... The accuracy of calculation of both INTERBALL spacecraft (SC) motion has been estimated at the IKI. ... The 30 days measuring intervals were used during the Tail probe (TP) orbital data treatment, and 15 days intervals - during the Auroral probe (AP) orbit determination. ... http://www.iki.rssi.ru/vprokhor/indap.htm for the Auroral probe; . http://www.iki.rssi.ru/vprokhor/indtp.htm for the Tail probe . ... http://www.iki.rssi.ru/vprokhor/ssc.htm , or http://www.iki.rssi.ru/vprokhor/amisan.htm . ...

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... Classes . Files . ... File List . File Members . measures . ... It is a simple 00060 // container with the selected method, and the mean epoch . br 00061 // The method is selected from one of the following: 00062 // ul 00063 // li Aberration ::STANDARD (at 1995/09/04 the IAU1980 definition) 00064 // li Aberration ::NONE 00065 // li Aberration ::B1950 00066 // /ul 00067 // Epochs can be specified as the MJD (with defined constants MeasData::MJD2000 00068 // and MeasData ...

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• Modifying Images by Models
• casacore: measures/Measures/SolarPos.h Source File
• VLBI Wiki | Main / ActionsLBA-Ops-2013

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

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• AI SPbU library of scattering codes
• Database of Optical Properties -- Level: subsubpage

... New offset/filter box. A new filter/box is available. ... It is lighter, smaller and sturdier than the filter/clock and offset boxes used till now. ... The offset is stabilized to a few parts in a million. ... Notice that only positions 0-3 are meaningful, while values of 4 and above will leave the signal unfiltered. The box has one input BNC, and two output BNC: one outputs the signal with the same polarity as the input, the other reverses the signal (remember that FIRPO has negative output). ...

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• FIRPO Help 5
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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

XMM-Newton Science Analysis System . ... CORR_RATE - The count rate after the following corrections have been applied; . 1) A further point-spread function correction may be applied, to extrapolate the counts from 12 to 35 pixels (presently only done for UV observations) 2) Correction for dead-time. 3) Correction for the OM sensitivity-degradation. A key-word TDS_CORR is added to the table to record the correction value. ... XMM-Newton SOC/SSC -- 2007-07-09 ...

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• Modification of Source-axes position angles
• Input Files

This module provides for the generation of Expires HTTP headers according to user-specified criteria. ... This module controls the setting of the Expires HTTP header in server responses. The expiration date can set to be relative to either the time the source file was last modified, or to the time of the client access. ... ExpiresByType . ExpiresDefault . The ExpiresDefault and ExpiresByType directives can also be defined in a more readable syntax of the form: . ... Module: mod_expires . ...

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• Apache module mod_log_forensic
• Apache's Handler Use
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... Directives | ... Apache HTTP Server Version 2.2 . ... This module controls the setting of the Expires HTTP header and the max-age directive of the Cache-Control HTTP header in server responses. The expiration date can set to be relative to either the time the source file was last modified, or to the time of the client access. ... access . ... If set to On , the headers will be added to served documents according to the criteria defined by the ExpiresByType and ExpiresDefault directives ( q.v. ). ...

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• Apache's Handler Use - Apache HTTP Server
• NVSS radio survey
• Software Modifications

The SAOtng graphical user interface is written in TCL using the NOAO widget server . A copy of the GUI specification is maintained in a file named saotng.gui , available in the SAOtng bin directory. If you are familiar with TCL, you can modify this file to create a new GUI and use it as your SAOtng interface. ... But if you create a modified version of saotng.gui, use: make crunch in the SAOtng directory to create the crunch.gui file. ...

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• *tprint* - Reading a Table File Created by imcnts

Astrophotography Forum Message . Forums: . ... Post . ... Modifying An Acuter Digitial Imager . ... Post Message | ... I just purchased an acuter digital imager, I read some where that you can take out the built 10mm lens. ... Acuter digital imager - erichollifield - November 8, 2004 - 02:40 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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• Rini Modified PlЖssl - MPL Eyepieces, care of Paul Rini, AstroGuide Listing
• The Hinge Mount - an Astronomy Net Astrophotography Forum Message

Geomagnetic disturbances can be monitored by ground-based magnetic observatories recording the three magnetic field components. The global Kp index is obtained as the mean value of the disturbance levels in the two horizontal field components, observed at 13 selected, subauroral stations . ... Geomagnetic activity is the occurrence of K variations. ... But K still remains a local index, describing disturbances in the vicinity of each observatory. ...

