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• W2018034653 abstract "A comparative analysis of the fine time structure of microwave and hard X-ray emissions from the flare event on 1992 November 5 is given. Based on wavelet analysis, quasi-periodic pulsations with a fundamental period of 6 s in both wave bands have been revealed. The anticorrelation of time profiles of microwave and hard X-ray emissions as well as time delays between the emission peaks in different wave bands are explained by the excitation of sausage oscillations of a flare loop modelling by a magnetic trap. It has been shown that the intermediate pitch angle diffusion regime of trapped electrons into the loss-cone should be realized in flare loops. The relation between time delays of emission peaks at different wave bands and the pulse duration has been investigated." @default.
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• W2018034653 date "2013-12-05" @default.
• W2018034653 modified "2023-09-24" @default.
• W2018034653 title "Oscillating Magnetic Trap and Non-Thermal Emission from Solar Flares" @default.
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• W2018034653 doi "https://doi.org/10.1093/pasj/65.sp1.s6" @default.
• W2018034653 hasPublicationYear "2013" @default.
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