CORRELATION BETWEEN MAGNETIC SHEAR AND MAGNETIC TENSION IN A SOLAR ACTIVE REGION

被引:5
|
作者
VENKATAKRISHNAN, P
NARAYANAN, RS
PRASAD, NDN
机构
[1] Indian Institute of Astrophysics, Bangalore
关键词
D O I
10.1007/BF00627596
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The difference between the magnetic tension and magnetic shear was calculated for four vector magnetograms of NOAA AR 4474. It was seen that this difference between the two independent angular measures of magnetic stress is less than 18-degrees for more than 50% of the pixels. Magnetic tension is thus found to be fairly well correlated with magnetic shear for AR 4474.
引用
收藏
页码:315 / 322
页数:8
相关论文
共 50 条
  • [41] Bayesian approach for modeling global magnetic parameters for the solar active region
    Poisson, M.
    Grings, F.
    Mandrini, C. H.
    Fuentes, M. Lopez
    Demoulin, P.
    ASTRONOMY & ASTROPHYSICS, 2022, 665
  • [42] Modeling the distribution of magnetic fluxes in field concentrations in a solar active region
    Carolus J. Schrijver
    Alan M. Title
    Hermance J. Hagenaar
    Richard A. Shine
    Solar Physics, 1997, 175 : 329 - 340
  • [43] What is the spatial distribution of magnetic helicity injected in a solar active region?
    Pariat, E.
    Nindos, A.
    Demoulin, P.
    Berger, M. A.
    ASTRONOMY & ASTROPHYSICS, 2006, 452 (02) : 623 - U49
  • [44] Measurements of Coronal Magnetic Field Strengths in Solar Active Region Loops
    Brooks, David H.
    Warren, Harry P.
    Landi, Enrico
    ASTROPHYSICAL JOURNAL LETTERS, 2021, 915 (01)
  • [45] A statistical study on property of spatial magnetic field for solar active region
    S. Liu
    Astrophysics and Space Science, 2014, 351 : 409 - 416
  • [46] What is the spatial distribution of magnetic helicity injected in a solar active region
    Pariat, E.
    Nindos, A.
    Démoulin, P.
    Berger, M.A.
    Astronomy and Astrophysics, 1600, 452 (02): : 623 - 630
  • [47] A magnetic bald-patch flare in solar active region 11117
    Chao-Wei Jiang
    Xue-Shang Feng
    Shi-Tsan Wu
    Qiang Hu
    ResearchinAstronomyandAstrophysics, 2017, 17 (09) : 53 - 62
  • [48] A coupled model for the emergence of active region magnetic flux into the solar corona
    Abbett, WP
    Fisher, GH
    ASTROPHYSICAL JOURNAL, 2003, 582 (01): : 475 - 485
  • [49] A model of magnetic fields in a large-scale solar active region
    Ji, HS
    Song, MT
    CHINESE ASTRONOMY AND ASTROPHYSICS, 2001, 25 (01) : 97 - 110
  • [50] Modeling the distribution of magnetic fluxes in field concentrations in a solar active region
    Schrijver, CJ
    Title, AM
    Hagenaar, HJ
    Shine, RA
    SOLAR PHYSICS, 1997, 175 (02) : 329 - 340