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Datoteka:Heliospheric-current-sheet.gif

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Opis izmjene

Opis
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
Izvor [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).
Ostale verzije http://wso.stanford.edu/gifs/HCS.html

Licenciranje

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:

Izvorna evidencija postavljanja

(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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Datum/vrijemeMinijaturaDimenzijeKorisnikKomentar
aktualna20:07, 3 oktobar 2013Minijatura verzije (20:07, 3 oktobar 2013)866 × 676 (172 kB)HohumLevels
06:11, 9 juni 2007Minijatura verzije (06:11, 9 juni 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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