Abstract
Response of the outer plasma sheet region to the substorm development on November 13, 1996 was studied with the plasma and magnetic field measurements obtained from INTERBALL-1 and GEOTAIL. In addition, the data from INTERBALL-2, LANL-080, -084 spacecraft and from Scandinavian and Siberian ground stations were used for the sub-storm timing. The solar wind and IMF which have been monitored by WIND spacecraft were rather variable during the early growth phase, but the remaining part of the growth phase as well as the expansion phase have been developed under stable southward IMF and relatively stable solar wind pressure. Few unusual features of substorm evolution have been revealed in our study. Measurements in the tail lobes and plasma sheet periphery during the growth phase showed that its behaviour differs from a classical scheme. Consideration of the total pressure behaviour during the substorm at distances 22 and 27.5 R E revealed cross-tail current substorm dynamics during the expansion phase. We concluded that current disruption impulsively propagated toward the tail from the near Earth plasma sheet region in accordance with the discrete character of the substorm development. In the course of the substorm the signatures of tailward propagating plasmoid were observed at northern and southern parts of the plasma sheet first by INTERBALL-1 (at 28 R E ) and later by GEOTAIL (at 22 R E ). Time delay in the registration of the plasmoid at two sides is hard to explain assuming the existence of only one plasmoid. This anomaly might be explained suggesting the asymmetric multiple plasmoid structure or (which is less probable) as signatures of completely different plasmoids. During the late expansion phase despite the enhanced convection at the dayside magnetosphere, the effective dissipation of energy in the disrupting current sheet resulted in the magnetotail collapse and in the plasma mantle approach to the INTERBALL-1 position.
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References
Baker D.N., Pulkkinen T.I., Angelopolous V., Baumjohann W. and McPherron R.L. (1996) Neutral line model of substorms: Past results and present view, J. Geophys. Res., 101, 12975–13010.
Bogott F.H. and Mozer F.S. (1973) Nightside energetic particle decreases at the synchronous orbit, J. Geophys. Res., 78, 8118–8127.
Caan M.N., McPherron R.L. and Russell C.T. (1978) The statistical magnetic signature of magnetospheric substorms,Planel. Space Sci., 26, 269–279.
Fairfield D.H. and Jones J. (1994) Variability of the tail lobe field strength J. Geophys. Res., 101, 7784–7791.
Hanasz J., Schreiber R., de Feraudy H., Mogilevsky M.M. and Romantsova T.V. (in press) Observations of the upper frequency cut-offs of the auroral kilometric radiation, Ann. Geophys.
Hones, E.W., Jr. (1992) Poleward leaping aurora, the substorm expansive and recovery phases and the recovery of the plasma sheet, Substorm 1, Bur. Space Egency, Spec. Publ., ESA SP-335,477.
Ieda A., Machida S., Mukai T., Saito Y., Yamamoto T., Nishida A., Terasawa T., and Kokubun S. (1998) Statistical analysis of the plasmoid evolution with Geotail observations, J. Geophys. Res., 103, 4453–4465.
Jacquey C., Sauvaud J.-A. and Dandouras J. (1991) Location and propagation of the magnetotail current disruption during substorm expansion - analysis and simulation of an ISEE multi-onset event, Geophys. Res. Lett., 18, 389–392.
Lutsenko V.N., Kudela K. and Sarris E.T. (1998) The DOK-2 experiment to study energetic particles by the Tail Probe and Auroral Probe satellites in the INTER-BALL project,Cosmic Research, 36, 93–102.
Nagai T., Fujimoto M., Saito Y., Machida S., Terasawa T., Nakamura R., Ya-mamoto T., Mukai T., Nishida A. and Kokubun S. (1998) Structure and dynamics of magnetic reconnection for substorm onsets with Geotail observations,J. Geophys. Res., 103, 4419–4440.
Nakai H. and Kamide Y. (1991) Estimating the long-term variations of the magnetotail pressure, J. Geophys. Res., 96, 23747–23751.
Nakai H. and Kamide Y. (1994) A model of the large-scale distribution of the neutral sheet current and its substrom-associated changes,J. Geophys. Res., 99, 2365–2373.
