6533b828fe1ef96bd1288c38
RESEARCH PRODUCT
Thermal conduction and modeling of static stellar coronal loops
Salvatore SerioAngela CiaravellaGiovanni Peressubject
PhysicsStellar magnetic fieldAstronomyAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCoronal loopAstrophysicsSolar physicsSurface gravityStarsSpace and Planetary ScienceStellar mass lossPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsLow MassAstrophysics::Galaxy AstrophysicsMain sequencedescription
We have modeled stellar coronal loops in static conditions for a wide range of loop length, plasma pressure at the base of the loop and stellar surface gravity, so as to describe physical conditions that can occur in coronae of stars ranging from low mass dwarfs to giants as well as on a significant fraction of the Main-Sequence stars.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 1993-05-01 | Solar Physics |