... I got all my tests for check_over to pass and moved on to writing the first test for do_kernel_square. ... I got all the tests working again and modified the pixmap code to create a float array instead of a double and use a half pixel grid. ... I got all the test cases to run and then modified the cdrizzlebox code to be zero based instead of one based. ... Dobox is the top of the hierarchy of code that needs to be tested for errors after rewriting map_value. ... And I got the tests to work again. ...

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• Archive for January
• RPS2 Demonstration
• Archive for February

This page was created by the IDL library routine mk_html_help . ... mk_html_help . at the IDL command line prompt. ... to calculate CHIANTI line intensities and continua, to create a synthetic spectrum. ... WRITTEN : Ver.1, 7-Nov-01, Giulio Del Zanna (GDZ) and Peter Young (PRY) MODIFICATION HISTORY: V.2, 7-Nov-01, GDZ . Fixed a small bug (now the spectrum plot is always plotted within the widget), and modified the option to add continua. ... Added extended details in the ascii output spectrum. ...

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• ...no longer exists.
• FIRPO Help 5

... The call to OMDETECT is changed in accordance with the new interface of OMDETECT (a few parameters have been removed) PARAM- file is set to OMDETECT-4.1 Version 1.22.9 -2002-05-29 ( VNY ) (+doc/omfchain_description.tex) documentation has been updated Version 1.22.8 -2002-05-27 (+src/omfchain.pl) The code for extraction of the ... Changed dependancy file to omfastshift 1.4 Version 1.2: 9 Oct 1998 Updated 'event-frame' locating algorithm in omfasttest.f90 and omfastshift. ...

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• http://xmm.vilspa.esa.es/sas/6.1.0/doc/rgsimplot/ChangeLog
• http://xmm.vilspa.esa.es/sas/5.4.1/doc/rgsimplot/ChangeLog
• http://xmm.vilspa.esa.es/sas/6.1.0/doc/omfchain/ChangeLog

... the radiative transfer equation (RTE) for the randomly-irregular magnetized plasma has been derived on the base of general grounds of the multiple scattering theory . ... Solutions of several absolute tasks of the scattering theory have been obtained (on the optical depth of the ionospheric plasma layer, on the value of radio wave anomalous attenuation, on anomalous refraction, on the backscattered signal intensity for the source being placed within a plasma layer). ...

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The two main numerical libraries in Fortran 90 are . NAG Numerical Libraries for Fortran 90 Users . IMSL Fortran 90 MP Library Both of these offer both a modified version of the Fortran 77 library, recompiled for Fortran 90, and a completely new library, using all the new facilities of Fortran 90. ... On the Sun using Sun OS 4.2.1 we also got completely wrong results when using library functions in single precision, since the C system on Sun converted all function calls into double precision. ...

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• Work notes
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• Fortran and Pascal

... 18sep08: bias for 3a/3b changed. Look at p2030 data (polA,polB summed) . 21sep08: bias for all beams changed. ... The wapps in 3 level mode take 100 MHz bw with 64usec sampling and 256 lags. alfa is centred at 1440 Mhz with the 100 Mhz 1390-1490 filter int. The total power was computed and then averaged to .1 seconds. ... Beam 6b is dead and p2030 is adding polA + polB. ... The a2010 data taken on 21sep08 was analyzed to check the stability of all the beams after the bias changes in alfa. ...

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• encoderOffsets
• datataking_software
• problems adjpwr with large birdies

... The MIDAS release 95NOV is the 10th official release of portable MIDAS. A number of new applications have been added to this version. ... After one year of working with the GNATS problem report database, new PR categories have been created, in particular for GUIs and for each context. ... Documentation for the EMMI calibration is provided with the command INITIALIZE/EMMI. ... For a more complete list of all updates/additions use the MIDAS command HELP [NEWS] after having installed this release. ...

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• The Modified Gauss--Newton Method.
• Interactive Editing of Tables
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. Other Relevant Links . Number counts have been illustrated earlier in the talk. QSO Clustering and Large-Scale Structure , Scott Croom et al . QSO Evolution and the Luminosity Function , B.J. Boyle et al . | Front page | . | << - Contamination | QSO close pairs - >> | . Robert J. Smith, ">rsmith@mso.anu.edu.au Last modified: Fri Sep 24 11:39:02 EST 1999 .

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• Dunk Proceedings - 2dF QSO Redshift Survey (Contamination)
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... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... For example, modified Newtonian dynamics (MOND) has no relativistic extension, and so makes no firm lensing predictions, but galaxy-galaxy lensing data can be used to empirically constrain the deflection law of a MONDian point-mass. ...

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• difx:startcorr.pl [ATNF VLBI Wiki]
• lbaops:tidnotes:fileprep [ATNF VLBI Wiki]
• VLBI Wiki | TidNotes / FilePrep

Next: Checking for disk errors Up: Filesystems Previous: Mounting and unmounting . ... A filesystem's correctness and validity can be checked using the fsck љ command. ... This allows e2fsck љ (the version of fsck љ for the ext2 filesystem) to avoid checking the filesystem if the flag indicates that the unmount was done (the assumption being that a proper unmount indicates no problems). ... Use fsck љ manually to check other filesystems, e.g., floppies. ...

