Magnetohydrodynamic Simulations for Solar Active Regions using Time-series Data of Surface Plasma Flow and Electric Field Inferred from Helioseismic Magnetic Imager Vector Magnetic Field Measurements-Reference-Cited by-同舟云学术

Magnetohydrodynamic Simulations for Solar Active Regions using Time-series Data of Surface Plasma Flow and Electric Field Inferred from Helioseismic Magnetic Imager Vector Magnetic Field Measurements

Published:2019-01-29 Issue:2 Volume:871 Page:L28
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Hayashi Keiji^ORCID,Feng Xueshang^ORCID,Xiong Ming^ORCID,Jiang Chaowei^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/aaffcf/pdf

Reference26 articles.

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

2. Coronal Magnetohydrodynamic Evolution Driven by Subphotospheric Conditions

3. The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches

4. THERMAL DIAGNOSTICS WITH THE ATMOSPHERIC IMAGING ASSEMBLY ON BOARD THE SOLAR DYNAMICS OBSERVATORY: A VALIDATED METHOD FOR DIFFERENTIAL EMISSION MEASURE INVERSIONS

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