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..127l&link_type=abstract

Solar Physics, Volume 129, Issue 1, pp.127-132

Physics

1

Scientific paper

We have carried out smoothing by averaging at one second intervals for the solar ultrafast fine structure (UFFS) data of Beijing Observatory at 2.84 GHz on May 16, 1981. The result is compared to the burst record with a time constant τ = 1 s. We find there is a difference of more than one order of magnitude in the flux calibration, and the burst curves are very different. So we are led to think that the UFFS data of the event are not likely to be reliable.

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