[1] R G Giovanelli. A theory of chromospheric flares[J]. Nature, 1946, 158(4003): 81-82.
[2] E N Parker. Sweet′s mechanism for merging magnetic fields in conducting fluids[J]. J Geophys Res, 1957, 62(4): 509-520.
[3] P Sweet. in B Lehnert, (ed.) Electromagnetic Phenomena in Cosmical Physics[M]. Cambridge: Cambridge University Press, 1958. 123-126.
[4] Y Ogawara, T Takano, T Kato,et al.. The SOLAR-A mission: an overview[J]. Sol Phys, 1991, 136(1): 1-16.
[5] T Kosugi, K Makishima, T Murakami, et al.. The hard X-ray telescope (HXT) for the SOLAR-A mission[J]. Sol Phys, 1991, 136(11): 17-36.
[6] S Tsuneta, L Acton, M Bruner, et al.. The soft X-ray telescope for the SOLAR-A mission[J]. Sol Phys, 1991, 136(11): 37-67.
[7] S Tsuneta, H Hara, T Shimizu, et al.. Observation of a solar flare at the limb with the YOHKOH soft X-ray telescope[J]. Pulbs Astr Soc Japan, 1992, 44(7): L63-L69.
[8] J Y Zhong, Yutong Li, XiaogangWang, et al.. Modelling loop-top X-ray source and reconnection outflows in solar flares with intense lasers[J]. Nature Phys, 2010, 6(10): 984-987.
[9] Quanli Dong, Shoujun Wang, Quanming Lu, et al.. Plasmoid ejection and secondary current sheet generation from magnetic reconnection in laser-plasma interaction[J]. Phys Rev Lett, 2012, 108(21): 215001.
[10] L S Shepherd, P A Cassak. Comparison of secondary islands in collisional reconnection to hall reconnection[J]. Phys Rev Lett, 2010, 105(01): 015004.
[11] D A Uzdensky, N F Loureiro, A A Schekochihin. Fast magnetic reconnection in the plasmoid-dominated regime[J]. Phys Rev Lett, 2010, 105(23): 235002.
[12] J Lin, Y-K Ko, L Sui, et al.. Direct observations of the magnetic reconnection site of an eruption on 2003 November 18[J]. Astrophys J, 2005, 622(4): 1251-1264.
[13] Q L Dong, D W Yuan, S J Wang, et al.. Energetic electron generation by magnetic reconnection in laboratory laserplasma interactions[J]. J Plasma Phys, 2012, 78(4): 497-500.
[14] J F Drake, M A Shay, W Thongthai, et al.. Production of energetic electrons during magnetic reconnection[J]. Phys Rev Lett, 2005, 94(9): 095001.
[15] T D Phan, J F Drake, M A Shay, et al.. Evidence for an elongated (>60 ion skin depths) electron diffusion region during fast magnetic reconnection[J]. Phys Rev Lett, 2007, 99(25): 255002.
[16] M A Shay, J F Drake, M Swisdak. Two-scale structure of the electron dissipation region during collisionless magnetic reconnection[J]. Phys Rev Lett, 2007, 99(15): 155002.
[17] F S Mozer, S D Bale, J P McFadden, et al.. New features of electron diffusion regions observed at subsolar magnetic field reconnection sites[J]. Geophys Res Lett, 2005, 32(24): L24102.
[18] D Ryutov, R P Drake, J Kane, et al.. Similarity criteria for the laboratory simulation of supernov hydrodynamics[J]. Astrophys J,1999, 518(2): 821-832.
[19] D Ryutov, R P Drake, B A Remington. Criteria for scaled laboratory simulations of astrophysical MHD phenomena[J]. Astrophys J Sup, 2000, 127(7): 465-468.
[20] R Wang, Q Lu, A Du, et al.. In situ observations of a secondary magnetic island in an ion diffusion region and associated energetic electrons[J]. Phys Rev Lett, 2010, 104(17): 175003