Amanote Research

Amanote Research

    RegisterSign In

Radiation-Accellerated Ions in Hot Star Winds: Heating and “Turbulence” Effects

Symposium - International Astronomical Union
doi 10.1017/s0074180900215696
Full Text
Open PDF
Abstract

Available in full text

Date

January 1, 1994

Authors
E. Ya Vilkoviskij
Publisher

Cambridge University Press (CUP)


Related search

The Basic Physics of Hot-Star Winds

Symposium - International Astronomical Union
1994English

Three-Dimensional Radiative Transfer in Clumped Hot Star Winds

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Turbulence Control Through Selective Surface Heating Using Microwave Radiation

2013English

Neglecting the Porosity of Hot-Star Winds Can Lead to Underestimating Mass-Loss Rates

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

Modelling Turbulence Effect in Formation of Zonal Winds

The Open Atmospheric Science Journal
2008English

Evidence for Azimuthal Asymmetry in Be Star Winds

International Astronomical Union Colloquium
1999English

Surface Mean Flow and Turbulence Structure in Tropical Cyclone Winds

English

Winds of Hot Stars in the Magellanic Clouds

Symposium - International Astronomical Union
1991English

Radar Observations of Winds and Turbulence in the Stratosphere and Mesosphere

Journals of the Atmospheric Sciences
Atmospheric Science
1974English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy