Súbor:Heliospheric-current-sheet.gif

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PopisHeliospheric-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.
Dátum	2000 or before
Zdroj	[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
Autor	Werner Heil, NASA (see "other version" below).
Ďalšie verzie	http://wso.stanford.edu/gifs/HCS.html

	This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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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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	Dátum/Čas	Náhľad	Rozmery	Používateľ	Komentár
aktuálna	18:07, 3. október 2013		866 × 676 (172 KB)	Hohum	Levels
	04:11, 9. jún 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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