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Science in China Series A: Mathematics

, Volume 45, Supplement 1, pp 19–24 | Cite as

Diagnosis of solar chromospheric magnetic field

  • Zhang Hongqi 
Article

Abstract

This paper discusses the measurements of the chromospheric magnetic field and the spatial configuration of the field at the lower solar atmosphere inferred by the distribution of the solar photospheric and chromospheric magnetic fields. Some questions in the study of the chromospheric magnetic field are also presented.

Keywords

sun chromosphere magnetic field 

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References

  1. 1.
    Zirin, H., Fine structure of solar magnetic field, Solar Phys., 1972, 22: 34–48.CrossRefGoogle Scholar
  2. 2.
    Geovanelli, R. G., An exploratory two-dimensional study of the coarse structure of network magnetic fields, Solar Phys., 1980, 68: 49–69.CrossRefGoogle Scholar
  3. 3.
    Geovanelli, R. G., Junes, H. P., The three-dimensional structure of atmospheric magnetic fields in two active regions, Solar Phys., 1982, 79: 267–278.CrossRefGoogle Scholar
  4. 4.
    Gabriel, A. H., A magnetic model of the chromosphere-corona transition region, in Chromospheric Fine Structure (ed. Athay, R. G.), IAU Symp. 56, Dordrecht: D. Redel Publ. Company, 1974, 295–298.Google Scholar
  5. 5.
    Zhang, H. Q., Zhang, M., Similarities between chromospheric and photospheric quiet-sun magnetograms, Solar Phys., 2000, 196: 269–277.CrossRefGoogle Scholar
  6. 6.
    Zhang, H. Q., Ai, G. X., Sakurai, T. et al., Fine structures of chromospheric magnetic field in a solar active region, Solar Phys., 1991, 136: 269–293.CrossRefGoogle Scholar
  7. 7.
    Zhang, M., Zhang, H. Q., A study of structures of small-scale magnetic flux tubes (I)—Solar disk center observation, Astrophys. Reports (Publ. Beijing Astron. Obs.), 1998, Special Issue 4: 85–92.Google Scholar
  8. 8.
    Zhang, M., Zhang, H. Q., A comparison between photospheric and chromospheric quiet-sun magnetograms, Solar Phys., 2000, 194: 29–33.CrossRefGoogle Scholar
  9. 9.
    Stenflo, J. O., Solar Magnetic Fields, Dordrecht: Kluwer Academic Publishers, 1994.Google Scholar
  10. 10.
    Zhang, M., Zhang, H. Q., Ai, G. X. et al., Different spatial structures between network regions and active regions indicated by TRACE 171-Å observations, Solar Phys., 1999, 190: 79–90.CrossRefGoogle Scholar
  11. 11.
    Chen, J., Ai, G., Zhang, H. et al., Analysis of solar flare in relation to the magnetic fields on Jan. 14, Publ. Yunnan Astron. Obs., 1989, Special Issue (Suppl.), 108–112.Google Scholar
  12. 12.
    Almeida, J. S., Chromospheric polarity reversal on sunspots—Are they consistent with weak line emission? Astron. Astrophys., 1997, 324: 763–769.Google Scholar
  13. 13.
    Li, W., Ai, G. X., Zhang, H. Q., Reversed-polarity-structures of chromospheric magnetic field, Solar Phys., 1994, 151: 1- 14.CrossRefGoogle Scholar
  14. 14.
    Zhang, H. Q., Solar chromospheric magnetic fields in active regions inferred by monochromatic images of the Stokes parameterV, Solar Phys., 1993, 146: 75–92.CrossRefGoogle Scholar
  15. 15.
    Zhang, H. Q., Spatial configuration of highly sheared magnetic structures in active region (NOAA 6659) in June 1991, Astrophys. J., 1996, 471: 1049–1057.CrossRefGoogle Scholar
  16. 16.
    Zhang, H. Q., Possibility of chromospheric reversal magnetic structures in solar active regions, Publ. Beijing Astron. Obs., 1995, 26: 13–20.Google Scholar
  17. 17.
    Alfven, H., Falthammer, R. C., Cosmical Electrodynamics, Oxford: Oxford University Press, 1963, 100–130.MATHGoogle Scholar

Copyright information

© Science in China Press 2003

Authors and Affiliations

  1. 1.National Astronomical ObservatoriesChinese Academy of SciencesBeijingChina

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