<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 3.2 Final//EN"> <!--Converted with LaTeX2HTML 98.1p1 release (March 2nd, 1998) originally by Nikos Drakos (nikos@cbl.leeds.ac.uk), CBLU, University of Leeds * revised and updated by: Marcus Hennecke, Ross Moore, Herb Swan * with significant contributions from: Jens Lippmann, Marek Rouchal, Martin Wilck and others --> <HTML> <HEAD> <TITLE>Computation of the Output Absorption Spectrum</TITLE> <META NAME="description" CONTENT="Computation of the Output Absorption Spectrum"> <META NAME="keywords" CONTENT="vol2"> <META NAME="resource-type" CONTENT="document"> <META NAME="distribution" CONTENT="global"> <META HTTP-EQUIV="Content-Type" CONTENT="text/html; charset=iso-8859-1"> <LINK REL="STYLESHEET" HREF="vol2.css"> <LINK REL="previous" HREF="node190.html"> <LINK REL="up" HREF="node184.html"> <LINK REL="next" HREF="node192.html"> </HEAD> <BODY > <!--Navigation Panel--> <A NAME="tex2html3805" HREF="node192.html"> <IMG WIDTH="37" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="next" SRC="icons.gif/next_motif.gif"></A> <A NAME="tex2html3802" HREF="node184.html"> <IMG WIDTH="26" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="up" SRC="icons.gif/up_motif.gif"></A> <A NAME="tex2html3798" HREF="node190.html"> <IMG WIDTH="63" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="previous" SRC="icons.gif/previous_motif.gif"></A> <A NAME="tex2html3804" HREF="node1.html"> <IMG WIDTH="65" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="contents" SRC="icons.gif/contents_motif.gif"></A> <BR> <B> Next:</B> <A NAME="tex2html3806" HREF="node192.html">Auxiliary Data</A> <B> Up:</B> <A NAME="tex2html3803" HREF="node184.html">Typical Run</A> <B> Previous:</B> <A NAME="tex2html3799" HREF="node190.html">Edition of the Table</A> <BR> <BR> <!--End of Navigation Panel--> <H2><A NAME="SECTION001337000000000000000"> Computation of the Output Absorption Spectrum</A> </H2> <P> This is the main step achieved by the command: <P><P> <BR> <DIV ALIGN="CENTER"> <!-- MATH: $\fbox{\tt COMPUTE/ABS \ \ SYNEMI \ \ SYNABS \ \ ABSC \ \ ABSP \ \ NAMEP}$ --> <IMG WIDTH="598" HEIGHT="31" ALIGN="BOTTOM" BORDER="0" SRC="img392.gif" ALT="\fbox{\tt COMPUTE/ABS \ \ SYNEMI \ \ SYNABS \ \ ABSC \ \ ABSP \ \ NAMEP}"></DIV> <P><P> <BR> <PRE><TT> SYNEMI : input emission spectrum <BR> SYNABS : output spectrum with synthetic absorption lines <BR> ABSC : table containing the cloud model <BR> ABSP : table containing the atomic data <BR> NAMEP : image containing the instrumental response <BR> <EM>Warning</EM> : this image must have the same step size as SYNEMI </TT></PRE> <P> <P> Then the program: <P> <DL COMPACT> <DT>1. <DD>Types: <BR> <P><P> <BR> PSF: FWHM a ANGSTROM <BR> STEP: b <BR> Where a and b are read from the description of the PSF; only as a check for the user. <DT>2. <DD>Computes: <BR> <P><P> <BR> The synthetic spectra according to the parameters of table ABSC. <BR> The output spectra are: <BR> <BR><P></P> <DIV ALIGN="CENTER"> <!-- MATH: \begin{displaymath} \left\{ \begin{array}{ll} SYNABS1 & \mbox {if option Voigtian profiles}\\ or & \\ SYNABS0 & \mbox {if option Maxwellian profiles} \end{array} \right. \end{displaymath} --> <IMG WIDTH="427" HEIGHT="84" SRC="img393.gif" ALT="\begin{displaymath}\left\{ \begin{array}{ll} SYNABS1 & \mbox {if option Voigtia... ...S0 & \mbox {if option Maxwellian profiles} \end{array} \right. \end{displaymath}"> </DIV> <BR CLEAR="ALL"> <P></P> and <BR> <BR><P></P> <DIV ALIGN="CENTER"> <!-- MATH: \begin{displaymath} \left\{ \begin{array}{ll} SYNABS1C & \mbox {convolution of \ above spectra}\\ or & \\ SYNABS0C \end{array} \right. \end{displaymath} --> <IMG WIDTH="453" HEIGHT="93" SRC="img394.gif" ALT="\begin{displaymath}\left\{ \begin{array}{ll} SYNABS1C & \mbox {convolution of \ above spectra}\\ or & \\ SYNABS0C \end{array} \right. \end{displaymath}"> </DIV> <BR CLEAR="ALL"> <P></P></DL> <P> <BR><HR> <ADDRESS> <I>Petra Nass</I> <BR><I>1999-06-15</I> </ADDRESS> </BODY> </HTML>