Abstract
The characteristics of the millisecond spikes with short duration and weak flux density which were observed with high time resolution (1 ms) at 1420, 2000 and 2840 MHz during the great type IV solar radio burst of 30 July 1990 are introduced in detail in this article. The time profiles of the spikes are statistically analyzed and the parameters of the spike source are also estimated.
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Wang, M., Xie, R. Millisecond spikes in a short decimetric solar radio burst. Solar Physics 185, 351–360 (1999). https://doi.org/10.1023/A:1005101001388
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DOI: https://doi.org/10.1023/A:1005101001388