Velocity of the solar wind at low heliographic latitudes

Details Velocity of the solar wind at low heliographic latitudes Velocity of the solar wind at low heliographic latitudes

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7618026t&link_type=abstract

Velocity of the solar wind at low heliographic latitudes NASA Transl. into ENGLISH from Astrometriya i Astrofizika (USSR), no. 2

Astronomy and Astrophysics

Astronomy

Solar Wind, Spectroheliographs, Wind Velocity, Aberration, Comet Tails, Plasma Density, Solar Activity

Scientific paper

Data from comet tail deflection observations were used to analyze the relationship between the solar-wind aberrational velocity and the heliographic latitude in the near-equatorial region. The aberrational velocities are found to vary with heliographic latitude, decreasing near the equator and increasing over active solar regions. Active solar-wind zones are found to shift in the course of the 11-year solar-activity cycle. The mean solar-wind aberrations velocity is greater near the solar-activity mimimum than near the maximum. The aberrational velocity at 0.5-2.5 AU is independent of heliocentric distance.

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