COCONUT simulations find open magnetic flux falls by up to 45% within 3 solar radii, matches in-situ observations, and varies by a factor of 1.4 during solar maximum.
A., Miki ´c, Z., Biesecker, D
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT
COCONUT simulations find open magnetic flux falls by up to 45% within 3 solar radii, matches in-situ observations, and varies by a factor of 1.4 during solar maximum.