Is Solar Convection Responsible for the Local Amplification and Structuring of Magnetic Fields? (Observational Test of the Hypothesis)

Proceedings of the International Astronomical Union - United Kingdom
doi 10.1017/s174392130700097x
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Cambridge University Press (CUP)

Related search

The Magnetic Structuring of the Solar Corona

Highlights of Astronomy
1995English

Turbulent Amplification of Interstellar Magnetic Fields

Symposium - International Astronomical Union
1991English

The Magnetic Fields of the Quiet Solar Photosphere

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

Magnetic Fields and Convection: New Observations

Symposium - International Astronomical Union
1983English

The Structure and Evolution of Global Solar Magnetic Fields

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2010English

Solar Magnetic Fields

Science
MultidisciplinaryPhilosophy of ScienceHistory
1965English

Stability of the Solar Tachocline With Magnetic Fields

Astronomische Nachrichten
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

Features in Ferrocolloid Convection in the Presence of Gravitational and Magnetic Fields

ВЕСТНИК ПЕРМСКОГО УНИВЕРСИТЕТА. ФИЗИКА
2018English

Thermomagnetic Convection Under Alternating Magnetic Fields

PAMM
2017English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy