Very long baseline interferometer measurements of plasma turbulence in the solar wind

Details Very long baseline interferometer measurements of plasma turbulence in the solar wind Very long baseline interferometer measurements of plasma turbulence in the solar wind

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jgr....9717141s&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 97, no. A11, p. 17,141-17,151.

Other

4

Plasma Turbulence, Solar Wind, Very Long Base Interferometry, Power Spectra, Very Large Array (Vla), Very Long Baseline Array (Vlba)

Scientific paper

Plasma turbulence in the solar wind is investigated using angular broadening VLBI measurements at 4.99 GHz of ten extragalactic compact radio sources (quasars). The measured broadening size was corrected for intrinsic source structures which were obtained from separate VLBI observations. It was found that the measured angular sizes are considerably less than those predicted by the Erickson's (1964) empirical relationship, as well as by two other models for the strength of scattering as a function of solar elongation. However, the measurements are in good agreement with a model for the spatial power spectrum of turbulence, proposed by Coles and Harmon (1989).

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