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Runaway Bride * * (out of * * * * )
Directed by Garry Marshall. Cast: Richard Gere, Julia Roberts, Joan Cusack, Paul Dooley, Rita Wilson, Hector Elizondo, Christopher Meloni, Jean Schertler, Laurie Metcalf. 1999 - 116 minutes. Rated PG (for mild profanity). Reviewed July 31, 1999.
1990's "Pretty Woman" became the most popular romantic comedy of all time not only because of the unmistakable chemistry between Richard Gere and Julia Roberts, but because of the surprising charm and innocence that it also possessed. It may not have been groundbreakingly original (and it wasn't), but it ably carried itself purely on the intelligence of the actors and screenplay. Over nine years have passed now, and although Roberts and Gere are a little bit older, they unfortunately aren't quite as wise in their project choices, as proven by their sophomore reunion with director Garry Marshall. Unlike "Pretty Woman," "Runaway Bride" constantly feels like a phony, artificially manufactured excuse just to get the two actors together once again. Apparently, the importance of the writing and story weren't at the top of everyone's minds when they decided to take on this lackluster endeavor.
Ike Graham (Richard Gere) is a once-divorced columnist for the USA Today who happens to be working for his ex-wife (Rita Wilson). Searching for a revitalizing, interesting story to write about, Ike is told by one of his buddies that there is a young lady in the small rural town of Hale, Maryland, who likes to dump grooms on their wedding day and run away. When the article finally is written, that woman, Maggie Carpenter (Julia Roberts), who doesn't purposefully hurt her fiances as much as she has trouble committing herself for a lifetime with one certain person, is humiliated and outraged. Writing a letter to the editor of the USA Today spotting fifteen--count 'em, 15!--factual errors, Ike is promptly fired for turning the paper into basically a tabloid. Fortunately, his best friend, Fisher (Hector Elizondo), comes up with a sure-fire way to save Ike's job: you see, Maggie is planning to get married in a week or two (her fourth attempt) with Bob (Christopher Meloni), a football coach and fitness nut, and if she once again backs out at the last minute, Ike's theory that he wrote in the paper will be confirmed.
When Ike arrives in Hale ("I think I'm in Mayberry!"), a quaint, old-fashioned kind of town, he gets a room at the motel in the town square and starts to pursue and question Maggie, a misunderstood woman who works at the local hardware store and is the butt of many "harmless" jokes with the townspeople (all of which know each other by name). At first despising the head-strong, determined Ike, she finally agrees for him to follow her around to see what makes her tick--for a sizable fee, of course, which must be a rip-off/ode to "Pretty Woman," where Gere payed Roberts (playing a prostitute) to spend six days with him while in L.A. Since Ike and Maggie are spending all of their time together, they start to get to know one another to the point that marriage with Ike sounds more appealing than marriage with Bob. But even if they go through with it, who is to say Maggie won't run again?
"Runaway Bride" lacks the smarts, wit, and spontaneity that the best romantic comedies have (just recently, the other Julia Roberts-starrer of the summer, "Notting Hill," had this). Simply put, this new film is stuck on auto-pilot, and therefore, comes off as a tiresome excursion into terrain that has been covered too many times to count. For one, you know going in that director Garry Marshall wouldn't dare make a movie with these two actors and not have them get together by the final act, so there is nary an ounce of suspense or interest generated from this major aspect of the story. To shake things up a little, Marshall and screenwriters Josann McGibbon and Sara Parriott should have went a similar route as Roberts' sweet 1997 career-revitalizing hit, "My Best Friend's Wedding," which had an upbeat resolution that was nonetheless more truthful and complicated than by just having the two romantic leads get together. Perhaps Marshall feared that audiences would get upset if Roberts and Gere didn't live happily ever after at the end, but it, no doubt, would have at least added a sprinkle of originality that is hopelessly absent from almost every scene in the overlong 116-minute running time. And that's another thing; the film may actually have worked on a minor level had it concluded with its natural ending, but instead, it proceeds to go on for another unnecessary fifteen minutes.
Once again, Julia Roberts and Richard Gere shine in their latest foray, but the romantic heat between the two that was so tangible in "Pretty Woman" isn't present nearly as much here, most likely because the writing, as mentioned, isn't as satisfying. Their roles of Ike and Maggie also happen to be the least interesting characters in the whole film, which is a glaring flaw that looms overhead most of the picture. No fault of Roberts and Gere, especially, who seems far more loose and care-free than I think I've ever seen him on film, but every time one of the supporting players would appear on-screen, things would brighten up considerably.
Joan Cusack, as always, is a comic delight and standout as Maggie's best friend and hairstylist at the "Curl Up and Dye" Salon (which, yes, garnered a big laugh). Cusack is not really wasted, particularly since she and Roberts have a subtle, honest scene together, but it is rather frustrating to constantly see Cusack, one of America's biggest current acting talents, cast in the "friend" role. Studio heads, take note: Give Cusack the lead in a movie, for once. Believe me, she has proven her worth and is fully capable of holding up a picture on her own. Why don't other people see this?
One compliment that probably should be given to the screenwriters is in the three-dimensional treatment given to the ex-wife character of Gere's, played by Rita Wilson in a memorable, superior performance to anything I've seen her in. Too often overacting or missing the mark (see her disappointing work in 1998's remake of "Psycho"), Wilson is perfect here as a woman who still cares for Gere, despite their divorce and avoidance to what went wrong with their marriage, and is able to have a warm, loving relationship with him. Of the other supporting actors, Hector Elizondo is not used nearly as well or effectively as he was in "Pretty Woman" and is given very little to do, while Laurie Metcalf is hilarious in her too-brief performance as the town baker, as is Jean Schertler as Roberts' lovable, if brazen, granny.
When you go to see a movie that features megastars Julia Roberts and Richard Gere and, yet, you mostly want them to disappear into the background so you can watch the people around them strut their stuff, what exactly does that tell you? In my opinion, it tells you that the screenplay needed an extensive rewrite to strengthen the two lead characters, who aren't nearly as flashy and absorbing as Cusack, Wilson, Metcalf, and Schertler. When Roberts and Gere finally do come together in the last scene, you are happy for them, but left with an uncertain feeling inside. If Roberts' Maggie really does have a lot of personal problems to work out, then how can you be so sure that she and Ike won't be making a trip to divorce court a week later? Or, better yet, and it is this plot contrivance that is the most difficult to swallow, why would Maggie be smitten with Ike in the second half when she thoroughly can't stand him in the former section because of the cruel things he wrote about her, in a country-wide newspaper, no less? Regretfully, "Runaway Bride" too often appears to be so concerned with big box-office receipts that everyone involved forgot about making the film actually good. Sorry, Julia, but don't worry, I still love ya! On second thought, who couldn't?
- Copyright 1999 by Dustin Putman. Http://hometown.aol.com/FilmFan16/index.html
The review above was posted to the
rec.arts.movies.reviews newsgroup (de.rec.film.kritiken for German reviews).
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belongs to the author.
Please direct comments/criticisms of the review to relevant newsgroups.
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Related links: index of all rec.arts.movies.reviews reviews


9-month-old boy found unresponsive at Roxbury day care
by EndPlayBOSTON - A child was found unresponsive after a medical incident Friday morning at an early childhood center in Roxbury, according to Children's Service of Roxbury.
The 9-month-old boy was found unresponsive shortly before 9:30 a.m. in a van at the CSR's early Childhood and Education Center.
Officials say the driver ran in to get a worker to take the child inside as 911 was called and employees began CPR.
Boston police say the incident is not considered suspicious.
The arriving paramedics took the child to Boston Medical Center. The child's condition was described as critical, but stable.
"At this time, our thoughts and primary concern is with the well-being of the child," spokesperson Sandra McCroom said in a letter. "The incident is currently under investigation, and we are gathering all the facts as quickly as we can."
CSR officials say the transportation van is not operated by the organization.
Parents were told they were allowed to pick up their children early if they wanted to.


--- title: (BFModel) getRecords keywords: documentation theme, jekyll, technical writers, help authoring tools, hat replacements last_updated: July 3, 2016 tags: [getting_started] sidebar: matlab_docs_sidebar permalink: bfmodel_getrecords.html folder: mydoc ---
getRecords Returns records of the given model RECORDS = getRecords(OBJ) returns the first 100 records for the given model. RECORDS = GETALL(OBJ, MAXCOUNT, OFFSET) returns a total of MAXCOUNT records starting at an OFFSET from the first record. You can use this to iteratively request many records. Example: M1 = BF.models(1); RECORDS = M1.GETALL()
| Access | public |
| Sealed | false |
| Static | false |


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Why do people have different blood types?
The types of proteins, glycoproteins and glycolipids found (or expressed) on the surface of red blood cells define blood types. In addition, blood types, or at least the genes responsible for them, are inherited. Karl Landsteiner described the original blood types--A, B and O--in 1900 and doctors now recognize 23 blood group systems with hundreds of different "types."


About Page This website is part of the course websoft course page on HKR website course repo on GitHub my forked course repo on GitHub


This page allows you to view all live or historical telemetry parameters in tabular format.
The view's default state is to plot 100 live telemetry parameters.
- Historical values can be displayed by using the time filter controls and clicking the filter button.
- Search the data shown in the table using the Search input field located at the top-right of the table.


Processing Video Files¶
Prepare video processing directory¶
Place trackHead.py
into a folder that contains the timestamps.csv and .mpg files that you want processed
Execute tracking script from the command line¶
Open a terminal window
Switch into your trackingEnv if you are not already in it
cd into your video processing directory
Run the trackHead.py script by entering the following:
python trackHead.py
Resulting Output¶
Annotated footage¶
All of the separate .mpg files will be combined into a single .mp4 that contains 3 frames stiched together.
The left frame is the original video footage. The center frame shows the pixels that remain after filtering for red and blue. The right frame places circlular marks at the centers of the filtered pixel clusters.
Tracked coordinates data¶
A .csv file that combines the timestamp.csv data with x,y coorindinates of the tracked LEDs.


