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Solar flare proton acceleration by Alfven turbulence

✍ Scribed by A.L. MacKinnon

Book ID
107880654
Publisher
Elsevier Science
Year
1991
Tongue
English
Weight
527 KB
Volume
34
Category
Article
ISSN
0083-6656

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πŸ“œ SIMILAR VOLUMES

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We show that protons can be accelerated to several GeV in ~I0 s by Alfven turbulence whose energy density is greater than a few erg/cmS. We also show that electrons can be accelerated to tens of MeV on similar time scales by whistler and Alfven turbulence.

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The data on optical, X-ray and gamma emission from proton flares, as well as direct observations of flare-associated phenomena, show energetic proton acceleration in the corona rather than in the flare region. In the present paper, the acceleration of protons and accompanying relativistic electrons