Source
* <TD> the sky coupling is the coupling efficiency to the sky of the WVR radiometer's. This column differs from the skyCoupling column because it contains one value for each of the individual channels of that spectralWindow. See the documentation of numChan for the size and the presence of this attribute. Note that in general one expects to see whether \b no sky coupling efficiency recorded or \b only \b one of the two forms scalar (skyCoupling) or array (skyCouplingSpectrum, numChan). </TD>
/*
* ALMA - Atacama Large Millimeter Array
* (c) European Southern Observatory, 2002
* (c) Associated Universities Inc., 2002
* Copyright by ESO (in the framework of the ALMA collaboration),
* Copyright by AUI (in the framework of the ALMA collaboration),
* All rights reserved.
*
* This library is free software; you can redistribute it and/or
* modify it under the terms of the GNU Lesser General Public
* License as published by the Free software Foundation; either
* version 2.1 of the License, or (at your option) any later version.
*
* This library is distributed in the hope that it will be useful,
* but WITHOUT ANY WARRANTY, without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU
* Lesser General Public License for more details.
*
* You should have received a copy of the GNU Lesser General Public
* License along with this library; if not, write to the Free Software
* Foundation, Inc., 59 Temple Place, Suite 330, Boston,
* MA 02111-1307 USA
*
* Warning!
* --------------------------------------------------------------------
* | This is generated code! Do not modify this file. |
* | If you do, all changes will be lost when the file is re-generated. |
* --------------------------------------------------------------------
*
* File FeedTable.h
*/