Skip to main content
SpringerLink
Log in

Diagnosis of solar chromospheric magnetic field

  • Published:
Science in China Series A: Mathematics Aims and scope Submit manuscript

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.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Log in via an institution

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Institutional subscriptions

Similar content being viewed by others

References

  1. Zirin, H., Fine structure of solar magnetic field, Solar Phys., 1972, 22: 34–48.

    Article  Google Scholar 

  2. Geovanelli, R. G., An exploratory two-dimensional study of the coarse structure of network magnetic fields, Solar Phys., 1980, 68: 49–69.

    Article  Google Scholar 

  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.

    Article  Google Scholar 

  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. Zhang, H. Q., Zhang, M., Similarities between chromospheric and photospheric quiet-sun magnetograms, Solar Phys., 2000, 196: 269–277.

    Article  Google Scholar 

  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.

    Article  Google Scholar 

  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. Zhang, M., Zhang, H. Q., A comparison between photospheric and chromospheric quiet-sun magnetograms, Solar Phys., 2000, 194: 29–33.

    Article  Google Scholar 

  9. Stenflo, J. O., Solar Magnetic Fields, Dordrecht: Kluwer Academic Publishers, 1994.

    Google Scholar 

  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.

    Article  Google Scholar 

  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.

  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. Li, W., Ai, G. X., Zhang, H. Q., Reversed-polarity-structures of chromospheric magnetic field, Solar Phys., 1994, 151: 1- 14.

    Article  Google Scholar 

  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.

    Article  Google Scholar 

  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.

    Article  Google Scholar 

  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. Alfven, H., Falthammer, R. C., Cosmical Electrodynamics, Oxford: Oxford University Press, 1963, 100–130.

    MATH  Google Scholar 

Download references

Author information

Authors and Affiliations

  1. National Astronomical Observatories, Chinese Academy of Sciences, 100012, Beijing, China

    Zhang Hongqi

Authors
  1. Zhang Hongqi
    View author publications

    You can also search for this author in PubMed Google Scholar

Corresponding author

Correspondence to Zhang Hongqi.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Zhang, H. Diagnosis of solar chromospheric magnetic field. Sci. China Ser. A-Math. 45 (Suppl 1), 19–24 (2002). https://doi.org/10.1007/BF02889679

Download citation

  • Received:

  • Revised:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02889679

Keywords

Search

Navigation