Thermal nonequilibrium limit cycles, previously seen in closed coronal loops, also occur in a transonic solar wind when foot-point heating exceeds about 3.5 times the global heating.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Simulation of Thermal Nonequilibrium Cycles in the Solar Wind
Thermal nonequilibrium limit cycles, previously seen in closed coronal loops, also occur in a transonic solar wind when foot-point heating exceeds about 3.5 times the global heating.