Coverage Summary for Class: PendingReadLacOp (org.apache.bookkeeper.client)
| Class | Method, % | Line, % |
|---|---|---|
| PendingReadLacOp | 0% (0/ 4) | 0% (0/ 56) |
| PendingReadLacOp$LacCallback | ||
| total | 0% (0/ 4) | 0% (0/ 56) |
1 /**
2 * Licensed to the Apache Software Foundation (ASF) under one
3 * or more contributor license agreements. See the NOTICE file
4 * distributed with this work for additional information
5 * regarding copyright ownership. The ASF licenses this file
6 * to you under the Apache License, Version 2.0 (the
7 * "License"); you may not use this file except in compliance
8 * with the License. You may obtain a copy of the License at
9 *
10 * http://www.apache.org/licenses/LICENSE-2.0
11 *
12 * Unless required by applicable law or agreed to in writing, software
13 * distributed under the License is distributed on an "AS IS" BASIS,
14 * WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
15 * See the License for the specific language governing permissions and
16 * limitations under the License.
17 */
18 package org.apache.bookkeeper.client;
19
20 import io.netty.buffer.ByteBuf;
21
22 import java.util.List;
23
24 import org.apache.bookkeeper.client.BKException.BKDigestMatchException;
25 import org.apache.bookkeeper.net.BookieSocketAddress;
26 import org.apache.bookkeeper.proto.BookieClient;
27 import org.apache.bookkeeper.proto.BookkeeperInternalCallbacks.ReadLacCallback;
28 import org.apache.bookkeeper.proto.checksum.DigestManager.RecoveryData;
29 import org.slf4j.Logger;
30 import org.slf4j.LoggerFactory;
31
32 /**
33 * This represents a pending ReadLac operation.
34 *
35 *
LAC is stored in two places on bookies.
36 * 1. WriteLac operation sends Explicit LAC and is stored in memory on each bookie.
37 * 2. Each AddEntry operation piggy-backs LAC which is stored on bookie's disk.
38 *
39 *
This operation returns both of those entries and we pick the latest LAC out of
40 * available answers.
41 *
42 *
This is an optional protocol operations to facilitate tailing readers
43 * to be up to date with the writer. This is best effort to get latest LAC
44 * from bookies, and doesn't affect the correctness of the protocol.
45 */
46
47 class PendingReadLacOp implements ReadLacCallback {
48 static final Logger LOG = LoggerFactory.getLogger(PendingReadLacOp.class);
49 LedgerHandle lh;
50 BookieClient bookieClient;
51 LacCallback cb;
52 int numResponsesPending;
53 volatile boolean completed = false;
54 int lastSeenError = BKException.Code.ReadException;
55 final DistributionSchedule.QuorumCoverageSet coverageSet;
56 long maxLac = LedgerHandle.INVALID_ENTRY_ID;
57 final List<BookieSocketAddress> currentEnsemble;
58
59 /*
60 * Wrapper to get Lac from the request
61 */
62 interface LacCallback {
63 void getLacComplete(int rc, long lac);
64 }
65
66 PendingReadLacOp(LedgerHandle lh, BookieClient bookieClient, List<BookieSocketAddress> ensemble, LacCallback cb) {
67 this.lh = lh;
68 this.bookieClient = bookieClient;
69 this.cb = cb;
70 this.numResponsesPending = ensemble.size();
71 this.coverageSet = lh.distributionSchedule.getCoverageSet();
72 this.currentEnsemble = ensemble;
73 }
74
75 public void initiate() {
76 for (int i = 0; i < currentEnsemble.size(); i++) {
77 bookieClient.readLac(currentEnsemble.get(i), lh.ledgerId, this, i);
78 }
79 }
80
81 @Override
82 public void readLacComplete(int rc, long ledgerId, final ByteBuf lacBuffer, final ByteBuf lastEntryBuffer,
83 Object ctx) {
84 int bookieIndex = (Integer) ctx;
85
86 // add the response to coverage set
87 coverageSet.addBookie(bookieIndex, rc);
88
89 numResponsesPending--;
90 boolean heardValidResponse = false;
91
92 if (completed) {
93 return;
94 }
95
96 if (rc == BKException.Code.OK) {
97 try {
98 // Each bookie may have two store LAC in two places.
99 // One is in-memory copy in FileInfo and other is
100 // piggy-backed LAC on the last entry.
101 // This routine picks both of them and compares to return
102 // the latest Lac.
103
104 // lacBuffer and lastEntryBuffer are optional in the protocol.
105 // So check if they exist before processing them.
106
107 // Extract lac from FileInfo on the ledger.
108 if (lacBuffer != null && lacBuffer.readableBytes() > 0) {
109 long lac = lh.macManager.verifyDigestAndReturnLac(lacBuffer);
110 if (lac > maxLac) {
111 maxLac = lac;
112 }
113 }
114 // Extract lac from last entry on the disk
115 if (lastEntryBuffer != null && lastEntryBuffer.readableBytes() > 0) {
116 RecoveryData recoveryData = lh.macManager.verifyDigestAndReturnLastConfirmed(lastEntryBuffer);
117 long recoveredLac = recoveryData.getLastAddConfirmed();
118 if (recoveredLac > maxLac) {
119 maxLac = recoveredLac;
120 }
121 }
122 heardValidResponse = true;
123 } catch (BKDigestMatchException e) {
124 // Too bad, this bookie did not give us a valid answer, we
125 // still might be able to recover. So, continue
126 LOG.error("Mac mismatch while reading ledger: " + ledgerId + " LAC from bookie: "
127 + currentEnsemble.get(bookieIndex));
128 rc = BKException.Code.DigestMatchException;
129 }
130 }
131
132 if (rc == BKException.Code.NoSuchLedgerExistsException || rc == BKException.Code.NoSuchEntryException) {
133 heardValidResponse = true;
134 }
135
136 if (rc == BKException.Code.UnauthorizedAccessException && !completed) {
137 cb.getLacComplete(rc, maxLac);
138 completed = true;
139 return;
140 }
141
142 if (!heardValidResponse && BKException.Code.OK != rc) {
143 lastSeenError = rc;
144 }
145
146 // We don't consider a success until we have coverage set responses.
147 if (heardValidResponse
148 && coverageSet.checkCovered()
149 && !completed) {
150 completed = true;
151 if (LOG.isDebugEnabled()) {
152 LOG.debug("Read LAC complete with enough validResponse for ledger: {} LAC: {}", ledgerId, maxLac);
153 }
154 cb.getLacComplete(BKException.Code.OK, maxLac);
155 return;
156 }
157
158 if (numResponsesPending == 0 && !completed) {
159 LOG.info("While readLac ledger: " + ledgerId + " did not hear success responses from all of ensemble");
160 cb.getLacComplete(lastSeenError, maxLac);
161 }
162 }
163 }


Week Three Day Two
This is random work from class on Wednesday.
List Tests
One
Two
Sub Item
Three
Anchors
Google
Home
Images


Now I'm up and running I have a list of applications around the house to start working through. One of the first is to monitor water cylinder temperature.
I can see the external temp sensor in the shop, but wondered what people have used to attach it to the cylinder or pipe work at the cylinder exit?
Any tips?
Re: Attaching thermal sensors to hot water cylinder?
I believe most people use a strap to hold the sensor in place, with some heat sink compound to assure a good thermal contact. I have also seen reports of purpose-designed pockets being used, though these are let into the tank top or sides rather than fixed on the pipework.
Re: Attaching thermal sensors to hot water cylinder?
Yes, I was thinking some kind of thermal paste/ grease and ty-wraps. (with a cover over it!)
Re: Attaching thermal sensors to hot water cylinder?
Hello!
I only used a piece of tape to kepp the sensors in place until the insulation material is in place around the cylinder and the sensors. The insulation will hold it in place forever. The sensors can measure a rise/fall of several degrees per second, but I've never seen such fast changes in my 800l cylinder.
The fastest changes that I measure are the temperatures of the solar system when the sun gets really hot and the pump starts working to heat up the boiler. Then I get 25°C to 60°C in about 90 seconds.
The fastest change in the boiler appears when somebody needs a bath, that can lead to a temperature drop of about 10°C in 10minutes.
So you see: all thermal systems with lots of water are very slow changing systems.
best regards
Juergen
Re: Attaching thermal sensors to hot water cylinder?
my cylinder have a pocket at the top... sadly not at the bottom
i used 2 dallas chips with the flat surface back to back and then heatshrinked it... i needed 2 anyway, one for the OpenTRV board and one for an emontx
fit very snug :-D


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A simple label or macro expander
Example use cases:
The supported command line options can be listed using the –help options.
shorthand --help
Source code can be found at github.com/rsdoiel/shorthand
The project website is rsdoiel.github.io/shorthand
If the content of the markdown file testdata/report.md was
Report Date: @now
# Topic: The current local time.
This report highlights the current local time of rendering this document
The current local time is @now
From the command line you can do something like this
shorthand -e ':bash: @now date' \
-e ":import: @report testdata/report.md" \
-e "@report" \
-e ':exit:' | pandoc -s > testdata/report.html
What this command does is launch the shorthand interpreter and it replaces all occurrences of “@now” in the markdown document with the output from the Unix program date.
The output (before piping to Pandoc) would look something like
Report Date: Sat Aug 29 11:25:48 PDT 2015
# Topic: The current local time.
This report highlights the current local time of rendering this document
The current local time is Sat Aug 29 11:25:48 PDT 2015
Notice that both “@now” are replace with the same date information.
You could also embed the shorthand definitions command straight in the markdown itself. with something like
@now :bash: date
Report Date: @now
# Topic: The current local time.
This report highlights the current local time of rendering this document
The current local time is @now
That makes the command line a little shorter
shorthand testdata/report.md | pandoc -s > testdata/report.html
shorthand can be installed with the go get command.
go get github.com/rsdoiel/shorthand/...


