Ultra-fast fine structures of a microwave outburst

Details Ultra-fast fine structures of a microwave outburst Ultra-fast fine structures of a microwave outburst

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sssmp..25..422z&link_type=abstract

Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences, vol. 25, Apr. 1982, p. 422-429.

Astronomy and Astrophysics

Astronomy

22

Astronomical Spectroscopy, Fine Structure, Microwave Spectra, Solar Radio Bursts, Solar Flares, Temporal Resolution

Scientific paper

Data acquired from 1 msec observations of a solar microwave outburst at 2.84 GHz on May 16, 1981 are discussed. An abundance of ultrafast fine structures (UFFS) was detected during the rise and highest peak phase, along with abrupt rising and falling of the flux density. A quasi-periodic oscillation lasting two seconds was confirmed, indicating that the variations and characteristics of the microbursts contain information on the physical events causing solar flares and bursts.

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