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1. Computing atmospheric absorption with AATM Bojan Nikolic web pages (r. 329)
... Bojan Nikolic web pages (r. 329) . ... Atmospheric Modelling for ALMA . This is also a very simple program (sharing some code with dispersive ) to compute the atmospheric absorption due to dry and wet components of the atmosphere. ... Invoking the help option: ./absorption --help Compute absorption by the atmosphere This program is part of AATM version 0.09 GPL license -- you have the right to the source code. ... Computing atmospheric absorption with AATM . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/alma/aatm-absorption.html -- 9.6 Кб -- 04.04.2016
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2. http://www.arcetri.astro.it/irlab/doc/library/recipes/bookcpdf/c4-0.pdf
Sample page from NUMERICAL RECIPES IN C: THE ART OF SCIENTIFIC COMPUTING (ISBN 0-521-43108-5) Copyright (C) 1988-1992 by Cambridge University Press.Programs Copyright (C) 1988-1992 by Numerical Recipes Software. ... Chapter 4. 4.0 Introduction Integration of Functions Numerical integration, which is also called quadrature, has a history extending back to the invention of calculus and before. ... Isaacson, E., and Keller, H.B. 1966, Analysis of Numerical Methods (New York: Wiley), Chapter 7. ...
[ Текст ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/recipes/bookcpdf/c4-0.pdf -- 46.8 Кб -- 23.03.2000
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3. Explanations for solar physics computing page
This document explains values, tables and other matters on solar physics computing pages. ... is040423.ete : SAHA-S tables, interpolation values: T, rho, X. Z is fixed at 0.02. See reference above. opal2005.etf : OPAL EOS, interpolation values: T, rho, X, Z. Downloaded from OPAL site , marked there as "2005", seems to be unpublished. opal2001.etf : OPAL EOS, interpolation values: T, rho, X, Z. Rogers F.J., Nayfonov A. Astrophys. ... The following values can be calculated: . ... dimensionless . ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/physics/phys-help.html -- 8.0 Кб -- 21.10.2009
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4. Computer Lab
... To introduce you to the Python programming language, and its Visual module (VPython), which allows 3D simulation. The computer labs are held in room BOZO 112, not in the usual physics lab. ... This lab will use the Python programming language. ... Click on the Windows button in the bottom left, select "Programs", then the "A-Z" list of programs. ... Later in the course you will need to write your own VPython programs for assessment - this lab is your chance to make sure you can do this. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/phys1101/ComputerLab/index.html -- 6.0 Кб -- 02.10.2012
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5. Cool Stars 10 - V. Kashyap and J. Drake: DEM Reconstructions
... Vinay Kashyap and Jeremy Drake . ... We describe a Markov-Chain Monte-Carlo process using a Metropolis algorithm to derive Differential Emission Measures (DEMs) and element abundances from EUV line fluxes. ... These 8 files all use the Ov applet. f1QFlRay.htm - Active Region Emission Measures, Feldman et al. abundances, Raymond ion balances . ... 154, The Tenth Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun , eds. R.A. Donahue & J.A. Bookbinder (San Francisco: ASP), 844 . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PINTofALE/papers/cs10_kashyav1/index.htm -- 7.1 Кб -- 02.10.2012
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6. Welcom to CONPAS workshop
... Dr. Ravil Nazirov is the head of the workshop, and Andrew Ananjev is the secretary of the workshop. ... The workshop is used to be held in the last decade of the month, preferably on Tuesdays. ... The next session will take place October 29, 1996 . ... There is "CONPAS" mailing list which you can join to discuss issues of problem solving and to be automatically notified of important dates and decisions with respect to the coming sessions. ... Secretary of the Workshop: Andrew Ananjev . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/CONPAS/Welcome.html -- 3.2 Кб -- 13.10.1997
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Еще в разделе: (Показать все результаты (>282) - www.iki.rssi.ru/ )

7. http://www.stsci.edu/documents/dhb/webvol2/c16_hspcalib.fm3.html
... Computing the true count rates for digital data. ... The following equation is used to find the count rate. x = ( raw counts / sample time ) . ... True count rates for digital data are corrected by using the first equation for a point source and the second for an extended source. a = ( y - pre_amp - darkrate ) / ( highvolt x pt_effic ) . ... True photocurrents (count rates for analog data) are corrected by the first equation for point sources and the second equation for extended sources. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/webvol2/c16_hspcalib.fm3.html -- 7.2 Кб -- 10.02.1998
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8. Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/kearnsk.html -- 12.3 Кб -- 03.11.2000
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9. BTA
. This is BTA "indome" main server computer tb.sao.ru . It is local address in SAO's Intranet. But it is visible from Internet through our Web-site proxy as: http://www.sao.ru/tb/ . BTA TSC online Web-pages located here: http://www.sao.ru/tb/tcs/ . BTA WebCameras: . "In-Dome" TV-camera . and it's last images . "Outdor" TV-camera . and it's last images . Also, one can find here some documents: .
[ Сохраненная копия ]  Ссылки http://www.sao.ru/tb/ -- 3.8 Кб -- 10.12.2010
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10. Computers
MOSCOW CENTER . ... We use servers based on the Intel PC architecture with Linux and FreeBSD as operating systems. The computers in the computer room are Toshiba Satellite notebooks that can boot either into Linux (and used as Unix X workstations) or into Windows. Hours of operation Monday 3:00pm--9:30pm Tuesday 3:00pm--9:30pm Wednesday 3:00pm--9:30pm Thursday 3:00pm--9:30pm Friday 3:00pm--9:30pm . If you see any errors on this page, please write us <compwww (at) mccme.ru> ...