Abstract
The gradients of line-of-sight magnetic fields in active region NOAA 6659 on 1991 June 8 have been calculated based on the photospheric and chromospheric magnetograms taken at Huairou Solar Observing Station. We found that high gradients coincided with high strengths of the transverse magnetic fields, implying a complicated configuration of the magnetic field in the lower atmosphere.
For this extraordinarily flare-prolific region, a possible relationship between the gradients and the flares was inferred.
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Ai, G.: 1987, Publ. Beijing Astron. Obs. 9, 27.
Ai, G., Li, W., and Zhang, H: 1982, Acta Astron. Sinica 23, 39.
Ai, G., Li, W., and Zhang, H: 1986, Publ. Beijing Astron. Obs. 8, 11.
Akhmedov, Sh. B., Gelfreikh, G. B., Bogod, V. M., and Korzhavin, A. N.: 1982, Solar Phys. 79, 41.
Allen, C. W.: Astrophysical Quantities, 3rd ed., Athlone Press, London.
Flaa, T., Osherovich, V. A., and Skumanich, A.: 1982, Astrophys. J. 261, 700.
Gopasyuk, S. I.: 1962, Izv. Krymsk. Astrofiz. Obs. 27, 110.
Hagyard M. and Rabin, D.: 1986, Adv. Space Res. 6, 7.
Hagyard, M. Venkatakrishnan, P., and Smith, J. B., Jr.: 1990, Astrophys. J. Suppl. Ser. 73, 159.
Hagyard, M., Cummings, N. P., West, E. A., and Smith, J. E.: 1982, Solar Phys. 81, 231.
Hagyard, M., Teuber, D., West, E., Tandberg-Hanssen, E., Henze, W., Beckers, J. M., Bruner, M., Hyder, C. L., and Woodgate, B. E.: 1983, Solar Phys. 84, 13.
Hagyard, M., Smith, J. B., Jr., Teuber, D., and West, E. A.: 1984, Solar Phys. 91, 115.
Henze, W., Tandberg-Hanssen, E., Hagyard, M., Woodgate, B. E., Shine, R. A., Beckers, J. M., Bruner, M., Gurman, J. B., Hyder, C. L., and West, E. A.: 1982, Solar Phys. 81, 231.
Koval, A. N. and Stepanyan, N. N.: 1972a, Soln. Dann. No. 1, 83.
Koval, A. N. and Stepanyan, N. N.: 1972b, Solar-Earth Phys. 3M, 210.
Liu, Y., Wang, J., and Yan, Y.: 1995, Publ. Beijing Astrophys. Obs. 26, 37.
Osherovich, V. A.: 1980, Solar Phys. 68, 297.
Osherovich, V. A.: 1984, Solar Phys. 90, 31.
Osherovich, V. A. and Flaa, T.: 1983, Solar Phys. 88, 109.
Schmieder, B., Hagyard, M., Ai, G., Zhang, H., Kalman, B., Gyori, L., Rompolt, B., and Machado, M. E.: 1994, Solar Phys. 150, 199.
Severny, A. B.: 1958, Izv. Krymsk. Astrofiz. Obs. 28, 22.
Severny, A. B.: 1960, Izv. Krymsk. Astrofiz. Obs. 22, 12.
Švestka, Z.: 1981, in E. R. Priest (ed.), Solar Flare Magnetohydrodynamics, Gordon and Breach, New York, p. 47.
Tandberg-Hanssen, E., Athay, R. G., Beckers, J. M., Brandt, J. C., Bruner, E. C., Chapman, R. D., Cheng, C. C., Gurman, J. B., Henze, W., Hyder, C. L., Michalitsianos, A. G., Shine, R. A., Schoolman, S. A., and Woodgate, B. E.: 1981, Astrophys. J. 244, L127.
Venkakrishnan, P., Hagyard, M., and Hathaway, D. H.: 1988, Solar Phys. 115, 88.
Wang, H., Tang, F., Zirin, H., and Ai, G.: 1991, Astrophys. J. 380, 282.
Yan, Y. and Wang, J.: 1995, Astron. Astrophys. 298, 277.
Zhang, H.: 1986, Acta Astrophys. Sinica 6, 295.
Zhang, H.: 1995, Astron. Astrophys. 297, 869.
Zhang, H. and Ai, G.: 1986, Acta Astron. Sinica 27, 217.
Zirin, H. and Wang, H.: 1993, Nature 363, 426.
Zhang, H. and Song, M.: 1992, Solar Phys. 138, 69.
Zhang, H. and Wang, T.: 1994, Solar Phys. 151, 129.
Zhang, H., Ai., G., Yan, X., Li, W., and Liu, Y.: 1994, Astrophys. J. 423, 828.
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Liu, Y., Wang, J., Yan, Y. et al. Gradients of the line-of-sight magnetic fields in active region NOAA 6659. Sol Phys 169, 79–89 (1996). https://doi.org/10.1007/BF00153835
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DOI: https://doi.org/10.1007/BF00153835