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- W1989757210 abstract "Abstract Using the data of the double quasi-periodic pulsation in the solar radio burst observed simultaneously by Nanjing University and Beijing Normal University with time resolutions of 1s and 10ms at 9.375 and 15 GHz, respectively, on 1990 May 23, at 0400–0451, along with the data of the associated phenomena in radio, optical and soft X-ray published in S.G.D., we propose a model of oscillation of Alfven and fast magneto-acoustic waves, triggered by interaction between nonthermal (microwave burst) and thermal (soft X-ray flare) processes in a flare loop, to account for the observed pulsation. As a by-product, average values of the physical quantities T, N, B of the burst source region are calculated." @default.
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- W1989757210 date "1993-07-01" @default.
- W1989757210 modified "2023-09-27" @default.
- W1989757210 title "A possible mechanism for the double quasi-periodic pulsation in solar radio bursts at short cm waves" @default.
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- W1989757210 doi "https://doi.org/10.1016/0275-1062(93)90100-4" @default.
- W1989757210 hasPublicationYear "1993" @default.
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