Ignore:
Timestamp:
Apr 13, 2000, 4:10:46 PM (25 years ago)
Author:
ansari
Message:

Sophie: adding documentation for Doxygen in the .cc files:wq

File:
1 edited

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  • trunk/SophyaLib/SkyT/derivblackbody.cc

    r893 r909  
    11//--------------------------------------------------------------------------
    22// File and Version Information:
    3 //      $Id: derivblackbody.cc,v 1.2 2000-04-12 10:24:52 ansari Exp $
     3//      $Id: derivblackbody.cc,v 1.3 2000-04-13 14:10:44 ansari Exp $
    44//
    55// Description:
     
    2020#include "derivblackbody.h"
    2121
    22 //----------------
    23 // Constructor --
    24 //----------------
     22
     23
     24/*! \class SOPHYA::DerivBlackBody <BR>
     25 * This class corresponds to the emission spectrum of a
     26 * dipole (since its emission spectrum is the derivation
     27 * of a blackbody spectrum wrt the temperature).
     28 */
     29
     30/*! Constructor: needs a temperature. Otherwise set to ConvTools::tcmb */
    2531DerivBlackBody::DerivBlackBody(double temperature)
    2632  : RadSpectra(10., 10000.)
     
    3440}
    3541
    36 
     42/*!
     43  The flux function is the derivation of the BlackBody
     44  flux function wrt the temperature (used e.g. for a Dipole)
     45  \f[
     46  I_\nu = {2 h_{pl} (1.10^9*\nu)^3  {h_{pl}1.10^9*\nu \over k T^2}
     47        {e^{{h_{pl}(1.10^9*\nu) \over kT}}\over c^2 (e^{{h_{pl}(1.10^9*\nu) \over kT}} -1)^2}}
     48  \f]
     49*/
    3750double
    3851DerivBlackBody::flux(double nu) const
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