SOLAR FLARE PROTON FLUXES IN THE LAST FEW MILLION YEARS
The authors describe a method for deducing the absolute solar cosmic-ray (flare) proton fluxes in the last few million years by means of He-3 in samples from three depths of lunar rocks. A figure shows concentration profiles of He-3 as a function of depth in lunar rocks 64435 and 61016.
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| Veröffentlicht in: | Current science (Bangalore) 1980-01, Vol.49 (10), p.391-391 |
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| container_end_page | 391 |
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| container_issue | 10 |
| container_start_page | 391 |
| container_title | Current science (Bangalore) |
| container_volume | 49 |
| creator | Venkatesan, T. R. Rao, M. N. |
| description | The authors describe a method for deducing the absolute solar cosmic-ray (flare) proton fluxes in the last few million years by means of He-3 in samples from three depths of lunar rocks. A figure shows concentration profiles of He-3 as a function of depth in lunar rocks 64435 and 61016. |
| format | Article |
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| fulltext | fulltext |
| identifier | ISSN: 0011-3891 |
| ispartof | Current science (Bangalore), 1980-01, Vol.49 (10), p.391-391 |
| issn | 0011-3891 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_18405996 |
| source | JSTOR Archive Collection A-Z Listing; EZB-FREE-00999 freely available EZB journals |
| subjects | LETTERS TO THE EDITOR Protons Solar flares |
| title | SOLAR FLARE PROTON FLUXES IN THE LAST FEW MILLION YEARS |
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