On the Predominance of the Radial Component of the Magnetic Field in the Solar Corona-Reference-Cited by-同舟云学术

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On the Predominance of the Radial Component of the Magnetic Field in the Solar Corona

Published:2001-09-10 Issue:2 Volume:558 Page:852-858
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Habbal Shadia Rifai,Woo Richard,Arnaud Jean

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/558/i=2/a=852/pdf

Reference29 articles.

1. Magnetic fields and the structure of the solar corona

2. Arnaud, J. 1983, Ph.D. thesis, Univ. Paris VI

3. Arnaud, J. 1984, in Proc. 4th European Meeting on Solar Physics (ESA SP-220), 115

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1. Coronal Magnetic Field Topology from Total Solar Eclipse Observations;The Astrophysical Journal;2020-06-03

2. Polarimeter for coronal magnetic field measurement: design and evaluation of polarization cross talk;Journal of Astronomical Telescopes, Instruments, and Systems;2019-10-17

3. Polarimetric Observations of the Sun;Astrophysics and Space Science Library;2019

4. Using a New Infrared Si x Coronal Emission Line for Discriminating between Magnetohydrodynamic Models of the Solar Corona During the 2006 Solar Eclipse;The Astrophysical Journal;2018-01-02

5. Diagnostics of Coronal Magnetic Fields through the Hanle Effect in UV and IR Lines;Frontiers in Astronomy and Space Sciences;2016-06-22

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