Interplanetary manifestation of the 'halo' coronal mass ejection of November 27, 1979

Details Interplanetary manifestation of the 'halo' coronal mass ejection of November 27, 1979 Interplanetary manifestation of the 'halo' coronal mass ejection of November 27, 1979

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985prian..32...11w&link_type=abstract

Nagoya University, Research Institute of Atmospherics, Proceedings (ISSN 0077-264X), vol. 32, March 1985, p. 11-28.

Physics

Interplanetary Space, Plasma Clouds, Solar Corona, Solar Wind, Stellar Mass Ejection, Directivity, Propagation Velocity, Solar Prominences, Solar Wind Velocity

Scientific paper

This paper presents a case study of a solar wind disturbance associated with the 'halo' coronal mass ejection (CME) of November 27, 1979, which was a 360-deg coronal density enhancement encircling the occulting disk (Howard et al., 1982). The principal sources of solar wind data are spacecraft observations and IPS observations. The interplanetary manifestation of the CME was a quasi-spherical solar wind disturbance. The total angular spread was greater than 70 deg at 1 AU heliocentric distance in the longitudinal direction.

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