2024-03-28T21:16:53Z
https://nagoya.repo.nii.ac.jp/oai
oai:nagoya.repo.nii.ac.jp:00020202
2023-01-26T04:16:14Z
879:1183:1640:1745
INTERPLANETETALY MANIFESTATION OF THE "HALO" CORONAL MASS EJECTION OF NOVEMBER 27, 1979
Watanabe, Takashi
open access
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° 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° at 1 AU heliocentric distance in the longitudinal direction.
The Research Institute of Atmospherics, Nagoya University
1985-03-25
eng
departmental bulletin paper
VoR
http://hdl.handle.net/2237/22115
https://nagoya.repo.nii.ac.jp/records/20202
0077-264X
Proceedings of the Research Institute of Atmospherics, Nagoya University
32
11
28
https://nagoya.repo.nii.ac.jp/record/20202/files/proria_32_11.pdf
application/pdf
3.0 MB
2018-02-21