Gamma-Ray Observations of Solar Flares with RHESSI Imaging Spectroscopy and the GRIPS instrument
<p> Solar flares can release ~1e33 ergs of power, accelerate particles to relativistic speeds, heat plasma to ~15 million K and catastrophically reorganize 1e5 km long field structures in 100s–1000s of seconds. Magnetic reconnection of large-scale field structures in the corona are t...
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| Language: | EN |
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University of California, Berkeley
2018
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| Online Access: | http://pqdtopen.proquest.com/#viewpdf?dispub=10620536 |