Identification of the different magnetic field contributions during a geomagnetic storm in magnetospheric and ground observations

被引:24
|
作者
Alberti, Tommaso [1 ]
Piersanti, Mirko [2 ]
Vecchio, Antonio [3 ]
De Michelis, Paola [4 ]
Lepreti, Fabio [1 ]
Carbone, Vincenzo [1 ]
Primavera, Leonardo [1 ]
机构
[1] Univ Calabria, Dept Phys, Arcavacata Di Rende, CS, Italy
[2] Univ Aquila, Dept Phys & Chem Sci, Laquila, Italy
[3] LESIA Observ Paris, 5 Pl Jules Janssen, F-92190 Meudon, France
[4] Ist Nazl Geofis & Vulcanol, Sect Geomagnetism Aeron & Enviromental Geophys, Rome, Italy
关键词
Magnetospheric physics; magnetosphere-ionosphere interactions; solar-wind magnetosphere interactions; storms and substorms; EMPIRICAL MODE DECOMPOSITION; 2003 HALLOWEEN SUPERSTORM; QUIET DAILY VARIATION; TEMPERATURE-CHANGES; ULF WAVES; SOLAR; IONOSPHERE; ATMOSPHERE; PRESSURE; FEATURES;
D O I
10.5194/angeo-34-1069-2016
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We used the empirical mode decomposition (EMD) to investigate the time variation of the magnetospheric and ground-based observations of the Earth's magnetic field during both quiet and disturbed periods. We found two timescale variations in magnetospheric data which are associated with different magnetospheric current systems and the characteristic diurnal orbital variation, respectively. On the ground we identified three timescale variations related to the solar-wind-magnetosphere high-frequency interactions, the ionospheric processes, and the internal dynamics of the magnetosphere. This approach is able to identify the different physical processes involved in solar-windmagnetosphere- ionosphere coupling. In addition, the largetimescale contribution can be used as a local index for the identification of the intensity of a geomagnetic storm on the ground.
引用
收藏
页码:1069 / 1084
页数:16
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