參考文獻 |
[1] Acuña, M., Curtis, D., Scheifele, J., Russell, C., Schroeder, P., Szabo, A., Luhmann, J., 2008. The STEREO/IMPACT magnetic field experiment. Space Science Reviews 136 (1-4), 203-226.
[2] Alexander, D., Richardson, I.G., Zurbuchen, T.H., 2006. A brief history of CME science, Coronal Mass Ejections. 3-11. Springer.
[3] Aschwanden, M., 2006. Physics of the solar corona: an introduction with problems and solutions. Springer Science & Business Media.
[4] Berger, M.A., Field, G.B., 1984. The topological properties of magnetic helicity. Journal of Fluid Mechanics 147, 133-148.
[5] Bothmer, V., Schwenn, R., 1994. Eruptive prominences as sources of magnetic clouds in the solar wind. Space Science Reviews 70 (1-2), 215-220.
[6] Bothmer, V., Schwenn, R., 1997. The structure and origin of magnetic clouds in the solar wind, Annales Geophysicae. 1-24.
[7] Brueckner, G., Howard, R., Koomen, M., Korendyke, C., Michels, D., Moses, J., Socker, D., Dere, K., Lamy, P., Llebaria, A., 1995. The large angle spectroscopic coronagraph (LASCO). Solar Physics 162 (1-2), 357-402.
[8] Burlaga, L., Fitzenreiter, R., Lepping, R., Ogilvie, K., Szabo, A., Lazarus, A., Steinberg, J., Gloeckler, G., Howard, R., Michels, D., Farrugia, C., Lin, R.P., Larson, D.E., 1998. A magnetic cloud containing prominence material: January 1997. Journal of Geophysical Research: Space Physics 103 (A1), 277-285.
[9] Burlaga, L., Klein, L., Sheeley, N., Michels, D., Howard, R., Koomen, M., Schwenn, R., Rosenbauer, H., 1982. A magnetic cloud and a coronal mass ejection. Geophysical Research Letters 9 (12), 1317-1320.
[10] Burlaga, L., Lepping, R., Jones, J., 1990. Global configuration of a magnetic cloud. Physics of magnetic flux ropes, 373-377.
[11] Burlaga, L., Sittler, E., Mariani, F., Schwenn, R., 1981. Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observations. Journal of Geophysical Research: Space Physics 86 (A8), 6673-6684.
[12] Burlaga, L.F., Behannon, K., 1982. Magnetic clouds: Voyager observations between 2 and 4 AU. Solar Physics 81 (1), 181-192.
[13] Cho, K.-S., Park, S.-H., Marubashi, K., Gopalswamy, N., Akiyama, S., Yashiro, S., Kim, R.-S., Lim, E.-K., 2013. Comparison of helicity signs in interplanetary CMEs and their solar source regions. Solar Physics 284 (1), 105-127.
[14] Delaboudiniere, J.-P., Artzner, G., Brunaud, J., Gabriel, A.H., Hochedez, J., Millier, F., Song, X., Au, B., Dere, K., Howard, R., 1995. EIT: extreme-ultraviolet imaging telescope for the SOHO mission. Springer.
[15] Domingo, V., Fleck, B., Poland, A.I., 1995. The SOHO mission: an overview. Solar Physics 162 (1-2), 1-37.
[16] Elsasser, W.M., 1956. Hydromagnetic Dynamo Theory. Reviews of Modern Physics 28 (2), 135-163.
[17] Feng, H., Wu, D., Lin, C., Chao, J., Lee, L., Lyu, L., 2008. Interplanetary small‐and intermediate‐sized magnetic flux ropes during 1995–2005. Journal of Geophysical Research: Space Physics 113 (A12).
[18] Galvin, A., Kistler, L., Popecki, M., Farrugia, C., Simunac, K., Ellis, L., Möbius, E., Lee, M., Boehm, M., Carroll, J., 2008. The Plasma and Suprathermal Ion Composition (PLASTIC) investigation on the STEREO observatories. Space Science Reviews 136 (1-4), 437-486.
[19] Goldstein, H., 1983. On the field configuration in magnetic clouds, NASA conference publication
[20] Gopalswamy, N., Yashiro, S., Akiyama, S., 2007. Geoeffectiveness of halo coronal mass ejections. Journal of Geophysical Research: Space Physics 112 (A6).
[21] Hale, G.E., Ellerman, F., Nicholson, S.B., Joy, A.H., 1919. The magnetic polarity of sun-spots. The Astrophysical Journal 49, 153.
[22] Howard, R., Michels, D., Sheeley Jr, N., Koomen, M., 1982. The observation of a coronal transient directed at Earth. The Astrophysical Journal 263, L101-L104.
[23] Howard, R., Sheeley, N., Koomen, M., Michels, D., 1985. Coronal mass ejections: 1979–1981. Journal of Geophysical Research: Space Physics 90 (A9), 8173-8191.
