Active regions in the solar wind from data of comet observations

Details Active regions in the solar wind from data of comet observations Active regions in the solar wind from data of comet observations

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7619036t&link_type=abstract

Active regions in the solar wind from data of comet observations NASA Transl. into ENGLISH from Astrometriya i Astrofiz. (USSR),

Astronomy and Astrophysics

Astronomy

Comet Tails, Solar Activity, Solar Wind, Chromosphere, Latitude, Solar Rotation

Scientific paper

Cases in which the aberrational velocities of the solar wind exceed the upper limit of solar wind velocity (1000 - 1500 km/sec) and when the angles between comet tail axis and the extended radius vector are negative were considered in the light of observational data. These phenomena were found to be related to the 27 day synodic rotation cycle of the sun and are often observed on the same day. A common physical agent is inferred.

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