Great Expectations (1998)
Director: Alfonso Cuaron Cast: Ethan Hawke, Gwyneth Paltrow, Hank Azaria, Chris Cooper, Anne Bancroft, Robert De Niro Rated R: Language, sexuality
by Nathaniel R. Atcheson<EMAIL_ADDRESS>This is one of those extremely rare cases in which I have actually read the source text from which a film is based. Dickens' Great Expectations was one of the books that I decided might be worth my time in high school (though I was wary after David Copperfield). I was pleasantly surprised by the novel, which I found to be an entertaining and very insightful look into the growth of one young boy named Pip.
The film version, for all who have not seen the preview, is a modernization of the story. Finn is the name of the character, and he is valiantly played by Ethan Hawke. The film opens in Florida and we are introduced to Finn (as a child, played by Jeremy James Kissner) in the famous scene with the escaped convict, played by Robert De Niro. Finn brings the convict food out of the goodness of his heart, but the convict is captured anyway. Later, we meet Finn's stepfather, Joe (Chris Cooper); Finn helps Joe with his day-to-day labor, and it becomes clear that, despite their lower-class living, they are at least somewhat content with their lives.
One day, Finn gets a call from the richest woman in Florida, Mrs. Dinsmore (Ms. Havisham in the book); she wants Finn to come and entertain her with his artistic talents. When he arrives at her home, he finds an eccentric, possibly psychotic, woman (Anne Bancroft) who lives in a great big, run-down house with her niece, Estella. The film takes off from there, going through the many love battles between Estella and Finn; Finn later ends up in New York as a successful artist, still trying to win Estella's love.
What I found most fascinating about the film is how close director Alfonso Cuaron came to creating the same images that I pictured as I read the book. Given that the book is from a different time period, I find this amazing. The cinematography and production design are truly striking, most notably in the scenes depicting Mrs. Dinsmore's lavishly decadent home. The courtyard in front of the house, ornamented with overgrown trees and vines; the rooms indoors, devoid of furniture but full of empty space--the locations in this film feel detached from time, as if we could look back on them in ten or thirty or one hundred years and they will all be the same.
I also think Hawke is the perfect choice to play Finn. Hawke has the kind of strength that this character needs, and he is capable of letting the audience know that a lot of what he does is just for show, that he isn't as strong and sure of himself as he seems. Ironically, this performance is not as powerful as I was expecting. The scenes in which he is drawing Estella are very well-done; sometimes, however, when he gets into situations in which he has to speak softly and be subtle, he drops the ball and makes some lines sound silly.
Gwyneth Paltrow plays Estella as an adult, and she does a great job in the role (though I pictured the character to look entirely different). I could see how some may say that she's one-dimensional, and often purely cruel, but Paltrow conveys just the right amount of inner torture, and it becomes clear that what she does to Finn is not out of spite, but out of habit. Supporting performances from Anne Bancroft, Chris Cooper, Hank Azaria, and Robert De Niro are all unique and colorful, and add a lot of life to the film.
Like all films, this one is not perfect. I wouldn't say that it doesn't live up to the book, because I think in many ways it does. What the film does that doesn't feel quite right is that it centers far too much on the relationship between the characters and not enough on just what Finn is doing and thinking in his life.
There are some truly brilliant scenes, though. My favorite in the film is probably the one in which Finn storms into a restaurant, approaches Estella, and says, "Would you like to dance?" with her fiancée sitting right there. After dancing for a few seconds, he takes her outside in the rain and they share a moment of passion--followed by sex, of course.
Great Expectations is thick on atmosphere and character, and in the end I found it to be an effective film. Unlike the cinematic tragedy of William Shakespeare's Romeo + Juliet, Cuaron has successfully updated a classic tale, and, despite a few flaws in content and story concentration, the result is an intelligent, insightful picture that both fans of the book and those not familiar with it can enjoy.
>From 0-10: 7 Grade: B
Visit FILM PSYCHOSIS at http://www.pyramid.net/natesmovies
Nathaniel R. Atcheson
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Seven O’Clock Stories
by Robert Gordon Anderson
“Third Night: Noisy Folks”
Additional Information
- Year Published: 1920
- Language: English
- Country of Origin: United States of America
- Source: Anderson, R. G. (1920). Seven O’Clock Stories. New York: G.P. Putnam’s Sons: The Knickerbocker Press.
-
Readability:
- Flesch–Kincaid Level: 4.6
- Word Count: 925
- Genre: Adventure
- Keywords: children's stories
- ✎ Cite This
Downloads
Do you remember what we were telling about last night when that little tongue told us to stop? The little tongue in the Clock-with-the-Wise-Face on the mantel?
Oh yes, the first cousins of the chickens who lived in the yard of the three happy children.
Their first cousins are called ducks. Most of them are white but a few are black. Their coats are very smooth, and the skin under them sends out little drops of oil like drops of perspiration. This keeps the water and the rain from wetting the ducks through and through. You have heard people say sometimes: “The way water runs off a duck’s back.” Well, now you know the reason why.
In rainy weather Hepzebiah wears a blue waterproof with a little hood but the ducks do not need anything like that.  If the White Wyandottes cannot get under the chicken coop or the barn quick enough when it rains, their feathers are all mussed up but the ducks seem always dressed in their best.
Their bills are different from their relatives’. They are not short and pointed like the chicken’s but broad and long.
And they have what are called web feet. Between the toes are pieces of skin, thick and tough like canvas. These web feet are like small oars or paddles. With them they can push against the water of the pond and swim quite fast.
The ducks are very fond of the pond but their cousins think it a dreadful place.
“Cluck, cluck,” say the White Wyandottes, “what a foolish way of spending your time, sailing on the water when there are fat, brown worms to dig for in the nice earth!”
You see animals, like people, like different things. The world wouldn’t be half so interesting if we all liked the same things, would it?
The other night Jehosophat felt very foolish when he came in to supper. His mother looked behind his ears and said: “Why you are just as afraid of the water as the chickens.”
Did you ever hear of such a thing!
Now the chickens have second cousins too. Their second cousins are the white geese.
They live on the other side of the tall fence that looks as if it were made of crocheted wire. Sometimes Jehosophat’s father opens the gate in the fence and lets the geese wander down to the pond.  This frightens Hepzebiah who always runs away. Then the geese waddle along in single file, that is one by one, like fat old ladies crossing a muddy street on their way to sewing society.
Jehosophat says that the chickens have third cousins too,—the swans. There they are, way out on the pond, sailing along like white ships. Their necks are very long and snowy white and they bend in such a pretty way. And their soft white wings look something like the wings of the angels on the Christmas cards.
Jehosophat, Marmaduke, and Hepzebiah do not like one barnyard neighbour very much. It is the guinea-hen.  She screeches horribly and Marmaduke calls her “Miss Crosspatch.”
But the turkey with his proud walk is just funny. And yet Farmer Green says he hasn’t any sense of humour. Ask your father how that can be if he is funny.
“Mr. Stuckup” the children call the turkey. He walks along slowly, swinging from side to side. His feathers are brownish-black or bronze, and his tail often spreads out like a fan. He has the funniest nose. It is red and soft and long and flops over his bill on his chest.
He calls “gobble, gobble, gobble,” all the time, yet he does not gobble as much as the busy White Wyandottes all around him who are forever looking for kernels of corn or worms or bugs.
But who is this magnificent creature coming along over the lawn under the cherry-tree?  He brought him from a land very far across the seas.
He is the peacock and is all green and gold and blue. On his head is a little crown of feathers. His tail, too, can spread out like a fan the way “Mr. Stuckup’s,” the turkey’s, does. But it is ever so much more beautiful. It is green and has hundreds of blue eyes in it. The three children call him the “Party Bird” for he is always so dressed up, but their father says he is “a bit of a snob.” He means that he is vain and will not have much to do with his plainer neighbours of the barnyard—
“One, two, three, four, five, six, seven.” There goes the clock again.
Tomorrow night, if you are good all day, we will tell you about the rest of the barnyard friends of the three happy children. Then the next night, about the exciting things that happened to them.
Good-night! Sweet Dreams!


{% extends "templates/post.html" %}
{% block post %}
{% filter markdown %}
[ScreenX TV](http://screenx.tv/) is a tool for broadcasting your terminal in
real time. The project is open source and currently in development.
Repos:
* [ScreenX TV Sandbox](https://github.com/yasulab/screenxtv-sandbox)
* [ScreenX TV Ruby Client](https://github.com/tompng/screenxtv-ruby-client)
* [ScreenX TV GCC Client](https://github.com/tompng/screenxtv-gcc-client)
* [ScreenX TV Internal Software](https://github.com/tompng/screenx)
ScreenX TV vs Codestre.am
-------------------------
[codestre.am](http://codestre.am) is another terminal broadcasting service I've
used in the past.
### Replays
One feature codestre.am has that ScreenX TV currently lacks
is video-on-demand for previous broadcasts. These stream replays are
particularly useful for bug reports and tutorials.
### Performance
codestre.am's servers are constantly under heavy load. Sometimes the
site will simply be unavailable for 30 minutes at a time. The lack of
reliability is a bit of a turn off. Currently, ScreenX TV seems to have almost
zero down-time. The site is extremely responsive. Broadcasting is very smooth,
consistent, and lag-free. This might be due to the lack of users, though. Only
time will tell.
### Ease of installation
Installing codestre.am was particularly annoying. The installation process was
plagued with npm and node.js errors. It took at least two hours of googling
error messages to finally get to where I was broadcasting.
ScreenX TV has three installation options. You can install via
* [GCC](https://github.com/tompng/screenxtv-gcc-client)
* [Ruby Gems](https://github.com/tompng/screenxtv-ruby-client)
* [curl script](https://github.com/yasulab/screenxtv-sandbox)
I've tried both the GCC and the curl script installations. Both work perfectly.
### Ease of use, features, and various issues
In order to broadcast, codestre.am would generate a random string for you to
pass to the `codestream` executable that you install via npm. ScreenX TV uses
a local configuration file.
codestre.am had huge issues in all my terminals - ranging from iTerm2 to
gnome-terminal. The terminal would display correctly on the stream, but my
screen would appear completely broken in the actual terminal. This resulted in
me hiding my terminal behind my browser window and looking at the browser to
work. This was a pretty severe inconvenience. ScreenX TV seems to work
perfectly in this regard.
codestre.am only let you broadcast in one size: About 630x330. ScreenX TV will
adjust the broadcast stream size as you adjust your terminal. If you stretch
your terminal, you will see the stream adjust in real-time.
Conclusion
----------
codestre.am is a finished product that feels like an unfinished product.
ScreenX TV is an unfinished product that feels like it could be everything
codestre.am tried to be once fully developed. If ScreenX TV can implement
replay support, I can see it changing how tutorials, debugging, and
pair-programming are handled.
{% endfilter %}
{% endblock post %}


