File:Heliospheric-current-sheet.gif
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Summary
DescriptionHeliospheric-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. |
Date | or before |
Source | [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 |
Author | Werner Heil, NASA (see "other version" below). |
Other versions | http://wso.stanford.edu/gifs/HCS.html |
Licensing
Public domainPublic domainfalsefalse |
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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Original upload log
(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
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 18:07, 3 October 2013 | 866 × 676 (172 KB) | Hohum | Levels | |
04:11, 9 June 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 |
File usage
The following pages on the English Wikipedia use this file (pages on other projects are not listed):
- Coronal mass ejection
- Current sheet
- ESA Vigil
- Geomagnetic storm
- Heliophysics
- Heliosphere
- Heliospheric current sheet
- Interplanetary magnetic field
- Interplanetary medium
- Solar flare
- Solar phenomena
- Solar wind
- Sunspot
- Van Allen radiation belt
- Talk:Solar System/Archive 5
- User:Mwolczko/sandbox
- User:SteveChervitzTrutane
- Template:Heliophysics
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