Two-dimensional Radiative Magnetohydrodynamic Simulations of Partial Ionization in the Chromosphere. II. Dynamics and Energetics of the Low Solar Atmosphere-Reference-Cited by-同舟云学术

Two-dimensional Radiative Magnetohydrodynamic Simulations of Partial Ionization in the Chromosphere. II. Dynamics and Energetics of the Low Solar Atmosphere

Published:2017-09-20 Issue:1 Volume:847 Page:36
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Martínez-Sykora Juan^ORCID,Pontieu Bart De^ORCID,Carlsson Mats^ORCID,Hansteen Viggo H.^ORCID,Nóbrega-Siverio Daniel^ORCID,Gudiksen Boris V.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/847/i=1/a=36/pdf

Reference88 articles.

1. The Magnetic Connection between the Convection Zone and Corona in the Quiet Sun

2. Instability by magnetic buoyancy

3. EFFECT OF SOLAR CHROMOSPHERIC NEUTRALS ON EQUILIBRIUM FIELD STRUCTURES

4. Emergence of a Flux Tube through a Partially Ionized Solar Atmosphere

5. Emergence of magnetic flux from the convection zone into the corona

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