FIELD: physics.
SUBSTANCE: information on X-ray solar radiation is continuously collected and analysed in the wavelength range of 0.1-0.8 nm, wherein during real-time prediction, X-ray bursts with intensity higher than 5*10-5 W/m2 are sought and for each such burst, the "protonness" parameter is determined from a given relationship and depending on its value and the helio-duration of the burst, the probability of observing, in the near-Earth environment, a solar proton event with proton energy greater than 30 MeV with intensity at the peak of the event higher than given levels is determined.
EFFECT: providing earlier forecast and providing better measurement of the burst evolution time and enabling prediction of onset after bursts of past events of different levels of intensity.
8 dwg
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Authors
Dates
2013-06-20—Published
2011-11-11—Filed