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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• SPECTRUM v3 - Examples
• Spectrum - control
• Atomic data for Stellar Atmospheres: lte_lines

... Different equations of state tables can be used, including SAHA-S equation of state. ... 1) separate input fields for X and Z are used, each line contains only T and rho; example: 2.17e6 0.18 . 2) each line contains T, rho, X and Z; separate input fields for X and Z are ignored; example: 2.17e6 0.18 0.74 0.018 . 3) each line contains T, rho, X, Z(CNO), Z(Ne), Z(FeSi); separate input fields for X and Z are ignored; example: 2.17e6 0.18 0.74 0.010 0.002 0.006 . ...

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• Solar modeling input physics (thermodynamics, opacity, nuclear reactions)
• Additional problems at the transition
• The layout of a program

function linespec_em,atom, wmin = wmin , wmax = wmax , nbin = nbin ,wlog=wlog,ww=ww,$ ikev=ikev, fstr = fstr , tlog = tlog ,EM=EM, _extra=e ;+ ;function linespec_em ; returns a spectrum of atomic lines for a 1-T EM. output will be in ; units of [erg,ph]/s/cm^2/[keV,Ang] ; ; if IKEV is set , WMIN , WMAX ,WW must be input in [keV] and the ; output will have units .../keV ; ; if NOPH is ...

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• http://hea-www.harvard.edu/PINTofALE/pro/apedance.pro
• http://hea-www.harvard.edu/PINTofALE/pro/linespec.pro
• http://hea-www.harvard.edu/PINTofALE/pro/show_line.pro

Focal line of the feed cabin No. ... Figure 1. The input parts of radiometers with primary feeds are placed on secondary mirror focal line taking into account a task to minimize losses in the front-end waveguides and reduce aberrational scatter at short wavelength range. ... From the right of the picture is a new developed three-frequency feed with matched phase center at the wavelengths 13, 31 and 49 cm, from the left is a new version radiometric system "MARS-2". ...

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• Advanced Pointer Topics
• Atlas and list of identified lines
• Exercises

... The syntax of the rtftohtml command is as follows: rtftohtml [-i] [-o filename] [-P extension] [-T] [-G][file] . ... Indicates that imbedded graphics
should be linked into the main document using an IMG tag. ... Use "extension" as the extension for any links to graphics files. ... If standard input is used, the body of the document will be written to standard output (unless overridden by the -o option.) If a file name appears, the output is written to "filename" with ".html" as an extension. ...

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• Command line editing with the Korn shell
• Deleting words and lines
• Removing duplicate lines with uniq

Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...

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• Eclipse map for Computer Ephemeris for 2016 (DE200/LE200).
• Eclipse map for Computer Ephemeris for 2014 (DE200/LE200).
• Eclipse map for Computer Ephemeris for 2015 (DE200/LE200).

Астрономическое образование с сохранением традиций . ... А.В.ЗАСОВ . ЗАДАЧИ АСТРОФИЗИЧЕСКОГО ПРАКТИКУМА . Для студентов 3 и 4 курсов астрономического отделения . ... Задача 01. Определение красного смещения галактики . ... Исследование объектива на оптической скамье . ... Спектры и показатели цвета звезд . ... Определение физических параметров газа в ядре сейфертовской галактики . ... Определение цвета и морфологии удаленной галактики - источнике гамма-всплеска . ...

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... title=' Eco Line Конверт на выписку Марсель - Eco Line - Eco LineКонверт на выписку Марсель' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> Компания Eco Line позаботилась о том, чтоб процесс выписки малыша был по-настоящему волнительным и радостным. ... Стефано Диониси ("Фаринелли - кастрат"), Андреа Продан ("Сицилийцы"), Фабрицио Джифуни в фильме Гвидо Кьезы "Обратная сторона войны". ... Но у войны есть и обратная сторона: . ... Цвет: разноцветный . ...

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• Rosenthal Studio-line Moon wei? Кофейная чашка 0,23 л - Rosenthal Studio Line -
• Rosenthal Studio Line Landscape Чайная чашка 0,23 л - Rosenthal Studio Line -
• Дутики FINN LINE - FINN LINE - FINN LINE Коврики в салон MITSUBISHI Pajero IV,

fitshdr - FITS-file headers manipulation tool fitshdr [options] [FITSfile_name] . ... fitshdr [options] --edit FITSfile_name . ... If You want to modify headers of FITSFILE using new FITS-header lines from HEADER file (or from stdin), You have to use this option (You can skip this option, if -H or --header option is used). ... Empty header lines are not displayed (in 'dump' mode only). --line-offsets . ... In 'dump' mode: file offset will be displayed for each header line. --no-line-offsets . ...

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• IDL programs
• Manpage of FITSHDR_EDIT

This module provides for forensic logging of the requests made to the server . ... Logging is done before and after processing a request, so the forensic log contains two log lines for each request. ... Module: mod_log_forensic . ... Each log entry is assigned unique ID which can be associated with the request using the normal CustomLog directive. mod_log_forensic creates a token called forensic-id , which can be added to the transfer log using the %{forensic-id}n format string. ...

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• Apache module mod_log_common
• Apache module mod_log_referer
• Configuration Files

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... Protected Member Functions | ... StelSkyImageTile Class Reference . Base class for any astro image with a fixed position. More... #include < StelSkyImageTile.hpp > . ... StelSkyImageTile (const QString &url, StelSkyImageTile *parent=NULL) . ... Definition at line 62 of file StelSkyImageTile.hpp . ... const QString &љ . ... Definition at line 100 of file StelSkyImageTile.hpp . ... Definition at line 114 of file StelSkyImageTile.hpp . ...

