Prefer a chat interface with context about you and your work?
Magnetohydrostatic equilibrium โ I. Three-dimensional open magnetic flux tube in the stratified solar atmosphere
A single open magnetic flux tube spanning the solar photosphere (solar radius R ) and the lower corona (R + 10 Mm) is modelled in magnetohydrostatic equilibrium within a realistic stratified atmosphere subject to solar gravity.Such flux tubes are observed to remain relatively stable for up to a day or โฆ