Open Access
Issue
J. Space Weather Space Clim.
Volume 5, 2015
Article Number A13
Number of page(s) 15
DOI https://doi.org/10.1051/swsc/2015016
Published online 16 June 2015
  • Adams, W.G. Comparison of simultaneous magnetic disturbances at several observatories. Philos. Trans. R. Soc. London, Ser., 183, 131–140, 1892. [CrossRef]
  • Akasofu, S.I., and S. Chapman. The sudden commencements of geomagnetic storms. URANIA, 44 (250), 321–358, 1959.
  • Araki, T. Global structure of geomagnetic sudden commencements, Planet. Space Sci., 25, 373–384, 1977. [CrossRef]
  • Araki, T. A physical model of the geomagnetic sudden commencement. In: M.J., Engebretson, K. Takahashi, and M. Scholer, Editors. Solar Wind Sources of Magnetospheric Ultra-Low-Frequency Waves, Geophys. Monogr. Ser., vol. 81, AGU, Washington DC, 183, 1994. [CrossRef]
  • Araki, T., T. Takeuchi, and Y. Araki. Rise time of geomagnetic sudden commencements – statistical analysis of ground geomagnetic data. Earth Planets Space, 56, 289–293, 2004. [CrossRef]
  • Araki, T., K. Keika, T. Kamei, H. Yang, and S. Alex. Nighttime enhancement of the amplitude of geomagnetic sudden commencements and its dependence on IMF-Bz. Earth Planets Space, 58, 45–50, 2006. [CrossRef]
  • Auster, H.U., K.H. Glassmeier, W. Magnes, O. Aydogar, W. Baumjohann, et al. The THEMIS fluxgate magnetometer. Space Sci. Rev., 141, 235–264, 2008, DOI: 10.1007/s11214-008-9365-9. [CrossRef]
  • Balogh, A., M.W. Dunlop, S.W.H. Cowley, D.J. Southwood, J.G. Thomlinson, et al. The cluster magnetic field investigation. Space Sci. Rev., 79, 65–92, 1997. [CrossRef]
  • Belian, R.D., G.R. Gisler, T. Cayton, and R. Christensen. High-z energetic particles at geostationary orbit during the great solar proton event series of October 1989. J. Geophys. Res., 97, 16897, 1992. [CrossRef]
  • Carpenter, D.L., and R.R. Anderson. An ISEE/whistler model of equatorial electron-density in the magnetosphere. J. Geophys. Res., 97, 1097–1108, 1992, DOI: 10.1097/91JA01549. [CrossRef]
  • Colburn, D.S., and C.P. Sonett. Discontinuities in the solar wind. Space Sci. Rev., 5, 43, 1966. [NASA ADS] [CrossRef]
  • Curto, J.J., T. Araki, and L.F. Alberca. Evolution of the concept of Sudden Storm Commencements and their operative identification. Earth Planets Space, 59, i–xii, 2007. [CrossRef]
  • Davis, T.N., and M. Sugiura. Auroral electrojet activity index AE and its universal time variations. J. Geophys. Res., 71 (3), 785–801, 1966, DOI: 10.1029/JZ071i003p00785. [CrossRef]
  • Ellis, W. On the simultaneity of magnetic variations at different places on occasions of magnetic disturbance, and on the relation between magnetic and earth current phenomena. Proc. Roy. Soc., 102, 191, 1892. [CrossRef]
  • Frank, L.A., K.L. Ackerson, W.R. Paterson, J.A. Lee, M.R. English, and G.L. Pickett. The Comprehensive Plasma Instrumentation (CPI) for the Geotail spacecraft. J. Geomagn. Geoelectr., 46, 23–37, 1994. [CrossRef]
  • Iyemori, T. Storm-time magnetospheric currents inferred from mid-latitude geomagnetic field variations. J. Geomagn. Geoelectr., 42, 1249–1265, 1990. [CrossRef]
  • Keika, K., R. Nakamura, W. Baumjohann, A. Runov, T. Takada, et al. Response of the inner magnetosphere and the plasma sheet to a sudden impulse. J. Geophys. Res., 113, A07S35, 2008, DOI: 10.1029/2007JA012763.
  • Keika, K., R. Nakamura, W. Baumjohann, V. Angelopoulos, P.J. Chi, et al. Substorm expansion triggered by a sudden impulse front propagating from the dayside magnetopause. J. Geophys. Res., 114, A00C24, 2009, DOI: 10.1029/2008JA013445.