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Pneumonia 'killed one child under five every 39 seconds last year'
by EuronewsPneumonia claimed the life of a child under five every 39 seconds last year, according to a new report.
Save the Children said the disease killed more than 800,000 children in this age group in 2018 and that it was a "forgotten global epidemic".
Most deaths occurred under the age of two, and almost 153,000 within the first month of life, said UNICEF.
Pneumonia is caused by bacteria, virus or fungi. The first symptoms are a heavy cough, diarrhoea, vomiting and serious breathing problems, as the lungs are filled with pus and fluid.
More children under the age of five died from the disease in 2018 than from any other: 437,000 children under five died due to diarrhoea and 272,000 to malaria.
However, this infection is preventable and can be cured.
“Every day, nearly 2,200 children under the age of five die from pneumonia, a curable and mostly preventable disease. Only through cost-effective protective, preventative and treatment interventions delivered to where children are will we be able to truly save millions of lives," said Henrietta Fore, executive director of UNICEF.
The disease can be prevented with vaccines, and easily treated with low-cost antibiotics if it is properly diagnosed. Children with severe cases of pneumonia may also require oxygen treatment, which is rarely available in the poorest countries to the children who need it.
The most vulnerable are those who live in poor conditions, in areas with high levels of air pollution or that suffer from malnutrition or HIV.
“This is a forgotten global epidemic that demands an urgent international response. Millions of children are dying for want of vaccines, affordable antibiotics, and routine oxygen treatment. The pneumonia crisis is a symptom of neglect and indefensible inequalities in access to health care", UK Chief Executive of Save the Children Kevin Watkins said.
In January, world leaders will meet in Spain at the Global Forum on Childhood Pneumonia to take global action.
Video editor • Sofia Sanchez Manzanaro


| Jump to DART Documentation Main Index |
The relationship between ROMS and DART is slightly different than most other models. ROMS has the ability to apply its own forward operator as the model is advancing (a capability needed for variational assimilation) which produces something the ROMS community calls 'verification' observations. The observation file that is input to ROMS is specified by the s4dvar.in:OBSname variable. The verification obs are written out to a netcdf file whose name is specified by the s4dvar.in:MODname variable. Since each ROMS model is advancing independently, a set of verification observation files are created during a DART/ROMS assimilation cycle. This set of files can be converted using convert_roms_obs to produce a DART observation sequence file that has precomputed forward operators (FOs). convert_roms_obs can also convert s4dvar.in:OBSname,MODname files to a DART observation sequence file that does not have the precomputed FOs.
The ROMS verification observation files must contain the obs_provenance as a global attribute and the following variables:
Note that the obs_provenance:flag_values, and obs_provenance:flag_meanings attributes are totally ignored - those relationships are specified by the global attribute obs_provenance.
Locations only specified by obs_Xgrid, obs_Ygrid, obs_depth are not supported.
The conversion of a (set of) ROMS verification observations requires metadata to
coordinate the relationship of the ROMS observation provenance to a DART observation
TYPE. ROMS provides significant flexibility when specifying the observation
provenance and it is simply impractical for DART to try to support all of them.
An example of the current practice is described in the
PROGRAMS section below.
Important: filter and
perfect_model_obs must also be informed which DART
observation types use precomputed forward operators. This is done by
setting the input.nml&obs_kind_nml
namelist. An example is shown at the end of the
PROGRAMS section below.
This namelist is read from the file input.nml. Namelists start with an ampersand '&' and terminate with a slash '/'. Character strings that contain a '/' must be enclosed in quotes to prevent them from prematurely terminating the namelist.
&convert_roms_obs_nml ens_size = 1 roms_mod_obs_files = '' roms_mod_obs_filelist = 'filelist.txt' dart_output_obs_file = 'obs_seq.out' append_to_existing = .false. use_precomputed_values = .true. add_random_noise = .false. pert_amplitude = 0.01 verbose = 0 type_translations = 'NULL' /
| Item | Type | Description |
|---|---|---|
| ens_size | integer | Number of ensemble members which are expected to be found when creating the expected obs values. This must match the number of ROMS "mod" files listed in either the 'roms_mod_obs_files' or 'roms_mod_obs_filelist' namelist items. It is an error if they are not the same length. |
| roms_mods_obs_files | character(len=256), dimension(100) | List of filenames, one per ensemble member, that contain the observation values for each ensemble member. These are output from the ROMS program. If listing the files explicitly in this list, 'roms_mod_obs_filelist' must be ' ' (null). |
| roms_mods_obs_filelist | character(len=256) | The name of an ASCII file which contains, one per line, a list of filenames, one per ensemble member, that contain the expected obs values for each ensemble member. The filenames should NOT be quoted. These are output from the ROMS program. If using a filelist, then 'roms_mod_obs_files' must be ' ' (null). |
| dart_output_obs_file | character(len=256) | The name of the DART obs_seq file to create. If a file already exists with this name, it is either appended to or overwritten depending on the 'append_to_existing' setting below. |
| append_to_existing | logical | If an existing 'dart_output_obs_file' is found, this namelist item controls how it is handled. If .true. the new observations are appended to the existing file. If .false. the new observations overwrite the existing file. |
| use_precomputed_values | logical | flag to indicate that the output DART observation sequence file should include the verification observation values from all of the ROMS observation files. If .true. this will result in the DART file having the precomputed FOs to be used in the DART assimilation. If .false. this will result in DART files having the instrument values only. |
| add_random_noise | logical | Almost always should be .false. . The exception is the first cycle of an assimilation if all the ROMS input files are identical (no ensemble currently exists). To create differences in the forward operator values (since they are computed by ROMS), we can add gaussian noise here to give them perturbed values. This should be set as well as the "perturb_from_single_instance = .true." namelist in the &filter_nml namelist. After the first cycle, both these should be set back to .false. . |
| pert_amplitude | real(r8) | Ignored unless 'add_random_noise' is .true. . Controls the range of random values added to the expected obs values. Sets the width of a gaussian. |
| verbose | integer | If greater than 0, prints more information during the conversion. |
| type_translations | character(256), dimension(2, 100) | A set of strings which control the mapping of ROMS observation types to DART observation types. These should be specified in pairs. The first column should be a string that occurs in the global attribute 'obs_provenance'. Note that the obs_provenance:flag_values and obs_provenance:flag_meanings attributes are ignored. The second column should be a DART specific obs type that is found in DART/assimilation_code/modules/observations/obs_kind_mod.f90, which is created by the DART preprocess program. |
The origin of the input observation files used by ROMS are completely unknown to me.
Only convert_roms_obs will be discussed here.
The global attribute obs_provenance is used to relate the observation provenance to DART observation TYPES. The ROMS 'MODname' netCDF file(s) must have both the obs_provenance variable and a obs_provenance global attribute. The exact strings must be repeated in the DART convert_roms_obs_nml:type_translations variable to be able to convert from the integer value of the obs_provenance to th DART type in the following example:
ncdump -h roms_mod_obs.nc (the output has been pruned for clarity)netcdf roms_mod_obs { dimensions: record = 2 ; survey = 5376 ; state_var = 8 ; datum = 2407217 ; variables: {snip} int obs_provenance(datum) ;obs_provenance:long_name = "observation origin" ; obs_provenance:flag_values = 1, 2, 3, 4, 5, 6, 7, 8, 9, 10 ;double obs_time(datum) ; obs_time:long_name = "time of observation" ; obs_time:units = "days since 1900-01-01 00:00:00 GMT" ; obs_time:calendar = "gregorian" ; double obs_lon(datum) ; obs_lon:long_name = "observation longitude" ; obs_lon:units = "degrees_east" ; double obs_lat(datum) ; obs_lat:long_name = "observation latitude" ; obs_lat:units = "degrees_north" ; double obs_depth(datum) ; obs_depth:long_name = "ROMS internal depth of observation variable" ; obs_depth:units = "meters or fractional z-levels" ; obs_depth:negative_value = "downwards" ; obs_depth:missing_value = 1.e+37 ; double obs_error(datum) ; obs_error:long_name = "observation error covariance" ; double obs_value(datum) ; obs_value:long_name = "observation value" ; double obs_scale(datum) ; obs_scale:long_name = "observation screening/normalization scale" ; obs_scale:_FillValue = 0. ; double NLmodel_value(datum) ; NLmodel_value:long_name = "nonlinear model at observation locations" ; NLmodel_value:_FillValue = 1.e+37 ; {snip} :obs_provenance = "\n", "1: gridded AVISO sea level anomaly (zeta)\n", "2: gridded Aquarius SSS (salinity)\n", "3: XBT from Met Office (temperature)\n", "4: CTD from Met Office (temperature)\n", "5: CTD from Met Office (salinity)\n", "6: ARGO floats (temperature)\n", "7: ARGO floats (salinity)\n", "8: glider UCSD (temperature)\n", "9: glider UCSD (salinity)\n", "10: blended satellite SST (temperature)" ; {snip}
Note the integer values that start the obs_provenance strings are used to
interpret the integer contents of the obs_provenance variable. They need not
be consecutive, nor in any particular order, but they must not appear more
than once.
The following is the relevent section of the DART input.nml:
&convert_roms_obs_nml ens_size = 32 roms_mod_obs_filelist = 'precomputed_files.txt' dart_output_obs_file = 'obs_seq.out' append_to_existing = .false. use_precomputed_values = .true. add_random_noise = .false. verbose = 1 type_translations = "gridded AVISO sea level anomaly (zeta)", "SATELLITE_SSH", "gridded Aquarius SSS (salinity)", "SATELLITE_SSS", "XBT from Met Office (temperature)", "XBT_TEMPERATURE", "CTD from Met Office (temperature)", "CTD_TEMPERATURE", "CTD from Met Office (salinity)", "CTD_SALINITY", "ARGO floats (temperature)", "ARGO_TEMPERATURE", "ARGO floats (salinity)", "ARGO_SALINITY", "glider UCSD (temperature)", "GLIDER_TEMPERATURE", "glider UCSD (salinity)", "GLIDER_SALINITY", "blended satellite SST (temperature)", "SATELLITE_BLENDED_SST" /
A complete list of DART observation TYPES is available in obs_def_ocean_mod.f90
Any or all of the DART observation types that appear in the second column of type_translations must also be designated as observations that have precomputed forward operators. This is done by setting the input.nml&obs_kind_nml namelist as follows:
&obs_kind_nml assimilate_these_obs_types = 'SATELLITE_SSH', 'SATELLITE_SSS', 'XBT_TEMPERATURE', 'CTD_TEMPERATURE', 'CTD_SALINITY', 'ARGO_TEMPERATURE', 'ARGO_SALINITY', 'GLIDER_TEMPERATURE', 'GLIDER_SALINITY', 'SATELLITE_BLENDED_SST' use_precomputed_FOs_these_obs_types = 'SATELLITE_SSH', 'SATELLITE_SSS', 'XBT_TEMPERATURE', 'CTD_TEMPERATURE', 'CTD_SALINITY', 'ARGO_TEMPERATURE', 'ARGO_SALINITY', 'GLIDER_TEMPERATURE', 'GLIDER_SALINITY', 'SATELLITE_BLENDED_SST' /
none
DART software - Copyright UCAR. This open source software is provided by UCAR, "as is", without charge, subject to all terms of use at http://www.image.ucar.edu/DAReS/DART/DART_download


