Abstract
From a large number of SOHO/MDI longitudinal magnetograms, three physical measures including the maximum horizontal gradient, the length of the neutral line, and the number of singular points are computed. These measures are used to describe photospheric magnetic field properties including nonpotentiality and complexity, which is believed to be closely related to solar flares. Our statistical results demonstrate that solar flare productivity increases with nonpotentiality and complexity. Furthermore, the relationship between the flare productivity and these measures can be well fitted with a sigmoid function. These results can be beneficial to future operational flare forecast models.
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Arnold, V.I.: 1973, Ordinary Differential Equations, MIT, Cambridge, Massachusetts.
Baum, P.J. and Bratenahl, A.: 1980, Solar Phys. 67, 245.
Baum, P.J., Bratenahl, A., Crockett, G., and Kamin, G.: 1979, Solar Phys. 62, 53.
Berger, T.E. and Lites, B.W.: 2003, Solar Phys. 213, 213.
Démoulin, P., Hénoux, J.C., and Mandrini, C.H.: 1994, Astron. Astrophys. 285, 1023.
Démoulin, P., van Driel-Gesztelyi, L., Schmieder, B., Hénoux, J.C., Csepura, G., and Hagyard, M.J.: 1993, Astron. Astrophys. 271, 292.
Démoulin, P., Mandrini, C.H., Hénoux, J.C., and Machado, M.E.: 1994, Solar Phys. 150, 221.
Falconer, D.A.: 2001, J. Geophys. Res. 106, 25185.
Fontenla, J., Ambasta, A., Kalman, B., and Csepura, G.: 1995, Astrophys. J. 440, 894.
Gallagher, P.T., Moon, Y.-J., and Wang, H.: 2002, Solar Phys. 209, 171.
Gary, G.A., Hagyard, M.J., and West, E.A.: 1990, Solar Polarimetry, Proceedings of the Workshop on Solar Polarimetry, National Solar Observatory, Sunspot, NM, p. 65.
Gorbachev, V.S. and Somov, B.B.: 1988, Solar Phys. 117, 77.
Gorbachev, V.S. and Somov, B.B.: 1989, Soviet Astron. 33(1), 57.
Hagyard, M.J.: 1988, Solar Phys. 115, 107.
Hagyard, M.J. and Rabin, D.M.: 1986, Adv. Space Res. 6, 7.
Leka, K.D. and Barnes, G.: 2003a, Astrophys. J. 595, 1277.
Leka, K.D. and Barnes, G.: 2003b, Astrophys. J. 595, 1296.
Mandrini, C.H., Démoulin, P., Hénoux, J.C., and Machado, M.E.: 1991, Astron. Astrophys. 250, 541.
Mandrini, C.H., Rovira, M.G., Démoulin, P., Hénoux, J.C., Machado, M.E., and Wilkinson, L.K.: 1993, Astron. Astrophys. 272, 609.
Marko, L.: 2003, Ind. Phys. 9(2), 24.
McIntosh, P.S.: 1990, Solar Phys. 125, 251.
Martres, M.-J., Michard, R., Soru-Iscovici, I., and Tsap, T.T.: 1968, Solar Phys. 5, 187.
Nitta, N., van Driel-Gesztelyi, L., Leka, K.D., and Shibata, K.: 1996, Adv. Space Res. 17, 201.
Sakurai, T., Shibata, K., Ichimoto, K., Tsuneta, S., and Acton, L.W.: 1992, Publ. Astron. Soc. Jpn. 44, L123.
Scherrer, P.H., Bogart, R.S., Bush, R.I., Hoeksema, J.T., Kosovichev, A.G., Schou, J., et al.: 1995, Sol.Phys. 162, 129.
Shi, Z. and Wang, J.: 1994, Astrophys. J. 149, 105.
Sweet, P.A.: 1958, Nuovo Cimento Suppl. Ser. X 8, 188.
Sweet, P.A.: 1969, Ann. Rev. Astron. Astrophys. 7, 149.
Tian, L. and Liu, Y.: 2003, Astron. Astrophys. 406, 337.
Tian, L., Wang, J., and Wu, D.: 2002, Solar Phys. 209, 375.
van Driel-Gesztelyi, L., Hofmann, A., Démoulin, P., Schmieder, B., and Csepura, G.: 1994, Solar Phys. 149, 309.
Wang, H.N.: 1997, Solar Phys. 174, 265.
Wang, H., Ewell, M.W., Jr., Zirin, H., and Ai, G.: 1994, Astrophys. J. 424, 436.
Wang, T., Qiu, J., and Zhang, H.: 1998, Astron. Astrophys. 336, 359.
Wang, H., Spirock, T.J., Qiu, J., Ji, H., Yurchyshyn, V., Moon, Y.-J., et al.: 2002, Astrophys. J. 576, 497.
Wang, J. and Shi, Z.: 1993, Solar Phys. 209, 375.
Wang, H.N. and Wang, J.: 1996, Astron. Astrophys. 313, 285.
Zhang, H., Ai, G., Yan, X., Li, W., and Liu, Y.: 1994, Astrophys. J. 423, 828.
Zhang, C.X. and Wang, J.: 2002, Solar Phys. 205, 303.
Zirin, H.: 1988, Astrophysics of the Sun, Cambridge University Press, Cambridge.
Zirin, H. and Liggett, M.A.: 1987, Solar Phys. 113, 267.
Zirin, H. and Wang, H.: 1993, Solar Phys. 144, 37.
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Cui, Y., Li, R., Zhang, L. et al. Correlation Between Solar Flare Productivity and Photospheric Magnetic Field Properties. Sol Phys 237, 45–59 (2006). https://doi.org/10.1007/s11207-006-0077-6
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DOI: https://doi.org/10.1007/s11207-006-0077-6