Variation of the mm Radio Emission in the Polar Zones of the Sun

Details Variation of the mm Radio Emission in the Polar Zones of the Sun Variation of the mm Radio Emission in the Polar Zones of the Sun

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.2.67k&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

We analyzed the radio emission at 37 GHz obtained from the polar zones of the Sun. These measurements were done at the Metsahovi Radiotelescope during 2005-2008.
In this work, we pay attention to the some characteristic of the enhanced temperature regions near the poles of the Sun.
Results obtained in this study showed that intensity of the mm radio emission changes in time interval beginning from 1 to 4 hours. Also, the FFT (Fast Fourier Transform) analyses showed that in the radio emission from the polar zones take place on 5-minute oscillations.

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