Coronal plasma flows and magnetic fields in solar active regions: Combined observations from SOHO and NSO/Kitt Peak

被引:0
|
作者
Marsch, E. [1 ,3 ]
Wiegelmann, T. [1 ]
Xia, L.D. [1 ,2 ]
机构
[1] Max-Planck-Inst. F. S., 37191 Katlenburg-Lindau, Germany
[2] Armagh Observatory, Armagh BT61 9DG, United Kingdom
[3] Univ. of Sci. and Technol. of China, Hefei, China
来源
Astronomy and Astrophysics | 1600年 / 428卷 / 02期
关键词
D O I
暂无
中图分类号
学科分类号
摘要
57
引用
收藏
页码:629 / 645
相关论文
共 33 条
  • [31] The Relationship Between Solar Coronal X-Ray Brightness and Active Region Magnetic Fields: A Study Using High-Resolution Hinode Observations
    Hazra, Soumitra
    Nandy, Dibyendu
    Ravindra, B.
    SOLAR PHYSICS, 2015, 290 (03) : 771 - 785
  • [32] The Relationship Between Solar Coronal X-Ray Brightness and Active Region Magnetic Fields: A Study Using High-Resolution Hinode Observations
    Soumitra Hazra
    Dibyendu Nandy
    B. Ravindra
    Solar Physics, 2015, 290 : 771 - 785
  • [33] 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
    Hayashi, Keiji
    Feng, Xueshang
    Xiong, Ming
    Jiang, Chaowei
    ASTROPHYSICAL JOURNAL LETTERS, 2019, 871 (02)