1D Solar Image Synthesis: A Multifrequency Analysis

Details 1D Solar Image Synthesis: A Multifrequency Analysis 1D Solar Image Synthesis: A Multifrequency Analysis

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap%26ss.282..255v&link_type=abstract

Astrophysics and Space Science, v. 282, Issue 1, p. 255-264 (2002).

Astronomy and Astrophysics

Astrophysics

Scientific paper

The radio emission from the solar corona is related to the configuration of the inner atmosphere. By studying the Sun at multiple frequencies, different layers of plasma in solar atmosphere are probed. We use the Mauritius Radio Telescope. The quiet Sun period, difference maps using synthesized 1D maps reveal a certain regular feature, the origin of which is not thoroughly understood and which is attributed to the solar differential rotation. For the active Sun period, the coronal emission is linked to the magnetic field configuration originating from the inner atmosphere. As expected, a strong correlation exists between the MRT 151 MHz and Nancay 164 MHz radio emission.

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