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The Monkees present The Mike & Micky Show Details: The Monkees
Book nowThe Monkees present The Mike & Micky Show Details: The Monkees
Book nowThe Monkees present The Mike & Micky Show Details: The Monkees
Book nowAs well as performing concerts around the world, we also love to gig at events that our fans host. We have performed at weddings, birthday parties, bar mitzvahs and many other types of events. If you have something in mind then....


|
NMEAParser
NMEA Parser Library - Monte Variakojis @VisualGPS
|
GGA Data. More...
#include <NMEAParserData.h>
Public Attributes | |
| int | m_nHour |
| hour More... | |
| int | m_nMinute |
| Minute. More... | |
| int | m_nSecond |
| Second. More... | |
| double | m_dLatitude |
| Latitude (Decimal degrees, S < 0 > N) More... | |
| double | m_dLongitude |
| Longitude (Decimal degrees, W < 0 > E) More... | |
| double | m_dAltitudeMSL |
| Altitude (Meters) More... | |
| GPS_QUALITY_E | m_nGPSQuality |
| GPS Quality. More... | |
| int | m_nSatsInView |
| Number of satellites in view. More... | |
| double | m_dHDOP |
| Horizontal Dilution of Precision. More... | |
| double | m_dGeoidalSep |
| Geoidal separation, the difference between the WGS-84 earth ellipsoid and mean-sea-level (geoid), "-" means mean-sea-level below ellipsoid (meters) More... | |
| double | m_dDifferentialAge |
| Age of differential GPS data, time in seconds since last SC104 type 1 or 9 update, null field when DGPS is not used. More... | |
| int | m_nDifferentialID |
| Differential reference station ID, 0000-1023. More... | |
| double | m_dVertSpeed |
| Derived vertical speed (THIS IS NOT PART OF THE NMEA SPECIFICATION. It is derived during parsing) More... | |
GGA Data.
Definition at line 175 of file NMEAParserData.h.
| double CNMEAParserData::_GGA_DATA_T::m_dAltitudeMSL |
Altitude (Meters)
Definition at line 181 of file NMEAParserData.h.
| double CNMEAParserData::_GGA_DATA_T::m_dDifferentialAge |
Age of differential GPS data, time in seconds since last SC104 type 1 or 9 update, null field when DGPS is not used.
Definition at line 186 of file NMEAParserData.h.
| double CNMEAParserData::_GGA_DATA_T::m_dGeoidalSep |
Geoidal separation, the difference between the WGS-84 earth ellipsoid and mean-sea-level (geoid), "-" means mean-sea-level below ellipsoid (meters)
Definition at line 185 of file NMEAParserData.h.
| double CNMEAParserData::_GGA_DATA_T::m_dHDOP |
Horizontal Dilution of Precision.
Definition at line 184 of file NMEAParserData.h.
| double CNMEAParserData::_GGA_DATA_T::m_dLatitude |
Latitude (Decimal degrees, S < 0 > N)
Definition at line 179 of file NMEAParserData.h.
| double CNMEAParserData::_GGA_DATA_T::m_dLongitude |
Longitude (Decimal degrees, W < 0 > E)
Definition at line 180 of file NMEAParserData.h.
| double CNMEAParserData::_GGA_DATA_T::m_dVertSpeed |
Derived vertical speed (THIS IS NOT PART OF THE NMEA SPECIFICATION. It is derived during parsing)
Definition at line 188 of file NMEAParserData.h.
| int CNMEAParserData::_GGA_DATA_T::m_nDifferentialID |
Differential reference station ID, 0000-1023.
Definition at line 187 of file NMEAParserData.h.
| GPS_QUALITY_E CNMEAParserData::_GGA_DATA_T::m_nGPSQuality |
GPS Quality.
Definition at line 182 of file NMEAParserData.h.
| int CNMEAParserData::_GGA_DATA_T::m_nHour |
hour
Definition at line 176 of file NMEAParserData.h.
| int CNMEAParserData::_GGA_DATA_T::m_nMinute |
Minute.
Definition at line 177 of file NMEAParserData.h.
| int CNMEAParserData::_GGA_DATA_T::m_nSatsInView |
Number of satellites in view.
Definition at line 183 of file NMEAParserData.h.
| int CNMEAParserData::_GGA_DATA_T::m_nSecond |
Second.
Definition at line 178 of file NMEAParserData.h.


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And another thing I want to say...
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This is the last slide.


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College of Engineering and Information Sciences
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Project: PCB milling machine!
o nosso grupo FabLab FCT:
For this week of mechanical design, our FabLab FCT group decided to make a PCB milling machine.

Once we have defined the concept, we begin to design and plan the materials we would need.
We thought of designing a milling machine for a platform with a dimension of 120x120 mm (standard size of the copper platform).
The machine will use the platform as Y axis and the drill for the X axis and Z axis. This allows us to have a good performance and smallest possible space.
We decided to recycle materials, such as engines and shafts from other machines we had in the lab to save costs.
List of required materials:
After having all the necessary materials, we started to draw the 3D materials with the correct dimensions and from there we created the design of our machine with the drilling and the fittings for all the components.
File: XXX
After having the final design, we export the equipment from the exterior of our machine to the laser machine.
Some missing components were produced in 3D and printed. Support for the platform was printed in 3D.


--- layout: archive title: Zulip Chat Archive permalink: /stream/113488-general/topic/greek.20letter.20tactic.html ---
Is there a tactic doing only that greek letter which transforms (λ a, f a) x
to f x
?
I think dsimp
with one of its special options does it, but I don't remember exactly what it is
that's eta reduction
no
beta
that's delta reduction
oh
beta it is then
I say alpha!
no, that's also eta reduction
We need printable DTT cheat sheets
it's not even DTT
-- (λ (a : X), f a) x = f x example : (λ a, f a) x = f x := by dsimp { eta := false, beta := false } -- (λ (a : X), f a) x = f x example : (λ a, f a) x = f x := by dsimp { eta := true, beta := false } -- f x = f x example : (λ a, f a) x = f x := by dsimp { eta := false, beta := true }
why isn't it eta?
@Andrew Ashworth
i don't know how dsimp does it, but I remember it as eta is the sorta useless thing that turns lam x, f x --> f
, while beta is (lam x, f x) y --> f y
basically eta only cleans up useless lambdas
An amazing feature I only discovered recently: set_option pp.beta true
will hide those useless (λ a, f a) x
in displayed types
The slightly annoying thing about that is sometimes it won't rewrite because it's not reduced, and you get frustrated trying to work out why.
You need to set pp.beta true in rw as well :-)
{% endraw %}Last updated: Apr 24 2020 at 19:02 UTC


{% extends parent_template|default:"patients/base_patients.html" %} {% block title %} {{ block.super }} | Unarchive Patient {% endblock %} {% block page_heading %} Unarchive Patient {% endblock %} {% block page_subheading %} {% endblock %} {% block page_breadcrumb %} {{ block.super }} {% if patient.archived %}
This patient is currently not archived so confirming that he/she should be unarchived will not lead to any changes to patient's details nor affect the services that can be logged for him/her.


{{/* gotype: github.com/JustaPenguin/assetto-server-manager.realPenaltyConfigurationTemplateVars */}} {{ define "title" }}Real Penalty Options{{ end }} {{ define "content" }}
Real Penalty is the popular server side app
designed to manage custom penalties for organised racing.
Real Penalty is not developed or maintained by {{ if $.IsHosted }}Emperor Servers{{ else }}the Server Manager authors{{ end }}.
If you have questions related to the operation of the Real Penalty tool itself, please ask on the
Real Penalty support thread.
These configuration options are applied globally - they are applied to the Real Penalty configuration files whenever a race setup is started by Server Manager.
{{ else }}Real Penalty is not installed. Please follow the instructions below to install Real Penalty, or contact your Server Administrator:
Real Penalty {{ $.RealPenaltySupportedVersion }}.zip
realpenalty
assetto
folder. If you are using multiserver, copy it inside each one of them. E.g. inside youracserver/servers/SERVER_00/assetto/
Note: these instructions and the integration provided are known to be compatible with {{ $.RealPenaltySupportedVersion }}
of Real Penalty.
Other versions may work. If you have problems with a more recent version than this,
please File an issue.