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• Stellarium: StelSkyPolygon Class Reference
• Stellarium: MultiLevelJsonBase Class Reference
• Stellarium: StelScriptMgr Class Reference

... As a result of BTA observations of 23 chemically peculiar stars with strong magnetic fields, it was found that in 22 of them the longitudinal magnetic field, measured from the hydrogen line cores are considerably lower (by about 1/3) than the value measured from metal lines in the same spectra. ... New approaches need to be developed in order to interpret the data. ... The Zeeman spectrum of a star with a strong magnetic field, 53 Cam. ...

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• V1494
• Figure 1
• Galaxy sector, archive 2013

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The real-time radiosignals characteristics calculation algorithm from current VS data is carried out according to the following scheme (V.P.Grozov ,G.V.Kotovitch,V.E.Nosov,S.N.Ponomartvhuk, S.V.Pushkarev,L.P.Sergeeva,V.V.Khakhinov. Real time decameters radio systems characteristics calculation by ionosphere vertical sounding data. ... ionogram and calculation results display on monitor; . ...

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• East Siberian Center for the Earth's Ionosphere Research. Maximum usable

... The software enables to browse HITRAN-86 or 96 databases. It enables input first 7 atmospheric gases. ... calculate atmospheric transmittance on any pressure level, . calculate instrument transmission functions through the atmosphere, . ... The software is supplied by standard atmospheric profiles, extracted from FASCODE_3.0 FORTRAN codes (dowloaded from PL/GP), and by instrument response function for IR channels of NOAA 14 satellite (both AVHRR and HIRS, downloaded from NOAA/NESDIS). ...

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• TDF Viewer (Satellite Data Format) REGIONAL DATA ARCHIVE (SMIS IKI RAN Project)
• TDF Viewer (Satellite Data Format)

echo 24 декабря br ; echo TABLE border=0 cellpadding=0 cellspacing=0 \n ; $ lines =file('day1.csv'); foreach ($ lines as $ line _num = $ line ) { $ line = rtrim($ line ); list($ time , $ dur , $ name , $ title ) = split( , , $ line ,4); print tr td align=right valign = top $ time /td td valign = top $ ...

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• http://hea.iki.rssi.ru/integral06/index.php~
• High Energy Astrophysics Department at IKI RAN
• Other WWW services

... The relationship of the mass and the observed galactocentric distance R -- (a), and that of the mass and the total dissipation velocity n taken from Gnedin, Ostriker (1997) -- (b). The dotted line in diagram (a) shows the "cone of survival" according to the paper by Surdin and Arkhipova (1998) . ... The solid line is a regression stright line for the main sequence of clusters, and the dotted line parallel to it separates the sequence of clusters of anomalously small mass shown by open triangles. ...

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• Population of Galactic globular clusters, figures
• Subsystems of the Galactic halo, figures
• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures

. (Data examples) . Russian . 4/03/1997 21:00 GMT . Image with coastal line and coordinate grid overlayed . (image size 784x521) . 6/03/1997 21:00 GMT . Image with coastal line and coordinate grid overlayed . (image size 512x512) . Moon disc captured by GOMS . (image size 1024x1024) . For information send a mail to: admin@planeta.rssi.ru . All rights reserved. © 1997-2002 SMIS IKI RAN and SRC PLANETA, Moscow, Russia.

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... 7 EPSC2012-52 2012 European Planetary Science Congress 2012 c Author(s) 2012 E P SC European Planetary Science Congress Properties of the impact-produced lunar exosphere during Perseid 2009 meteor shower A.A. Berezhnoy (1), O.R. Baransky (2), K.I. Churyumov (2), T.K. Churyumova (2), V.V. Kleshchenok (2), E.A. Kozlova (1), V. Mangano (3), V.O. Ponomarenko (2), Yu.V. Pakhomov (4), V.V. Shevchenko (1), Yu.I. Velikodsky (5) (1) Sternberg Astronomical Institute, Universitetskij pr., ... 12/13, 2009. ...

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• http://selena.sai.msu.ru/Greg/Publications/ms40/81_Ushkin_Michael.pdf

... Phys., 45, 409-419 10.02.2010 , . PLHR: o 50 / 60 / 100 / 120 o MLR: o 50 / 60 / 100 / 120 o o , - PorojДrvi 17/11/1993 Total power -5 dB 1,8 -15 1,7 -25 1,6 14.09 14.11 Time(UT) -35 14.13 Frequency (kHz) 4,2 4,1 4,0 07.30 -30 -40 07.45 Time(UT) 07.00 10.02.2010 Frequency (kHz) PorojДrvi 25/01/1993 Total power 4,3 -20 dB , . ... 10.02.2010 , . ... f1 < < fn < fn+ 1 20 ms 128 Frequency (kHz) 1,8 1,8 Frequency (kHz) 4 dB 0 -20 1,7 1,7 1,6 0 10.02.2010 30 Time(sec) 60 1,6 -40 0 0,3 Time(sec) 0,6 , . ...

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• Солнечный ветер для всех

THE INTERNATIONAL WORKSHOP "MASTER GlOBAL ROBOTIC NET" . ... From left to right, 1 st line: Oleg Gress ( Irkutsk State University ), Vadim Krushinskiy ( Ural Federal University ), Artem Burdanov ( Ural Federal University ), Alexander Popov ( Ural Federal University ), Alexander Parkhomenko ( Kislovodsk solar station of the Pulkovo observatory RAS ), Maria Pruzhinskaya ( Lomonosov MSU , SAI ), Nicolas Lodieu ( Instituto de Astrofisica de Canarias ), Denis Denisenko SAI ) . ...

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