Fine Time Structures in Solar Radio Bursts: A Summary of Observations at Four Frequencies

Details Fine Time Structures in Solar Radio Bursts: A Summary of Observations at Four Frequencies Fine Time Structures in Solar Radio Bursts: A Summary of Observations at Four Frequencies

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ap%26ss.272..369x&link_type=abstract

Astrophysics and Space Science, v. 272, Issue 4, p. 369-381 (2000).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

29 fine time structures (FTS) are found in 103 radio bursts observed with YRSOS of high temporal resolution of 1 ms at 4 frequencies (1.42, 2.00 (or2.13), 2.84 and 4.00 (or 4.26) GHz) from January 1990 to January 1994. The various morphologies of FTSs occurring in different phases of flares and the different FTS in the same event may reflect the transitional property of the low-frequency microwave bursts. Most FTSs are probably consisted with the four characteristics observed previously in literatures. The typical and representative events of FTSs and occurrence frequency of each kind are presented in order to explain the multiplicity, breadth and observational characteristics of FTSs in the range of long centimeter to short decimeter wavelengths.

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