Forward Modeling of MOSES Response to the Solar Atmosphere

Details Forward Modeling of MOSES Response to the Solar Atmosphere Forward Modeling of MOSES Response to the Solar Atmosphere

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.5507c&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #55.07; Bulletin of the American Astronomical Society, Vol. 34, p.733

Astronomy and Astrophysics

Astronomy

Scientific paper

Using high resolution TRACE data, we have generated a suite of models
for EUV intensity and line profiles in He II and Si XI. The models are
used to simulate the response of the Multi-Order Solar EUV Spectrograph
(MOSES) rocket instrument to realistic solar features. This research is
supported by NASA Grant NAG5-10997.

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