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http://xmm.vilspa.esa.es/sas/8.0.0/doc/ssclib/node119.html.
http://xmm.vilspa.esa.es/sas/8.0.0/doc/ssclib/node119.html.
1. Generating a set of points along an ellipse locus
... subroutine calcEllipseFromAngle(xSemi, ySemi, angleDeg, xVals, yVals) real(single), intent(in) :: xSemi, ySemi, angleDeg real(single), intent(out) :: xVals(:), yVals(size(xVals)) end subroutine calcEllipseFromAngle . ... The subroutine returns points evenly distributed in . ... subroutine calcEllipseFromPhase(xAmp, yAmp, phase, xVals, yVals) real(single), intent(in) :: xAmp, yAmp, phase real(single), intent(out) :: xVals(:), yVals(size(xVals)) end subroutine calcEllipseFromPhase . ...
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Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/doc/ssclib/node119.html -- 5.0 Кб -- 15.08.2005
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2. Tools - Random numbers
... Tools . ... In order to generate random numbers that follow a normal distribution, one first needs to create two uniform random numbers $u_{1}$ and $u_{2}$, in the range of 0 to 1. ... begin{equation*} g_{1} = \sqrt{-2 \ln(u_{1})} \cos(2 \pi u_{2}) \end{equation*} . ... Random numbers following a power law, $P(x) \propto x^{n}$, can be generated from a single uniform random number, $u$, in the range of 0 to 1 through the following transform : . ...
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Ссылки http://www.atnf.csiro.au/people/Tobias.Westmeier/tools_random_numbers.php -- 6.2 Кб -- 10.04.2016
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3. The AstroStat Slog Blog Archive chi-square distribution [Eqn]
... Archives . ... Reduced and Processed Data . ... 2 distribution plays an incredibly important role in astronomical data analysis, but it is pretty much a black box to most astronomers. ... Comment ( RSS ) | ... I guess in the typical analysis we call chi2 a ?random variable? that follows the chi2 distribution: . ... where D(i) is the observed data, M(i) is the model predicted data and we ?silently? assume that D(i) is normally distributed and each i measurement is independent. ... Chandra Blog . ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2008/eotw-chisq-distribution/index.html -- 23.3 Кб -- 01.03.2014
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4. Simulations of Pinhole Imaging for AXAF: Distributed Processing Using the MPI
... The pinhole simulation program is a computationally and memory intensive task. ... A parallel version was developed instead, to enable distributed processing on a cluster of workstations. The program makes use of the Message Passing Interface (MPI) standard for parallel processing, implemented as an API (Application Programming Interface) to the Local Area Multicomputer (LAM) programming environment developed at the Ohio Supercomputer Center. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/nguyend.html -- 11.5 Кб -- 03.11.2000
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5. Procedure to be followed by DMD secretary for DFS Group documentation
Procedure to be followed by DMD secretary for DFS Group documentation . Initial email comes from author requesting document number. ... An email is then sent by the DMD secretary to the Technical Archive (tecarch@eso.org) with the same information, to request the last 4 digits of the document number (the 'chronological number'). ... Some time will pass and then the author, using the DFS Group tool 'WebCheck', will post a web readable version of the document on the DFS Group website. ...
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Ссылки http://www.eso.org/projects/dfs/team/DMD_Archive_procedure_notes.html -- 9.2 Кб -- 21.01.2002
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6. Monitoring Options
... Statistic files are managed using file generation sets and scripts in the ./scripts directory of this distribution. ... Each valid update appends a line of the following form to the current element of a file generation set named peerstats : . ... This keyword allows the (otherwise constant) filegen filename prefix to be modified for file generation sets, which is useful for handling statistics logs. filegen name [ file filename ] [ type typename ] [ flag flagval ] [ link | ...
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Ссылки http://www.sai.msu.su/~er/xntp/monopt.html -- 9.3 Кб -- 21.12.2007
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7. Specification
Symbolic circuit-matrix processor and evaluator . ... This software is reliable over the range of benchmark circuit complexity (both *.CIR and *.MAT file). ... SYMBOL is a symbolic-algebra package which in contrast to REDUCE, MACSYMA, MAPLE, MATHEMATICA, MathLAB, MathCAD and other known multi-purpose systems is especially intended for analysis of any lumped, linear, time-invariant circuit. ... pure ASCII text . ... CIRSYM - SYMbolic CIRcuit processor used to format ASCII text file *.out for CALCSYM. ...
