Physics
Scientific paper
Nov 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...45..189k&link_type=abstract
Solar Physics, vol. 45, Nov. 1975, p. 189-197. Research supported by the Conselho Nacional de Pesquisas, Comissao de Aperfeicoam
Physics
2
Microwave Emission, Solar Flares, Solar Radio Bursts, Ionospheric Disturbances, Radio Telescopes, Solar Activity Effects
Scientific paper
The active region McMath 10433 was the source of several flares and radio outbursts during the early part of July 1974. This region was tracked continuously for several periods during the month at 22.2 GHz using a telescope with a 4-min beam. Comparison with results obtained simultaneously with a normal 7-GHz solar-patrol instrument indicates that there is important burst activity occurring at levels below the detection limit of normal solar-patrol instruments. The time-development morphology of these bursts is similar to those normally observed and has enabled the simple events to be reinterpreted. A completely new type of event - the fast absorption - has also been recognized. The correlation of the microwave events with sudden-phase-anomaly events observed in VLF propagation is also discussed.
Blakey J. R.
Iacomo Jr. P.
Kaufmann Patrik
Koppe E. H.
Marques Dos Santos P.
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