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Vertical evolution of auroral acceleration at substorm onset
被引:19
|作者:
Morioka, A.
[1
]
Miyoshi, Y.
[2
]
Tsuchiya, F.
[1
]
Misawa, H.
[1
]
Yumoto, K.
[3
]
Parks, G. K.
[4
]
Anderson, R. R.
[5
]
Menietti, J. D.
[5
]
Honary, F.
[6
]
机构:
[1] Tohoku Univ, Planetary Plasma & Atmospher Res Ctr, Sendai, Miyagi 980, Japan
[2] Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan
[3] Kyushu Univ, Space Environm Res Ctr, Fukuoka 812, Japan
[4] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[5] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[6] Univ Lancaster, Dept Commun Syst, Lancaster, England
关键词:
Magnetospheric physics;
Auroral phenomena;
Magnetosphere-ionosphere interactions;
Storms and substorms;
PARALLEL ELECTRIC-FIELDS;
ALFVEN-WAVE ACCELERATION;
KILOMETRIC RADIATION;
MAGNETOSPHERIC SUBSTORMS;
IMAGE-FUV;
SATELLITE;
PARTICLE;
REGION;
SIGNATURES;
BURSTS;
D O I:
10.5194/angeo-27-525-2009
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
This study describes the onset process of auroral substorms in connection with the vertical evolution of auroral particle acceleration, on the basis of auroral kilometric radiation (AKR) dynamics. We show that the auroral acceleration process at substorm onset basically consists of two stages: (1) appearance/intensification of a low-altitude acceleration region at 4000-5000 km accompanied by initial brightening and (2) breakout of high-altitude field-aligned acceleration above the pre-existing low-altitude acceleration region at 6000-12 000 km, which is followed by auroral breakup and poleward expansion. It is also revealed that this two-stage evolution of auroral acceleration corresponds to the two-step reinforcement of field-aligned current.
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页码:525 / 535
页数:11
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