INTRODUCTION TO COSMOLOGY (V.A.Sirota)
|
- Introduction: objects, scales
- Methods of distance determinaiton
- Hierarchical structure
- Hubble expansion
- Geometry of the Universe
- Cosmological principle
- Robertson-Walker metric
- Red shift
- Friedmann models
- Cosmological constant
- Horizons
- Recombination and cosmic ray background
- Spectrum transformation under free expansion
- Hot Universe
- Saha formula and eviations from it in expanding Universe
- Planck spectrum distortion
- Reionization
- Zeldovich-Sunyaev effect
- Cosmic ray background anisotropy
- Dipole and short-scale anisotropy
- Doppler peaks
- Sachs-Wolfe effect
- Silk damping
- Nucleosynthesis
- Temperature history of the Universe
- Jeans theory
- Fluctuation growth in the expanding Universe
- Formation of galaxies
- Dark matter
- Pros. Candidates
- Gravitational lenses and microlensing
- Zeldovich–Harrison spectrum
- Zeldovich pancakes
- Gurevich–Zybin theory
- LITERATURE:
- S. Weinberg. Gravitation and Cosmology
- L.D. Landau, E.M. Lifshitz. Field Theory
- Ya.B. Zeldovich, I.D. Novikov. Structure and Evolution of the Universe
- F.J.A. Peebles. Large-scale Structure of the Universe
- Perlmutter et al. Ap.J. 517, 565 (1999) – cosmological constant
- A.D. Chernin. (UFN) 171(11), 1153-1175 (2001)
- Kurt, Zeldovich, Sunyaev. JETP 55(1) 278 (1968) - recombination
- Zeldovich, Sunyaev. Comments on Astrophys. and Space Phys. v.2, 173 (1970) – Zeldovich–Sunyaev effect
- J.Silk. Ap.J. 151, 459 (1968)
- S.Weinberg. Ap.J. 168, 175 (1971) - Silk damping
- Sachs, Wolfe. Aph.J. 147, 73 (1967) - Sachs-Wolfe effect
- P.de Bernardis et al. astro-ph/0011468 - observations of anisotropy of cosmic ray background
- Ishkhanov, Kapitonov, Tyutin. Nucleosynthesis in the Universe
|
|


