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Journal ArticleDOI

The Angular Momentum of the Solar Wind

Edmund J. Weber, +1 more
- 01 Apr 1967 - 
- Vol. 148, pp 217-227
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TLDR
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 effects

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Journal ArticleDOI

The multi-scale nature of the solar wind

TL;DR: The role of expansion effects, non-equilibrium distribution functions, collisions, waves, turbulence, and kinetic microinstabilities for the multi-scale plasma evolution are discussed.
Journal ArticleDOI

Some problems of pulsar physics or I'm madly in love with electricity

TL;DR: In this paper, a review of the theory of pulsar magnetospheres and their emission is presented, with particular attention paid to the total amount of electronpositron plasma created and its momentum distribution.
Journal ArticleDOI

Rotation and Magnetic Activity in a Sample of M-Dwarfs

TL;DR: In this paper, rotational broadening and chromospheric activity in a sample of 123 M-dwarfs were analyzed using spectra taken at the W.M. Keck Observatory as part of the California Planet Search program.
Journal ArticleDOI

Radio Emission and Particle Acceleration in SN 1993J

TL;DR: In this paper, a fit to the individual spectra by a synchrotron spectrum, suppressed by external free-free absorption and synchoretron self-absorption, gives a superior fit to models based on pure free free free absorption.
Journal ArticleDOI

MHD simulations of jet acceleration from Keplerian accretion disks: the effects of disk resistivity

TL;DR: In this article, the effects of the disk magnetic resistivity, parametrized through an alpha-prescription, in determining the properties of the inflow-outflow system were investigated.