Physics
Scientific paper
Nov 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..161..393k&link_type=abstract
Solar Physics, Volume 161, Issue 2, pp.393-405
Physics
5
Scientific paper
Recent technical progress of solar radio spectrography is concerned with digital data recording, the achievement of high time and frequency resolution, and with an improved coverage of the radio range at short and long wavelengths. A spatially-distributed network of radio spectrographs allows for complementary information about solar events and periods of activity selected for detailed investigation. By modern radio spectrographs a wealth of not yet adequately classified spectral fine structures can be observed, some of them potentially intimately related to effects of fragmentation of flare energy and/or to processes related to coronal heating. Requirements for the choice of technical parameters of solar spectrographs for checking theoretical models of fundamental processes of energy release are reflected in modern instruments. Prospects for future observations are briefly included.
Kruger Andrew
Voigt W.
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