Ultra-low-frequency background radiation of the Galaxy.

Details Ultra-low-frequency background radiation of the Galaxy. Ultra-low-frequency background radiation of the Galaxy.

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...293..565f&link_type=abstract

Astronomy and Astrophysics 293, 565-571 (1995)

Astronomy and Astrophysics

Astrophysics

16

Interstellar Medium: General, Radiation Mechanisms: Non Thermal, Background Radiations, Radio Continuum: Ism

Scientific paper

The paper examines the lowest frequency observations of the galactic radio noise published by Brown (1973) and their relationship to the properties of the local interstellar medium. We find that the Razin cut-off frequency in the warm gas is about 0.3MHz and nearly constant, which provides a sharp decrease of the galactic spectrum at f<0.6MHz. The synchrotron emissivity in the tenuous (coronal) gas is found to be much less than that in the warm gas, while it is responsible for the observed excess of the emission at 0.13

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