Other
Scientific paper
Nov 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...274..910k&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 274, Nov. 15, 1983, p. 910-915. Sponsorship: Swiss National Science Foundat
Other
33
H Alpha Line, Microwave Emission, Solar Flares, Solar Radio Bursts, Energy Transfer, Time Lag, Visible Spectrum
Scientific paper
The authors investigate the evolution of an Hα flare and the corresponding microwave burst, both observed with high time resolution and available in digital form. The evolution can clearly be divided into three parts, each of them characterized by a specific mechanism of energy transport. It is shown that one specific Hα kernel has no time delay with respect to the microwave event, whereas the other kernels are delayed as much as 30 s. These facts can be used to establish different transport mechanisms of energy.
Kaempfer N.
Magun Andreas
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