Image:Heliospheric-current-sheet.gif

From Wikipedia, the free encyclopedia

Wikimedia Commons logo This is a file from the Wikimedia Commons. The description on its description page there is shown below.
Commons is a freely licensed media file repository. You can help.
Description

The en:heliospheric current sheet 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.

Source

[1] from http://lepmfi.gsfc.nasa.gov/mfi/hcs/hcs_shape.html.

Date

2005-11-20 (first version); 2005-11-24 (last version)

Author

Werner Heil (see "other version" below).

Permission
(Reusing this image)

PD-LAYOUT; PD-USGOV-NASA.

Other versions http://wso.stanford.edu/gifs/HCS.html

[edit] License information

Public domain
This file is in the public domain because it was created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (NASA copyright policy page or JPL Image Use Policy).

Deutsch | English | Español | Français | Nederlands | Português | Русский | ‪中文(简体)‬ | ‪中文(繁體)‬ | +/-

Warning sign
Warnings:

[edit] 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/TimeDimensionsUserComment
current04:11, 9 June 2007866×676 (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)
The following pages on the English Wikipedia link to this file (pages on other projects are not listed):