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Ссылки http://astrometric.sai.msu.ru/~symbol/specification.html -- 11.5 Кб -- 06.10.2004
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8. Distributed Unconsciousness (DU) - an Astronomy Net God Science Forum Message
God Science Forum Message . ... God and Science ћ SETI ћ Software ћ UFO ћ XEphem . ... God and Science | ... Distributed Unconsciousness (DU) . ... Posted by Michael Trout on May 2, 2006 09:10:07 UTC . ... Link: - h0riz0ndu - May 3, 2006 - 04:54 UTC . ... Consciousness? - imback - June 12, 2006 - 05:02 UTC . ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
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Ссылки http://www.astronomy.net/forums/god/messages/32271.shtml -- 14.5 Кб -- 09.04.2016
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9. http://www.stsci.edu/ops/swat/safing/12358/seventh-healthandsafety-start.txt
Date: Sun, 23 Dec 2012 16:55:13 -0500 From: Bill Workman Cc: Bill Workman Subject: Fwd: SCI Flash Report: H&S SMS Successfully Intercepted following SWSP Safemode Recovery Activities For those of you not on the flash distribution, the 12 hour H&S SMS began executing at 358/21:00:00 UT (4pm EST) as planned. ... The Science recovery schedule is built and SMS generation/review is underway as I write. ... The Science Recovery SMS start time is 359/09:00:00 UT. ... EST). ...
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Ссылки http://www.stsci.edu/ops/swat/safing/12358/seventh-healthandsafety-start.txt -- 3.4 Кб -- 31.12.2012
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10. DUST: Dust::CarbSD Class Reference
... Classes . Files . Class List . Class Hierarchy . Class Members . Dust :: CarbSD . include < sizedist.hxx > . Collaboration diagram for Dust::CarbSD: . ... List of all members. CarbSD ( dust_sdpars &sdpars) . double . operator() (double a) . A class representation of the size distribution of carbonaceous grains . The documentation for this class was generated from the following files: . ... Generated on Fri Jul 11 07:32:09 2008 for DUST by 1.5.5 ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/devman/dust/classDust_1_1CarbSD.html -- 4.6 Кб -- 11.07.2008
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11. http://star.arm.ac.uk/~ambn/abstract240.html
We have modelled the spectral energy distribution of the carbon-rich star UU~Aurigae, which shows an excess flux in the far infrared and sub-millimeter regions, in terms of a detached shell generated by an episode of higher (than the current) mass loss rate. Two different compositions for the detached shell were used: oxygen-rich and carbon-rich dust grains. ...
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Ссылки http://star.arm.ac.uk/~ambn/abstract240.html -- 2.1 Кб -- 04.12.1996
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12. http://www.gao.spb.ru/english/personal/malkin/publ/zm08g.pdf
... Between them, the following points are touched: ICRF-2 structure, ICRF Core sources selection, and some expected user's requirements. ... Suggested total number of sources is close to the number of sources already observed in the IVS and VCS sessions, and for most of them reliable positions are derived, mostly for declination > -40 deg. ... So, results of source position time series analysis heavily depend on method used for time series computation and should be used with care. ...
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Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm08g.pdf -- 2058.3 Кб -- 27.10.2008
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13. Format Documentation of kpyymm.tab Files
The most recent kpyymm.tab (yymm stands for year and month, each expressed with two digits) files are distributed per e-mail half-monthly by Dr. H.-J. Linthe, mailto:kp_index@gfz-potsdam.de Both recent and past tables are supplied as an archive on the FTP servers . ... Since many observatories are interested mainly in the international quietest and most disturbed days, beginning August 1996 three extra lines have been added to the end of the table containing these values in an easy to read form. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/KP_INDEX/tab_fmt.html -- 5.7 Кб -- 21.12.2007
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14. Space Telescope-European Coordinating Facility
... The European HST Archive has been moved to ESA's European Space Astronomy Centre ( ESAC ), Spain, where most of ESA's Space Science Archives are located and operated from. ... The Space Telescope European Coordinating Facility (ST-ECF), jointly operated by ESA and the European Southern Observatory ( ESO ) was, until the end of 2010, the European HST science facility, supporting the European astronomy community in exploiting the research opportunities provided by the Hubble Space Telescope. ...