✅
My To-Do List Tracker
H
Humber Web Development
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HTTP5101
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8.2
psb_error — Prints the error stack content and aborts execution
call
psb_error
(
icontxt
)
Type:
Asynchronous.
On Entry
icontxt
the communication context.
Scope:
global
Type:
optional
Intent:
in
.
Specified as: an integer.
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| nc_create_par {pbdNCDF4} | R Documentation |
Creates a new parallel NetCDF file on a parallel file system, given the variables the new file is to contain.
nc_create_par(filename, vars, force_v4 = TRUE, verbose = FALSE, comm = 0L, info = 0L)
filename |
Name of the NetCDF file to be created. |
vars |
Either an object of class |
force_v4 |
If |
verbose |
If |
comm |
a communicator number from pbdMPI. |
info |
a info number from pbdMPI. |
See nc_create
for details.
The parallel version is able to coordinate with other
nc_create_par
instances
for more efficient operation in parallel.
An object of class ncdf4
, which has the fields described
in nc_open
.
George Ostrouchov, Pragneshkumar Patel<EMAIL_ADDRESS>Wei-Chen Chen, and Drew Schmidt.
Programming with Big Data in R Website: http://r-pbd.org/
nc_open_par
, nc_var_par_access
,
ncdim_def
, ncvar_def
.
## Not run: ### Under command mode, run the demo with 2 processors by ### (Use Rscript.exe for windows system) mpiexec -np 2 Rscript -e "demo(ncwrite,'pbdNCDF4',ask=F,echo=F)" mpiexec -np 2 Rscript -e "demo(ncread,'pbdNCDF4',ask=F,echo=F)" ## End(Not run)


AlmondJS is a small part of RequireJS, which has no provision to download dependencies on demand. Hence it only supports bundled modules.
Also no configuration required.
As of now, most amd-module bundlers (Rollup, js-bundler, amd-bundler, Parcel.js) suck. (No no. I am not wrong. Hence, there must be some issue with plugin, Node.js, Browser, Computer, Electricity, Gravity, Space or Time)
Hence manually bundled them in one file.
You can write your own bundler as well. All you have to do for bundling is,
There is an added advantage of bundling. Double-click and run the file. No need of server as no lazy loading.
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Sdec
Provides a simple interface to SPHDEC (XDM 0.9) based algorithms. Currently only works for TI:s G711 decoder due to assumptions made. Typical usage (G.711, no error checking):
More...
Detailed Description
Provides a simple interface to SPHDEC (XDM 0.9) based algorithms. Currently only works for TI:s G711 decoder due to assumptions made. Typical usage (G.711, no error checking):
#include <xdc/std.h>
#include <ti/sdo/ce/Engine.h>
#include <ti/sdo/ce/CERuntime.h>
#include <ti/sdo/dmai/Dmai.h>
#include <ti/sdo/dmai/Buffer.h>
#include <ti/sdo/dmai/Loader.h>
#include <ti/sdo/dmai/ce/Sdec.h>
Sdec_Handle hSd;
Loader_Handle hLoader;
Buffer_Handle hOutBuf;
Engine_Handle hEngine;
SPHDEC_Params params = Sdec_Params_DEFAULT;
SPHDEC_DynamicParams dynParams = Sdec_DynamicParams_DEFAULT;
Loader_Attrs lAttrs = Loader_Attrs_DEFAULT;
Buffer_Attrs bAttrs = Buffer_Attrs_DEFAULT;
CERuntime_init();
Dmai_init();
hEngine = Engine_open("myengine", NULL, NULL);
hSd = Sdec_create(hEngine, "g711dec", ¶ms, &dynParams);
hOutBuf = Buffer_create(Sdec_getOutBufSize(hSd), &bAttrs);
lAttrs.readSize = Sdec_getInBufSize(hSd);
lAttrs.readBufSize = lAttrs.readSize * 2;
hLoader = Loader_create("myfile.g711", &lAttrs);
Loader_prime(hLoader, &hInBuf);
while (1) {
Sdec_process(hSd, hInBuf, hOutBuf);
Loader_getFrame(hLoader, hInBuf);
if (Buffer_getUserPtr(hInBuf) == NULL) break;
}
Loader_delete(hLoader);
Buffer_delete(hOutBuf);
Sdec_delete(hSd);
Engine_close(hEngine);
Typedef Documentation
Handle through which to reference a Speech Decode algorithm.
Function Documentation
| Sdec_Handle Sdec_create |
( |
Engine_Handle |
hEngine, |
|
|
Char * |
codecName, |
|
|
SPHDEC_Params * |
params, |
|
|
SPHDEC_DynamicParams * |
dynParams | |
|
) |
| | |
Creates a Speech Decode (XDM 0.9) algorithm instance.
- Parameters:
-
| [in] | hEngine | An opened engine containing the algorithm to create. |
| [in] | codecName | The name of the algorithm to open. Corresponds to the string name given in the .cfg file. |
| [in] | params | XDM parameters to use while creating the codec. |
| [in] | dynParams | XDM dynamic parameters to use while creating the codec. |
- Return values:
-
| Handle | for use in subsequent operations (see Sdec_Handle). |
| NULL | for failure. |
Decodes a Speech buffer.
- Parameters:
-
| [in] | hSd | The Sdec_Handle to use for decoding. |
| [in] | hInBuf | The Buffer_Handle for the buffer containing the encoded data. |
| [in] | hOutBuf | The Buffer_Handle for the buffer to fill with decoded data. |
- Return values:
-
| Dmai_EOK | for success. |
| Negative value | for failure, see Dmai.h. |
Deletes a Speech Decode algorithm instance.
- Parameters:
-
- Return values:
-
| Dmai_EOK | for success. |
| Negative value | for failure, see Dmai.h. |
Get the SPHDEC handle from the Sdec module instance.
- Parameters:
-
| [in] | hSd | The Sdec_Handle for which to get the SPHDEC handle. |
- Return values:
-
| Handle | to the speech decode algorithm, see the XDM documentation for SPHDEC. |
Get the input buffer size required by the codec.
- Parameters:
-
| [in] | hSd | The Sdec_Handle for which to get the buffer size. |
- Return values:
-
| Size | in bytes of the input buffer required. |
Get the output buffer size required by the codec.
- Parameters:
-
| [in] | hSd | The Sdec_Handle for which to get the buffer size. |
- Return values:
-
| Size | in bytes of the output buffer required. |
Variable Documentation
Default XDM parameters for a Speech Decode algorithm.
size = sizeof(SPHDEC_Params),
dataEnable = 0,
compandingLaw = ISPEECH_ALAW,
packingType = 0
Default XDM dynamic parameters for a Speech Decode algorithm.
size = sizeof(SPHDEC_DynamicParams),
postFilter = 0


Fix that Web Site!
I can’t recall how many times I’ve entered a domain name in a browser, say ‘domain.com’, only to wait 30 seconds and get an ugly 502 Bad gateway error in return. The problem? Enter http://domain.com instead of http://www.domain.com and see what happens.
- you are served the expected website, the url stays the same
- you are redirected to http://www.domain.com or some other url
- you get a 502, Bad gateway timeout
I don’t know if it’s laziness, lack of knowledge or simply host providers being plain rubbish, but it’s an annoying problem that can be solved extremely simply!
Most of websites that are not configured properly often get away with it as many internet users believe that ‘www’ is a compulsory part of any web URL.
In fact it’s only because of an old practice of naming hosts according to the services they provide, in our case a web site, with www. FTP using ftp.domain.come etc. But it has nothing to do with any technical issue or any standard. Not many (if any) ‘Mr average’ know this!
One of the problems is that with the advent of new web browsers that suggest you URLs from your history, or even perform straight away an interactive search of web resources that match your typing, it is very easy to fall into the usual consumer laziness and let the browser find everything for you. That way, you get into the habit of accessing a website just by typing the domain name, without www or any other prefix, and sometimes even without the top level domain (The ‘.com’ or other ‘.something’).
I’m the first to do it and that’s why I probably end up on these poorly configured web servers from time to time. But I am still quite astonished to it see happen, as it can seriously lead to some misunderstanding from the average user. If I don’t know anything of internet, don’t care about ‘www’s, just type a domain name in my browser and get an error page, I’m not going to try very long to search for how to access that site!
That problem has a simple solution though.
First, if you have access to them, check your DNS records. This step might not be compulsory, but it won’t harm to check them anyways. Your domain will have an A record to point your domain name to the IP of the host of your web site:
domain.com A <IP_ADDRESS>
You can also add either an A or a CNAME record for the www sub-domain. The syntax differs:
domain.com A <IP_ADDRESS> www.domain.com A <IP_ADDRESS> www.domain.com CNAME domain.com.
Second, check your web server configuration that it actually is accepting requests from sub-domains and serving the proper files. In Apache, for example, you can set it up by adding a virtual host:
Listen 80 NameVirtualHost * <VirtualHost *> ServerName www.domain.com DocumentRoot /home/httpd/htdocs/ </VirtualHost> <VirtualHost *> ServerName domain.com DocumentRoot /home/httpd/htdocs/ </VirtualHost>
or using a server alias:
Listen 80 NameVirtualHost * <VirtualHost *> ServerName domain.com ServerAlias www.domain.com DocumentRoot /home/httpd/htdocs/ </VirtualHost>
So yes, I admit, you have to have access to the DNS entries and the configuration files of the server. But even if you don’t and it’s down to the host provider to configure the DNS and the web server files, it is very easy to set these up properly.
Ok, again, you might argue that you could serve a different version of the site with http://domain.com and http://www.domain.com, but if you don’t and there is no redirection in place, just make sure you don’t serve a 502.


(To be filled by the officer who is in service with government / statutory body / local authority)
I confirm that the information above is correct. I decided
for this applicant.


