Long-term, solar flare fluence forecasting
The problem of forecasting solar flare proton fluences is discussed and some projection techniques are proposed for long-duration space missions. The proton energy ranges considered are > 10 and > 30 MeV. Results of modeling the proton fluences are compared with available observational data.
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| Veröffentlicht in: | Radiation measurements 1996, Vol.26 (3), p.455-456 |
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| container_end_page | 456 |
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| container_issue | 3 |
| container_start_page | 455 |
| container_title | Radiation measurements |
| container_volume | 26 |
| creator | Getselev, I.V. Morozova, E.I. Moszhukhina, A.R. Pisarenko, N.F. Polyanskaya, M.G. Timofeev, G.A. |
| description | The problem of forecasting solar flare proton fluences is discussed and some projection techniques are proposed for long-duration space missions. The proton energy ranges considered are > 10 and > 30 MeV. Results of modeling the proton fluences are compared with available observational data. |
| doi_str_mv | 10.1016/1350-4487(96)00020-0 |
| format | Article |
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| fulltext | fulltext |
| identifier | ISSN: 1350-4487 |
| ispartof | Radiation measurements, 1996, Vol.26 (3), p.455-456 |
| issn | 1350-4487 1879-0925 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_15436958 |
| source | Elsevier ScienceDirect Journals |
| subjects | Data processing Mathematical models Q1 |
| title | Long-term, solar flare fluence forecasting |
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