[24] Howard, T.A., Tappin, S.J., 2008. Three-Dimensional Reconstruction of Two Solar Coronal Mass Ejections Using the STEREO Spacecraft. Solar Physics 252 (2), 373-383.
[25] Howard, T.A., Tappin, S.J., 2009. Interplanetary Coronal Mass Ejections Observed in the Heliosphere: 3. Physical Implications. Space Science Reviews 147 (1-2), 89-110.
[26] Hu, Q., Qiu, J., Dasgupta, B., Khare, A., Webb, G., 2014. Structures of interplanetary magnetic flux ropes and comparison with their solar sources. The Astrophysical Journal 793 (1), 53.
[27] Hudson, H.S., Bougeret, J.L., Burkepile, J., 2006. Coronal Mass Ejections: Overview of Observations. Space Science Reviews 123 (1-3), 13-30.
[28] Jeong, H., Chae, J., 2007. Magnetic helicity injection in active regions. The Astrophysical Journal 671 (1), 1022.
[29] Ji, H., 1999. Turbulent dynamos and magnetic helicity. Physical review letters 83 (16), 3198.
[30] Jian, L., Russell, C., Luhmann, J., Skoug, R., 2008. Evolution of solar wind structures from 0.72 to 1AU. Advances in Space Research 41 (2), 259-266.
[31] Jian, L., Russell, C.T., Luhmann, J.G., Skoug, R.M., 2006. Properties of Interplanetary Coronal Mass Ejections at One AU During 1995 – 2004. Solar Physics 239 (1-2), 393-436.
[32] Kataoka, R., Miyoshi, Y., 2006. Flux enhancement of radiation belt electrons during geomagnetic storms driven by coronal mass ejections and corotating interaction regions. Space Weather 4 (9), n/a-n/a.
[33] Kilpua, E., Jian, L., Li, Y., Luhmann, J., Russell, C., 2012. Observations of ICMEs and ICME-like solar wind structures from 2007–2010 using near-Earth and STEREO observations. Solar Physics 281 (1), 391-409.
[34] Kilpua, E., Pomoell, J., Vourlidas, A., Vainio, R., Luhmann, J., Li, Y., Schroeder, P., Galvin, A., Simunac, K., 2009. STEREO observations of interplanetary coronal mass ejections and prominence deflection during solar minimum period, Annales Geophysicae. 4491-4503.
[35] Kilpua, E.K.J., Jian, L.K., Li, Y., Luhmann, J.G., Russell, C.T., 2011. Multipoint ICME encounters: Pre-STEREO and STEREO observations. Journal of Atmospheric and Solar-Terrestrial Physics 73 (10), 1228-1241.
[36] Klein, L.W., Burlaga, L.F., 1982. Interplanetary magnetic clouds At 1 AU. Journal of Geophysical Research 87 (A2), 613.
[37] Kopp, R., Pneuman, G., 1976. Magnetic reconnection in the corona and the loop prominence phenomenon. Solar Physics 50 (1), 85-98.
[38] Krieger, A., Timothy, A., Roelof, E., 1973. A coronal hole and its identification as the source of a high velocity solar wind stream. Solar Physics 29 (2), 505-525.
[39] Kumar, A., Rust, D.M., 1996. Interplanetary magnetic clouds, helicity conservation, and current-core flux-ropes. Journal of Geophysical Research: Space Physics 101 (A7), 15667-15684.
[40] Lepping, R., Acũna, M., Burlaga, L., Farrell, W., Slavin, J., Schatten, K., Mariani, F., Ness, N., Neubauer, F., Whang, Y., 1995. The WIND magnetic field investigation. Space Science Reviews 71 (1-4), 207-229.
[41] Lepping, R., Berdichevsky, D., Wu, C.-C., Szabo, A., Narock, T., Mariani, F., Lazarus, A., Quivers, A., 2006. A summary of WIND magnetic clouds for years 1995-2003: model-fitted parameters, associated errors and classifications, Annales Geophysicae. 215-245.
[42] Lepping, R.P., Jones, J.A., Burlaga, L.F., 1990. Magnetic field structure of interplanetary magnetic clouds at 1 AU. Journal of Geophysical Research 95 (A8), 11957.
[43] Longcope, D., Beveridge, C., Qiu, J., Ravindra, B., Barnes, G., Dasso, S., 2007. Modeling and measuring the flux reconnected and ejected by the two-ribbon flare/CME event on 7 November 2004. Solar Physics 244 (1-2), 45-73.
[44] Low, B., 1996. Solar activity and the corona. Solar Physics 167 (1-2), 217-265.
[45] Lundquist, S., 1950. Magneto-hydrostatic fields. Arkiv for Fysik 2 (4), 361-365.
