Magnetic fields and flows between 1 AU and 0.3 AU during the primary mission of HELIOS 1

Details Magnetic fields and flows between 1 AU and 0.3 AU during the primary mission of HELIOS 1 Magnetic fields and flows between 1 AU and 0.3 AU during the primary mission of HELIOS 1

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stin...7817964b&link_type=abstract

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Computer Science

Helios 1, Interplanetary Magnetic Fields, Magnetic Flux, Ion Temperature, Photosphere, Solar Corona, Solar Wind

Scientific paper

The recurrent flow and field patterns observed by HELIOS 1, and the relation between these patterns and coronal holes are discussed. Four types of recurrent patterns were observed: a large recurrent stream, a recurrent slow (quiet) flow, a rapidly evolving flow, and a recurrent compound stream. There recurrent streams were not stationary, for although the sources recurred at approximately the same longitudes on successive rotations, the shapes and latitudinal patterns changed from one rotation to the next. A type of magnetic field and plasma structure characterized by a low ion temperature and a high magnetic field intensity is described as well as the structures of stream boundaries between the sun at approximately 0.3 AU.

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