Large-scale propagation properties of an interplanetary disturbance in association with a 'halo' coronal mass ejection on 27 November 1979

Details Large-scale propagation properties of an interplanetary disturbance in association with a 'halo' coronal mass ejection on 27 November 1979 Large-scale propagation properties of an interplanetary disturbance in association with a 'halo' coronal mass ejection on 27 November 1979

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nuria..36...11s&link_type=abstract

Nagoya University, Research Institute of Atmospherics, Proceedings (ISSN 0077-264X), vol. 36, March 1989, p. 11-28.

Physics

2

Interplanetary Space, Solar Corona, Solar Wind Velocity, Stellar Mass Ejection, Coronagraphs, Propagation Velocity, Scintillation, Solar Activity

Scientific paper

Propagation properties of an interplanetary disturbance in association with a halo coronal mass ejection (CME), which was observed with the Solwind coronagraph from 08:22 to 09:58 UT on November 27, 1979, are examined utilizing IPS and spacecraft observations. Detailed model-fitting showed that a dip of the propagation speed of the disturbance was situated in the radial direction of the heliospheric current sheet. Quick deceleration of the disturbance along the current sheet is suggested.

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