FNAS UAH UVSP and complimentary data analysis and modeling

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Coronal Loops, Magnetic Field Configurations, Solar Atmosphere, Solar Flares, Solar Maximum Mission, Sunspots, Ultraviolet Spectrometers, X Ray Spectra, Data Reduction, Energy Consumption, Gas Jets, High Temperature, Magnetohydrodynamics, Mathematical Models, Sequencing

Scientific paper

Several data sets obtained by the UVSP and HXIS instruments on board SMM were studied. From these data, several events of sequences of events were selected that are specially representative of the plethora of active region energetic phenomena that was simultaneously observed by UVSP and HXIS. The selection criteria was to have available both types of observations in active region flares that are not so bright that the UVSP instrument was switched off for protection, and at the same time flares that are not so dim in X-Rays that HXIS will have collected significant data. Another criteria of secondary importance was to select events where auxiliary optical data is available.

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