Lêer:Heliospheric-current-sheet.gif

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Oorspronklike lêer ‎(866 × 676 piksels, lêergrootte: 172 KG, MIME-tipe: image/gif)

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Opsomming

Beskrywing
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.
Datum or before
Bron [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
Outeur Werner Heil, NASA (see "other version" below).
Ander weergawes http://wso.stanford.edu/gifs/HCS.html

Lisensiëring

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.)
Warnings:

Oorspronklike oplaailogboek

(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

Lêergeskiedenis

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Datum/TydDuimnaelDimensiesGebruikerOpmerking
huidig18:07, 3 Oktober 2013Duimnaelskets vir weergawe vanaf 18:07, 3 Oktober 2013866 × 676 (172 KG)HohumLevels
04:11, 9 Junie 2007Duimnaelskets vir weergawe vanaf 04:11, 9 Junie 2007866 × 676 (172 KG)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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