Theoretical motivation for high spatial resolution, hard X-ray observations during solar flares

Details Theoretical motivation for high spatial resolution, hard X-ray observations during solar flares Theoretical motivation for high spatial resolution, hard X-ray observations during solar flares

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sfcp.nasa..132e&link_type=abstract

In NASA. Marshall Space Flight Center Solar Flares and Coronal Physics Using P/OF as a Research Tool p 132-138 (SEE N86-24614

Physics

1

Impulses, Solar Flares, Solar X-Rays, Spatial Resolution, Bremsstrahlung, Electrons, High Energy Interactions, Pinhole Occulter Facility

Scientific paper

The important role played by hard X-ray radiation as a diagnostic of
impulsive phase energy transport mechanism is reviewed. It is argued
that the sub-arc second resolution offered by an instrument such as the
Pinhole/Occulter Facility (P/OF) can greatly increase our understanding
of such mechanisms.

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