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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 |
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Original file (866 × 676 pixels, file size: 172 KB, MIME type: image/gif)
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
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 |
The following other wikis use this file:
View more global usage of this file.