𝔖 Bobbio Scriptorium
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Energy budget in coronal holes

✍ Scribed by Giancarlo Noci

Book ID
104644496
Publisher
Springer
Year
1973
Tongue
English
Weight
237 KB
Volume
28
Category
Article
ISSN
0038-0938

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✦ Synopsis

It is shown that the constancy of the ratio between conductive flux and pressure squared as one goes from quiet regions to 'holes' (regions of exceptionally low density and temperature) in the solar corona, observed in the case of the first well-studied coronal hole, implies that a strong solar wind is likely to originate in coronal holes.

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