Module: ActiveSupport::Cache::SerializerWithFallback
Do not use. This module is for internal use only.
| Relationships & Source Files | |
| Namespace Children | |
|
Modules:
| |
| Extension / Inclusion / Inheritance Descendants | |
|
Included In:
| |
| Defined in: | activesupport/lib/active_support/cache/serializer_with_fallback.rb |
Constant Summary
-
SERIALIZERS =
# File 'activesupport/lib/active_support/cache/serializer_with_fallback.rb', line 166{ passthrough: PassthroughWithFallback, marshal_6_1: Marshal61WithFallback, marshal_7_0: Marshal70WithFallback, marshal_7_1: Marshal71WithFallback, message_pack: MessagePackWithFallback, }
Class Method Summary
Instance Method Summary
- #load(dumped)
- #marshal_load(payload) (also: #_load) private
Class Method Details
.[](format)
[ GitHub ]# File 'activesupport/lib/active_support/cache/serializer_with_fallback.rb', line 9
def self.[](format) if format.to_s.include?("message_pack") && !defined?(ActiveSupport::MessagePack) require "active_support/message_pack" end SERIALIZERS.fetch(format) end
Instance Method Details
#load(dumped)
[ GitHub ]# File 'activesupport/lib/active_support/cache/serializer_with_fallback.rb', line 17
def load(dumped) if dumped.is_a?(String) case when MessagePackWithFallback.dumped?(dumped) MessagePackWithFallback._load(dumped) when Marshal71WithFallback.dumped?(dumped) Marshal71WithFallback._load(dumped) when Marshal70WithFallback.dumped?(dumped) Marshal70WithFallback._load(dumped) else Cache::Store.logger&.warn("Unrecognized payload prefix #{dumped.byteslice(0).inspect}; deserializing as nil") nil end elsif PassthroughWithFallback.dumped?(dumped) PassthroughWithFallback._load(dumped) else Cache::Store.logger&.warn("Unrecognized payload class #{dumped.class}; deserializing as nil") nil end end
#marshal_load(payload) (private) Also known as: #_load
[ GitHub ]# File 'activesupport/lib/active_support/cache/serializer_with_fallback.rb', line 39
def marshal_load(payload) Marshal.load(payload) rescue ArgumentError => error raise Cache::DeserializationError, error. end


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abstract class AnimationEngine
Animation Engine abstract
Author
vikramezhil
<init> |
Animation Engine abstract AnimationEngine() |
animationRunning |
abstract var animationRunning: Boolean |
animDurationInMilliSecs |
val animDurationInMilliSecs: Long |
idleFrequency |
val idleFrequency: Float |
minFrequencies |
val minFrequencies: Array<Float> |
outOfBoundsMinFrequency |
val outOfBoundsMinFrequency: Float |
animate |
Starts animating the view abstract fun animate(frequency: Float): Unit |
idle |
Starts idle mode for the view abstract fun idle(): Unit |
start |
Starts the animation abstract fun start(frequency: Float): Unit |
stop |
Stops the animation abstract fun stop(switchToIdle: Boolean): Unit |
BounceAnimationDriver |
Bounce Animation Driver class BounceAnimationDriver : AnimationEngine |


--- layout: post status: publish published: true title: Podcast 4.03 - Spring Training 2012 is underway author: display_name: Corey Fineran login: Corey email<EMAIL_ADDRESS>url: '' author_login: Corey author_email<EMAIL_ADDRESS>wordpress_id: 6847 wordpress_url: http://ivyenvy.com/?p=6847 date: '2012-03-06 22:52:20 +0000' date_gmt: '2012-03-07 04:52:20 +0000' categories: - Podcast - Spring Training tags: - Alfonso Soriano - Spring Training - Mesa - Brett Jackson - Blake Dewitt - Hohokam Stadium - Hohokam - Fitch Park - Anthony Rizzo - Joe Martin comments: [] ---
Andy and Corey discuss the three games of Spring Training that we've heard, but not seen. We consider the reasons that Soriano sees himself someone that leads by example and how the rest of us see him. While there aren't many position battles this year in Mesa, we briefly discuss Blake DeWitt and his attempt to earn a spot on the team.
The Cubs are hitting the ball well and neither of us have much hope that it's a sign the team will be an offensive powerhouse this year. Brett Jackson has been a source of offensive production between the intrasquad games and the first few Spring Training games. We both look forward to the televised Spring Training games, so we can see Brett Jackson and Anthony Rizzo in action.
We do a segment with Joe Martin, who is covering the action in Mesa for us. Joe talks about the promising things he saw at the game on Sunday. He went to Fitch Park today to watch the minor league camp and witnessed a quite interesting training session that at least one player took very seriously.


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We love to work with other great brands to
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Linux, my favorite OS - I admin that windows is just a big mistake. Do not be scared of
the truth because we need to restart the human foundation in truth And I love you like
Kanye loves Kanye I love Rick Owens’ bed design but the back is...


Contract Talks Initiated For In-Demand Striker
by Soccer LadumaPSL clubs that are still interested in signing Joseph Mhlongo might have to look elsewhere, should the negotiations between Black Leopards and the player’s handlers yield positive results.
In fearing of losing the forward on a free to Absa Premiership rivals, Lidoda Duvha have opened up negotiations with the player’s representatives with a view of keeping him at the club beyond his current spell, as reported in edition 1149 of Soccer Laduma.
Read: Chiefs Midfielder Could Be Followed To PSL…
Mhlongo has entered into the last year of his contract with Lidoda Duvha, with his existing deal set to expire in June next year.
In recent weeks, the 29-year-old has been linked with a number of clubs in Mzansi’s topflight, including AmaZulu, Kaizer Chiefs and Orlando Pirates.
However, indications are that Leopards view the player as an integral part of their team and want to keep him.
Mhlongo’s representative, Ratshibvumo Mulovhedzi, confirmed to the Siya crew that negotiations between the player’s camp and Leopards have been initiated.
 We are negotiating about a new contract and we are getting there,” confirmed the representative.
Read: Another SAFA Official Accepts Role Elsewhere
“Yes, we have not yet finalised, but we are getting there. The club gave us their offer and we have made them our counter-offer. They are in the process of making a decision and we are waiting for them,” concluded Mulovhedzi.


--- layout: post title: What about a geoprocessing tip of the week? date: 2011-02-09 20:48:47.000000000 -06:00 type: post published: true status: publish categories: - Geoprocessing with Python tags: [] meta: _edit_last: '15714693' _wpas_done_fb: '1' _wpas_done_twitter: '1' author: login: broberts65 email<EMAIL_ADDRESS>display_name: Bob Roberts first_name: '' last_name: '' ---
Would anybody be interested if I did a Python geoprocessing tip of the week? Maybe every week cover one of the gp commands?


Suggestions of which likelihood and inference method to use is implicitly given by default,
- GPR uses Gaussian likelihood and exact inference.
- GPC uses Erf likelihood and EP inference.
- FITC model uses same default with corresponding FITC inference.
- GPMC calls GPC and thus uses the default setting of GPC
You can change to other likelihood or inference methods using:
model.useLikelihood(newLik)
model.useInference(newInf)
To be consistent with Gaussian Processes community, we use the name “Laplace” for both Laplace likelihood and Laplace inference. Please note the differences.


Money Game. Should Red double? If doubled, should White take?
pips Red=90 White=150
(CorrectAnswer= 0/0, ErrorScore= 0)
This one comes from the Battersea chouette. This is the sort of position where I used to take a roll but in recent months I have been applying Woolsey's Law much more rigorously and with a any sniff of gammon I am likely to double.
Two of us doubled, the other two members waited. We rolled 52, hit the checker on the 2-pt. White fanned (the other two players cashing their sure point) and we coasted to gammon. QED.
What's more XG supports us. Not doubling here is a double blunder and more. Red leads in the race, position and threat and it's extremely volatile. it just cries out for a double.
Of course you will lose some games from here and starting with something like 55 certainly doesn't help but you need to think ”what can go right?” rather than ‘what can go wrong?” Optimists make better backgammon players than pessimists!
Two of us doubled, the other two members waited. We rolled 52, hit the checker on the 2-pt. White fanned (the other two players cashing their sure point) and we coasted to gammon. QED.
What's more XG supports us. Not doubling here is a double blunder and more. Red leads in the race, position and threat and it's extremely volatile. it just cries out for a double.
Of course you will lose some games from here and starting with something like 55 certainly doesn't help but you need to think ”what can go right?” rather than ‘what can go wrong?” Optimists make better backgammon players than pessimists!
Cube analysis 2-ply cubeless equity +0.662 0.821 0.027 0.000 - 0.179 0.008 0.000 Cubeful equities: 1. Double, pass +1.000 2. Double, take +1.202 (+0.202) 3. No double +0.991 (-0.009) Proper cube action: Double, pass


My name is Brock Cowen. I graduated from Cameron University in 2014 and have lived in Austin ever
since. I am 29 years old now and run the QA for an ipad based Point of Sale company in Austin called
UNION. In QA I do both black and white box testing on our multiple products that make up UNION,
including our web browser run portal, iOS based app that runs the POS and all of our different hardware
ranging from printers and cash drawers to Ingenico card swipers. I also test our mobile payments app
that integrates with our point of sale. I have created test plans for all of our products and utilize
tools such as Charles and MITM Proxy, New Relic, Paper Trail, GitHub and Jira to track and diagnose
issues that I am experiencing. I also, often, query the database and read through the couchbase
documents to do my testing.
In my spare time I like to go to movies and play disc golf. I also enjoy traveling and take
any chance I get to go somewhere new.
I am trying to get into the field of full stack web development because I would like to make the
transition into more of the development side of things. With having worked at a startup
for the last 5 years I have quite a bit of experience in the tech industry and a solid understanding of
the development cycle.
I got married this last August to my girlfriend of five years. We live in a house on the
north side of Austin
with our 2 dogs, Moose and Boulder.  We like to take them
camping every chance we get and will often times bring them to Yard Bar where we meet up with our
friends for a drink and let the dogs play there.


Ladle project page | Official Lua website | LuaSocket website | CGILua website
Ladle is a lightweight web server written in the Lua programming language using the TCP functionality offered by LuaSocket. Ladle requires the following modules in Lua's package.path to work properly:
package.path


The Problem: The MPI-1.1 standard says, in the discussion of MPI_INTERCOMM_CREATE, both that
The groups must be disjoint
and that
The leaders may be the same process.
To further muddy the waters, the reason given for ``The groups must be
disjoint'' is based on concerns about the implementation of
MPI_INTERCOMM_CREATE that are not applicable for the case where
the leaders are the same process.
The Fix: Delete the text:
(the two leaders could be the same process)
from the discussion of MPI_INTERCOMM_CREATE.
Replace the text:
All inter-communicator constructors are blocking and require that the local
and remote groups be disjoint.
The groups must be disjoint for several reasons. Primarily, this is the
intent of the intercommunicators --- to provide a communicator for
communication between disjoint groups. This is reflected in the
definition of MPI_INTERCOMM_MERGE, which allows the user to
control the ranking of the processes in the created intracommunicator;
this ranking makes little sense if the groups are not disjoint. In
addition, the natural extension of collective operations to
intercommunicators makes the most sense when
the groups are disjoint.
( End of advice to users.)
All inter-communicator constructors are blocking and require that the local
and remote groups be disjoint in order to avoid deadlock.
with
Advice to users.


