Hard X-rays Associated with CMEs

Details Hard X-rays Associated with CMEs Hard X-rays Associated with CMEs

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh32b..03h&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH32B-03

Astronomy and Astrophysics

Astronomy

7509 Corona, 7513 Coronal Mass Ejections, 7519 Flares, 7534 Radio Emissions, 7554 X Rays, Gamma Rays, And Neutrinos

Scientific paper

In principle we can use hard X-ray bremsstrahlung (> few keV) to study the non-thermal tail of the electron distribution function in the solar corona. This approach is less sensitive than the techniques of radio astronomy, because of the low emissivity and low detection sensitivity for hard X-rays, but observations of major events are now possible; HESSI should greatly improve the breadth of such observations. These highly energetic flare events commonly are associated with CMEs. The view offered by such observations complements the radio techniques in interesting ways. This talk reviews data from several coronal hard X-ray events observed by the Yohkoh Hard X-ray Telescope and other instruments in the context of the radio observations.

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