A STATISTICAL PROPERTY OF SOLAR PROTON FLARES

Wang Jja-long

doi:10.11728/cjss1993.04.313

Volume 13 Issue 4

Dec. 1993

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Wang Jja-long. A STATISTICAL PROPERTY OF SOLAR PROTON FLARES[J]. Chinese Journal of Space Science, 1993, 13(4): 313-315. doi: 10.11728/cjss1993.04.313

Citation:

Wang Jja-long. A STATISTICAL PROPERTY OF SOLAR PROTON FLARES[J]. Chinese Journal of Space Science, 1993, 13(4): 313-315. doi: 10.11728/cjss1993.04.313

Wang Jja-long. A STATISTICAL PROPERTY OF SOLAR PROTON FLARES[J]. Chinese Journal of Space Science, 1993, 13(4): 313-315. doi: 10.11728/cjss1993.04.313

Citation:

Wang Jja-long. A STATISTICAL PROPERTY OF SOLAR PROTON FLARES[J]. Chinese Journal of Space Science, 1993, 13(4): 313-315. doi: 10.11728/cjss1993.04.313

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A STATISTICAL PROPERTY OF SOLAR PROTON FLARES

doi: 10.11728/cjss1993.04.313 cstr: 32142.14.cjss1993.04.313

Wang Jja-long

Beijing Observatory, Academia Sinica, 100080

Received Date: 1993-02-16
Rev Recd Date: 1900-01-01
Publish Date: 1993-12-24

Abstract

Abstract

Astatistical study of solar proton flares in this paper reveals a property of proton flares that most of the solar proton flares studied and the solar disk center are located on the same side of the neutral line of the large scale, averaged line of sight component of solar magnetic fields in the photosphere. This finding would be of some significance for proton flare research and prediction.
- Sun proton flares,
- Solar magnetic fields,