The need for hard X-ray imaging observations at the next solar maximum

Details The need for hard X-ray imaging observations at the next solar maximum The need for hard X-ray imaging observations at the next solar maximum

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988fnsm.work..145e&link_type=abstract

In NASA, Goddard Space Flight Center, Max 1991: Flare Research at the Next Solar Maximum. Workshop 1: Scientific Objectives p 14

Physics

Imaging Techniques, Mathematical Models, Prediction Analysis Techniques, Solar Activity, X Rays, Acceleration (Physics), Canonical Forms, International Sun Earth Explorers, Solar Maximum Mission, Transport Theory

Scientific paper

Canonical models of solar hard X-ray bursts; associated length and time
scales; the adequacies and inadequacies of previous observations;
theoretical modeling predictions; arcsecond imaging of solar hard X-rays
are outlined.

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