LARGE-SCALE PROPAGATION PROPERTIES OF AN INTERPLANETARY DISTURBANCE IN ASSOCIATION WITH A "HALO" CORONAL MASS EJECTION ON 27 NOVEMBER 1979
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説明
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 27 November 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.
収録刊行物
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- Proceedings of the Research Institute of Atmospherics, Nagoya University
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Proceedings of the Research Institute of Atmospherics, Nagoya University 36 11-28, 1989-03-25
The Research Institute of Atmospherics, Nagoya University
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詳細情報 詳細情報について
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- CRID
- 1050845763733832832
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- NII論文ID
- 120005607707
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- HANDLE
- 2237/22013
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- ISSN
- 0077264X
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- 本文言語コード
- en
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- 資料種別
- departmental bulletin paper
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- データソース種別
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- IRDB
- CiNii Articles