Sources of magnetic fields in recurrent interplanetary streams

Details Sources of magnetic fields in recurrent interplanetary streams Sources of magnetic fields in recurrent interplanetary streams

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978jgr....83.4177b&link_type=abstract

Journal of Geophysical Research, vol. 83, Sept. 1, 1978, p. 4177-4185.

Physics

25

Interplanetary Magnetic Fields, Magnetic Field Configurations, Plasma Dynamics, Satellite Observation, Solar Activity, Lines Of Force, Photosphere, Plasma Diagnostics, Solar Corona, Time Response

Scientific paper

The paper examines sources of magnetic fields in recurrent streams observed by the Imp 8 and Heos spacecraft at 1 AU and by Mariner 10 en route to Mercury between October 31, 1973 and February 9, 1974, during Carrington rotations 1607-1610. Although most fields and plasmas at 1 AU were related to coronal holes and the magnetic field lines were open in those holes, some of the magnetic fields and plasmas at 1 AU were related to open field line regions on the sun which were not associated with known coronal holes, indicating that open field lines may be more basic than coronal holes as sources of the solar wind. Magnetic field intensities in five equatorial coronal holes, certain photospheric magnetic fields, and the coronal footprints of the sector boundaries on the source surface are characterized.

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