The Coronal Global Evolutionary Model: Using HMI Vector Magnetogram and Doppler Data to Model the Buildup of Free Magnetic Energy in the Solar Corona-Reference-Cited by-同舟云学术

The Coronal Global Evolutionary Model: Using HMI Vector Magnetogram and Doppler Data to Model the Buildup of Free Magnetic Energy in the Solar Corona

Published:2015-06 Issue:6 Volume:13 Page:369-373
ISSN:1542-7390
Container-title:Space Weather
language:en
Short-container-title:Space Weather

Author:

Fisher G. H.¹,Abbett W. P.¹,Bercik D. J.¹,Kazachenko M. D.¹,Lynch B. J.¹,Welsch B. T.¹,Hoeksema J. T.²,Hayashi K.²³,Liu Y.²,Norton A. A.²,Dalda A. Sainz⁴,Sun X.²,DeRosa M. L.⁵,Cheung M. C. M.⁵

Affiliation:

1. Space Sciences Laboratory; University of California, Berkeley; Berkeley California USA

2. Solar Observatories Group, W.W. Hansen Experimental Physics Laboratory; Stanford University; Stanford California USA

3. Solar Terrestrial Environment Laboratory; Nagoya University; Aichi Japan

4. Stanford-Lockheed Institute for Space Research; Stanford California USA

5. Solar and Astrophysics Laboratory; Lockheed Martin Advanced Technology Center; Palo Alto California USA

Funder

NSF

NASA

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Reference21 articles.

1. The magnetic connection between the convection zone and corona in the quiet Sun;Abbett;Astrophys. J.,2007

2. Radiative cooling in MHD models of the quiet Sun convection zone and corona;Abbett;Sol. Phys.,2012

3. The Helioseismic and Magnetic Imager (HMI) vector magnetic field pipeline: SHARPs-Space-weather HMI active region patches;Bobra;Sol. Phys.,2014

4. Local helioseismology in the SDO HMI/AIA data analysis pipeline;Bogart;Astron. Nachr.,2007

5. A method for data-driven simulations of evolving solar active regions;Cheung;Astrophys. J.,2012

Cited by 51 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A Statistical Study of Magnetic Flux Emergence in Solar Active Regions Prior to Strongest Flares;Research in Astronomy and Astrophysics;2024-04-01

2. Simulating the Photospheric to Coronal Plasma Using Magnetohydrodynamic Characteristics. I. Data-driven Boundary Conditions;The Astrophysical Journal Supplement Series;2024-02-01

3. MHD Simulations of the Solar Corona to Determine the Conditions for Large Solar Flares and the Acceleration of Cosmic Rays during Them;Physics;2023-08-22

4. Hybrid Data-driven Magnetofrictional and Magnetohydrodynamic Simulations of an Eruptive Solar Active Region;The Astrophysical Journal;2023-07-24

5. Effects of optimisation parameters on data-driven magnetofrictional modelling of active regions;Astronomy & Astrophysics;2023-07