Microflares observed with UVSP and HXIS

Details Microflares observed with UVSP and HXIS Microflares observed with UVSP and HXIS

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..289p&link_type=abstract

In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 289-2

Computer Science

Flux Density, Remote Sensing, Solar Corona, Solar Flares, Solar Maximum Mission, Space Plasmas, Distribution Functions, Heating, Solar Radio Emission, Solar X-Rays, Ultraviolet Spectrometers, X Ray Spectroscopy

Scientific paper

A review of an analysis of SMM (Solar Maximum Mission) microflare observations is presented. The data, from the UVSP (Ultraviolet Spectrometer and Polarimeter) and HXIS (Hard X-ray Imaging Spectrometer) instruments, show that there are counterparts to UV microflares in x-ray emission characteristic of 107 K plasma. Implications of the x-ray/UV relationship for flare distribution functions and coronal heating are discussed, and examples of similar events in SMM quiet Sun data are shown.

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