[46] Möstl, C., Farrugia, C.J., Kilpua, E.K.J., Jian, L.K., Liu, Y., Eastwood, J.P., Harrison, R.A., Webb, D.F., Temmer, M., Odstrcil, D., Davies, J.A., Rollett, T., Luhmann, J.G., Nitta, N., Mulligan, T., Jensen, E.A., Forsyth, R., Lavraud, B., de Koning, C.A., Veronig, A.M., Galvin, A.B., Zhang, T.L., Anderson, B.J., 2012. Multi-Point Shock and Flux Rope Analysis of Multiple Interplanetary Coronal Mass Ejections around 2010 August 1 in the Inner Heliosphere. The Astrophysical Journal 758 (1), 10.
[47] Marubashi, K., 1986. Structure of the interplanetary magnetic clouds and their solar origins. Advances in Space Research 6 (6), 335-338.
[48] Marubashi, K., Lepping, R.P., 2007. Long-duration magnetic clouds: a comparison of analyses using torus- and cylinder-shaped flux rope models. Annales Geophysicae 25 (11), 2453-2477.
[49] Michalek, G., Gopalswamy, N., Lara, A., Yashiro, S., 2006. Properties and geoeffectiveness of halo coronal mass ejections. Space Weather 4 (10).
[50] Moldwin, M., Ford, S., Lepping, R., Slavin, J., Szabo, A., 2000. Small‐scale magnetic flux ropes in the solar wind. Geophysical Research Letters 27 (1), 57-60.
[51] Mulligan, T., Russell, C.T., Luhmann, J.G., 1998. Solar cycle evolution of the structure of magnetic clouds in the inner heliosphere. Geophysical Research Letters 25 (15), 2959-2962.
[52] Ogilvie, K., Chornay, D., Fritzenreiter, R., Hunsaker, F., Keller, J., Lobell, J., Miller, G., Scudder, J., Sittler Jr, E., Torbert, R., 1995. SWE, a comprehensive plasma instrument for the Wind spacecraft. Space Science Reviews 71 (1-4), 55-77.
[53] Parker, E.N., 1955. The Formation of Sunspots from the Solar Toroidal Field. The Astrophysical Journal 121, 491.
[54] Phillips, J., Bame, S., Barnes, A., Barraclough, B., Feldman, W., Goldstein, B., Gosling, J., Hoogeveen, G., McComas, D., Neugebauer, M., 1995. Ulysses solar wind plasma observations from pole to pole. Geophysical Research Letters 22 (23), 3301-3304.
[55] Pizzo, V., 1978. A three-dimensional model of corotating streams in the solar wind, 1. Theoretical foundations. Journal of Geophysical Research: Space Physics 83 (A12), 5563-5572.
[56] Riley, P., Schatzman, C., Cane, H., Richardson, I., Gopalswamy, N., 2006. On the rates of coronal mass ejections: Remote solar and in situ observations. The Astrophysical Journal 647 (1), 648.
[57] Sauvaud, J.A., Larson, D., Aoustin, C., Curtis, D., Médale, J.L., Fedorov, A., Rouzaud, J., Luhmann, J., Moreau, T., Schröder, P., Louarn, P., Dandouras, I., Penou, E., 2007. The IMPACT Solar Wind Electron Analyzer (SWEA). Space Science Reviews 136 (1-4), 227-239.
[58] Scherrer, P., Bogart, R., Bush, R., Hoeksema, J.-a., Kosovichev, A., Schou, J., Rosenberg, W., Springer, L., Tarbell, T., Wolfson, C., 1995. The solar oscillations investigation-Michelson Doppler imager. Solar Physics 162 (1-2), 129-188.
[59] Smith, E.J., Wolfe, J.H., 1976. Observations of interaction regions and corotating shocks between one and five AU: Pioneers 10 and 11. Geophysical Research Letters 3 (3), 137-140.
[60] Tripathi, D., Bothmer, V., Cremades, H., 2004. The basic characteristics of EUV post-eruptive arcades and their role as tracers of coronal mass ejection source regions. Astronomy & Astrophysics 422 (1), 337-349.
[61] Van Ballegooijen, A., Martens, P., 1989. Formation and eruption of solar prominences. The Astrophysical Journal 343, 971-984.
[62] Wilson, R.M., Hildner, E., 1986. On the association of magnetic clouds with disappearing filaments. Journal of Geophysical Research 91 (A5), 5867.
[63] Woltjer, L., 1958. On hydromagnetic equilibrium. Proceedings of the National Academy of Sciences 44 (9), 833-841.
[64] Woltjer, L., 1958. A theorem on force-free magnetic fields. Proceedings of the National Academy of Sciences 44 (6), 489-491.
[65] Yan, L., Luhmann, J., Lynch, B., Kilpua, E., 2014. Magnetic clouds and origins in STEREO era. Journal of Geophysical Research: Space Physics 119 (5), 3237-3246.
[66] Yashiro, S., Gopalswamy, N., Mäkelä, P., Akiyama, S., 2013. Post-eruption arcades and interplanetary coronal mass ejections. Solar Physics 284 (1), 5-15.
[67] Zhang, G., Burlaga, L.F., 1988. Magnetic clouds, geomagnetic disturbances, and cosmic ray decreases. Journal of Geophysical Research 93 (A4), 2511. |