Observations and analyses of solar pulsations in the low part of microwaves.

Details Observations and analyses of solar pulsations in the low part of microwaves. Observations and analyses of solar pulsations in the low part of microwaves.

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999acasn..40..263w&link_type=abstract

Acta Astron. Sin., Vol. 40, No. 3, p. 263 - 271

Astronomy and Astrophysics

Astronomy

Solar Microwave Bursts: Morphology, Solar Microwave Bursts: Periods

Scientific paper

The twelve pulsation events recorded by the solar radio synchronous observation system of four frequencies (1420, 2000, 2840 and 4000 MHz) with high time resolution at Yunnan Observatory from Dec. 1989 to Jan. 1994 are investigated. Several characteristics of the microwave pulsations in this band are found, such as the long period (about 50 s) and short period (dozens of ms) pulsations. The morphology, period and bandwidth of pulations are analyzed. A discussion of these characteristics is presented.

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