Journal ArticleDOI
The Angular Momentum of the Solar Wind
Edmund J. Weber,Leverett Davis +1 more
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Steady state model of solar wind flow in equatorial plane solved for radial and azimuthal motions, taking into account pressure gradient, magnetic field and gravitational effects as discussed by the authors.Abstract:
Steady state model of solar wind flow in equatorial plane solved for radial and azimuthal motions, taking into account pressure gradient, magnetic field and gravitational effectsread more
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Journal ArticleDOI
Kinetic aspects of the Jovian current sheet
TL;DR: In this paper, self-consistent two-dimensional particle simulations are used to examine the structure and dynamics of the current sheet in the middle and outer regions of the Jovian magnetotail.
Journal ArticleDOI
Magnetically Driven Outflows in a Starburst Environment
Elisabete M. de Gouveia Dal Pino,Elisabete M. de Gouveia Dal Pino,Gustavo Medina Tanco,Gustavo Medina Tanco +3 more
TL;DR: In this article, the authors investigate the possibility that the observed collimated outflows in luminous infrared galaxies (LIGs) and some Seyfert galaxies can be produced in a starburst (SB) environment.
Journal ArticleDOI
Stellar versus Galactic: the intensity of cosmic rays at the evolving Earth and young exoplanets around Sun-like stars
TL;DR: In this paper, a 1.5D stellar wind model combined with a spatially 1D cosmic ray transport model was used to study the evolution of the stellar cosmic ray spectrum as a function of stellar rotation.
Journal ArticleDOI
Multi-Component MHD Model of Hot Jupiter Envelopes
Andrey Zhilkin,Dmitri Bisikalo +1 more
TL;DR: In this paper, a numerical model of a hot Jupiter extended envelope based on the approximation of multi-component magnetic hydrodynamics is presented, where the main attention is focused on the problem of implementing the completed MHD stellar wind model.
Posted ContentDOI
An Extended and Fragmented Alfv\'en Zone in the Young Solar Wind
TL;DR: In this article , the authors explore the possibility that the critical transition between sub-Alfvénic periods and super-Alignments in the solar atmosphere takes place in fragmented and disconnected subvolumes within a general Alfvén critical zone.