journal article Jun 26, 2014

Plasmoid-induced-reconnection and fractal reconnection

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References
68
[1]
Akiyama, S. and H. Hara, X-ray eruptive structures associated with small flares, Adv. Space Res., 26, 465–468, 2000. 10.1016/s0273-1177(99)01107-2
[2]
Anzer, U. and G. W. Pneuman, Magnetic reconnection and coronal transients, Solar Phys., 79, 129–147, 1982. 10.1007/bf00146978
[3]
Benz, A. O. and M. J. Aschwanden, Characteristics of the impulsive phase of flares, in Proc. Eruptive Solar Flares, IAU Colloq. No. 133, edited by Z. Svestka, B. V. Jackson, and M. E. Machado, Lecture Notes in Physics 399, Springer-Verlag, Berlin, pp. 106–115, 1992. 10.1007/3-540-55246-4_84
[4]
Biskamp, D., Magnetic reconnection via current sheets, Phys. Fluids, 29, 1520–1531, 1986. 10.1063/1.865670
[5]
Biskamp, D., Nonlinear Magnetohydrodynamics, 392 pp., Cambridge Univ. Press, 1992. 10.1017/cbo9780511599965
[6]
Biskamp, D. and H. Welter, Magnetic arcade evolution and instability, Solar Phys., 120, 49–77, 1989. 10.1007/bf00148534
[7]
Carmichael, H., A process for flares, in Proc. AAS-NASA Symp. on the Physics of Solar Flares, edited by W. N. Hess, Washington, NASA, NASA-SP 50, pp. 451–456, 1964.
[8]
Chen, P. F., K. Shibata, and T. Yokoyama, Global destabilization due to localized reconnection: a mechanism for coronal mass ejections, Earth Planets Space, 53, this issue, 611–614, 2001. 10.1186/bf03353279
[9]
Cheng, C. Z. and G. S. Choe, Solar flare mechanism based on magnetic arcade reconnection and island merging, Earth Planets Space, 53, this issue, 597–604, 2001. 10.1186/bf03353277
[10]
Choe, G. S. and L. Lee, Evolution of solar magnetic arcades. I. Ideal MHD evolution under footpoint shearing, ApJ, 472, 360–371, 1996. 10.1086/178069
[11]
Choe, G. S. and C. Z. Cheng, A model of solar flares and their homologous behavior, ApJ, 541, 449–467, 2000. 10.1086/309415
[12]
Dere, K., G. E. Brueckner, R. A. Howard, D. J. Michels, and J. P. Delaboudiniere, LASCO and EIT observations of helical structure in coronal mass ejections, ApJ, 516, 465–474, 1999. 10.1086/307101
[13]
Drake, J., private communication, 2000.
[14]
Forbes, T. G., Numerical simulation of a catastrophe model for coronal mass ejections, J. Geophys. Res., 95, 11919–11931, 1990. 10.1029/ja095ia08p11919
[15]
Forbes, T. G. and L. Acton, Reconnection and field line shrinkage in solar flares, ApJ, 459, 330–341, 1996. 10.1086/176896
[16]
Hanaoka, Y., H. Kurokawa, S. Enome et al., Simultaneous observations of a prominence eruption followed by a coronal arcade formation in radio, soft X-rays, and H alpha, PASJ, 46, 205–216, 1994.
[17]
Heyvaerts, J., E. R. Priest, and D. Rust, An emerging flux model for the solar flare phenomenon, ApJ, 216, 123–137, 1977. 10.1086/155453
[18]
Hirayama, T., Theoretical model of flares and prominences, I. Evaporating flare model, Solar Phys., 34, 323–338, 1974. 10.1007/bf00153671
[19]
Hirayama, T., Magnetic morphologies of solar flares, in Lecture Note in Physics, No. 387, Flare Physics in Solar Activity Maximum 22, edited by Y. Uchida et al., pp. 197–201, Springer, New York, 1991. 10.1007/bfb0032639
[20]
Horiuchi, R., W. Pei, and T. Sato, Collisionless driven reconnection in an open system, Earth Planets Space, 53, this issue, 439–445, 2001. 10.1186/bf03353254
[21]
Hoshino, M., K. Hiraide, and T. Mukai, Strong electron heating and non-Maxwellian behavior in magnetic reconnection, Earth Planets Space, 53, this issue, 627–634, 2001. 10.1186/bf03353282
[22]
Hundhausen, A., Coronal mass ejections, in The Many Faces of the Sun: A Summary of the Results from NASA’s Solar Maximum Mission, edited by K. T. Strong, J. L. R. Saba, B. M. Haisch, and J. T. Schmelz, pp. 143–200, Springer, New York, 1999. 10.1007/978-1-4612-1442-7_5
[23]
Ichimaru, S., Electrical resistivity of electromagnetically turbulent plasma and reconnection rate of magnetic fields, ApJ, 202, 524–531, 1975. 10.1086/154002
[24]
Kahler, S. W., R. L. Moore, S. R. Kane, and H. Zirin, Filament eruptions and the impulsive phase of solar flares, ApJ, 328, 824–829, 1988. 10.1086/166340
[25]
Kitabata, H., T. Hayashi, T. Sato et al., Impulsive nature in magnetohydrodynamic driven reconnection, J. Phys. Soc. Japan, 65, 3208–3214, 1996. 10.1143/jpsj.65.3208
[26]
Kopp, R. A. and G. W. Pneuman, Magnetic reconnection in the corona and the loop prominence phenomenon, Solar Phys., 50, 85–98, 1976. 10.1007/bf00206193
[27]
