On the Origin of Long Time-Scale Pulsar Scintillations - Part Three - the Density Fluctuations in Our Galaxy

Details On the Origin of Long Time-Scale Pulsar Scintillations - Part Three - the Density Fluctuations in Our Galaxy On the Origin of Long Time-Scale Pulsar Scintillations - Part Three - the Density Fluctuations in Our Galaxy

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.190..385h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 190, P. 385, 1980

Astronomy and Astrophysics

Astronomy

7

Scientific paper

We discuss the form of the spectrum of density fluctuations in the interstellar medium. A simple stratified model of the Galaxy is considered, and the variation of scattering with galactic latitude and longitude is discussed. The density fluctuations have a scale height ˜71 pc. Scattering and diffuse Hα emission in the Galaxy appear to be correlated.

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