The physical conditions in the source of a type I solar radio noise storm

Details The physical conditions in the source of a type I solar radio noise storm The physical conditions in the source of a type I solar radio noise storm

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..840g&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Sept. 1988, p. 840-844. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Noise Storms, Solar Atmosphere, Solar Radio Emission, Electron Density Profiles, Solar Activity, Solar Cycles, Solar Magnetic Field, Solar Wind, Very Large Array (Vla)

Scientific paper

A two-dimensional map of the radio source of a May 20, 1966 radio noise storm at frequencies close to 200 MHz is compared with the distribution of the electron density on this day and magnetic field strength calculations. It is shown that the radio emission of the noise storm in the meter wave-length range is generated close to the upper hybrid frequency.

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