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15. Image: The procedure is as follows: put a coin into special box, pull a cord
. Album : Фотоальбом Сергея Аюкова :: Travels to distant places and countries :: 1997/08 Japan (Kyoto, Nara) :: 17/08 Kyoto streets. Maruyama park . Up . << Prev . The procedure is as follows: put a coin into special box, pull a cord (the bells will chime), clap hands and bow. Don't forget to tell god about your wishes. You see the woman at the left in the end of the prayer. Next >> . Photo album generated by album from Dave's MarginalHacks on Wed Jun 5 20:38:35 2013 .
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Ссылки http://crydee.sai.msu.ru/album/trips/1997.08.Japan/17.Maruyama/tn/a24l.jpg.index.html -- 5.6 Кб -- 05.06.2013
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16. How do neutron stars generate steady magnetic fields? | Astronomy.com
... Tonight's Sky . ... Observing . ... Sky this Month . ... Star Atlas . ... stars . ... Observing Podcasts . ... Astronomy for Kids . ... Observing springtime deep-sky objects with a large telescope . ... How do neutron stars generate steady magnetic fields? ... How can a neutron star exist if those neutrons are just going to pieces? Get instant access to subscriber content on Astronomy.com! ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...
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Ссылки http://www.astronomy.com/magazine/ask-astro/2007/02/how-do-neutron-stars-generate-steady-magnetic-fields -- 62.8 Кб -- 10.04.2016
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17. Ionospheric plasma-wave interaction
. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere and radiowave propagation: structure . The main page . Information . Publications: . 2011 - 2015 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2000 - 2004 . 1995 - 1999 . Participation in International symposiums and conferences: . 2013 - 2015 . 2011 - 2012 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2002 - 2004 . N.V. Pushkov . 09/04/2016 23:52 MSK . webmaster@izmiran.ru .
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Ссылки http://www.izmiran.rssi.ru/ionosphere/satellite_inv/plasma.shtml -- 9.4 Кб -- 09.04.2016
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18. Chapter 30. Acknowledgements
Chapter 30. Acknowledgements . ... These carry the following copyright notice: . ... This software was developed by the Computer Systems Engineering group at Lawrence Berkeley Laboratory under DARPA contract BG 91-66 and contributed to Berkeley. ... All advertising materials mentioning features or use of this software must display the following acknowledgement: This product includes software developed by the University of California, Berkeley and its contributors. ...
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Ссылки http://www.naic.edu/~phil/hardware/nvidia/doc/driverInstall/chapter-30.html -- 6.2 Кб -- 30.10.2009
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19. Nonequilibrium distributions
Results on nonequilibrium distributions of charged particles and radioisotope sources of current are as the following: . the new power-law distribution of charged particles in nonequilibrium media, for example, in the thin metalic films, under powerful energy source pumping were obtained ( together with V.I.Karas, V.M.Kontoriovich, V.E.Novikov); . ...
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Ссылки http://www.iki.rssi.ru/mss04/s5.htm -- 2.8 Кб -- 04.03.2004
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/mss04/s5.htm -- 2.8 Кб -- 04.03.2004
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/mss04/s5.htm -- 2.8 Кб -- 04.03.2004
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20. Following a rainbow back to the Big Bang | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Space Flight . ... Some 13.7 billion years ago, a mere millionth of a second after the Big Bang, the first hydrogen and helium nuclei condensed out of a hot, dense soup of quarks and gluons. ... In the very last few kilometres some of the light was scattered by a myriad of water droplets (containing hydrogen nuclei which had existed almost since the Big Bang) slowly descending through the air following a rainshower. ...
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Ссылки http://www.armaghplanet.com/blog/following-a-rainbow-back-to-the-big-bang.html -- 42.2 Кб -- 09.04.2016
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