Dispersion analysis of solar wind velocity

Details Dispersion analysis of solar wind velocity Dispersion analysis of solar wind velocity

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....61...13l&link_type=abstract

Astronomy and Astrophysics, vol. 61, no. 1, Oct. 1977, p. 13-16.

Astronomy and Astrophysics

Astrophysics

2

Diffraction Patterns, Scintillation, Solar Wind Velocity, Wave Dispersion, Astrometry, Diurnal Variations, Spectrum Analysis

Scientific paper

Three site observations of interplanetary scintillations are used to estimate the dispersion in diffraction-pattern velocity. The mean velocity and dispersion change considerably from day to day. For the eight source days analyzed, the standard deviation of velocity varied from 17% to 37% of the mean. If the temporal spectrum is used to estimate the spatial spectrum, then to the extent that the dispersion in diffraction-pattern velocity is not constant, a correction must be applied. This may occur for frequencies below 1 Hz.

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