Kusano, K., Y. Suzuki, and K. Nishikawa, A solar flare triggering mechanism based on the Woltjer-Taylor minimum energy principle, ApJ, 441, 942–951, 1995. 10.1086/175413
[28]
Lee, L. C. and Z. F. Fu, Multiple X line reconnection, I. A criterion for the transition from a single X line to a multiple X line reconnection, J. Geophys. Res., 91, 6807–6815, 1986. 10.1029/ja091ia06p06807
[29]
Lin, J. and T. G. Forbes, Effects of reconnection on the coronal mass ejection process, J. Geophys. Res., 105, 2375–2392, 2000. 10.1029/1999ja900477
[30]
Magara, T., K. Shibata, and T. Yokoyama, Evolution of eruptive flares. I. Plasmoid dynamics in eruptive flares, ApJ, 487, 437–446, 1997. 10.1086/304592
[31]
Magara, T. and K. Shibata, Evolution of eruptive flares. II. The occurrence of locally enhanced resistivity, ApJ, 514, 456–471, 1999. 10.1086/306929
[32]
Masuda, S., T. Kosugi, H. Hara, S. Tsuneta, and Y. Ogawara, A loop-top hard X-ray source in a compact solar flare as evidence for magnetic reconnection, Nature, 371, 495–496, 1994. 10.1038/371495a0
[33]
Mikic, Z., D. C. Barnes, and D. D. Schnack, Dynamical evolution of a solar coronal magnetic field arcade, ApJ, 328, 830–847, 1988. 10.1086/166341
[34]
Moore, R. L. and G. Roumeliotis, Triggering of eruptive flares: destabilization of the preflare magnetic field configuration, in Lecture Note in Physics, No. 399, Eruptive Flares, edited by Z. Svestka, B. V. Jackson, and M. E. Machado, pp. 69–78, Springer, New York, 1992.
[35]
Morimoto, T. and H. Kurokawa, private communication, 2000.
[36]
Nitta, S., S. Tanuma, K. Maezawa, and K. Shibata, Fast magnetic reconnection in free space: self-similar evolution process, ApJ, 550, 1119–1130, 2001. 10.1086/319774
[37]
Nitta, N., A study of major solar flares observed by Yohkoh, in Magnetic Reconnection in the Solar Atmosphere, ASP Conference Series; Vol. 111, edited by R. D. Bentley and J. T. Mariska (1997), pp. 156–161, 1996. 10.1007/978-94-009-0315-9_30
[38]
Ohyama, M. and K. Shibata, Preflare heating and mass motion in a solar flare associated with hot plasma ejection: 1993 November 11 C9.7 flare, PASJ, 49, 249–261, 1997. 10.1093/pasj/49.2.249
[39]
Ohyama, M. and K. Shibata, X-ray plasma ejection associated with an impulsive flare on 1992 October 5: physical conditions of X-ray plasma ejection, ApJ, 499, 934–944, 1998. 10.1086/305652
[40]
Ohyama, M. and K. Shibata, Timing and occurrence rate of X-ray plasma ejections, JASTP, 62, 1509–1514, 2000.
[41]
Ono, Y., M. Inomoto, Y. Ueda, T. Matsuyama, and Y. Murata, Fast compression of a current sheet during externally driven magnetic reconnection, Earth Planets Space, 53, this issue, 521–526, 2001. 10.1186/bf03353264
[42]
Priest, E. R., C. E. Parnel, and S. F. Martin, A converging flux model of an X-ray bright point and an associated canceling magnetic feature, ApJ, 427, 459–474, 1994. 10.1086/174157
[43]
Scholer, M., Undriven magnetic reconnection in an isolated current sheet, J. Geophys. Res., 94, 8805–8812, 1989. 10.1029/ja094ia07p08805
[44]
Schumacher, J. and B. Kliem, Dynamic current sheets with localized anomalous resistivity, Phys. Plasmas, 3, 4703–4711, 1996. 10.1063/1.872037
[45]
Shibata, K., S. Nozawa, and R. Matsumoto, Magnetic reconnection associated with emerging magnetic flux, PASJ, 44, 265–271, 1992.
[46]
Shibata, K., S. Masuda, M. Shimojo, H. Hara et al., Hot plasma ejections associated with compact-loop solar flares, Ap. J. Lett., 451, L83-L85, 1995. 10.1086/309688
[47]
Shibata, K., New observational facts about solar flares from Yohkoh studies—Evidence of magnetic reconnection and a unified model of flares, Adv. Space Res., 17, (4/5)9-18, 1996. 10.1016/0273-1177(95)00534-l
[48]
Shibata, K., Rapidly time variable phenomena: Jets, explosive events, and flares, 1997, in Proc. 5-th SOHO workshop, ESA, SP-404, pp. 103–112, 1997.
[49]
Shibata, K., A unified model of flares, in Proc. Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond, edited by T. Watanabe et al., pp. 187–196, 1998. 10.1007/978-94-011-5220-4_32
[50]
Shibata, K., Evidence of magnetic reconnection in solar flares and a unified model of flares, Astrophys. Sp. Sci., 264, 129–144, 1999. 10.1023/a:1002413214356

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Published
Jun 26, 2014
Vol/Issue
53(6)
Pages
473-482
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Kazunari Shibata, Syuniti Tanuma (2014). Plasmoid-induced-reconnection and fractal reconnection. Earth, Planets and Space, 53(6), 473-482. https://doi.org/10.1186/bf03353258