Fail:Heliospheric-current-sheet.gif

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Ringkasan

KeteranganHeliospheric-current-sheet.gif	English: The heliospheric current sheet (HCS) results from the influence of the Sun's rotating magnetic field on the plasma in the interplanetary medium (solar wind). The wavy spiral shape has been likened to a ballerina's skirt. Русский: Гелиосферный токовый слой является результатом воздействия вращающегося магнитного поля Солнца на плазму (солнечный ветер), находящуюся в межпланетной среде. Волнистую спиральную форму можно уподобить юбке балерины.
Tarikh	2000 or before
Sumber	[1] ^{[dead link]} from http://lepmfi.gsfc.nasa.gov/mfi/hcs/hcs_shape.html ^{[dead link]}. https://web.archive.org/web/20090423072931/https://lepmfi.gsfc.nasa.gov/mfi/hcs/hcs_shape.html
Pengarang	Werner Heil, NASA (see "other version" below).
Versi lain	http://wso.stanford.edu/gifs/HCS.html

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(All user names refer to en.wikipedia)

2005-11-24 11:08 Iantresman 800×560×8 (39813 bytes) == Summary == [[Heliospheric current sheet]], the largest structure in the Solar System, resulting from the influence of the [[Sun]]'s rotating magnetic field on the [[plasma]] in the [[interplanetary medium]] (Solar Wind). The wavy [[Parker spiral|spiral
2005-11-20 13:32 Iantresman 800×560×8 (40735 bytes) [[Heliospheric current sheet]], the largest structure in the Solar System, resulting from the influence of the Sun's rotating magnetic field on the plasma in the [[interplanetary medium]] (Solar Wind). The wavy spiral shape has been likened to a ballerina

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	Tarikh/Waktu	Gambar kenit	Ukuran	Pengguna	Komen
semasa	18:07, 3 Oktober 2013		866 × 676 (172 KB)	Hohum	Levels
	04:11, 9 Jun 2007		866 × 676 (172 KB)	Chanueting	{{Information \|Description=The en:heliospheric current sheet results from the influence of the en:Sun's rotating magnetic field on the plasma in the en:interplanetary medium (solar wind). The wavy [[:en:Parker spira

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