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JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 110, A09S25, doi:10.1029/2005JA011070, 2005

Geotail observations of signatures in the near-Earth magnetotail for the extremely intense substorms of the 30 October 2003 storm

Y. Miyashita

Solar-Terrestrial Environment Laboratory, Nagoya University, Toyokawa, Japan


Y. Miyoshi

Solar-Terrestrial Environment Laboratory, Nagoya University, Toyokawa, Japan


Y. Matsumoto

21st Century Center of Excellence Program, Graduate School of Environmental Studies, Nagoya University, Nagoya, Japan


A. Ieda

Solar-Terrestrial Environment Laboratory, Nagoya University, Toyokawa, Japan


Y. Kamide

Solar-Terrestrial Environment Laboratory, Nagoya University, Toyokawa, Japan


M. Nosé

Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University, Kyoto, Japan


S. Machida

Department of Geophysics, Kyoto University, Kyoto, Japan


H. Hayakawa

Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan


R. W. McEntire

Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA


S. P. Christon

Focused Analysis and Research, Columbia, Maryland, USA


D. S. Evans

Space Environment Center, NOAA, Boulder, Colorado, USA


O. A. Troshichev

Arctic and Antarctic Research Institute, St. Petersburg, Russia


Abstract

Two coronal mass ejections associated with the X17 and X10 solar flares reached the Earth's environment at very high speeds on 29 and 30 October 2003, respectively, causing very intense geomagnetic storms (Dst ∼ −400 nT). The present study focused on the main phase of the 30 October storm during which the Geotail spacecraft was within the near-Earth magnetotail at X ∼ −8 R E . A number of extremely intense substorms occurred during this period. In one of them, the intensity of the westward auroral electrojet exceeded 3000 nT, which was one of the largest magnitudes ever observed. The energetic particle observations from the low-altitude, polar-orbiting NOAA satellites indicate that the auroral oval shifted equatorward to magnetic latitudes much lower than usual, as low as 50°. Throughout the interval, the magnetic field in the near-Earth magnetotail, and possibly the plasma density, was much larger than usual, indicating a considerable degree of energy accumulation in the lobe region and compression of the plasma sheet and very intense cross-tail currents. The dense plasma may be responsible for the intense auroral electrojet and the intense ring current. Very large, rapid dipolarizations occurred in relation to the intense substorms. High-energy particle fluxes were an order of magnitude higher than usual, and their increases took place immediately after the dipolarizations. Fast tailward flows with large southward magnetic fields as well as fluxes of energetic heavy ions (oxygen) were also observed, suggesting that the magnetic reconnection took place in the near-Earth magnetotail, associated with the very intense substorms. This location is much closer to the Earth than usual, probably as close to the Earth as ever reported. These magnetotail and auroral observations as well as other results reported previously suggest that the entire magnetosphere was considerably distorted during the storm.

Received 13 February 2005; accepted 6 June 2005; published 3 September 2005.

Keywords: superstorm; Geotail; dipolarization.

Index Terms: 2788 Magnetospheric Physics: Magnetic storms and substorms (7954); 2744 Magnetospheric Physics: Magnetotail; 2784 Magnetospheric Physics: Solar wind/magnetosphere interactions; 2704 Magnetospheric Physics: Auroral phenomena (2407); 2723 Magnetospheric Physics: Magnetic reconnection (7526, 7835).

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Citation: Miyashita, Y., et al. (2005), Geotail observations of signatures in the near-Earth magnetotail for the extremely intense substorms of the 30 October 2003 storm, J. Geophys. Res., 110, A09S25, doi:10.1029/2005JA011070.