Hard X-ray imaging from the solar probe

Details Hard X-ray imaging from the solar probe Hard X-ray imaging from the solar probe

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978clus.nasa..132h&link_type=abstract

In JPL A Close-up of the Sun p 132-142 (SEE N78-32964 23-92)

Astronomy and Astrophysics

Astronomy

Mission Planning, Solar Probes, Solar Wind, Solar X-Rays, X Ray Imagery, X Ray Telescopes, Energetic Particles, Particle Interactions, Solar Electrons, Solar Flares, X Ray Astronomy

Scientific paper

The solar probe offers a platform with particular advantages for studying solar nonthermal plasma processes via the observations of hard X-radiation from energetic electrons in the chromosphere and corona, these include (1) high sensitivity, (2) a second line of sign (in addition to the earth's) that can aid in three dimensional reconstruction of the source distribution, and, (3) the possibility of correlation with direct measurements of the nonthermal particles from the probe itself.

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