Comments
-
Greg Hurrell
Thanks for the request, Joseph. I have two thoughts about this:
1. Computational complexity
One is that the amount of computation required to calculate this "shortest string" would be absolutely enormous. Consider a typical project with anywhere from a few hundred to several thousand files in it, and think about how many possible permutations of search strings you would need to consider and compare in order to determine the best/shortest string for each file.
Imagine a path which has 40 or 50 characters in it, like
spec/controllers/issues_controller_spec.rb
; there are perhaps thousands of search strings of lengths ranging from as little as 1 to as many as 42 characters which could conceivably match this path:- one-letter strings: s, p, e, c, /, o, n, t, r, l, i, u, _, ., b
- two-letter strings: sp, se, sc, s/, so, sn ... pe, pc, p/, po ...
- three-letter stings: ...
The number of permuations is absolutely enormous, and for each of these you would need to calculate a "score" between 0.0 and 1.0 indicating the ranking for that path given that search pattern. Multiply that by 4 or 5,000 paths in the project and we're already talking about millions of scores.
Once you've got all these score you then need to grind through them and figure out which one is the shortest "winning" score for each path, and it's quite possible that there will be a tie and you'll then have to decide which one is the "best" or most intuitive one which you should show as a hint to the user. The amount of work needed to perform this comparison would grow exponentially as the number of files in the project increases.
I don't actually think this could be viably done for anything but the most trivial projects; for real-world projects with typical file counts in the hundreds and thousands performance would quickly degrade to the point of being untenable.
2. The right way to solve the problem
My other thought is that if finding files with Command-T isn't intuitive and easy for you, then the solution is not having you look at or memorize a list of shortcuts (which in themselves may not seem at all intuitive to you; you may end up asking yourself, why did the program end up choosing those letters for that path?). I think instead you'd benefit much more from a deeper understanding of how results are scored, and when you understand the way the algorithm works, it becomes much easier to find what you're looking for.
I'll try to sum it up for you in a nutshell here:
- Command-T looks at characters in the entire path, not just the file name (ie. if you want to open
foo/bar
then you're not limited to typing "bar" but can type "fb" instead) - by including characters from the initial path components rather than just the filename you help narrow down the range of possible matches (ie. given file
spec/models/issue_spec.rb
you will probably narrow down the search more decisively by typing "smi" than by typing "iss") - some characters are weighted more heavily in the scoring algorithm; that is, characters which appear immediately after a slash or an underscore will be given more weight than those buried in the middle of a run of letters (ie. given file
lib/authentication/ssl_wrapper.rb
a string like "lasw" will score more highly than one like "bclr"; both of those strings match the path, but the first one is a "better" match because the matching characters fall after boundary characters)
As a general rule of thumb the most important things to remember are:
- characters that follow "boundary" markers (like "/" and "_") are the most important ones, and are the ones that you should prefer when typing your search string
- as the number of files in the project grows, the more important it becomes to provide letters from higher up in the path components (eg. in a 10-file project then it is fine to type "bar" in order to find
foo/bar
, but in a 10,000-file project if you want to openfoo/bing/bang/bong/buzz/bar
then you'd best get in the habit of typing something like "fbbbbbar" rather than just "bar")
Hope this helped.
-
anonymous
Wincent,
Thanks for the thoughtful response. Agreed on point 1 - way too computationally complex.
As an alternative, what if users could create their own file of mappings and command-T could process those are overrides to its own algorithm? That way, for those fifteen or so files that I am constantly going to, I can have those mappings memorized and count on just my fingers to get me where I need to go, rather than viewing the output from Command-T and verifying that I've highlighted the file I want.
So, billing_report.php could have the mapping "br". I type in "br" and that file is auto-selected. Type "Enter" and bam, it opens. Just as easily I should be able to alternatively choose "bphp" as the mapping, update my mappings file, and have that work.
What are your thoughts on this approach?
-Joseph
-
Greg Hurrell
Take a look at ticket #1541 ('"Learn" from previous selections'). The idea proposed there is that the plug-in remembers which files you choose for any given search string and then in future searches adds a "bonus" to the score of such items when you enter that same search string again.
So in your example, you type "br", wanting to open
billing_report.php
, and it's not the top search result so you actually end up using the cursor keys to move down and select it. The next time you type "br", Command-T applies a small bonus tobilling_report.php
, pushing it slightly higher up the results listing. You again use the cursor keys to move down and select it and so the bonus is bumped up a little higher. Next time you type "br", the bonus is big enough to makebilling_report.php
the top result.What do you think of that one? I'm inclined to think that this would be a nice, intuitive way to transparently give you the behavior you're looking for without obliging users to spend time maintaing a special mappings file.
The only tricky part of this would be fine-tuning the implementation details (how much should the "bonus" fluctuate up or down when you select a file or later select a different one?) but nothing insurmountable.
-
joseph
Created , edited
The bonus is an interesting idea, though the bottom line is that it will take some time for the program to learn. Plus, what if I want to use a keystroke series that is not a match for the resource - it will never appear in the matches.
I delved into the Command-T source code last night and put a little something together. Let me know what you think. My co-worker and I are already using this and we like it a good bit. Eager to hear your thoughts, Wincent.
Inside controller.rb:
Add this line near the other requires:
require 'yaml'
Change this function:
def list_matches matches = @finder.sorted_matches_for @prompt.abbrev, :limit => match_limit override_file = "command-t-overrides.yaml" if File.file?(override_file) file_contents = IO.read(override_file) ruby_obj = YAML::load(file_contents) overrides = ruby_obj["overrides"] overrides.each_pair do |k,v| if @prompt.abbrev == k matches.insert(0, v) end end end @match_window.matches = matches end
And then in my directory where I usually launch vim, I have my command-t-overrides.yaml file:
overrides: { pr : scripts/billing/payment_report.php, br : scripts/billing/billing_report.php, cto : command-t-overrides.yaml }
-
Greg Hurrell
Nice to see you could implement this without having to make deep changes to the algorithm, but instead just insert it at a higher layer.
A few suggestions:
- wouldn't
command-t-overrides.yaml
be better as an invisible dot-file? - do you really need to wrap things inside the "overrides" hash? (if the file contains only key-value pairs
YAML::load
will return a hash anyway); if you're envisioning additional future possible uses for this file, of which shortcut overrides would be just one, then it should probably be called.command-t.yaml
and not have "overrides" in the file name at all - I'd suggest reading the overrides file once only at the beginning of the search, rather than for each key press (
list_matches
is called once for each new key press)
- wouldn't
Add a comment
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Lisa Kieffer
Unafffiliated
April 2019 - present: Solutions Consultant on Search Ads at Google -- Boulder, CO April 2018 - April 2019: Account Strategist at Google -- Boulder, CO May 2014 - May 2019: Business Manager and Bookkeeper at Boulder Swing Dance -- Boulder, CO April 2014 - August 2016: President and Treasurer Swing Dance Club at the University of Colorado Boulder -- Boulder, CO (unpaid student organization) May 2015 - July 2015: Summer Research Assistant in Political Science at the University of Colorado Boulder -- Boulder, CO February 2013 - May 2013: Resident Hall Assistant at the University of Delaware -- Newark, DE May 2012 - May 2013: Public Relations Officer for Swing Dance Club at the University of Delaware -- Newark, DE (unpaid student organization) September 2010 - July 2011: Barista at Barnes and Noble Booksellers -- Boulder, CO
BA from University of Colorado Boulder in Political Science (May 2017) BA from University of Colorado Boulder in Psychology (May 2017) Credits towards BS in Apparel Design at the University of Delaware (attended August 2011 - May 2013) High school diploma: Fairview High School (May 2010)
80301
In 2020 I donated $15 to the Biden/Harris campaign, but have not previously volunteered with an organization nor donated money.
My experience is primarily with student organizations during my time at university. These would include - University of Colorado Swing Dance Club Student Organization - University of Colorado Model United Nation Student Organization - University of Delaware Swing Dance Club Student Organization - National Honor Society Member through the University of Delaware
I have experience with organizing student and growing organizations of various sizes, and advocating for these student groups with the wider university systems especially with funding and growing membership numbers. During my 2 years on the board with CU Swing Dance I was able to develop a core leadership group, and increase membership attendance from 15/week to 60/week handling an annual budget of $10K. I've taken these student organization skills into the corporate environment to leverage people's passions to create a feeling of belonging and coming to a strong team decision that can move forward with a clear sense of ownership. While I would be new to the political organization sphere, I think that could play to the groups' advantage as I would not have any strong previous political alliances beyond the success of our state and nation to be beholden to. During the course of my experiences in developing and advocating roles I have found that being able to step back and listen to all sides of concern, without the weight of preference upon me, has allowed me to respond with more compassion with a fair balance of facts to make data driven decisions to benefit all involved.
I think it's important that all voices in all of our diverse communities are heard and have the opportunity to self-advocate within a larger political system. As a Colorado native, I have seen first hand how so many of our communities have changed, and how some voices have been lost as a result. I think during this unique time, when we need to unite our community perhaps more now than ever, we must first start by acknowledging our differences and ensuring those differences can be represented, not squashed. I would like to serve my Colorado community, my home, as we move into this next chapter. I would like to work to ensure that the commission comes to decisions that will serve all those we represent, while we might be a small this is not a small undertaken to identify and proactively prevent issues for our growing state. I also think that I could be a strong, well informed voice for a younger generation full of future voters. Politics for so long has been the "old boys club" which is no longer serving our country. We are more diverse and the decisions about our political future should have influence from those who it will impact the longest. While age may provide wisdom, it can also be wise to change how we evaluate current systems, the systems that many believe have failed those it's meant to serve. T
While individuals may disagree on many topics on the political spectrum we come here with a common goal: to serve our communities. I think the best way to build consensus is to first identify the shared goals for this organization before getting to detail oriented. By building a shared common language and framework of operations we can discuss the more contentious topics with respect for each other and respect for our core goals. Furthermore I am an empathetic person, we will all be coming here with our own story that shapes how we view the world and make decisions. By removing any "us vs them" mentality it will allow the whole commision to move forward successfully. Additionally I am not preemptively hoping for a specific outcome. This allows me to look at the whole picture without seeking confirmation bias, it allows me to listen to opinions openly without seeking points of pure rebuttal. This will allow me to unitilize facts and data to come to decisions, to hear all sides and provide an unbiased and fair opinion.
Making data driven decisions is key to ensuring a sustainable outcome. During my degrees I was often working with large data sets to provide insights and I can rely on my understanding of statistics to guide my decisions. As part of my professional career I continue to use large data sets to ensure that we're making good business decisions without the detriment of the people it will impact. We often need to make decisions that have a trade off, and being able to find a way that objectively helps the most people without undue detriment to those not directly benefiting needs to be based on as much data as possible. Additionally, solving a problem starts with making sure we're asking the right questions. Looking at data will only serve us fully if we're asking the right type of questions. To do this we must engage in expansive thinking before we can move to deductive thinking.
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HOpS is a tool for simulating the optics of a field of heliostats. HOpS was developed as part of the RE<C Initiative at Google, focused on developing concentrated solar power.
A heliostat is an actuated reflector (either flat or concave) designed to reflect sunlight onto a target surface, which may itself be flat or curved. In the context of concentrating solar energy production, the target may be
HOpS computes the visibility relationships between optical elements including the sun, heliostats, and discretized segments of the target surface. It simulates passing "packets" of light between each of these elements in order to compute irradiance data for the heliostats and the target.
HOpS was written as part of a larger effort in renewable energy research and development that focused on concentrating solar thermal production of electricity.
Our goals included optical simulation of a heliostat field over the course of an entire year with ten-minute granularity. Existing heliostat simulation tools were difficult to adapt to our needs. Optics simulation tools generally fall into two categories: raytracers and analytic approximations. Raytracers are very accurate, but because they need to compute flux using a statistically significant sample of rays, they require a lot of computation to arrive at a result. Analytic approximations, such as DELSOL, are very fast but allow only limited configurability and accuracy.
HOpS falls somewhere between the two categories, but closer to the analytic end of the spectrum: It passes data representing packets of light from one optical element to another, allowing it to compute shadowing and blocking masks precisely as vector-based objects, without the need for casting millions of light rays as a raytracer would.
HOpS is intended for use by researchers or designers of heliostat fields. It allows
There are so many optical simulation tools, covering various domains, that it be fruitless to attempt a comprehensive list here. Below is a small selection of tools which are relevant to concentrating solar applications.
Raytracers:
Analytic approximations:
The RE<C project used HOpS to lay out potential heliostat fields for the technology we designed. Because our heliostats employ pitch-roll actuation kinematics rather than conventional azimuth-elevation, they exhibit different shadowing and blocking characteristics than conventional heliostats do. We used HOpS to model this effect by comparing azimuth-elevation heliostats to pitch-roll heliostats for several different field configurations.
With a little scripting, we also used HOpS to gauge the benefit of
allowing heliostats in a tesselated field with regularly-placed receivers to
switch their aim from one receiver to another to maximize total flux through
the receivers' apertures, rather than always aiming at the nearest receiver.
This strategy can provide increased power by balancing cosine loss
(inefficiency due to canted reflectors) against spillage (reflected flux lost
because it doesn't pass through a receiver's aperture and thus doesn't strike
the receiver). We accomplished this by running HOpS seven times on a hexagonal
field assumed to be the basic unit of tesselation. For each run we used a
different receiver position: the center of the hexagon and the centers of the
six adjacent hexagons. We used HOpS' --heliostat_flux_on_target
flag (see below) to measure the flux from each heliostat that reaches the
receiver (through its aperture) and the --disable_field_masking
flag in order to be agnostic regarding the exact placement of heliostats and
their shadowing and blocking. Then, for each heliostat at each time step, we
took the highest flux-on-target value for that heliostat amongst all seven
receivers, assigning that heliostat to that receiver for that time step.
For a field located at Barstow's latitude, with parallel edges separated by 120 meters and with one pair of edges aligned east-west, receiver apertures of diameter 1.5 meters, level with the horizon and 42 meters above the centers of the mirrors, allowing retargeting yields 13% more flux on target on the winter solstice, 7% more on an equinox, and 5% more on the summer solstice than having each heliostat tied to its single closest receiver.
Features that would be very nice to add to HOpS include:
src/receiver_surfaces.cc
.HOpS is known to build on Ubuntu and Darwin. It depends on the following packages, which must be installed first:
It's best to install google-gflags
before
google-glog
, so that the google-glog
library will be
built with support for command-line flags. (Otherwise, you'll have to set the
environment variable GLOG_logtostderr=1
in place of using the
the command-line flag --logtostderr
discussed below.)
Once these are installed (and the protobuf compiler
protoc
is in your PATH
),
checkout the HOpS source code using the instructions
here.
Next, change to the resulting directory, then run
autoreconf --force --install --verbose ./configure
to construct a Makefile for your system. Then run
make hops
to build the hops
executable, or
make check
to build the executable and build and run the unittests.
./hops [--logtostderr] \ --layout_file=... \ --start_time=... --end_time=... --time_step=... \ [--disable_field_masking] \ [--heliostat_aiming_error=...] \ [--heliostat_facets_per_side=...] \ [--heliostat_flux_in=...] \ {other output flags}
For example, to simulate sixty minutes in the life of the field in
src/examples/curved_receiver_oblique_layout
, with receiver
irradiance output to my_receiver_irradiance
and field efficiency
output to my_heliostat_efficiency
, you might run something like
this:
./hops --logtostderr \ --layout_file=src/examples/curved_receiver_oblique_layout \ --start_time=1321395400 --end_time=1321399000 --time_step=60 \ --receiver_irradiance=my_receiver_irradiance \ --heliostat_efficiency=my_heliostat_efficiency
hops
reads a field configuration from a text protocol buffer
in the format defined in src/field_layout.proto
. The flag to
specify the file to load is --layout_file
.
The basic elements of a field configuration file are as follows:
sun
describes the location of the sun in the sky. It can be
either automatic, in which case you must use field_location
to specify the location of the field on Earth, or manual, in which case
you must specify a list of sun_config
messages, each of
which gives the sun's position in the sky (as a vector in field
coordinates, of arbitrary magnitude) as a sun_vector
message
and a corresponding direct normal insolation in watts per square
meter as a dni
value. In the automatic case, the sun's
position is computed using NREL's SOLPOS library, and DNI is
calculated using extraterrestrial DNI from SOLPOS multiplied by a
clear-sky atmospheric attenuation factor given by Rozenberg's equation;
see src/sun_calculators.cc
for more details.heliostat
and heliostat_block
are messages that
let you create individual heliostats or lattice-aligned blocks of
heliostats, respectively. In a heliostat
message, you can
specify reflectivity
, focal_length
,
actuation
kinematics (as DIRECT
,
AZI_ELE
