coronal mass ejection
significant release of plasma and magnetic field from the solar corona
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coronal mass ejection
Summary
coronal mass ejection ranks in the top 1% of general entities by monthly Wikipedia readership (4,326 views/month).[1]
Key Facts
- coronal mass ejection is a type of astrophysical process[2].
- coronal mass ejection is a type of electromagnetic pulse[3].
- coronal mass ejection is part of solar phenomena[4].
- coronal mass ejection's Commons category is recorded as Coronal mass ejection[5].
- coronal mass ejection's facet of is recorded as space weather[6].
- coronal mass ejection's facet of is recorded as Sun's magnetic field[7].
- coronal mass ejection's has immediate cause is recorded as Solar dynamo[8].
- coronal mass ejection's has effect is recorded as geomagnetic storm[9].
Body
Definition and Type
Recorded subclass of include astrophysical process[2] and electromagnetic pulse[3].
Use and Application
coronal mass ejection is part of solar phenomena[4].
Why It Matters
coronal mass ejection ranks in the top 1% of general entities by monthly Wikipedia readership (4,326 views/month).[1] It has Wikipedia articles in 27 language editions, a strong signal of global cultural recognition.[10] It is known by 17 alternative names across languages and contexts.[11]