Currently, sci.esa.int is under review and not being updated. For the latest information and news from ESA science missions and scientific results, please visit esa.int. For a comprehensive overview of ESA’s Science Programme and its missions, please refer to science.esa.int. For in-depth technical information aimed at ESA's scientific communities, you may also wish to consult cosmos.esa.int.

Asset Publisher

Back Coronal Mass Ejection

Coronal Mass Ejection


Date: 23 December 1996
Satellite: SOHO
Depicts: Coronal Mass Ejection
Copyright: SOHO/LASCO (ESA/NASA)

A frame from a movie obtained with the SOHO/LASCO outer coronagraph C3. The field of view of this instrument encompasses 32 diameters of the Sun. To put this in perspective, the diameter of the images is 45 million kilometers at the distance of the Sun, or half of the diameter of the orbit of Mercury. The Sun is located in the constellation Sagittarius. The centre of the Milky Way is visible, as well as the dark interstellar dust rift, which stretches from south to north. The cloudy solar wind can be seen along the ecliptic plane, both over the east and the west limb of the Sun, stronger over the latter. The coronal mass ejection has now stretched out over the whold field of view to a distance of 22.5 million kilometres
Last Update: 1 September 2019
21-Jan-2026 19:44 UT

ShortUrl Portlet

Shortcut URL

https://sci.esa.int/s/8r0aP9w

Also Available As

Related Images

Related Videos

Related Publications

Related Links

Documentation