Interstellar scattering medium - Determination of the distribution profile by a space tomography method

Details Interstellar scattering medium - Determination of the distribution profile by a space tomography method Interstellar scattering medium - Determination of the distribution profile by a space tomography method

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..963b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Nov. 1988, p. 963-969. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

2

Interstellar Matter, Plasma Turbulence, Pulsars, Tomography, Wave Scattering, Cosmic Plasma, Electron Density Profiles, Milky Way Galaxy, Radio Emission

Scientific paper

Data concerning pulsar radiation scattering are used in the space tomography method to construct profiles of the scattering medium for the inner regions of the Galactic disk for three different distributions of average electron density. The existence of two main components of turbulent plasma distribution is confirmed: an oscillating component and a monotonically increasing component in the direction of the Galactic center. Also, several problems associated with the space tomography method and the accuracy of the results are examined.

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