Low-frequency solar radiophysics with LOFAR and FASR

Details Low-frequency solar radiophysics with LOFAR and FASR Low-frequency solar radiophysics with LOFAR and FASR

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004p%26ss...52.1381b&link_type=abstract

Planetary and Space Science, Volume 52, Issue 15, p. 1381-1389.

Physics

8

Scientific paper

Low-frequency radio observations offer unique diagnostics of the solar corona and solar wind. After a prolongued hiatus, there is renewed interest in this important frequency regime. Two new ground-based instruments will provide critical new low-frequency observations: the low-frequency array (LOFAR) and the frequency agile solar radiotelescope (FASR). This brief topical review summarizes low-frequency radio phenomena that will be accessible to detailed study by LOFAR and FASR in the coming decade. Energy release, drivers of space weather, and studies of the solar wind are emphasized. Both instruments are expected to play important roles in both basic research problems and national and international space weather capabilities. While FASR is a solar-dedicated instrument, LOFAR is not. Solar observing requirements for LOFAR are briefly discussed.

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