Correlation of near-Earth proton enhancements >100 MeV with parameters of solar microwave bursts

Author:

Гречнев Виктор1,Grechnev Victor2,Киселев Валентин1,Kiselev Valentin2,Мешалкина Наталия1,Meshalkina Nataliya2,Черток Илья3,Chertok Il'ya4

Affiliation:

1. Институт солнечно-земной физики СО РАН

2. Institute of Solar Terrestrial Physics SB RAS

3. Институт земного магнетизма, ионосферы и распространения радиоволн им. Н.В. Пушкова РАН

4. Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation RAS

Abstract

We analyze the relations between various combinations of peak fluxes and fluences of solar microwave bursts at 35 GHz recorded with the Nobeyama Radio Polarimeters during 1990–2015, and corresponding parameters of proton enhancements with E>100 MeV exceeding 0.1 pfu registered by GOES monitors in near-Earth environment. The highest correlation has been found between the microwave and proton fluences. This fact reflects a dependence of the total number of protons on the total duration of the acceleration process. In the events with strong flares, the correlation coefficients of proton fluences with microwave and soft X-ray fluences are higher than those with speeds of coronal mass ejections. The results indicate a statistically larger contribution of flare processes to acceleration of high-energy protons. Acceleration by shock waves seems to be less important at high energies in events associated with strong flares, although its contribution probably prevails in weaker events. The probability of a detectable proton enhancement was found to directly depend on the peak flux and duration of the microwave burst, that can be used for diagnostics of proton enhancements based on microwave observations.

Publisher

Infra-M Academic Publishing House

Subject

Space and Planetary Science,Atmospheric Science,Geophysics

Reference50 articles.

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