Fractal properties of the IMF and the Earth's magnetotail field

• Kabin K.

  Space Physics Research Laboratory, Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan

• Papitashvili V. O.

  Space Physics Research Laboratory, Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan

抄録

The time series of the interplanetary and Earth's magnetotail magnetic fields are analyzed. The data subsets taken by the IMP 8 spacecraft outside and inside of the Earth's magnetosphere show clearly the fractal properties: their “box dimensions” are found to be close to 1.7 and 1.5 respectively. It is shown that data gaps have a little effect on the results. The magnetic field increment distributions are found to be non-Gaussian, but self-affine.

収録刊行物

• Ｅａｒｔｈ，　Ｐｌａｎｅｔｓ　ａｎｄ　Ｓｐａｃｅ

  Ｅａｒｔｈ，　Ｐｌａｎｅｔｓ　ａｎｄ　Ｓｐａｃｅ 50 (1), 87-90, 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

キーワード

• Space and Planetary Science
• Geology

詳細情報

• CRID: 1390001206508906880
• NII論文ID: 10002205719
• NII論文ID: 130003955859
• NII書誌ID: AA11211921
• DOI: 10.1186/bf03352089
• ISSN: 18805981
• ISSN: 13438832
• Web Site: https://link.springer.com/content/pdf/10.1186/BF03352089.pdf
• Web Site: https://link.springer.com/article/10.1186/BF03352089/fulltext.html
• Web Site: http://link.springer.com/content/pdf/10.1186/BF03352089
• 本文言語コード: en
• データソース種別:
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• 抄録ライセンスフラグ: 使用不可