On the interpretation of the 2.84 GHz solar UFFS data of May 16, 1981

Details On the interpretation of the 2.84 GHz solar UFFS data of May 16, 1981 On the interpretation of the 2.84 GHz solar UFFS data of May 16, 1981

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..129..127z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 129, Sept. 1990, p. 127-132.

Physics

2

Fine Structure, Millimeter Waves, Solar Flares, Solar Radio Bursts, Solar X-Rays, Polarization Characteristics, Solar Cycles, Solar Oscillations

Scientific paper

Smoothing has been conducted by averaging at 1-second intervals for the solar ultrafast fine structure (UFFS) data of Beijing Laboratory at 2.84 GHz on May 16, 1981. The result obtained is compared to the burst record with a time constant of 1 sec. There is a difference of more than one order of magnitude in the flux calibration, and the burst curves are very different; the UFFS data of the event are therefore not likely to be reliable.

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