Amanote Research

Amanote Research

    RegisterSign In

Height Variation of Magnetic Field and Plasma Flows in Isolated Bright Points

Astronomy and Astrophysics - France
doi 10.1051/0004-6361/201935856
Full Text
Open PDF
Abstract

Available in full text

Categories
AstrophysicsAstronomyPlanetary ScienceSpace
Date

October 1, 2019

Authors
Christoph Kuckein
Publisher

EDP Sciences


Related search

Magnetic Topological Analysis of Coronal Bright Points

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Coronal Bright Points

Symposium - International Astronomical Union
1976English

Magnetic Field in Reentry Flows in 2D: Eleven Species

Journal of Advances in Mathematics and Computer Science
2017English

Magnetic Reconnection at 3D Null Points: Effect of Magnetic Field Asymmetry

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2010English

Magnetic Field in Expanding Quark-Gluon Plasma

Physical Review C
High Energy PhysicsNuclear
2018English

Links Between Magnetic Fields and Plasma Flows in a Coronal Hole

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2005English

Magnetic Field Topologies of the Bright, Weak-Field Ap Stars Theta Aurigae and Eps Ursae Majoris

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Substructure of Quiet Sun Bright Points

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2010English

Variation of Coronal Magnetic Field and Solar Flare Eruption

2019English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy