The determination of radio-halo size on the basis of fluctuations of diffuse radio emission

Details The determination of radio-halo size on the basis of fluctuations of diffuse radio emission The determination of radio-halo size on the basis of fluctuations of diffuse radio emission

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..490l&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, June 1991, p. 490-494. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Diffuse Radiation, Galactic Structure, Halos, Magnetohydrodynamic Turbulence, Synchrotron Radiation, Cross Correlation, Magnetic Field Configurations, Radio Astronomy

Scientific paper

A novel method for determining the size of the Galactic radio halo based on a statistical study of synchrotron fluctuations is presented. H II regions are used as distance indicators. A knowledge of radio-halo size will enhance the possibilities of the statistical method of investigating MHD turbulence based on a study of the correlation functions of diffuse synchrotron radiation.

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