On thermosolutal-convective instability in a stellar atmosphere. II. FLR and Hall effects
type: Item
instance of: scholarly article
title: On thermosolutal-convective instability in a stellar atmosphere. II. FLR and Hall effects
zbMATH Open document ID: 0619.76058
DOI: 10.1007/BF00639375
author: R. C. Sharma
author: J. N. Misra
published in: Astrophysics and Space Science
publication date: 1986-01-01T00:00:00Z
review text: [For part I see the authors, ibid. 126, 21-28 (1986; Zbl 0606.76056).] Thermosolutal-convective instability of a stellar atmosphere in the presence of a stable solute gradient is considered to include the effects, separately, due to finite Larmor radius (FLR) and Hall currents in the presence of a uniform horizontal magnetic field. The criteria derived for monotonic instability are found to hold true in the presence of FLR and Hall effects.
Mathematics Subject Classification ID: 76E20
Mathematics Subject Classification ID: 76E15
Mathematics Subject Classification ID: 85A05
Mathematics Subject Classification ID: 76M99
zbMATH DE Number: 4005856
zbMATH Keywords: Thermosolutal-convective instability
zbMATH Keywords: stellar atmosphere
zbMATH Keywords: stable solute gradient
zbMATH Keywords: finite Larmor radius
zbMATH Keywords: Hall currents
MaRDI profile type: Publication
cites work: Magnetohydrodynamic Equations for Finite Larmor Radius
cites work: On thermosolutal-convective instability in a stellar atmosphere. I. Effect of rotation and magnetic field
description: scientific article; zbMATH DE number 4005856