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• Geomagnetic Indices Kp, ap, Ap, Cp and C9
• Format Documentation of *.wdc Files
• Format Documentation of kpyymm.tab Files

. This pagee is under construction and we would appreciate your comments. Last Modified: April 18, 1996 . Tapasi Ghosh /

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• pulsedPwrIntoAlfa
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• Simulations of 3 ALFA Surveys

... Start and end times (of the observation, or of the integration for a given group). Exposure time per pixel (i.e., the integration time which contributes to the counts in each pixel), for the whole observation, or a given group. ... The determination of FOS start and stop times from header information is limited to an accuracy of +0.125 to -0.255 seconds (see Chapter 32). ... FPKTTIME 2 - group_elapsed_time . ... Group exposure time per pixel . ... start time = FPKTTIMEgroup - elapsed time group . ...

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• http://www.stsci.edu/spst/lrpg/documentation/unix_migration/mupid/task-dataaccess-usecase.html
• Beginner's IDL - Line Plots
• Python: module move_it

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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• Specifications
• Dynamic HTML in Communicator
• Fortran 90 for the Fortran 77 Programmer

... Bojan Nikolic web pages (r. 329) . Understanding Infrared emission from galaxies . This page contains a description and links for download of software that may be used for modelling various aspect of absorption and emission of radiation by interstellar dust. ... Also, some basic modelling of radiation fields and similar supporting code . ... dust-1.0.1 . ... Modelling absorption and emission of radiation by interstellar dust . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• OptInt PmWiki : PmWiki / Custom InterMap
• OptInt PmWiki : PmWiki / Initial Setup Tasks
• OptInt PmWiki : PmWiki / Skins

In order to calculate the line profile of a given absorption line for atomic species Z with a wavelength LAMBDA (in Angstroms) and a microturbulent velocity VT (in km/s). ... mode . ... 1) The input model may contain more than one model (i.e. it may be an entire grid of models). Spectrum will cycle through this grid NMOD times, omitting NSKIP-1 models from the . ... However, the input data following MODE must be repeated NMOD times in order to obtain equivalent results for each model in the grid. ...

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• Stellar Atmospheres Software
• Atomic data for Stellar Atmospheres: lte_lines
• Armagh Observatory

... From the chain visibility point of view, it is very recommended to look at the Javascript movies , especially if the frame rate can be not regulated in your MPEG player. ... The non-CH-associated large-scale chains visible on the SOHO/EIT images at three wavelengths of 171, 195 and 284 as well as on the MLSO/HAO He I 10830 spectroheliogram of December 16, 1997. ... The SOHO/EIT movies at 171 and 195 show the chain dynamics on June 1-3, 1998. ... Javascript movie (230 KB), SOHO/EIT, 171 . ...

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• Chains and CMEs

... Each document which is or can be circulated outside DMD division has to be issued according to the following Technical Archive procedure. ... Identify the type of document according to the ESO Documentation Type definition list . ... Get the chronological four-digit number from Technical Archive (pday@eso.org phone 6462 or tecarch@eso.org), specifying: the document type, PSC, document title, author(s), issue and issue date. ... ESO document number (i.e. VLT-SPE-ESO-19100-1836). ... issue number . ...

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• DFS Department internal procedure for issue of documentation
• recommended DFS development tools
• DFS To-Do list rules

. Other Relevant Plots . Several new Radio-loud BAL QSOs . A unique Q+A QSO . | Front page | . | << - Close pairs | Talk summary - >> | . 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 (Close Pairs)
• Dunk Proceedings - 2dF QSO Redshift Survey (Summary)
• Dunk Proceedings - 2dF QSO Redshift Survey (Radio-loud BAL QSOs)

... Byte-by-byte Description of files: star -S1.txt , star -S2.txt, star -S3.txt ------------------------------------------------------------------------------- Bytes Format Units Label Explanations 1- 4 I4 --- YYYY Year of the date 6- 7 I2 --- MM Month of the date 9- 10 I2 d DD Day of the date 13- 14 I2 h h Hour of the day 18- 24 F7,2 d JD* Julian day of the date , JD*=JD-2450000.5 28- 31 F4.1 degrees M-S Apparent distance between ...

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• http://lnfm1.sai.msu.ru/neb/nss/SatStar/expl-J.txt
• IDL programs
• Data bases of Natural Satellites. Documentation. Structure