, or PITCH_ROLL
), and the shape of the
reflector (either as a rectangle with width
and
height
or as a sequence of vertex
coordinate
pairs. A heliostat
also needs a location
and
an aim
point in field coordinates. Its frame's
orientation can be changed (thus affecting its actuation kinematics)
using a frame_orientation
message. A
heliostat_block
message, instead of having a
location
, takes parameters specifying the spacing and number
of heliostats in the x and y directions.receiver
defines the type
,
location
, and orienatation (via the direction
field) of the field's receiver. type
is a string specifying
which receiver shape from src/receiver_surfaces.cc
to use;
at present this is "flat" for a square plate three meters on a side, or
"alec" for a curved surface (a quadratic surface of revolution used as
an early model by one of our team members) with a radius at its mouth of
1.68 meters. The parameter resolution
specifies the number
of discrete elements in each of two axes into which to divide the
receiver surface for the simulation; for example, with
resolution
set to 10, the receiver will be divided into 100
discrete elements. If you care only about properties of the field or
about flux delivered through the aperture, it's best to use the "flat"
receiver with resolution
set to 1.aperture
specifies the location
and
radius
of a circular aperture to be placed near the
receiver, along with an orientation specified by the normal
direction. (Actually, due to the fact that we model all shapes in HOpS
as polygons, the aperture is approximated by a regular icosagon.)
If no aperture
message is specified, light from heliostats
may strike the receiver from any direction. Be aware when using a curved
receiver that, as an optimization, HOpS does not calculate blocking
between receiver elements. Thus, if you use a curved receiver without
also using an aperture to provide blocking, you may get incorrect
results.Reflector curvature is defined by the single parameter
focal_length
. Reflectors are assumed to be ideal flat Fresnel
reflectors (by analogy with the Fresnel lens), rather than spherical or
parabolic. This approximation is valid as long as the size of a heliostat is
much smaller than the distance between the heliostat and the receiver.
The three systems of heliostat actuation kinematics are as follows:
DIRECT
means that the reflector is tilted directly from
a horizontal orientation by the shortest path to the desired normal.AZI_ELE
models a conventional heliostat with a vertical
azimuth axis and a horizontal elevation axis that rotates with
azimuth.PITCH_ROLL
models the heliostats designed by the RE<C
team, which have a horizontal pitch axis and a roll axis that rotates
with pitch in the plane orthogonal to the pitch axis.Coordinates in a field configuration file may be expressed in any of the
following systems, which are defined in
math/coordinates3d.h
:
CARTESIAN
takes coordinates in (x, y, z) tuples.
The x-axis points east, the y-axis points north, and the z-axis points
up.CYLINDRICAL
takes coordinates in (ρ, φ, z) tuples.
ρ is distance from the z-axis. φ is measured in radians from
the x-axis (east), increasing towards the y-axis (north).SPHERICAL
takes coordinates in (r, θ, φ) tuples.
θ is inclination (or colatitude) meausured in radians. That is,
vectors with θ equal to π/2 lie in the x-y plane. φ is as
above.ASTRONOMICAL
takes coordinates in (altitude, azimuth,
elevation) tuples. Altitude is vector magnitude, the same as r in
spherical coordinates. Azimuth is a compass bearing (measured in degrees
from the y-axis and increasing towards the x-axis). Elevation (sometimes
called latitude) is an angle measured in degrees from the x-y plane, with
positive values corresponding to the positive z-direction.src/examples
contains the following example configuration
files:
curved_receiver_oblique_layout
models a square field of
heliostats with azimuth-elevation kinematics and trapezoidal
reflectors, aimed at a curved receiver located south of the field
and having an aperture with a 1.68 meter radius.
The sun moves automatically, with the field
presumed to be located in Barstow, California.flat_receiver_overhead_layout
models a square field
heliostats with pitch-roll kinematics and rectangular reflectors,
aimed at a flat plate receiver located 50 meters above the center of the
field, without any aperture between the heliostats and the receiver.
Again, the sun moves automatically, with the field presumed to be located
in Barstow, California.two_heliostats_layout
models two heliostats with
differently-shaped reflectors, positioned underneath a flat plate
receiver. Two different locations of the sun in the sky are specified,
together with values of direct normal insolation in watts per square
meter.--logtostderr
is recommended for visibility into what the
program is doing and its progress.
The flags --start_time
, --end_time
, and
--time_step
govern time in the simulation. If the layout file
specifies an automatic sun, these times should be expressed in Unix time
(seconds since the epoch at 00:00:00 UTC on 1 January 1970). If the layout
file specifies manual sun positions,
just set --end_time
to the index of the last position in the list
(that is, the length of the list minus 1) and leave --start_time
and --time_step
at their defaults (of 0 and 1 respectively).
--disable_field_masking
ignores all shadowing and blocking
effects within the field (but apertures still block). It can dramatically
increase the program's speed for a first-approximation simulation.
--heliostat_aiming_error
is a value in radians, with default
zero. At each time step, each heliostat's aim is set to a direction differing
from the ideal aim by a random amount drawn from a two-dimensional normal
distribution with this value of standard deviation.
--heliostat_facets_per_side
enables discrete convolution
of the mirror shape with the sun shape in order to produce a more
realistic reflection. The default value of 1 treats each heliostat as
a single infinitesimal facet producing a perfect reflection of the sun.
(It's infinitesimal only for the purpose of calculating the reflected image;
shadowing and blocking are always computed for the full area of the reflecting
surface.) Values of 4 or 5 have been found to produce fairly accurate images
for receiver resolutions of about 10 by 10.
The output of hops
is saved to text files formatted
for plotting with the pm3d
module in gnuplot
.
Outputs are enabled, and their filenames specified, using command-line flags
to hops
.
Each row of output has five columns, separated by spaces, with
"
as a quote character: The timestamp, x and y coordinates for
plotting the results, the value being output, and a string describing the value
(which should be the same for each row but is repeated for convenience).
A single blank line separates blocks of data with constant y coordinate
(this is needed by pm3d
), and two blank lines separate blocks
of data with constant time.
For heliostats' output, the x and y coordinates are each heliostat's x and y coordinates in the field.
--heliostat_flux_in
outputs flux in watts incident on each
heliostat surface.
--heliostat_irradiance_in
outputs irradiance in watts per
square meter incident on each heliostat surface.
--heliostat_shadowing
outputs percent of light traveling
towards each heliostat shadowed by other heliostats.
--heliostat_blocking
outputs the percent of light emitted by
each heliostat blocked by other optics (either heliostats or the aperture).
Note that this is not the conventional definition of blocking, which includes
only heliostats!
--heliostat_flux_on_target
outputs the flux in watts from
each heliostat that strikes the receiver surface.
--heliostat_efficiency
outputs the percent of flux incident
on each heliostat that that heliostat delivers to the receiver surface.
For receiver elements' output, the x and y coordinates are equal-area
projections defined in src/receiver_surfaces.cc
.
--aperture_flux_spill
outputs the flux in watts that passes
outside the aperture.
--receiver_flux
outputs the flux in watts incident on each
element of the receiver surface.
--receiver_irradiance
outputs the irradiance in watts per
square meter incident on each element of the receiver surface.
The script src/plot_results.sh
can be used to turn
output files into heat maps. It requires gnuplot
to be in
your PATH
. Invoke it using:
src/plot_results.sh OUTPUT_FILENAME
The results will be saved to .png files with names formatted as
OUTPUT_FILENAME_TIMESTAMP.png
.
If the output file to be plotted contains more than 5 time
steps and mencoder
is in your PATH
,
plot_results.sh
will assemble the resulting plots into a .avi
movie file using mencoder
.
Below are example plots of heliostat efficiency (percent
of flux incident on a heliostat actually delivered to the
receiver) and receiver irradiance for the configuration defined in
src/examples/curved_receiver_oblique_layout
. The heliostat
efficiency plot is a heat map of the heliostat field itself; the receiver
is located south of the field at coordinates (0,0).
These plots were produced by the following invocation
of hops
, with the resolution parameter in
src/examples/curved_receiver_oblique_layout
changed from
10 to 60 to give a more detailed plot of the receiver:
./hops --layout_file=src/examples/curved_receiver_oblique_layout \ --start_time=1321570800 --end_time=1321570800 \ --receiver_irradiance=receiver_irradiance \ --heliostat_efficiency=heliostat_efficiency src/plot_results.sh receiver_irradiance src/plot_results.sh heliostat_efficiency
Note that the dates displayed above the plots are converted from the
presumed Unix timestamps in the data file output by hops
. Thus,
in the case of a configuration file specifying manual sun positions, these
dates will be relative to the start of the Unix epoch and not otherwise
meaningful.
HOpS works by passing data structures representing packets of light
from one optical element to another. These IncidentLight
structures, defined in src/optic.h
, record the intensity and
direction of the light, as well as a blocking mask and a const
pointer to the source object. The sun object illuminates each heliostat,
and each heliostat illuminates each element of the receiver that's visible
to it.
The advantages to this approach are that it is completely deterministic, and for some configurations it can be a great deal faster than ray tracing. The runtime scales with the product of the number of heliostat facets and the number of receiver elements, so for a detailed picture of a single heliostat's image or flux-through-aperture for a large field of heliostats, this approach can be ten to a hundred times faster than ray tracing.
Shadowing (masking of sunlight incident on a heliostat) and blocking
(masking of light reflected by a heliostat) are calculated deterministically,
with the resulting masks represented as Polygons
objects (declared
in math/polygons.h
).
Because the shadowing and blocking masks for a given reflector (or facet) are known exactly, we intersect them to compute the total blocking mask, avoiding double-counting and giving us a precise measure of shadowing and blocking for every heliostat.
The image produced by any reflective surface can be determined by integrating over the surface: Each infinitesimal reflective element produces a perfect image of the source, and the resulting image is therefore a convolution.
We can approximate this convolution operation by dividing a heliostat's
reflector into discrete facets, each of which is treated as a perfect
infinitesimal reflector. This is enabled using the
--heliostat_facets_per_side
flag.
In our case, the source is always the sun, which we approximate as a regular dodecagon of the Sun's true size and distance from Earth, subtending an angular diameter of about half a degree or nine milliradians. For automatic sun positioning, the distance is determined exactly; for manual sun positioning it is assumed to be 1 AU.
For an in-depth look at the convolution, see the appendix.
The simulation operates on optical elements (the class Optic
).
An Optic
is a flat object with a polygonal shape (a
Polygon
structure or Polygons
object),
has a location and an orientation, and can receive packets of light
(IncidentLight
structures).
Optic
has four subclasses: Sun
,
Heliostat
, Aperture
, and
ReceiverElement
. Additionally, a Sun
object owns a SunCalculator
object, which determines the
Sun
's position in the sky either automatically (in the
case of the SOLPOS
subclass) or manually (in the case of
the SunPositionList
subclass). Each Heliostat
object owns a set of HeliostatFacet
objects which represent
a division of the reflector surface into finitely many facets, allowing
the simulation to produce more accurate solar images through discrete
convolution. To see this effect in action, set up a field with just
one heliostat and compare the receiver_flux
between the
default --heliostat_facets_per_side=1
and a more realistic
--heliostat_facets_per_side=5
.
These Optic
elements are owned by containers of class
OpticContainer
.
OpticContainer
has three subclasses: Sky
,
Field
, and Receiver
.
OpticContainer
objects are linked together
by OpticContainerConnection
objects. An
OpticContainerConnection
stores visibility information.
Suppose we have an OpticContainerConnection
that connects
OpticContainer
X to OpticContainer
Y. For each
Optic
pair (x, y), where x is in X and y is in Y, the
OpticContainerConnection
stores a list of Optic
objects in X that are capable of blocking, and a list of Optic
objects in Y that are capable of shadowing, the path from x to y.
OpticContainerConnection
is also the class responsible for
orchestrating the communication of IncidentLight
structures
from one OpticContainer
to another.
Here is a sketch of the relationships between these objects:
Solid arrows denote ownership. The dashed arrows represent the visibility
relationship between OpticContainer
objects encapsulated in
the OpticContainerConnection
objects.
Below is a partial class-level call graph for a Simulate()
step, illustrating the sequence of method calls. The Simulate()
method in the Simulation
object first calls the
UpdateSelf()
method in each of its OpticContainer
members, which in turn call UpdateSelf()
on their
Optic
members. These methods don't perform any optical
calculations; they simply clear the data the Optic
objects stored
at the previous timestep and allow the Sun
to move in the sky and
each Heliostat
to reorient itself to stay on target. Then
Simulation
calls the Simulate()
method in each of its
OpticContainerConnection
members. These objects recalculate their
cached visibility information if necessary, then pass light from each source
Optic
to each destination Optic
by calling
OutputIrradiance
on a source Optic
to calculate
output irradiance and store it in an IncidentLight
structure, followed by ReceiveIncidentLight
on a destination
Optic
.
OutputIrradiance
in turn calls TransferIrradiance
to
calculate the "transfer function" that converts each of an Optic
object's incoming IncidentLight
packets into an irradiance value
for an outgoing IncidentLight
packet. This is nonzero only
for Heliostat
objects, which use this method to compute the
sun's reflected image and combine this with their reflectivity, shadowing,
and blocking to produce an "irradiance on target" value.
HOpS proved to be a very useful tool for the RE<C project. By scripting it to run on a thousand machines in parallel, we were able to run comparative simulations of many different field configurations very quickly.
For example, at one point we wanted to compare the performance of four
different field layouts with three different receiver heights, three different
aperture diameters, and three different magnitudes of heliostat aiming error,
or 108 combinations in all. We simulated sixty days of real insolation data at
5-minute granularity, with 8970 time steps for each run. We needed to know
only the values of flux through the aperture (--receiver_flux
) and
flux spilled at the aperture (--aperture_flux_spill
), and so we
were able to use a single-element receiver (resolution
set to 1 in
the configuration files), allowing the simulation to run far faster than any
ray tracer could. Using one thousand machines, the whole experiment,
including plotting of the results, took less than two hours, or about 7.5
machine-seconds per time step. By comparison, the commercial ray tracer
LightTools, running on a modern desktop, takes about a minute per time step for
a similar simulation.
In testing HOpS during development, we compared its results to those
produced by LightTools. In our use cases, we found agreement to within one
part in a thousand with --heliostat_facets_per_side=5
.
Due to its design, HOpS' runtime scales with the product of the total number of heliostat facets and the number of receiver elements. Thus, it may take a long time to produce a detailed receiver flux map for a large field of heliostats.
In this appendix, we explore in depth the issue of imaging the sun in a canted curved reflector. This will provide a useful background for understanding how heliostats focus light and the limitations of their performance, as well as the convolution that HOpS uses to produce reflected images of the sun.
The effect we describe here is usually termed astigmatism, not to be confused with coma, which is a next-order optical aberration which becomes important only for optical systems in which the focal length of the reflector (or lens) is comparable to its width.
Imagine an ideal mirror with focal length f, where f is much larger than the width of the mirror. This means that parallel normal incident rays reflect to meet at a point A a distance f from the mirror surface. This is illustrated by the blue rays in the following diagram. (We shall use Greek letters for angles, capital Roman letters for points, and lower-case Roman letters for lengths.)
Here the focal point is A, and the mirror is BC (drawn as a flat surface because the curvature is assumed small). Assume WLOG that the rays strike at the edges of the mirror, a distance
apart.
But what if the rays are parallel to each other but not normal to the mirror? At what distance from the mirror do they intersect? Adding the new non-normal rays in red to the diagram above, we get:
Let the angle between the incident red rays and the vertical be α and the point of intersection of the reflected red rays be A′.
Let the angle between the left-hand reflected red ray and the line BC be
.Likewise we have
for the right-hand reflected ray. Then the angle at A′ is
,the same as the angle at A. Therefore the isosceles triangles ABC, A′B′C, and A′BC′ are all similar.
The distance from A′ to the mirror could be measured to one edge of the mirror or to the other, or to some point in between.  Let f′ be the height of a triangle similar to these two triangles whose base passes through O; we will define this to be the distance we seek.
 Let δ be the angle CBC′. Since A′BC′ is similar to ABC, it is clear that
and so
.Now we can calculate the length of the triangle bases B′C and BC′, and from there determine g and h.
Let
be the length of BF and
be the length of FC (which is the same as EB′). Then using the triangle CFC′, we can calculate the length of FC′ (and BE) to be
.Now we know that
and
.Therefore, by triangle similarity,
and
.Since O is the midpoint of BC, OO′ is midway between B′C and BC′. Hence the distance A′O′ is the mean of g and h. That is,
.The above derivation works for two dimensions, with a one-dimensional mirror surface. In three dimensions, with a two-dimensional mirror surface, there is one direction in the mirror plane in which the incident rays are normal and a direction orthogonal to that one in which they aren't. Therefore there are two focal lengths at work: the ordinary focal length f, and the astigmatic focal length f′. In one direction, the rays focus at distance f, and in the other direction, they focus at distance f′.
The parallel incident rays in the discussions above may be considered as coming from a distant point source. The image of this point source formed at a distance x from the mirror is a diagonal linear transformation (that is, a scaling-and-squeezing) of the mirror surface, as depicted in the diagram below. (The dotted lines should be centered within the dashed quadrilaterals, but perspective drawing is hard.)
The scale factor along the normal direction is
,and the scale factor along the astigmatic direction is
.A negative value for a scale factor means that the image is flipped in that axis.
The image of a source of finite extent (the sun, for example) is the locus of the images of all the rays from the source; that is, a convolution of the above transformation of the mirror's shape with the source's shape.
The extent of this image in either direction is therefore the width of a point reflection of the source (ie. its angular width φ times the distance of the image from the mirror) plus the width of the image of the mirror under the above linear transformation.
In particular, if the mirror has width dn in the normal direction and width da in the astigmatic direction, then the extent of the image in the normal direction is
,and the extent of the image in the astigmatic direction is
.The minimum total image spread is the isotropic case cn = ca, or
,which gives
and thus
.


