Birefringence effect in the solar corona

Details Birefringence effect in the solar corona Birefringence effect in the solar corona

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..605f&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Solar Radio Emission, Microwave Millisecond Pulsations, Group Delay

Scientific paper

Group delay between two magnetoionic modes is discovered and spectrally confirmed for the first time for quasiperiodic narrowband millisecond solar radio pulsations. Analysis of cross- and auto-delays proves that both (X and O) modes originate at the same source, so the radiation is weakly polarized originally. This finding allows to specify the emission mechanism of the pulsations to be nonlinear plasma mechanism operating at the second harmonics. Physical parameters of the solar corona are determined by the use of the theory of nonlinear plasma mechanism, they agree well with independent observations of solar millisecond pulsations.

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