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- Dubinin Eduard
- Max-Planck-Institut für Aeronomie Space Research Institute, Russian Academy of Sciences International Space Science Institute (ISSI)
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- Sauer Konrad
- Max-Planck-Institut für Aeronomie International Space Science Institute (ISSI)
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- Delva Magda
- Space Research Institute, Austrian Academy of Sciences International Space Science Institute (ISSI)
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- Skalsky Aleksandr
- Space Research Institute, Russian Academy of Sciences International Space Science Institute (ISSI)
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A noticeable bending of the magnetic field lines in the Martian upstream region is observed. Variations of the field are controlled by the IMF and the foreshock geometry. The sign of ΔB changes at the crossing of the tangent surface, which borders foreshock and the undisturbed solar wind. Perturbations of the magnetic field are centered at the plane which is normal to the tangent surface and intersects the bow shock at the tangent point. All observed signatures suggest that the current, providing field variations, is localized near the tangent surface. Although, two models are discussed, neither of them is able to explain all observed features satisfactorily.
収録刊行物
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- Earth, Planets and Space
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Earth, Planets and Space 50 (3), 295-302, 1998
地球電磁気・地球惑星圏学会 、公益社団法人 日本地震学会、特定非営利活動法人 日本火山学会、日本測地学会、日本惑星科学会
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詳細情報
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- CRID
- 1390001206510840448
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- NII論文ID
- 10002206317
- 130003780711
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- NII書誌ID
- AA11211921
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- ISSN
- 18805981
- 13438832
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- 本文言語コード
- en
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- データソース種別
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- JaLC
- Crossref
- CiNii Articles
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- 抄録ライセンスフラグ
- 使用不可