Ohtani S., Kokubun S. and Russell C.T. (1992) Radial expansion of the tail current disruption during substorms: A new approach to the substorm onset region,J. Geophys. Res., 97, 3129–3136.
Opgenoorth H.J., Pellinen R.J., Maurer H. et al. (1980) Ground-based observations of onset of localized field-aligned currents during auroral breakup around magnetic midnight,J. Geophys. Res., 48, 3101–115.
Ostapenko A.A. and Maltsev Yu.P. (1998) Three-dimensional magnetospheric response to variations in the solar wind dynamic pressure, Geophys. Res. Lett., 25, 261–263.
Petrukovich A.A., Sergeev V.A., Zelenyi L.M. et al. (1998) Two spacecraft observations of a reconnection pulse during an auroral breakup,J. Geophys. Res., 103, 47–59.
Pulkkinen T.I., Baker D.N., Pellinen R.J., Buchner J., Koskinen H.E.J., Lopez R.E., Dyson R.L. and Frank L.A. (1992) Particle scaterring and current sheet stability in the geomagnetic tail during the substorm growth phase,J. Geophys. Res., 97, 19283–19297.
Pulkkinen T. L, Baker D.N., Toivanen P.K., Pellinen R.J., Friedel R.H.W. and Korth A. (1994) Magnetospheric field and current distribution during the substorm recovery phase, J. Geophys. Res., 99, 10995–10966.
Ranta H., Ranta A., Collis R.N. and Hargreaves J.K. (1981) Development of the auroral absorption substorm: studies of pre-onset phase and sharp onset using an extensive riometer network,Planel. Space Sci., 29, 1287–1313.
Rostoker G., Akasofu S.-I., Foster J. et al. (1980) Magnetospheric substorms: definitions and signatures, J. Geophys. Res., 85, 1663–1668.
Sauvaud J.-A. and Winckler J.R. (1980) Dynamics of plasma, energetic particles, and fields near synchronous orbit in the night time sector during magnetospheric substorms,J. Geophys. Res., 85, 2043–2056.
Sckopke N., Paschmann G., Rosenbauer H. and Fairfield D.H. (1976) Influence of the interplanetary magnetic field on the occurrence and thickness of the plasma mantle, J. Geophys. Res., 81, 2687–2691.
Sergeev V.A. and Yahnin A.G. (1979) The features of the auroral bulge expansion,Planet. Space Sci., 27, 1429–1440.
Sergeev V.A. and Yahnin A.G. (1979) A detail study of the microsubstorm onsets, Geomagnetic Research (in Russian), 24, 90–100.
Sergeev V.A., Yahnin A.G. and Hones E.W., Jr. (1982) On the plasma sheet current changes during substorms as inferred from the data of IMP- 8 satellite, Cosmic Research (in Russian), 20, 636–639.
Wang Z. and Ashour-Abdalla M. (1992) Topological variation in the magnetic field line at the dayside magnetopause, J. Geophys. Res., 97, 8245–8255.
Yahnin A.G., Sergeev V.A., Pellinen R.J., Baumjohann W., Kaila K.U., Ranta H., Kangas J. and Raspopov O.M. (1983) Substorm time sequence and microstructure on 11 November 1976, J.Geophys.Res., 53, 182–197.
Yahnin A.G., Bosinger T., Kangas J. and Belian R.D. (1990) Some implications on substorm dynamics inferred from correlations between multiple flux peaks of drifting proton clouds and ground observations, Ann. Geophys., 8, 327–336.
Zelenyi L.M. and Kuznetsova M.M. (1984) Generation of the plasma sheet large-scale instabilities by plasma flows at the boundary of the magnetosphere, Plasma Physics, 10, 326–334.
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Borodkova, N.L. et al. (1999). Multi-Point Substorm Observations of the Outer Plasma Sheet Dynamics on November 13, 1996. In: Sibeck, D.G., Kudela, K. (eds) Interball in the ISTP Program. NATO Science Series, vol 537. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4487-2_2
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DOI: https://doi.org/10.1007/978-94-011-4487-2_2
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