@article{oai:nagoya.repo.nii.ac.jp:00020202,
 author = {Watanabe, Takashi},
 journal = {Proceedings of the Research Institute of Atmospherics, Nagoya University},
 month = {Mar},
 note = {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.},
 pages = {11--28},
 title = {INTERPLANETETALY MANIFESTATION OF THE "HALO" CORONAL MASS EJECTION OF NOVEMBER 27, 1979},
 volume = {32},
 year = {1985}
}