New medical centre offering free ‘mole mapping’
by Staff WriterA NEW Perth medical centre is celebrating its opening by offering free ‘mole mapping’ to its first 100 skin check patients.
Floreat Forum General Practice was officially opened on Saturday.
And to celebrate the launch, the team is offering free mole mapping using their leading edge machine.
The head-to-toe check, valued at $200, provides a comprehensive scan of your skin allowing the doctors to thoroughly assess and diagnose suspicious spots and record any changes over time.
The new medical centre is family owned, offers bulk billing for all patients and extended operating hours, opening seven days a week, for both appointments and walk-ins.
The new facility has nine consulting rooms for doctors, a dedicated Clinipath pathology centre and a separate surgery room for minor medical procedures.
Floreat Forum General Practice is located in the centre of the main mall at Floreat Forum Shopping Centre, with convenient external access off the Floreat Avenue lane-way and a new internal entrance directly into the shopping mall opposite Lenard’s.
Floreat Forum General Practice operates Monday to Thursday, 8am-9pm, Friday, 8am-6pm and 9am-1pm on weekends.
The practice can be contacted on 9269 9029.


|
|
TwoLevelQueue< vid_t > | active_queue |
| |
|
ulong_t * | new_paths_curr |
| |
|
ulong_t * | new_paths_prev |
| |
|
int * | active |
| |
|
int | iteration_static |
| |
|
ulong_t * | num_paths_data |
| |
|
ulong_t ** | num_paths |
| |
|
ulong_t * | num_paths_curr |
| |
|
ulong_t * | num_paths_prev |
| |
|
double * | KC |
| |
|
double * | lower_bound |
| |
|
double * | upper_bound |
| |
|
double | alpha |
| |
|
double | alphaI |
| |
|
double | lower_bound_const |
| |
|
double | upper_bound_const |
| |
|
int | K |
| |
|
int | max_degree |
| |
|
int | iteration |
| |
|
int | max_iteration |
| |
|
int | num_active |
| |
|
int | num_prev_active |
| |
|
int | nV |
| |
|
bool * | is_active |
| |
|
double * | lower_bound_unsorted |
| |
|
double * | lower_bound_sorted |
| |
|
int * | vertex_array_unsorted |
| |
|
int * | vertex_array_sorted |
| |
The documentation for this struct was generated from the following file:
- /home/fbusata3/HornetAlg/include/Dynamic/KatzCentrality/Katz.cuh


This interactive visualization allows you to explore the contents of a dense array of values by viewing its slices and its 3 dimensional iso-surfaces.
Adjust the isosurface threshold value by moving the colored slider or by clicking on on the slice images.
Rotate the 3 dimensional views by dragging over the dot cloud.


Radio buttons
Reference by name
Do you want to see a smile?
Yes
No
:)
Radio button with an inital value
2+2=
4
6
So bad at math?


