A Tilted-Dipole MHD Model of the Solar Corona and Solar Wind

Journal of Geophysical Research - United States
doi 10.1029/2002ja009777
Full Text
Abstract

Available in full text

Date
Authors
Publisher

American Geophysical Union (AGU)

Related search

Turbulent Dissipation in the Solar Wind and Corona

AIP Conference Proceedings
AstronomyPhysics
2003English

MHD Modeling of the Interaction Between the Solar Wind and Solar System Objects

Lecture Notes in Computer Science
Computer ScienceTheoretical Computer Science
2006English

The Solar Corona

Nature
Multidisciplinary
1941English

The Solar Corona

Highlights of Astronomy
1980English

MHD Turbulence in the Solar Wind and Interplanetary Dynamo Effects

Symposium - International Astronomical Union
1993English

MHD Shock Waves and Turbulence in Collisionless Solar Wind Plasma

2019English

A Mechanical Theory of the Solar Corona.

Publications of the Astronomical Society of the Pacific
AstrophysicsAstronomyPlanetary ScienceSpace
1890English

3D Multi-Fluid MHD Studies of the Solar Wind Interaction With Mars

Geophysical Research Letters
EarthPlanetary SciencesGeophysics
1999English

Waves in the Solar Corona

Symposium - International Astronomical Union
2004English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy