Radio Wave Scattering in the Solar Wind

Details Radio Wave Scattering in the Solar Wind Radio Wave Scattering in the Solar Wind

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...19712801d&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #128.01; Bulletin of the American Astronomical Society, Vol. 33, p.710

Astronomy and Astrophysics

Astronomy

Scientific paper

We have observed 60 VLBA calibrator sources affected to varying degrees by scattering in the solar wind. Our goal was to map the properties of solar wind turbulence over a wide range of solar elongations ranging from a few degrees to over 100 degrees in as short a time as possible. The final aim is to get information about (a) the anisotropy in the solar wind, (b) variation of scattering size with solar distance and (c) spectrum of the density of fluctuations on the VLBA scales. Each source was observed at two epochs at three wavelengths each time using the full VLBA. We present some preliminary findings.

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