EventGadget()
语法
GadgetNumber = EventGadget()概要
After an event of type #PB_Event_Gadget (returned by WindowEvent() or WaitWindowEvent()), use this function to determine which gadget has been triggered.
参数
无.
返回值
Returns the #Gadget number associated to the event.
参阅
WindowEvent(), WaitWindowEvent()
已支持操作系统
所有


CSPICE_ILUMIN computes the illumination angles (phase, solar incidence,
and emission) at a specified surface point of a target body.
This routine supersedes cspice_illum, which lacks an input
argument for the target body-fixed frame name.
Given:
method is a short string providing parameters defining
the computation method to be used. In the syntax
descriptions below, items delimited by brackets
are optional.
[1,c1] = size(method); char = class(method)
or
[1,1] = size(method); cell = class(method)
`method' may be assigned the following values:
'ELLIPSOID'
The illumination angle computation uses a
triaxial ellipsoid to model the surface of the
target body. The ellipsoid's radii must be
available in the kernel pool.
'DSK/UNPRIORITIZED[/SURFACES = <surface list>]'
The illumination angle computation uses
topographic data to model the surface of the
target body. These data must be provided by
loaded DSK files.
The surface list specification is optional. The
syntax of the list is
<surface 1> [, <surface 2>...]
If present, it indicates that data only for the
listed surfaces are to be used; however, data
need not be available for all surfaces in the
list. If absent, loaded DSK data for any surface
associated with the target body are used.
The surface list may contain surface names or
surface ID codes. Names containing blanks must
be delimited by double quotes, for example
'SURFACES = "Mars MEGDR 128 PIXEL/DEG"'
If multiple surfaces are specified, their names
or IDs must be separated by commas.
See the Particulars section below for details
concerning use of DSK data.
Neither case nor white space are significant in
`method', except within double-quoted strings
representing surface names. For example, the string
' eLLipsoid ' is valid.
Within double-quoted strings representing surface names,
blank characters are significant, but multiple
consecutive blanks are considered equivalent to a single
blank. Case is not significant. So
"Mars MEGDR 128 PIXEL/DEG"
is equivalent to
" mars megdr 128 pixel/deg "
but not to
"MARS MEGDR128PIXEL/DEG"
target name of the target body. `target' is case-insensitive, and
leading and trailing blanks in `target' are not significant.
Optionally, you may supply a string containing the integer ID
code for the object. For example both "MOON" and "301" are
legitimate strings that indicate the moon is the target body.
[1,c2] = size(target); char = class(target)
et epoch specified in ephemeris is seconds past J2000, at which
the apparent illumination angles at the specified surface point
on the target body, as seen from the observing body, are to be
computed.
[1,1] = size(et); double = class(et)
fixref name of body-fixed, body-centered reference frame associated
with the target body. The input surface point `spoint' and the
output vector 'srfvec' are expressed relative to this reference
frame.
[1,c3] = size(fixref); char = class(fixref)
'fixref' is case-insensitive, and leading and trailing
blanks are not significant.
abcorr aberration correction to be used in computing the location of
the surface point, the orientation of the target body, and the
location of the Sun.
[1,m] = size(abcorr); char = class(abcorr)
For remote sensing applications, where the apparent
illumination angles seen by the observer are desired,
normally either of the corrections
'LT+S'
'CN+S'
should be used. These and the other supported options
are described below. `abcorr' may be any of the
following:
'NONE' No aberration correction.
'LT' Correct the position of the input
surface point SPOINT and orientation of
target body for light time, and correct
the position of the Sun as seen
from the target for light time.
'LT+S' Correct the position of the surface
point SPOINT for light time and stellar
aberration, correct the orientation of
the target body for light time, and
correct the position of the Sun as seen
from the target for light time and
stellar aberration.
'CN' Converged Newtonian light time
correction. In solving the light time
equation, the 'CN' correction iterates
until the solution converges. Both the
position of the surface point SPOINT c
and rotation of the target body, as
well as the position of the Sun as seen
from the target, are corrected for
light time.
'CN+S' Converged Newtonian light time and
stellar aberration corrections. This
option produces a solution that is at
least as accurate at that obtainable
with the 'LT+S' option. Whether the
'CN+S' solution is substantially more
accurate depends on the geometry of the
participating objects and on the
accuracy of the input data. In all
cases this routine will execute more
slowly when a converged solution is
computed.
Neither case nor white space are significant in
`abcorr'. For example, the string
'Lt + s'
is valid.
obsrvr name of the observing body. This is typically a spacecraft,
the earth, or a surface point on the earth. `obsrvr' is
case-insensitive, and leading and trailing blanks in `obsrvr'
are not significant. Optionally, you may supply a string
containing the integer ID code for the object. For example both
'EARTH' and '399' are legitimate strings that indicate the
earth is the observer.
[1,c4] = size(obsrvr); char = class(obsrvr)
`obsrvr' may be not be identical to `target'.
spoint a surface location on the target body, expressed in Cartesian
coordinates, relative to the body-fixed target frame designated
by `fixref'.
[3,1] = size(spoint); double = class(spoint)
`spoint' need not be visible from the observer's
location at the epoch `et'.
The components of `spoint' have units of km.
the call:
[trgepc, srfvec, phase, solar, emissn] = cspice_ilumin( method, ...
target, et, fixref, ...
abcorr, obsrvr, spoint)
returns:
trgepc "surface point epoch." 'trgepc' is defined as follows: letting
'lt' be the one-way light time between the observer and the
input surface point 'spoint', 'trgepc' is either the epoch
et-lt or 'et' depending on whether the requested aberration
correction is, respectively, for received radiation or omitted.
'lt' is computed using the method indicated by 'abcorr'.
[1,1] = size(trgepc); double = class(trgepc)
'trgepc' is expressed as seconds past J2000 TDB.
srfvec the position vector from the observer at 'et' to 'spoint'.
'srfvec' is expressed in the target body-fixed reference frame
designated by 'fixref', evaluated at 'trgepc'.
[3,1] = size(srfvec); double = class(srfvec)
The components of 'srfvec' are given in units of km.
One can use the function norm to obtain the
distance between the observer and 'spoint':
dist = norm( srfvec )
The observer's position 'obspos', relative to the
target body's center, where the center's position is
corrected for aberration effects as indicated by
'abcorr', can be computed with:
obspos = spoint - srfvec
To transform the vector 'srfvec' from a reference frame
'fixref' at time 'trgepc' to a time-dependent reference
frame 'ref' at time 'et', the routine 'cspice_pxfrm2' should be
called. Let 'xform' be the 3x3 matrix representing the
rotation from the reference frame 'fixref' at time
'trgepc' to the reference frame 'ref' at time 'et'. Then
'srfvec' can be transformed to the result 'refvec' as
follows:
xform = cspice_pxfrm2 ( fixref, ref, trgepc, et )
refvec = xform * srfvec
phase phase angle at 'spoint', as seen from 'obsrvr' at time 'et'.
This is the angle between the spoint-obsrvr vector and the
spoint-sun vector. Units are radians. The range of 'phase' is
[0, pi].
[1,1] = size(phase); double = class(phase)
solar solar incidence angle at 'spoint', as seen from 'obsrvr' at
time 'et'. This is the angle between the surface normal vector
at 'spoint' and the spoint-sun vector. Units are radians. The
range of 'solar' is [0, pi].
[1,1] = size(solar); double = class(solar)
emissn emission angle at 'spoint', as seen from 'obsrvr' at time 'et'.
This is the angle between the surface normal vector at 'spoint'
and the spoint-observer vector. Units are radians. The range of
'emissn' is [0, pi].
[1,1] = size(emissn); double = class(emissn)
Any numerical results shown for this example may differ between
platforms as the results depend on the SPICE kernels used as input
and the machine specific arithmetic implementation.
Find the phase, solar incidence, and emission angles at the
sub-solar and sub-spacecraft points on Mars as seen from the Mars
Global Surveyor spacecraft at a specified UTC time.
Use both an ellipsoidal Mars shape model and topographic data
provided by a DSK file. For both surface points, use the "near
point" and "nadir" definitions for ellipsoidal and DSK shape
models, respectively.
Use converged Newtonian light time and stellar aberration
corrections.
The topographic model is based on data from the MGS MOLA DEM
megr90n000cb, which has a resolution of 4 pixels/degree. A
triangular plate model was produced by computing a 720 x 1440
grid of interpolated heights from this DEM, then tessellating
the height grid. The plate model is stored in a type 2 segment
in the referenced DSK file.
Use the meta-kernel shown below to load the required SPICE
kernels.
KPL/MK
File: illum_t2.tm
This meta-kernel is intended to support operation of SPICE
example programs. The kernels shown here should not be
assumed to contain adequate or correct versions of data
required by SPICE-based user applications.
In order for an application to use this meta-kernel, the
kernels referenced here must be present in the user's
current working directory.
The names and contents of the kernels referenced
by this meta-kernel are as follows:
File name Contents
--------- --------
de430.bsp Planetary ephemeris
mar097.bsp Mars satellite ephemeris
pck00010.tpc Planet orientation and
radii
naif0011.tls Leapseconds
mgs_ext12_ipng_mgs95j.bsp MGS ephemeris
megr90n000cb_plate.bds Plate model based on
MEGDR DEM, resolution
4 pixels/degree.
\begindata
KERNELS_TO_LOAD = ( 'de430.bsp',
'mar097.bsp',
'pck00010.tpc',
'naif0011.tls',
'mgs_ext12_ipng_mgs95j.bsp',
'megr90n000cb_plate.bds' )
\begintext
Example(1):
function illumf_t2()
%
% Load kernel files.
%
cspice_furnsh( 'illum_t2.tm' )
%
% Convert the UTC request time string to seconds past
% J2000 TDB.
%
utc = '2003 OCT 13 06:00:00 UTC';
et = cspice_str2et( utc );
%
% Assign observer and target names. The acronym MGS
% indicates Mars Global Surveyor. See NAIF_IDS for a
% list of names recognized by SPICE.
%
% Also set the target body-fixed frame and
% the aberration correction flag.
%
target = 'Mars';
obsrvr = 'MGS';
fixref = 'IAU_MARS';
abcorr = 'CN+S';
ilumth = {'Ellipsoid', 'DSK/Unprioritized' };
submth = {'Near Point/Ellipsoid', 'DSK/Nadir/Unprioritized' };
for i=1:numel(ilumth)
%
% Find the sub-solar point on the Earth as seen from
% the MGS spacecraft at et. Use the 'near point'
% style of sub-point definition.
%
[ssolpt, trgepc, srfvec] = ...
cspice_subslr( submth(i), ...
target, et, fixref, ...
abcorr, obsrvr );
%
% Now find the sub-spacecraft point.
%
[sscpt, trgepc, srfvec] = ...
cspice_subpnt( submth(i), ...
target, et, fixref, ...
abcorr, obsrvr );
%
% Find the phase, solar incidence, and emission
% angles at the sub-solar point on the Earth as seen
% from MGS at time et.
%
[ trgepc, srfvec, sslphs, sslsol, sslemi ] = ...
cspice_ilumin( ilumth(i), ...
target, et, fixref, ...
abcorr, obsrvr, ssolpt );
%
% Do the same for the sub-spacecraft point.
%
[ trgepc, srfvec, sscphs, sscsol, sscemi ] = ...
cspice_ilumin( ilumth(i), ...
target, et, fixref, ...
abcorr, obsrvr, sscpt );
%
% Convert the angles to degrees and write them out.
%
sslphs = sslphs * cspice_dpr;
sslsol = sslsol * cspice_dpr;
sslemi = sslemi * cspice_dpr;
sscphs = sscphs * cspice_dpr;
sscsol = sscsol * cspice_dpr;
