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ߞߐߕߐ߮:Heliospheric-current-sheet.gif

ߞߐߕߐ߮ ߓߊߛߎ߲ ‏(߈߆߆ × ߆߇߆ ߖߌ߬ߦߊ߬ߘߊ߲ߕߊ߸ ߞߐߕߐ߮ ߢߊ߲ߞߊ߲: ߁߇߂ KB߸ MIME ߛߎ߮ߦߊ:image/gif)

ߘߐ߬ߛߙߋ ߣߌ߲߬ ߦߋ߫ ߦߊ߲߬ ߠߋ߫ Wikimedia Commons ߖߊ߬ߕߋ߬ߘߐ߬ߛߌ߮ ߕߐ߭ ߟߎ߬ ߞߏ߬ߣߌ߲ ߘߌ߫ ߛߴߊ߬ ߟߊߓߊ߯ߙߊ߫ ߟߊ߫. ߊ߬ ߕߐ߯ ߛߓߍߟߌ ߦߙߐ ߞߐߕߐ߮ ߞߊ߲߬ߛߓߍߟߌ ߞߐߜߍ ߟߋ߬ ߦߋ߫ ߘߎ߰ߟߊ ߘߐ߫ ߣߌ߲߬.

ߟߊߘߛߏߣߍ߲

ߕߐ߯ߟߊߘߏ߲
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.
ߕߎ߬ߡߊ߬ߘߊ or before
ߛߎ߲ [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
ߛߓߍߦߟߊ Werner Heil, NASA (see "other version" below).
Other versions http://wso.stanford.edu/gifs/HCS.html

ߟߊ߬ߘߌ߬ߢߍ߬ߟߌ ߦߴߌ ߘߐ߫

Public domain 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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ߞߍߛߊ߲ߞߏ߁߈:߀߇, ߃ ߞߏ߲ߓߌߕߌ߮ ߂߀߁߃ߡߊ߬ߦߟߍ߬ߡߊ߲߬ߠߌ߲ ߠߊߘߐ߯ߦߊߣߍ߲ ߕߎ߬ߡߊ߬ߘߊ ߣߌ߲߬ ߁߈:߀߇, ߃ ߞߏ߲ߓߌߕߌ߮ ߂߀߁߃ ߠߊ߫߈߆߆ × ߆߇߆ (߁߇߂ KB)HohumLevels
߀߄:߁߁, ߉ ߥߊ߬ߛߌ߬ߥߙߊ ߂߀߀߇ߡߊ߬ߦߟߍ߬ߡߊ߲߬ߠߌ߲ ߠߊߘߐ߯ߦߊߣߍ߲ ߕߎ߬ߡߊ߬ߘߊ ߣߌ߲߬ ߀߄:߁߁, ߉ ߥߊ߬ߛߌ߬ߥߙߊ ߂߀߀߇ ߠߊ߫߈߆߆ × ߆߇߆ (߁߇߂ 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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