Coronal mass ejection | Wikipedia audio article
Channel: wikipedia tts
Date: 2019-03-26

This is an audio version of the Wikipedia Article:
https://en.wikipedia.org/wiki/Coronal_mass_ejection


00:00:47 1 Description
00:01:34 2 Cause
00:03:08 3 Impact on Earth
00:04:53 4 Physical properties
00:07:44 5 Association with other solar phenomena
00:09:21 6 Theoretical models
00:10:32 7 Interplanetary coronal mass ejections
00:11:51 8 Related solar observation missions
00:12:02 8.1 NASA mission iWind/i
00:13:02 8.2 NASA mission iSTEREO/i
00:13:41 8.3 NASA mission iParker Solar Probe/i
00:14:02 9 History
00:14:11 9.1 First traces
00:15:32 9.2 First clear detections
00:17:06 9.3 1989-present
00:19:57 10 Future risk
00:20:20 11 Stellar coronal mass ejections
00:21:18 12 See also



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SUMMARY
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A coronal mass ejection (CME) is a significant release of plasma and accompanying magnetic field from the solar corona. They often follow solar flares and are normally present during a solar prominence eruption. The plasma is released into the solar wind, and can be observed in coronagraph imagery.Coronal mass ejections are often associated with other forms of solar activity, but a broadly accepted theoretical understanding of these relationships has not been established. CMEs most often originate from active regions on the Sun's surface, such as groupings of sunspots associated with frequent flares. Near solar maxima, the Sun produces about three CMEs every day, whereas near solar minima, there is about one CME every five days.