sscemi = sscemi * cspice_dpr;
fprintf( [ '\n' ...
' cspice_ilumin method: %s\n' ...
' cspice_subpnt method: %s\n' ...
' cspice_subslr method: %s\n' ...
'\n' ...
' Illumination angles at the ' ...
'sub-solar point:\n' ...
'\n' ...
' Phase angle (deg): %15.9f\n' ...
' Solar incidence angle (deg): %15.9f\n' ...
' Emission angle (deg): %15.9f\n'],...
char(ilumth(i)), ...
char(submth(i)), ...
char(submth(i)), ...
sslphs, ...
sslsol, ...
sslemi );
if ( i == 0 )
fprintf( [ ' The solar incidence angle ' ...
'should be 0.\n' ...
' The emission and phase ' ...
'angles should be equal.\n' ] );
end
fprintf( [ '\n' ...
' Illumination angles at the ' ...
'sub-s/c point:\n' ...
'\n' ...
' Phase angle (deg): %15.9f\n' ...
' Solar incidence angle (deg): %15.9f\n' ...
' Emission angle (deg): %15.9f\n'],...
sscphs, ...
sscsol, ...
sscemi );
if ( i == 0 )
fprintf( [ ' The emission angle ' ...
'should be 0.\n' ...
' The solar incidence ' ...
'and phase angles should be equal.\n' ] );
end
fprintf ( '\n' );
end
%
% It's always good form to unload kernels after use,
% particularly in Matlab due to data persistence.
%
cspice_kclear
MATLAB outputs:
cspice_ilumin method: Ellipsoid
cspice_subpnt method: Near Point/Ellipsoid
cspice_subslr method: Near Point/Ellipsoid
Illumination angles at the sub-solar point:
Phase angle (deg):<PHONE_NUMBER>85
Solar incidence angle (deg): 0.000000000
Emission angle (deg):<PHONE_NUMBER>85
Illumination angles at the sub-s/c point:
Phase angle (deg):<PHONE_NUMBER>40
Solar incidence angle (deg):<PHONE_NUMBER>41
Emission angle (deg): 0.000000002
cspice_ilumin method: DSK/Unprioritized
cspice_subpnt method: DSK/Nadir/Unprioritized
cspice_subslr method: DSK/Nadir/Unprioritized
Illumination angles at the sub-solar point:
Phase angle (deg):<PHONE_NUMBER>78
Solar incidence angle (deg): 0.967122745
Emission angle (deg):<PHONE_NUMBER>99
Illumination angles at the sub-s/c point:
Phase angle (deg):<PHONE_NUMBER>59
Solar incidence angle (deg):<PHONE_NUMBER>67
Emission angle (deg): 0.117861156
Mice contains four routines that compute illumination angles:
cspice_illumf (same as cspice_illumg, except that illumination
and visibility flags are returned)
cspice_illumg (same as this routine, except that the caller
specifies the illumination source)
cspice_ilumin (this routine)
cspice_illum (deprecated)
cspice_illumf is the most capable of the set.
Illumination angles
===================
The term "illumination angles" refers to following set of
angles:
phase angle Angle between the vectors from the
surface point to the observer and
from the surface point to the
illumination source.
incidence angle Angle between the surface normal at
the specified surface point and the
vector from the surface point to the
illumination source.
emission angle Angle between the surface normal at
the specified surface point and the
vector from the surface point to the
observer.
The diagram below illustrates the geometric relationships
defining these angles. The labels for the incidence, emission,
and phase angles are "inc.", "e.", and "phase".
*
illumination source
surface normal vector
._ _.
|\ /| illumination
\ phase / source vector
\ . . /
. .
\ ___ /
. \/ \/
_\ inc./
. / \ /
. | e. \ /
* <--------------- * surface point on
viewing vector target body
location to viewing
(observer) location
Note that if the target-observer vector, the target normal vector
at the surface point, and the target-illumination source vector
are coplanar, then phase is the sum of the incidence and emission
angles. This rarely occurs; usually
phase angle < incidence angle + emission angle
All of the above angles can be computed using light time
corrections, light time and stellar aberration corrections, or no
aberration corrections. In order to describe apparent geometry as
observed by a remote sensing instrument, both light time and
stellar aberration corrections should be used.
The way aberration corrections are applied by this routine
is described below.
Light time corrections
======================
Observer-target surface point vector
------------------------------------
Let `et' be the epoch at which an observation or remote
sensing measurement is made, and let et-lt ("lt" stands
for "light time") be the epoch at which the photons
received at `et' were emitted from the surface point `spoint'.
Note that the light time between the surface point and
observer will generally differ from the light time between
the target body's center and the observer.
Target body's orientation
-------------------------
Using the definitions of `et' and `lt' above, the target body's
orientation at et-lt is used. The surface normal is
dependent on the target body's orientation, so the body's
orientation model must be evaluated for the correct epoch.
Target body -- illumination source vector
-----------------------------------------
The surface features on the target body near `spoint' will
appear in a measurement made at `et' as they were at et-lt.
In particular, lighting on the target body is dependent on
the apparent location of the illumination source as seen
from the target body at et-lt. So, a second light time
correction is used to compute the position of the
illumination source relative to the surface point.
Stellar aberration corrections
==============================
Stellar aberration corrections are applied only if
light time corrections are applied as well.
Observer-target surface point body vector
-----------------------------------------
When stellar aberration correction is performed, the
direction vector `srfvec' is adjusted so as to point to the
apparent position of `spoint': considering `spoint' to be an
ephemeris object, `srfvec' points from the observer's
position at `et' to the light time and stellar aberration
corrected position of `spoint'.
Target body-illumination source vector
--------------------------------------
The target body-illumination source vector is the apparent
position of the illumination source, corrected for light
time and stellar aberration, as seen from the target body
at time et-lt.
Using DSK data
==============
DSK loading and unloading
-------------------------
DSK files providing data used by this routine are loaded by
calling cspice_furnsh and can be unloaded by calling cspice_unload or
cspice_kclear. See the documentation of cspice_furnsh for limits on
numbers of loaded DSK files.
For run-time efficiency, it's desirable to avoid frequent
loading and unloading of DSK files. When there is a reason to
use multiple versions of data for a given target body---for
example, if topographic data at varying resolutions are to be
used---the surface list can be used to select DSK data to be
used for a given computation. It is not necessary to unload
the data that are not to be used. This recommendation presumes
that DSKs containing different versions of surface data for a
given body have different surface ID codes.
DSK data priority
-----------------
A DSK coverage overlap occurs when two segments in loaded DSK
files cover part or all of the same domain---for example, a
given longitude-latitude rectangle---and when the time
intervals of the segments overlap as well.
When DSK data selection is prioritized, in case of a coverage
overlap, if the two competing segments are in different DSK
files, the segment in the DSK file loaded last takes
precedence. If the two segments are in the same file, the
segment located closer to the end of the file takes
precedence.
When DSK data selection is unprioritized, data from competing
segments are combined. For example, if two competing segments
both represent a surface as a set of triangular plates, the
union of those sets of plates is considered to represent the
surface.
Currently only unprioritized data selection is supported.
Because prioritized data selection may be the default behavior
in a later version of the routine, the UNPRIORITIZED keyword is
required in the `method' argument.
Syntax of the `method' input argument
-----------------------------------
The keywords and surface list in the `method' argument
are called "clauses." The clauses may appear in any
order, for example
'DSK/<surface list>/UNPRIORITIZED'
'DSK/UNPRIORITIZED/<surface list>'
'UNPRIORITIZED/<surface list>/DSK'
The simplest form of the `method' argument specifying use of
DSK data is one that lacks a surface list, for example:
'DSK/UNPRIORITIZED'
For applications in which all loaded DSK data for the target
body are for a single surface, and there are no competing
segments, the above string suffices. This is expected to be
the usual case.
When, for the specified target body, there are loaded DSK
files providing data for multiple surfaces for that body, the
surfaces to be used by this routine for a given call must be
specified in a surface list, unless data from all of the
surfaces are to be used together.
The surface list consists of the string
'SURFACES ='
followed by a comma-separated list of one or more surface
identifiers. The identifiers may be names or integer codes in
string format. For example, suppose we have the surface
names and corresponding ID codes shown below:
Surface Name ID code
------------ -------
"Mars MEGDR 128 PIXEL/DEG" 1
"Mars MEGDR 64 PIXEL/DEG" 2
"Mars_MRO_HIRISE" 3
If data for all of the above surfaces are loaded, then
data for surface 1 can be specified by either
"SURFACES = 1"
or
'SURFACES = "Mars MEGDR 128 PIXEL/DEG"'
Double quotes are used to delimit the surface name
because it contains blank characters.
To use data for surfaces 2 and 3 together, any
of the following surface lists could be used:
'SURFACES = 2, 3'
'SURFACES = "Mars MEGDR 64 PIXEL/DEG", 3'
'SURFACES = 2, Mars_MRO_HIRISE'
'SURFACES = "Mars MEGDR 64 PIXEL/DEG", Mars_MRO_HIRISE'
An example of a `method' argument that could be constructed
using one of the surface lists above is
'DSK/UNPRIORITIZED/SURFACES = "Mars MEGDR 64 PIXEL/DEG", 3'
Aberration corrections using DSK data
-------------------------------------
For irregularly shaped target bodies, the distance between the
observer and the nearest surface intercept need not be a
continuous function of time; hence the one-way light time
between the intercept and the observer may be discontinuous as
well. In such cases, the computed light time, which is found
using iterative algorithm, may converge slowly or not at all.
In all cases, the light time computation will terminate, but
the result may be less accurate than expected.
Please refer to the Aberation Corrections Required Reading (ABCORR.REQ)
for detailed information describing the nature and calculation of the
applied corrections.
For important details concerning this module's function, please refer to
the Mice routine cspice_ilumin.
MICE.REQ
ABCORR.REQ
DSK.REQ
FRAMES.REQ
NAIF_IDS.REQ
PCK.REQ
SPK.REQ
TIME.REQ
-Mice Version 1.1.0, 04-APR-2017, EDW (JPL)
Changed field name, in 'ilumin' return argument, corresponding
to the 'solar' incidence angle from "solar to "incdnc" (incident).
This change corresponds to the modification made to the MiceIlum
return structure.
Particulars updated to refer to Aberration Corrections
Required Reading document.
I/O updated to describe use of DSKs.
-Mice Version 1.0.4, 12-MAR-2012, SCK (JPL), EDW (JPL)
References to the new 'cspice_pxfrm2' routine were added to the
'I/O returns' section. A problem description was added to the
'Examples' section.
Edited I/O section to conform to NAIF standard for Mice documentation.
-Mice Version 1.0.3, 29-APR-2011, EDW (JPL)
Corrected minor typo in header and another in the usage string.
-Mice Version 1.0.2, 12-MAY-2009, EDW (JPL)
Edited I/O section; added 'fixref' description.
-Mice Version 1.0.1, 30-DEC-2008, EDW (JPL)
Added typography markers to usage string descriptor.
Minor edit to Example comments.
Corrected misspellings.
-Mice Version 1.0.0, 14-FEB-2008, EDW (JPL)
illumination angles
lighting angles
phase angle
emission angle
solar incidence angle
|


