The fate of sunward streaming protons associated with coronal mass ejections

Details The fate of sunward streaming protons associated with coronal mass ejections The fate of sunward streaming protons associated with coronal mass ejections

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...145..139s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 145, no. 1, April 1985, p. 139-143.

Astronomy and Astrophysics

Astrophysics

8

Solar Corona, Solar Protons, Solar X-Rays, Stellar Mass Ejection, Particle Acceleration, Solar Magnetic Field, Solar Wind

Scientific paper

It is suggested that the sunward streaming protons accelerated in the travelling interplanetary shock which accompanies a coronal mass ejection have sufficient energy to power the long duration solar X-ray event frequently correlated with the ejections. The energy flux of such protons over a 104s period is estimated to be comparable to the total energy content of the X-ray emitting plasma during the long decay of a typical event.

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