[55.07] Forward Modeling of MOSES Response to the Solar Atmosphere

AAS 200th meeting, Albuquerque, NM, June 2002
Session 55. Solar Data Analysis and Calibration
Display, Wednesday, June 5, 2002, 10:00am-7:00pm, SW Exhibit Hall

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[55.07] Forward Modeling of MOSES Response to the Solar Atmosphere

M. J. S. Cirtain, C. C. Kankelborg (Physics Department, Montana State University), M. Reiser (Physics Department, University of Wisconsin - Stevens Point)

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.

If you would like more information about this abstract, please follow the link to http://solar.physics.montana.edu/MOSES/public/moses.html. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.

The author(s) of this abstract have provided an email address for comments about the abstract: mcirtain@physics.montana.edu

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