Long-term evolution of coronal magnetic fields based on noise storm continuum observations in the 20th and 21st cycle

Details Long-term evolution of coronal magnetic fields based on noise storm continuum observations in the 20th and 21st cycle Long-term evolution of coronal magnetic fields based on noise storm continuum observations in the 20th and 21st cycle

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.285..157b&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Reconnection in Space Plasma, Volume 2 p 157-161 (SEE N89-24974 1

Physics

Solar Corona, Solar Cycles, Solar Magnetic Field, Solar Radio Bursts, Solar Storms, Sunspots

Scientific paper

Based on the noise storms of cycles 20 and 21, the long-term variations of the radiation signatures of sunspot groups during a solar cycle were studied. The results suggest that nonpotential loops favoring the emission of a strong type 1 continuum at the low frequencies (less than 100MHz) tend to exist more frequently above the sunspot groups in the later phase of a solar cycle.

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