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--- layout: post title: Blogging with Emacs org-mode and Github Pages tagline: Blogging the way you should categories: computers tags: web org-mode emacs org blog github bitbucket git ---
Lately, I've become enamoured of writing things in text files and avoiding proprietary formats as much as possible, but I still like to be able to render the text into nicer formats for printing (PDF) or sharing (HTML). There are many lightweight mark-up languages that support this, markdown and friends, but I prefer Emacs org-mode for its power with including source code, literate programming, strong LaTeX support, and table editing.
Not surprisingly, org-mode
has a powerful publishing facility that,
when combined with Jekyll and GitHub, can produce pretty a pretty
reasonable blog with categories, tags, archives, and comments, all
separate from the content.
Because the source material in org-mode
can contain comments,
code-snippets you don't want published, or other content intended
for the author and collaborators, I keep the source separate from
the publishing location.
Although we won't use this content for a little while, it's important to make sure this works before getting too far. Also, the initial push of content to GitHub can take a little while to be recognized by GitHub, so this will give GitHub some time while we do other things.
To set up a username.github.io web page1 you need to get
a "blank" Jekyll set up and push it to GitHub. Later we'll
hard-code the local location of this repository in your .emacs
file, so you might as well choose a good location for it now. On
my MacOS computer, I have it in ~/Documents/
.
The following four commands
/username/.github.io
_config.yml
that you should edit and fill in the fields that need to be
filled in.
git clone https://github.com/plusjade/jekyll-bootstrap.git ${USER}.github.io cd ${USER}.github.io git remote set-url origin git@github.com:${USER}/${USER}.github.com.git (edit _config.yml) git push origin master
If you wait a little while and then go to http://username.github.io (replacing username with your GitHub user name) you'll see the default Jekyll pages. Don't worry, you'll replace them soon enough.
As mentioned, I like to keep my source files separate from the
published content, because org-mode
can selectively export
during the publishing step, but anyone can read a text file.
I keep my source content in another Git repository, although I
keep that one at BitBucket because they let me have private
repositories at no cost. You could also just keep them on your
harddrive as files, or in a local revision control system.
Anywhere that can be seen by Emacs as the same time as seeing the
Git repository username.github.io
will work.
For the sake of the examples below, I have all of the blog
postings in one directory (blog/
) and all of the images in an
images
directory in the blog
directory (blog/images/
).
As with the location of the cloned username.github.io
directory,
these paths will be hard-coded in your .emacs
file, so you
should choose a good location for them now.
Writing a blog posting is like writing any other document in
org-mode
(which is what makes it so great), but there are three
details to which you should pay attention.
Jekyll, which is the formatting engine at GitHub that turns your
the raw HTML from the org-mode
export into formatted web pages,
does not use Org's #TITLE:
, #DESCRIPTION:
, or other export
template fields, it uses its own. However, Org does share that and
you can reference those fields, by including things like { {
{title} } }
or { { {keywords} } }
(but without the extra space;
that's there to prevent expansion in my example)2. NB: This
expansion doesn't seem to work in Org-Move version 8. The options
are described in the Jekyll documentation and must be exported when
Org exports as HTML. At the top of this document is a block that
looks like:
#+BEGIN_HTML --- layout: page title: { { {title} } } tagline: Blogging the way you should categories: computers tags: web org-mode emacs org blog github bitbucket git --- #+END_HTML
The layout
field is worth looking at. It has two options: page
and post
. page
makes it a standard web page—there are no
dates, comments, or other sort of bloggy things. post
makes it a
more bloggy post, enabling comments if you have them enabled in
_config.yml
and adding a date near the top of the file and
Previous, Archive, Next buttons at the bottom of the page.
Once you have the Jekyll header (which, frankly, is a lot easier
to do than the preceding section merits), the rest of your
document is standard org-mode
paragraphs, sections, links,
embedded code, etc.
The layout on the GihHub site will take the first paragraph or section and put that in the index, saving the rest for the click-through; I think it looks nice to have a paragraph before the first section that your reader will see on the main page, instead of a table of contents or a section heading and the first part of the section.
The filename needs to be of the format
YYYY-MM-DD-the-actual-title
for accurate parsing by Jekyll.
The publishing template that will be in your .emacs
file will
move images around between your source content and the publishing
location. This can lead to some confusion between standard HTML
rendering, publishing to the Jekyll location, and LaTeX or other
export formats.
Jekyll can support images in its assets/
that are referenced in
the blog posts like
, but the
"root-ed" path doesn't work well with normal org-mode
exports.
While there are likely more elegant solutions, I set up different export options depending on the type of export. For example:
#+BEGIN_HTML  #+END_HTML #+BEGIN_LATEX \includegraphics[width=0.8\textwidth]{images/YYYY-MM-DD-picture-name.jpg} #+END_LATEX
Although the image file names don't need the YYYY-MM-DD
format
the same way, they help me keep things organized.
Other files you'd like to reference can also be put in the
/assets
directory.
With a written blog posting, you can remove the examples from
username.github.io/_posts
and leave the empty directory. It will
be re-populated when you publish your blog post.
org-mode
has a "publish" facility3 that is configured in
your .emacs
file in two sections, once for the rendered HTML and
one for the static content (usually images).
(require 'org-publish) (setq org-publish-project-alist '(("org-acaird" (name1) ;; Path to your org files. :base-directory "~/Documents/blog" (srcdir) :base-extension "org" (extension) ;; Path to your Jekyll project. :publishing-directory "~/Documents/acaird.github.io/_posts" (destination) :recursive t ;; this was for org-mode pre-version 8 ;;:publishing-function org-publish-org-to-html ;; this is for org-mode version 8 and on :publishing-function org-html-publish-to-html :headline-levels 4 :html-extension "html" :body-only t ;; Only export section between   (body-only) ) ("org-static-acaird" (name2) :base-directory "~/Documents/blog/images" (imgsrc) :base-extension "css\\|js\\|png\\|jpg\\|gif\\|pdf\\|mp3\\|ogg\\|swf\\|php" (imgext) :publishing-directory "~/Documents/acaird.github.io/assets" (imgdest) :recursive t :publishing-function org-publish-attachment) ("blog" :components ("org-acaird" "org-static-acaird")) (combo) ))
While this is mostly readable, there are a few things to point out that you might want to edit.
.org
files go
.org
, but
you can add to it following the pattern in line imgext if you
use files that end in .txt
or something else
.html
files will be written
on export
org-mode
)
blog
) to use for exporting
Once your .emacs
file has those lines in it and they are
evaluated, you can type C-c C-e
to bring up the export menu.
From the menu, choose X
and when prompted, enter the name
defined in line combo above.
That will export the HTML to the username.github.io/_posts
directory (as defined in line destination above) and copy the
images to the destination defined in line imgdest above.
Once the files are in the proper locations in the
username.github.io
directory, they need to be added to the
repository and pushed to GitHub for publishing.
To publish your newly created HTML files, go to your
username.github.io
directory and git add
and git commit
your
new files and git push
them to Github.
After waiting a few minutes for GitHub to process your file, you'll see the title and the first bit of text at http://username.github.io and clicking the title will show you the full post.
Jekyll supports themes to change the look of your blog pages. There are some sample themes at http://themes.jekyllbootstrap.com/ with installation instructions.
Jekyll themes are installed into your username.github.io
directory and repository and when it is pushed to GitHub, the
theme you have chosen is applied.
Jekyll uses rake
(Ruby mAKE) to install and manage themes;
rake
comes with MacOS and, likely, with Linux. For Windows you
might have to install Ruby.
To install the theme called the-minimum
from
http://themes.jekyllbootstrap.com/, follow these steps
cd
into your username.github.io
directory
rake theme:install
git
"https://github.com/jekyllbootstrap/theme-the-minimum.git"=
git commit -a
Jekyll can use Disqus to support blog comments. This is described
in the _config.yml
file in your username.github.io
directory.
At www.google.com/analytics you can set up an analytics page for
your github.io
pages; the end of the set-up results in a
tracking ID that is a 13 character (at least, mine is) string.
Add that string to the analytics:
section of _config.yml
and push the changes to GitHub. After a few days, if anyone looks
at your blog, you'll see some nice statistics at Google.
analytics : provider : google google : tracking_id : 'AA-12345678-9'
Most of this came from http://jekyllbootstrap.com
More documentation on this in org-mode
is at
http://orgmode.org/org.html#Macro-replacement
More on the org-mode
publishing is at
http://orgmode.org/worg/org-tutorials/org-publish-html-tutorial.html


Good_Witch
Cassie Nightingale, Middleton's favorite enchantress, and her young-teenage daughter Grace, who shares that same special intuition as her mom, welcome Dr. Sam Radford and his son to town. When the New York transplants move in next to the Grey House, they are immediately spellbound by the mother-daughter duo next door, but Sam and Cassie quickly find they may not see eye to eye. With her signature charm, Cassie attempts to bring everyone together, ensuring all of Middleton is in for new changes, big surprises and, of course, a little bit of magic!Based on the Good Witch series of cable movies.


{% extends "home/base.html" %} {% load static %} {% block content %}
Follow the 4 steps for uploading simulations.
For more information on this form, see the docs.


--- layout: default ---
Where Cooper County Youth Fairgrounds
16899 Dunkles Drive.
Boonville Mo. 65233
When March 30th 9:00am to 3:pm.
Free admission for buyers.
Sellers, tables are $7 non electric hookups, $10 electric hookup.
For info or to reserve table call Tom WA0E<PHONE_NUMBER>. Dwight
N0QOK<PHONE_NUMBER>
Talk in's on W0BRC 147.360+
HAMFESTS ARE FUN!
IF $ CAN'T BUY HAPPINESS, THEN EXPLAIN HAMFESTS


To use this feature, select Report | All Measurements. This feature allows you to review any measurement of any type. It functions the same way as the other report options except that you get a list of all the measurements.
More:
Batch Script Generation


Register the application for remote push notifications and handle registration request results.
Click to copy the blue snippets and then paste them into your code.#import "AppDelegate.h" @implementation AppDelegate - (BOOL)application:(UIApplication *)application didFinishLaunchingWithOptions:(NSDictionary *)launchOptions { UIUserNotificationType types = (UIUserNotificationTypeBadge | UIUserNotificationTypeSound | UIUserNotificationTypeAlert); UIUserNotificationSettings *mySettings = [UIUserNotificationSettings settingsForTypes:types categories:nil]; // In iOS 8, this is when the user receives a system prompt for notifications in your app [[UIApplication sharedApplication] registerUserNotificationSettings:mySettings]; [[UIApplication sharedApplication] registerForRemoteNotifications]; return YES; } - (void)application:(UIApplication *)application didRegisterForRemoteNotificationsWithDeviceToken:(NSData *)deviceToken { // We have our devide push token now. } - (void)application:(UIApplication *)application didFailToRegisterForRemoteNotificationsWithError:(NSError *)error { // Something went wrong and you better to look into error description. } @end


Add class content-scroll
in div, which has textarea child that has class n-textarea
. Also you can change the width and height of textarea by overriding class name ".content-scroll" if you
want as in following example.
<form role="form">

Scrolling text area
<textarea id="ta-scroll" class="n-textarea">TEXT TEXT TEXT TEXT TEXT TEXT TEXT</textarea>

