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Derivation of the MC diameter after flux rope fitting
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Version 2
Version 2 2019-02-11, 09:52
Version 2 2019-02-11, 09:52
Version 1 2019-01-17, 10:50
Version 1 2019-01-17, 10:50
journal contribution
posted on 2019-02-11, 09:52
authored by
Tanja Amerstorfer
Tanja Amerstorfer
This is a short derivation of how the diameter of a magnetic cloud can be calculated after the flux rope was fitted by using the Lundquist or the Gold-Hoyle fitting method.
No warranty is given or implied!
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Categories
Solar physics
Keywords
magnetic clouds
fitting
interplanetary coronal mass ejections
flux rope
Space and Solar Physics
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CC BY 4.0
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