Energy and nuclear charge dependence of abundance enhancements of solar cosmic ray heavy ions in three large solar events
The differential flux and energy spectra of solar cosmic-ray heavy ions of He, C, O, Ne, Mg, Si, and Fe were determined in the energy interval E=3-30 MeV amu super(-) super(1) for two large solar events of Jan. 24, 1971, and Sept. 1, 1971, in rocket flights made from Ft. Churchill. From these data,...
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Veröffentlicht in: | Solar physics 1983-11, Vol.89 (1), p.163-180 |
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