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Geisa inital import

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12<CENTER><P><B><FONT COLOR="#FF0000"><FONT SIZE=+1>GEISA-97 Introduction</FONT></FONT></B></P></CENTER>
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17<CENTER><P><A NAME="intoduct"></A><B><FONT COLOR="#000000">INTRODUCTION</FONT></B></P></CENTER>
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19<P><FONT COLOR="#000000">Adequate tools are required to perform reliable
20radiative transfer calculations to meet the needs of communities involved
21in understanding the atmospheres of the Earth and other planets. In particular,
22accurate spectral analyses of Earth or planetary spectra observed by new
23generations of high spectral resolution vertical atmospheric sounders will
24result in an improved knowledge of their atmospheric and surface properties.
25The performance of instruments like AIRS (Atmospheric Infrared Sounder)
26in the USA (JPL, 1991), and IASI (Infrared Atmospheric Sounding Interferometer)
27in Europe (Phulpin et al., 1997), which have a better vertical resolution
28and accuracy compared to presently existing satellite infrared temperature
29sounders, is directly related to the quality of the spectroscopic parameters
30of the optically active atmospheric gases since these are essential input
31in the forward models used to simulate recorded radiance spectra. The ARA
32(Atmospheric Radiation Analysis) group at LMD (Laboratoire de M&eacute;t&eacute;orologie
33Dynamique du CNRS, France) developed the GEISA (Gestion et Etude des Informations
34Spectroscopiques Atmosph&eacute;riques: Management and Study of Atmospheric
35Spectroscopic Information) computer accessible database system (Chedin
36et al., 1982; Husson et al., 1992, 1994), in 1974. This early effort implemented
37the so-called line-by-line and layer-by-layer approach for forward radiative
38transfer modeling action. This activity is of interest to research groups
39involved in direct and inverse radiative transfer studies. </FONT></P>
40
41<P><FONT COLOR="#000000">The role of molecular spectroscopy in modern atmospheric
42research has entered a new phase with the advent of highly sophisticated
43spectroscopic instruments and computers. Retrieval of the concentrations
44of radiatively active molecular species from observed spectra of planetary
45atmospheres using available spectroscopic databases and atmospheric models
46has become fairly routine. The molecular spectroscopist is constantly on
47demand to deliver data that are not only appropriate but essential for
48the analyses of the planetary atmospheric observations. GEISA is dedicated
49to meeting that aim.</FONT></P>
50
51<P><FONT COLOR="#000000">Currently, GEISA is involved in activities, with
52the purpose of assessing the IASI (Infrared Atmospheric Sounding Interferometer)
53measurement capabilities and its own database quality, within the ISSWG
54(IASI Sounding Working Group), in the frame of the CNES (Centre National
55d'Etudes Spatiales, France)/EUMETSAT (EUropean organization for METeorological
56SATellites) European Polar System (EPS), by simulating high-resolution
57adiances and/or using experimental data, as described in Jacquinet-Husson
58et al., 1998a. </FONT></P>
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60<CENTER><P><A HREF="geisa_index_gs03.html"><IMG SRC="/icons-geisa/prev.gif" BORDER=0 HEIGHT=50 WIDTH=91></A><B><FONT COLOR="#800080"><FONT SIZE=+1>MAIN&nbsp;PAGE</FONT></FONT></B></P></CENTER>
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