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• Filesystems galore
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... In the western literature this method is now called ``coupled dipole method" (CDM). ... Thus, a system of equations relative to the fields scattered by the elementary domains can be obtained, and summation of these fields gives the total scattering field. ... A subtle difference between both methods is in the fact that in the first method one works with the fields which excite a dipole (without the field of the dipole), whereas in the second method one uses the real fields in a given domain. ...

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• Spherical particles
• Generalizations of the RDG approximation
• Cylinders

Stellarium 0.12.3 . ... Classes . ... ClassљList . ... SatellitesListModel Class Reference . A model encapsulating a satellite list. ... Tell the model that its internal data structure is about to be modified. ... Tell the model that its internal data has been modified. ... The model keeps a pointer to the satellite list, not a copy, so every time that list is modified outside the model (i.e. satellites are added or removed), you need to call beginSatellitesChange() and endSatellitesChange() . ...

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• Stellarium: File and Directory Structure
• Stellarium: /home/aw/devel/stellarium/trunk/doc/fileStructure.doxygen Source

XmCCD Copyright 2007-2013 John Kielkopf ======================================= Development Log =============== March 9, 2002 Version 1.0.0 * Support for SBIG cameras using the first public SBIG library * Basic panel for operation with ds9 +--------------------------+ May 22, 2002 Version 1.1.0 * Updated to use libudrv 4.35 +--------------------------+ May 24, 2004 Version 1.2.0 * USB support +--------------------------+ March 1, 2005 ...

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• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/CHANGELOG
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.2/CHANGELOG
• http://www.astro.louisville.edu/software/sbig/xmccd-5.1/CHANGELOG

. Next: Fonts used in the Up: General information Previous: About Contents . This is not only a manual on how to use the software, but a reference as well on how the procedures work. Study of the Programmer's reference sections should enable you to write and add your own procedures to the software, or create modified copies of existing routines which replace the latter if they are compiled during a session. Christian Hummel 2015-04-28

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• HISTORY moveProducts
• Migration to the SL6.3 System
• QA rules: DFS commissioning kick-off

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... A most promising problem is to investigate the interaction of two VHF powerful radiowave beams in the ionosphere, whose difference frequency is equal to the plasma frequency in some ionospheric area (that is, the difference frequency is taken in the range 1-8 MHz). ... Two-frequency interaction effects are based on radiowave non-linear mixing, which is rather complicated when describing and modelling the experiment. ...

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• East Siberian Center of Earth Ionosphere Research. Chirp ionosonde.
• East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
• Ionogram path coding structure

... His early works dealt with statistical methods especially in atmospheric, geomagnetic and ionospheric tides. In 1928, Bartels became professor in Eberswalde; in 1936, he became director of the Potsdam Geophysical Institute and full professor at Berlin university. ... With these statistical methods, he was able to disprove many widely accepted geophysical models on the one hand and develop some very useful and easy to apply geophysical indices on the other. ...

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• Geomagnetic Indices Kp, ap, Ap, Cp and C9
• New Mirrors
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Make a copy of your shell start up file before editing it to change environment or shell variables. You can always return to using this copy if you find that the modified file is not working and you are unable to fix the problem. For example: cd cp .profile old_profile ue .profile . The first command changes you to your home directory, where a copy of the file .profile is made in old_profile . ... To revert to using the original .profile you simply copy it back. ...

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• Problems linking files
• Did You Know?
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MAIN CHARACTERISTICS BASIC MODIFICATIONS TEST RESULTS . ... integrated drop tests in order to verify the strength of DM modified shell and equipment attachment points, functional check of new chairs and DM structure, determination of shock impacts onto the crew to verify landing safety; . ... nominal landing with the main parachute system (MPS) - drop #1 took place on December 24, 1998; . ... reduction of shock g-loads values at landing in accordance with decrease of landing speeds. MAIN | ...

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• S.P. Korolev RSC Energia - International Space Station
• S.P.Korolev RSC Energia - MARTIAN MISSION
• RSC "Energia" - History

chandra_acis_ao9.par ; generate an ACIS spectrum for a source using a DEM , ; and optionally rescale the DEM to produce the same ; counts as a ROSAT / PSPC observation ; ;calling sequence ; .run initale ; @chandra_acis_ao9.par ; ;(LL/VK; modified from chandra_acis_ao5.par, Feb04) ;(LL ... density [cm^-3] T_components = [6.9, 7.4] ;log(T[K]) components in the EM EM_components = [5.1d12, 6.1d12] ;Emission Measure [cm^-3] obs_rate = 0.1 ; ROSAT / ...

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• http://hea-www.harvard.edu/PINTofALE/ardb/chandra_acis_ao7.par
• The Chandra Multiwavelength Project (ChaMP)
• The AstroStat Slog Blog Archive working together to tackle hard problems in

... E-mail: ladyn@issp.ac.ru . ... N.V. Demeneva, S.I. Bredikhin, A.I. Ivanov, D.V. Matveev, V.V. Kharton, Gold medal of the XIX Moscow international Innovation technologies and inventions salon "Archimed-2016" for the project "Contact electrode material for solid oxide fuel cell bataries and its preparation process" . ... H.В. Деменева, С.И. Бредихин 'Формирование оксидных пленок и диффузионные процессы в приповерхностных слоях' Электрохимия, том 50, ?8, 808-813 (2014) ... top . ...

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• Institutes of Chernogolovka
• Astronomy: Olympiad of Scientific Centres: Institutes of Chernogolovka
• II-VI compound crystal growth, HPVB & HPVZM basics