  • Kokubun, S. Characteristics of storm sudden commencement at geostationary orbit. J. Geophys. Res., 88, 10025–10033, 1983. [CrossRef]
  • Kokubun, S., T. Yamamoto, M.H. Acuña, K. Hayashi, K. Shiokawa, and H. Kawano. The Geotail magnetic-field experiment. J. Geomagn. Geoelectr., 46, 7–21, 1994. [CrossRef]
  • Lepping, R.P., M.H. Acuña, L.F. Burlaga, W.M. Farrell, J.A. Slavin, et al. The Wind magnetic field investigation. Space Sci. Rev., 71, 207–299, 1995, DOI: 10.1007/BF00751330. [NASA ADS] [CrossRef]
  • Lin, R.P., K.A. Anderson, S. Ashford, C. Carlson, D. Curtis, et al. A three-dimensional plasma and energetic particle investigation for the Wind spacecraft, Space Sci. Rev., 71, 125–153, 1995, DOI: 10.1007/BF00751328. [NASA ADS] [CrossRef]
  • Matsushita, S. Studies on sudden commencements of geomagnetic storms using IGY data from United States stations. J. Geophys. Res., 65, 1423–1435, 1960. [CrossRef]
  • Rodés, L. On the non-simultaneity of magnetic storms. Terr. Mag. Atmos. Electr., 27 (4), 161–166, 1922. [CrossRef]
  • Samsonov, A.A., D.G. Sibeck, N.V. Zolotova, H.K. Biernat, S.H. Chen, et al. Propagation of a sudden impulse through the magnetosphere initiating magnetospheric Pc5 pulsations. J. Geophys. Res., 116, A10216, 2011, DOI: 10.1029/2011JA016706. [CrossRef]
  • Shue, J.H., P. Song, C.T. Russell, J.T. Steinberg, J.K. Chao, et al. Magnetopause location under extreme solar wind conditions. J. Geophys. Res., 103, 17691–17700, 1998. [NASA ADS] [CrossRef]
  • Siscoe, G.L., V. Formisano, A.J. Lazarus. Relation between geomagnetic sudden impulses and solar wind pressure changes – an experimental investigation. J. Geophys. Res., 73, 15, 1968.
  • Smith, C.W., J. L’Heureux, N.F. Ness, M.H. Acuña, L.F. Burgala, and J. Scheifele. The ACE magnetic fields experiment. Space Sci. Rev., 86, 613–632, 1998, DOI: 10.1023/A:1005092216668. [NASA ADS] [CrossRef]
  • Sugiura, M., and D.J. Poros. Hourly values of equatorial Dst for years 1957 to 1970, Rep. X-645-71-278, Goddard Space Flight Center, Greenbelt, Maryland, 1971.
  • Tanakade, A. Short preliminary report on three sudden commencements of geomagnetic storms. Comptes Rendues Assemblée de Lisbone, 1933, UGGI, Assoc. Magnetism Electr. Bull., 9, 149–157, 1934.
  • Tsunomura, S., and T. Araki. Numerical analysis of equatorial enhancement of geomagnetic sudden commencement. Planet. Space Sci., 32 (5), 599–604, 1984. [CrossRef]
  • Tsurutani, B.T., and R.P. Lin. Acceleration of >47 keV ions and >2 keV electrons by interplanetary shocks at 1 AU, J. Geophys. Res., 90 (A1), 1–11, 1985. [NASA ADS] [CrossRef]
  • Tsurutani, B.T., E. Echer, F.L. Guarnieri, and J.U. Kozyra. CAWSES November 7–8, 2004, superstorm: complex solar and interplanetary features in the post-solar maximum phase. Geophys. Res. Lett., 35, L06S05, 2008, DOI: 10.1029/2007GL031473. [CrossRef]
  • Tsurutani, B.T., G.S. Lakhina, O.P. Verkhoglyadova, W.D. Gonzalez, E. Echer, et al. A review of interplanetary discontinuities and their geomagnetic effects. J. Atmos. Sol. Terr. Phys., 73, 5, 2011, DOI: 10.1016/j.jastp.2010.04.001. [CrossRef]
  • Tsurutani, B.T., E. Echer, K. Shibata, O.P. Verkhoglyadova, A.J. Mannucci, et al. The interplanetary causes of geomagnetic activity during the 7–17 March 2012 interval: a CAWSES II overview. J. Space Weather Space Clim., 4, A02, 2014, DOI: 10.1051/swsc/2013056. [CrossRef] [EDP Sciences]
  • Tsyganenko, N.A. A magnetospheric field model with a warped tail current sheet. Planet. Space Sci., 37, 5–20, 1989. [NASA ADS] [CrossRef]
  • Volwerk, M., J. Berchem, Y.V. Bogdanova, O.D. Constantinescu, M.W. Dunlop, et al. Interplanetary magnetic field rotations followed from L1 to the ground: the response of the Earth’s magnetosphere as seen by multi-spacecraft and ground-based observations. Ann. Geophys., 29, 1549–1569, 2011. [CrossRef]
  • Vorotnikov, V.S., C.W. Smith, Q. Hu, A. Szabo, R.M. Skoug, et al. Automated shock detection and analysis algorithm for space weather application. Space Weather, 6, S03002, 2008, DOI: 10.1029/2007SW000358. [CrossRef]
  • Wanliss, J.A., and K.M. Showalter. High-resolution global storm index: Dst versus YM-H. J. Geophys. Res., 111, A02202, 2006, DOI: 10.1029/2005JA011034.
  • Wilken, B., C.K. Goertz, D.N. Baker, P.R. Higbie, and T.A. Fritz. The SSC on July 29, 1977 and its propagation within the magnetosphere. J. Geosphys. Res., 87, 5901–5910, 1982. [CrossRef]

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