IS liaison to ASG slain in Sulu clash
by Francisco TuyayAn Islamic-trained bomb expert who had been liaising between the global terror network and the Abu Sayyaf bandit group in Mindanao was killed Friday in a military operation in Patikul, Sulu, the military said Saturday.
The man was identified as Talha Jumsah, alias Abu Talha, considered a high-value target of the military in Sulu, slain during a 20-minute battle with army elite Scout Rangers in Sitio Tubig Amu. Barangay Tanum, Patikul at about 7:15 a.m. the other day.
His body was recovered 800 meters away from the encounter site during a clearing operation in the aftermath of the fighting with soldiers from the Ist Scout Ranger Battalion and the 1101st Infantry Brigade.
''Abu Talha is a high-value target of the AFP in Sulu. Accordingly, he is an ISIS-trained Improvised Explosive Device expert who served as an instructor to the ASG in the fabrication of a more lethal and destructive IEDs that caused tremendous casualties during the suicide bombings in Sulu,” Major Gen. Corleto Vinluan Jr., commander of Joint Task Force Sulu, said.
“He also served as the financial conduit and liaison between foreign and local terrorist communication lines,” Vinluan added. Vinluan attributed the killing of Abu Talha on the information shared with the government by the civilian community in Patikul town.
The encounter, Vinluan said, was a follow-up operation against ASG bandits and their movements in the bushy area in Sitio Tubig Amu.
The ASG extremists and Talha were monitored by the troops and intercepted the terrorists whiuch sparked the gunfight. Operating troops recovered personal belongings, cooking and dining utensils, a backpack, and uniform while blood stains were also seen in the encounter site.
Three soldiers were wounded but are now in stable condition in Camp Teodulfo Bautista Station Hospital in Busbus, Jolo.
''The death of Abu Talha will surely cause demoralization in the ASG ranks in Sulu. It could not have been made possible without the support of the Tausug community who reported the presence of the armed terrorists and volunteered to serve as guides during the conduct of combat operations,” said Brig. Gen. Antonio Nafarrete, commander of the 1101st Infantry Brigade.
Vinluan lauded the operating units who carried out the combat operations to stop Abu Talha as he gave stern waming that the AFP in Sulu would not stop in hunting down the remaining ASG members in Sulu until all of them were brought to justice.
''I am reiterating my appeal to them to surrender and live a normal life instead of being hunted down as fleeing criminals and a disgrace to the peace-loving Tausug Community. One by one, we will hunt you down,” Vinluan emphasized.
The ISIS-inspired ASG has launched suicide bombings in military posts in Mindanao since January this year that killed three soldiers at a military post while a female, two Egyptians and a Moroccan, were killed in failed suicide bombing attempts.
President Rodrigo Duterte had ordered the military to “destroy” the ASG following the deadly blasts at a Roman Catholic Cathedral in Jolo, Sulu that left more than 20 people dead.
Duterte told the soldiers to crush the ASG by “whatever means.”
The military is presently hunting down at least three more foreigners they believed as suicide bombers.
READ: 8 soldiers injured, Abu bandits killed in Sulu clash
READ: 2 Abu Sayyaf killed, 2 hurt in clash with troops in Sulu


--- layout: archive title: Zulip Chat Archive permalink: /stream/113488-general/topic/.22missing.22.20theorems.html ---
I have noticed that there seems to be a mismatch between the theorems in the set
and finset
module in mathlib. I would expect them to share a lot of theorems (and indeed they do), but there are also theorems in one which are not in the other, when they might be expected to be in both.
For example, in set
(in data/set/basic.lean
) there is:
theorem union_diff_distrib {s t u : set α} : (s ∪ t) \ u = s \ u ∪ t \ u
However, there is no similarly typed theorem for finset
.
Is there a reason for this?
I'm planning a PR to add this sort of thing soon, as far as I can tell it's just the case that no-one's gotten round to it yet
Is there a corresponding lemma for a suitable type of lattices?
Is there a corresponding lemma for a suitable type of lattices?
You mean in mathlib?
The suitable type is boolean algebras, but there is no \
operator on boolean algebras, only unary complementation and lattice meet a ⊓ -b
it might make sense to define a - b
but I'm not a big fan of overloading the algebraic operators because they could conflict with other possible meanings for the expression (e.g. A - B
in sets meaning the set of all subtractions of elements of A and B)
@Mario Carneiro Can't we overload \
in this case?
Last updated: Apr 24 2020 at 19:02 UTC


$$
Alumini Grant
ASPRS
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(make-instance 'http-url :host "foo.com" :port "8000" :scheme "HTTP" :path "/bar") => url (parse-urlstring "http://foo.com:8000/") => url (merge-url an-existing-url "/relative?url") => url
url-scheme url-endpoint url-path url-query url-fragment
also url-host url-port ( url-endpoint = url-host ":" url-port )
These also have SETF methods. The behaviour of (setf url-scheme) is undefined, however, and it will probably go away unless somebody suggests a sensible one.
Relative URLs are not implemented as objects - if we don't know what scheme they have, we don't know how to parse them. We do have a procedure merge-url that merges a base url with a string, though, which caters for most uses.
(merge-url url string)
will create and return a new URL from STRING according to the rules for creating relative URLs. Note that this is a complex operation which takes a whole RFC to describe, and it's unlikey that we do it correctly in weird cases. Relative URLs with authority components containing non-standard hosts are currently known to be broken.
In addition, there is also append-url which is very crude. It functions similarly to merge-url, but it is not recommended that you use it. The ONE time it is recommended is when you want to concatenate a URL with a string that begins with a slash.
(let ((url (parse-urlstring "http://example.com/my/example"))) (format t "merge: ~A~%" (merge-url url "/is/here")) (format t "append: ~A~%" (append-url url "/is/here"))) merge: #<HTTP-URL "http://example.com/is/here" {9506011}> append: #<HTTP-URL "http://example.com/my/example/is/here" {95073B9}>


CMPSC311 Project Submission Portal
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Morse code audio generator
Dih-dah sounds generated using morse-code-wav
Awesome video on Morse code
Source Code


CPU On both servers
Disk I/O on both servers
IPv4 traffic on both servers
Netdata statistics on both servers
registry.my-netdata.io
your netdata server


Modify your Account
If you need help to get your georide token or the ID of your tracker, go to the help page.
{% extends "map/base/base.html" %} {% load static %} {% block title %}
If you need help to get your georide token or the ID of your tracker, go to the help page.


Main Title of Web Page
Menu Html Css JavaScript
Content goes here
First name:
Last name:
Account:
Pwd:
我就是一个文本框
Name:
E-mail:
Comment:
RUNOOB.COM
JavaScript can react to events. Like the click of a button.
Click Me!
my can't react?
Click!


TESTING USE ONLY TESTING USE ONLY TESTING USE ONLY TESTING USE ONLY TESTING USE ONLY TESTING USE ONLY
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spod
`Prev `__
S
`Next `__
--------------
**spod**: n.
[UK]
1. A lower form of life found on `*talker
system* <../T/talker-system.html>`__\ s and
`*MUD* <../M/MUD.html>`__\ s. The spod has few friends in
`*RL* <../R/RL.html>`__ and uses talkers instead, finding communication
easier and preferable over the net. He has all the negative traits of
the computer geek without having any interest in computers per se.
Lacking any knowledge of or interest in how networks work, and
considering his access a God-given right, he is a major irritant to
sysadmins, clogging up lines in order to reach new MUDs, following
passed-on instructions on how to sneak his way onto Internet (“Wow! It's
in America!”) and complaining when he is not allowed to use busy routes.
A true spod will start any conversation with “Are you male or female?”
(and follow it up with “Got any good numbers/IDs/passwords?”) and will
not talk to someone physically present in the same terminal room until
they log onto the same machine that he is using and enter talk mode.
Compare `*newbie* <../N/newbie.html>`__,
`*tourist* <../T/tourist.html>`__, `*weenie* <../W/weenie.html>`__,
`*twink* <../T/twink.html>`__, `*terminal
junkie* <../T/terminal-junkie.html>`__, `*warez
d00dz* <../W/warez-d00dz.html>`__.
2. A `*backronym* <../B/backronym.html>`__ for “Sole Purpose, Obtain a
Degree”; according to some self-described spods, this term is used by
indifferent students to condemn their harder-working fellows. Compare
the defiant adoption of the term `*geek* <../G/geek.html>`__ in the
mid-1990s by people who would previously have been stigmatized by it.
Spods in the positive sense are talker users who've accumulated a large
amount of spod time, that is, they spend a lot of time logged in to that
talker (for example, my spod time on Uberworld as of this moment is 131
days, 15 hours and 20 minutes). Spods are generally highly knowledgeable
about talkers and SGXStalker coding, as well as computers and the
internet in general.
3. [Glasgow University] An otherwise competent hacker who spends way too
much time on talker systems.
4. [obs.] An ordinary person; a `*random* <../R/random.html>`__. This is
the meaning with which the term was coined, but the inventor informs us
he has himself accepted sense 1.
--------------
+----------------------------+----------------------------+----------------------------+
| `Prev `__ | `Up <../S.html>`__ | `Next `__ |
+----------------------------+----------------------------+----------------------------+
| splork! | `Home <../index.html>`__ | spoiler |
+----------------------------+----------------------------+----------------------------+


---
layout: post
title: ''
date: '2008-04-20T10:22:00-07:00'
tags:
tumblr_url: http://alexhwilliams.tumblr.com/post/32334063/judys-birthday-second-try-at-getting-video
---
Judy’s birthday — second try at getting video uploaded from Flip camera. Saved file. Converted AVI to MP4 and saved as a Quicktime movie. Video would not play when saved for iPod. Resolution quality decreases when saved in .mov format.