wind Turbine is capable of producing over 1000 watts, but it is an experimental version at this time.
The diameter of the spinning blades is 5 feet and the windmill weighs about 25 pounds. 100 feet of hanging cable is included with the windmill. Also included are the bridge rectifier and digital panel meter showing volts, amps, watts, and kilowatts.
The RW-X will charge batteries up to 24 volts. The power output of the windmill in watts is equal to the voltage times the current. If you are charging a 24-volt system and the current is 10 amps, the power will be 240 watts (24 volts x 10 amps). To charge a 12-volt system with 240 watts will require 20 amps of current. This amount of current requires a larger wire size. And the size of the wire selected is an important design consideration. For this reason, we are not including the power cord. If you plan to purchase the RW-X, you will need to perform tests to determine the appropriate wire size to use for your application.
Only individuals with knowledge of how electricity works should purchase the RW-X.
There are 4 units available for purchase at this time.


MY FAMILY (MI FAMILIA) A film review by James Berardinelli Copyright 1995 James Berardinelli
RATING (0 TO 10): 8.7
U.S. Availability: wide release 5/3/95 Running Length: 2:07 MPAA Classification: R (Violence, profanity, sex, nudity)
Starring: Jimmy Smits, Eduardo Lopez Rojas, Jenny Gago, Edward James Olmos, Esai Morales, Constance Marie, Lupe Ontiveros, Jacob Vargas, Scott Bakula, Mary Steenburgen Director: Gregory Nava Producer: Anna Thomas Screenplay: Gregory Nava and Anna Thomas Cinematography: Edward Lachman Music: Mark McKenzie and Pepe Avila Released by New Line Cinema In English and Spanish with subtitles
MY FAMILY, the portrait of a Mexican-American family living in East Los Angeles, boasts a series of distinguished thematic antecedents, including Francis Ford Coppola's THE GODFATHER and Zhang Yimou's TO LIVE. Here, as in the 1972 gangster saga, the significance of family is a central issue, although each movie chooses to explore this differently. In THE GODFATHER, Vito and Michael Corleone struggled to hold their household together regardless of outside pressures; in MY FAMILY, family unity gives meaning to existence.
Although vastly different from THE GODFATHER, TO LIVE is also echoed by MY FAMILY. The 1994 Chinese film followed two characters from early marriage to old age, observing keenly that though lives end, life continues. Here, the setting is different, but the message is the same. MY FAMILY never shrinks from tragedy, but it doesn't wallow in it, either.
One highlighted truth is the commonality of the human experience. Though the focus is one specific family, every issue confronted by the characters is universal. As is true in all good "ethnic" motion pictures, the central culture provides a rich and resonant backdrop to stories capable of touching anyone, regardless of heritage or upbringing. Certain emotions, beliefs, and hopes cross racial lines, and it is through these that MY FAMILY finds its strength.
This film, which is epic in scale (although not in length--the running time is just over two hours), canvasses sixty years and three generations. Major events take place in three periods: the late 1920s and early 1930s, the late 1950s, and the 1980s. The third era is the longest and most detailed, but valuable background is presented in the other two. MY FAMILY requires the totality of its story for the climactic moments to attain their full dramatic impact, especially since writer/director Gregory Nava (EL NORTE) refuses cheap, theatrical methods of audience manipulation.
MY FAMILY opens in 1926 Mexico, as Jose Sanchez heads north to California to find a long-lost relative. Once there, he meets and marries Maria, who bears him a son and daughter. She is pregnant with their third child when immigration officials illegally deport her. The rest of this segment concentrates on her attempts to return to her husband and family.
The 1958 and 1980s episodes present the fortunes of two of the Sanchez children: Chucho (Esai Morales) and Jimmy (Jimmy Smits). Chucho is a brash youth who leads a gang, incurs the wrath of his father when he sells marijuana, and is constantly skirting trouble with the police. Jimmy idolizes his older brother and eventually follows in his footsteps, but the underlying pain of one shared, tragic moment haunts Jimmy's future. It is only during a watershed scene, when the anger and grief are released, that Jimmy is able to agree that "tomorrow matters."
Never before has Jimmy Smits shown the range and aptitude he displays here. As the emotional fulcrum of MY FAMILY, he is consistent, with no evidence of over- or underacting. Esai Morales and Constance Marie, who play two of Jimmy's siblings, bring fire, energy, and a touch of humor to their roles. In the parts of the aging Jose and Maria, Eduardo Lopez Rojas and Jenny Gago offer unforced performances salted with joy and pathos. Edward James Olmos as Paco, one of six Sanchez children, is the narrator (I could have done without the lengthy and intrusive voiceovers). Other cast members include Scott Bakula and Mary Steenburgen.
MY FAMILY constantly builds upon itself. Each scene has meaning not only because of what comes before it, but for what it adds to all that comes after. The film runs the audience through a range of emotions from laughter to tears, but the tone retains a sense of hopefulness. Nava has a clear vision that is achieved through the exceptional work of his cast and crew.
MY FAMILY is amazingly rich, with themes that are topical-yet- timeless, a solidly-constructed story to give them vitality, and superlative production values. Cinematographer Edward Lachman has photographed all three eras differently, and his visual flair adds another layer to this production. MY FAMILY gives us culture shock and class distinctions, metaphors involving owls and bridges, and the struggle between traditional values and modern ethics. It never dwells on gang violence, crime, or racism; but ignores none of these three. Above all, however, it is faithful to its title, presenting the newest portrait of an ancient truth--of all the ties that bind humans to each other, none is more lasting than that of birth and blood.
- James Berardinelli<EMAIL_ADDRESS>The review above was posted to the
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