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New Results from the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) Mission

Published online by Cambridge University Press:  26 May 2016

R. P. Lin
R. P. Lin*
Affiliation:
Physics Department and Space Sciences Laboratory, Univ. of California/Berkeley, Berkeley, CA, USA 94720-7450

Abstract

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The primary scientific objective of RHESSI Small Explorer mission is to investigate the physics of particle acceleration and energy release in solar flares, through imaging and spectroscopy of X-ray/gamma-ray continuum and gamma-ray lines emitted by accelerated electrons and ions, respectively. Here we briefly describe the mission and summarize the new solar observations, including the first hard X-ray imaging spectroscopy, the first high resolution spectroscopy of solar gamma-ray lines, and the first imaging of solar gamma-ray lines and continuum.

Type
Part 2: Results from New Instrumentation
Information
Symposium - International Astronomical Union , Volume 219: Stars as Suns : Activity, Evolution and Planets , 2004 , pp. 41 - 54
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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