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Detailed Reference Information |
Nonnast, J.H., Armstrong, T.P. and Kohl, J.W. (1982). A study of solar flux soft x rays and their relation to particle events observed with IMP 8. Journal of Geophysical Research 87: doi: 10.1029/JA087iA06p04327. issn: 0148-0227. |
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Data from the Johns Hopkins University Applied Physics Laboratory charged particle measurement experiment aboard IMP 8 was used to study solar flare events and find correlations between soft X rays (4--17 ¿) and particle events. The results show that a greater probability exists of observing a proton event if the observed soft X ray flare has a relatively large decay time. It is also found that the H&agr; brightening area is a good indicator of the strength of the soft X ray burst. Results also show that the strength of the soft X ray burst can be used to estimate a probability that a proton event will occur, along with the strength of that particle event. |
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American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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