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High energetic solar proton flares on the declining phase of solar cycle 22

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Abstract

The year 1991 is a part of the declining phase of the solar cycle 22, during which high energetic flares have been produced by active regions NOAA/USAF 6659 in June. The associated solar proton events have affected the Earth environment and their proton fluxes have been measured by GOES space craft. The evaluation of solar activity during the first half of June 1991, have been carried out by applying a method for high energetic solar flares prediction on the flares of June 1991. The method depends on cumulative summation curves according to observed H-alpha flares, X-ray bursts, in the active region 6659 during one rotation when the energetic solar flares of June 1991 have occurred. It has been found that the steep trend of increased activity sets on several tens of hours prior to the occurrence of the energetic flare, which can be used, together with other methods, for forecasts of major flares. All the used data at the present work are received from NOAA, Boulder, Colorado, USA.

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Shaltout, M.A.M. High energetic solar proton flares on the declining phase of solar cycle 22. Astrophys Space Sci 228, 67–75 (1995). https://doi.org/10.1007/BF00984967

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  • DOI: https://doi.org/10.1007/BF00984967

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