Physics
Scientific paper
Jun 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993acasn..34..189h&link_type=abstract
Acta Astronomica Sinica (ISSN 0001-5245), vol. 34, no. 2, p. 197-201
Physics
1
Flux (Rate), Solar Flux, Solar Physics, Solar Radio Bursts, Statistical Analysis, Sun, Energy Conservation, Frequency Stability, Narrowband, Wave-Particle Interactions
Scientific paper
The main purpose of this work is to explain the statistical relationship, for example, the repetition rate of the pulsation is proportional to the increase of the radio flux. On the assumption of energy conservation in wave-particle interaction, the saturation time is inversely proportional to the increase of the radio flux, which can be used to explain the R-S relationship. The other predictions are also consistent with the pulsation at 3 cm band, such as the modulation degree is directly proportional to the period of an individual pulsation and is inversely proportional to the radio burst flux, the burst energy corresponding to individual pulsation increases with the increase of the radio burst flux. The differences of the time scale and the value of the gradient in the R-S relationship at 3 cm and 1.36 cm are also explained.
Huang Guang Li
Li Jian-Ping
Qin Zhi-Hai
Wang Ren-Ying
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