Coronal Mass

Some articles on coronal mass, coronal:

Solar Wind - Emission - Coronal Mass Ejection
... by large, fast-moving bursts of plasma called interplanetary coronal mass ejections, or ICMEs ... ICMEs are the interplanetary manifestation of solar coronal mass ejections, which are caused by release of magnetic energy at the Sun ...
Coronal Mass Ejection
... A coronal mass ejection (CME) is a massive burst of solar wind and magnetic fields rising above the solar corona or being released into space ... Coronal mass ejections are often associated with other forms of solar activity, most notably solar flares, but a causal relationship has not been established ...
Coronal Mass Ejection - Physical Properties
... A typical coronal mass ejection may have any or all of three distinctive features a cavity of low electron density, a dense core (the prominence, which appears as a bright region on coronagraph images ... solar minimum, CMEs form primarily in the coronal streamer belt near the solar magnetic equator ... Coronal mass ejections reach velocities between 20km/s to 3200km/s with an average speed of 489km/s, based on SOHO/LASCO measurements between 1996 and 2003 ...

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