Solar flare nuclear gamma rays and interplanetary proton events

Cliver, E. W.; Forrest, D. J.; Mcguire, R. E.; Vonrosenvinge, T. T.; Reames, D. V.; Cane, H. V.; Kane, S. R.

NASA NTRS · 19920075518

Solar flare nuclear gamma rays and interplanetary proton events

Cliver, E. W.·Forrest, D. J.·Mcguire, R. E.·Vonrosenvinge, T. T.·Reames, D. V.·Cane, H. V.·Kane, S. R.

Abstract

We compared flare gamma ray line (GRL) events and solar energetic proton (SEP) events for the period from Feb. 1980 - Jan. 1985 and substantiated earlier results showing a lack of correlation between gamma-ray-producing ions and interplanetary protons. This poor correlation results primarily from several large SEP events that originated in flares without detectable gamma ray emission. The converse case of GRL events unassociated with SEP events is rare. We present evidence which suggests that the ratio of trapped to escaping protons in GRL/SEP flares depends on the spatial scale size of the flare. We affirm the result of Bai and Dennis (1985) that GRL flares are generally accompanied (75 percent) by metric Type 2 bursts.

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BibTeX RIS

Cliver, E. W., Forrest, D. J., Mcguire, R. E., Vonrosenvinge, T. T., Reames, D. V., Cane, H. V., Kane, S. R.. 1987-01-01. Solar flare nuclear gamma rays and interplanetary proton events. https://ntrs.nasa.gov/citations/19920075518

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