</form>
// Change the textarea width and height if you want


Club Championship 2017 Event 1
| Hard 5 |
25 February 17 |
|
5 |
miles |
| Name |
Position |
Road bike |
Actual Time |
Avg. mph |
| |
|
|
|
|
| Matt
Plews |
1 |
|
00:17:11 |
17.46 |
| Hans van
Nierop |
2 |
|
00:17:47 |
16.87 |
| Lawrence
Cox |
3 |
|
00:18:33 |
16.17 |
| Peter
Bentley |
4 |
|
00:18:43 |
16.03 |
| Matt
Crabtree |
5 |
|
00:18:45 |
16.00 |
| Julian
Twynham |
6 |
|
00:19:00 |
15.79 |
| Isaac
Hudson |
7 |
1 |
00:19:37 |
15.29 |
| Luke
Marlow |
8 |
|
00:19:59 |
15.01 |
| Adrian
Killworth |
9 |
|
00:20:12 |
14.85 |
| Linda
Hubbard |
10 |
|
00:20:17 |
14.79 |
| Ed
Grandidge |
11 |
2 |
00:20:59 |
14.30 |
| Simon
Ward |
12 |
|
00:21:28 |
13.98 |
| Vic
Barnett |
13 |
3 |
00:21:53 |
13.71 |
| Carl
Roberts |
14 |
|
00:22:01 |
13.63 |
| Chris
Dainty |
15 |
4 |
00:22:07 |
13.56 |
| Jill
Postlethwaite |
16 |
5 |
00:22:16 |
13.47 |
| Stuart
Dawkins |
17 |
6 |
00:22:46 |
13.18 |
| Steven
Coulam |
18 |
|
00:22:48 |
13.16 |
| Dan High |
19 |
7 |
00:23:08 |
12.97 |
| Neville
Brooks |
20 |
|
00:24:07 |
12.44 |
| Jennifer
Clegg |
21 |
|
00:24:19 |
12.34 |
| Stewart
Holland |
22 |
8 |
00:24:48 |
12.10 |
| John
Welsford |
23 |
9 |
00:25:07 |
11.94 |
| John
Ridgway |
24 |
10 |
00:25:23 |
11.82 |
| Sophie
Alexander |
25 |
11 |
00:28:16 |
10.61 |
| Ben
Brant |
26 |
12 |
00:31:02 |
9.67 |
|
|
|
|
|


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Summoner Belthus
I've never fought anyone foolish enough to try to carry on a conversation during a battle. I guess I don't mind, but are you sure you are OK? It appears that my creature is getting the better of yours...? Oops! There he goes again!


Frisbee? Fun? Friends? We’ve got it all! La WUFA is Williams College’s ultimate frisbee team for female and non-binary students. In the fall, we welcome new team members, learn the beautiful game of Ultimate, and casually practice for our Spring season competing nationally at the USAU (USA Ultimate) DIII level. Interested in joining WUFA? No experience necessary! Fill out our interest form here, or email<EMAIL_ADDRESS>if you want to get in contact. Hope to see you soon out on the sunny, grassy fields of Poker Flats (or an equally exciting Zoom “field”)!


About
Simple realtime messaging system. Contains an API to send message through sockets, where clients can subscribe. It's lighter than Apache Kafka because we have simple needs here.
Links
Github repository: https://github.com/thefirstspine/messaging/
Service URL: https://messaging.thefirstspine.fr/


FLASH
check
/crossdomain.xml
any other site can perform two-way interaction
<allow-access-from domain="*" />
SILVERLIGHT
check
/clientaccesspolicy.xml
JAVA
Java same-origin policy is that other domains that share the IP address of the originating domain are considered to be same-origin under some circumstances.
HTML5 and XMLHTTPRequest
In response to the OPTIONS request, the server may use headers like the following to specify the types of cross-domain requests that are allowed:
Access-Control-Allow-Origin: http://wahh-app.com
Access-Control-Allow-Methods: POST, GET, OPTIONS
Access-Control-Allow-Headers: X-PINGOTHER
Access-Control-Max-Age: 1728000
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FROM DR SANI MUSTAPHA, THE MANAGER OF AUDIT AND ACCOUNTING DEPT, BANK OF AFRICA OUAGADOUGOU, BURKINA-FASO. DEAR FRIEND, I AM DR SANI MUSTAPHA. I WORK IN THE BANK OF AFRIC(B.O.A.),OUAGADOUGOU, BURKINA FASO.I HAVE A BUSINESS WHICH WILL BE BENEFICIAL TO BOTH OF US.  AND ALSO TO TAKE MY WIFE TO USA FOR TREATMENT OF LIVER DAMAGE. THIS MONEY WAS OWNED BY ONE OF THE CUSTOMERS IN OUR BANK.THE MAN'S NAME IS CALLED ANDREAS SCHRANNER FROM Munich,Germany.A BUSINESS COMMERCIALIST IN WEST-AFRICAN REGIONS.  BELOW IS THE( website http://news.bbc.co.uk/1/hi/world/europe/859479.stm) AND SINCE THEN,NO CLAIM HAS BEEN PLACED IN HIS BANK ACCOUNT BALANCE. I WANT TO TRANSFER THIS MONEY OUT OF THE COUNTRY BUT SUCH FUND CAN NOT BE TRANSFERRED WITHOUT A NEXT OF KIN ATTACHED TO THE FUND. THE FUND COULD BE TRANSFERRED IN THESE WAY;YOU SHALL PRESENT YOURSELF AS BUSINESS ASSOCIATES TO THE DECEASED PERSON[ANDREAS SCHRANNER] AS DETAILS SHALL BE THAT YOU ARE THE CARE-TAKER BUSINESS ASSOCIATES TO MR.ANDREAS SCHRANNER AND HIS PROPERTIES. I SHALL MAKE AVAILABLE TO YOU MATERIALS AND INFORMATION WITH WHICH A SUCCESSFUL CLAIM SHALL BE PLACED ON THE FUND. I SHALL BE YOUR GUIDIANCE AND INSTRUCTOR THROUGHOUT THE DURATION OF THIS TRANSACTION SO AS TO ENSURE A SWIFT AND SURE TRANSFER OF THE FUND TO YOUR BANK ACCOUNT.  BEST REGARDS, DR SANI MUSTAPHA, _________________________________________________________________ MSN Hotmail : créez votre adresse e-mail gratuite & à vie ! http://www.msn.fr/newhotmail/Default.asp?Ath=f


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In Alloy, "*bar" denoted the reflexive transitive closure of bar. It is equavalent to (iden + ^bar) where ^ is the (non-reflexive) transitive closure operator.


WEEK 25 THURSDAY
Year 1 (Year 2)
FIRST READING Haggai 1:1-8
“Build the house, that I may take pleasure in it.”
The beginning of the Book of the Prophet Haggai
In the second year of Darius the king, in the sixth month, on the first
day of the month, the word of the LORD came by Haggai the prophet to Zerubbabel the son of Shealtiel,
governor of Judah, and to Joshua the son of Jehozadak,
the high priest, "Thus says the LORD of hosts: This people say the time
has not yet come to rebuild the house of the LORD." Then the word of the
LORD came by Haggai the prophet, "Is it a time for you yourselves to dwell
in your panelled houses, while this house lies in ruins? Now therefore thus
says the LORD of hosts: Consider how you have fared.  "Thus says the LORD
of hosts: Consider how you have fared. Go up to the hills and bring wood and
build the house, that I may take pleasure in it and that I may appear in my
glory, says the LORD.
The word of the Lord
RESPONSORIAL PSALM Psalm 149:1-2.3-4.5-6a and 9bc (R. 4a)
R. The Lord takes delight in his people.
Sing a new song to the LORD, his praise in the assembly of the faithful.
Let
R. The Lord takes delight in his people.
Let them praise his name with dancing, and make music with timbrel and harp. For the LORD takes delight in his people;
he crowns the poor with salvation.
R. The Lord takes delight in his people.
Let the faithful exult in glory, and rejoice as they take their rest.
Let the praise of God be in their mouths. This is an honour
for all his faithful.
R. The Lord takes delight in his people.
FIRST READING Eccesiastes 1:2-11
“There is nothing new under the sun.”
A reading from the Book of Ecclesiastes
Vanity of vanities, says the Preacher, vanity of
vanities! All is vanity. What does man gain by all the toil at which he toils
under the sun? A generation goes, and a generation comes, but the earth remains
for ever. The sun rises and the sun goes down, and hastens to the place where
it rises. The wind blows to the south, and goes round to the north; round and
round goes the wind, and on its circuits the wind returns. All streams run to
the sea, but the sea is not full; to the place where the streams flow, there
they flow again.  What has
been is what will be, and what has been done is what will be done; and there is
nothing new under the sun. Is there a thing of which it is said, "See,
this is new"? It has been already, in the ages before us. There is no
remembrance of former things, nor will there be any
remembrance of later things yet to happen among those who come after.
The word of the Lord
RESPONSORIAL PSALM Psalm 90:3-4.5-6.12-13.14 and 17 (R. 1)
R. O Lord, you have been our refuge, from generation to generation.
You turn man back to dust, and say, 'Return, O
children of men.' To your eyes a thousand years are like yesterday, come and
gone, or like a watch in the night.
R. O Lord, you have been our refuge, from generation
to generation.
You sweep them away like a dream, like grass which
is fresh in the morning. In the morning it sprouts and is fresh; by evening it
withers and fades.
R. O Lord, you have been our refuge, from generation
to generation.
Then teach us to number our days,
that we may gain wisdom of heart. Turn back, O LORD! How long? Show pity
to your servants.
R. O Lord, you have been our refuge, from generation
to generation.
At dawn, fill us with your merciful love; we shall
exult and rejoice all our days. Let the favour of the Lord our God be upon us;
give success to the work of our hands. O give success
to the work of our hands.
R. O Lord, you have been our refuge, from generation
to generation.
R. Alleluia. I am the way, and the truth, and the life, says the Lord; no one comes to the Father, but by me. R. Alleluia.
GOSPEL Luke 9:7-9
“John I beheaded; but who is this about whom I hear such things?”
A reading from the holy Gospel according to Luke
At that time: Herod the tetrarch heard of all that was done by Jesus, and
he was perplexed, because it was said by some that John had been raised from
the dead, by some that Elijah had appeared, and by others that one of the old
prophets had risen. Herod said, "John I beheaded;
but who is this about whom I hear such things?" And he sought to see him.
The Gospel of the Lord


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