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Microflares observed with UVSP and HXISA 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 10(exp 7) 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.
Document ID
19930022216
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Porter, Jason G. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
September 6, 2013
Publication Date
November 1, 1992
Publication Information
Publication: ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition
Subject Category
Solar Physics
Accession Number
93N31405
Distribution Limits
Public
Copyright
Other
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