Confirmation of existence of the small-scale field-aligned currents in middle and low latitudes and an estimate of time scale of their temporal variation
被引:19
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作者:
Iyemori, Toshihiko
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机构:
Kyoto Univ, Grad Sch Sci, Kyoto, JapanKyoto Univ, Grad Sch Sci, Kyoto, Japan
Iyemori, Toshihiko
[1
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Nakanishi, Kunihito
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Kyoto Univ, Grad Sch Sci, Kyoto, JapanKyoto Univ, Grad Sch Sci, Kyoto, Japan
Nakanishi, Kunihito
[1
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Aoyama, Tadashi
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Kyoto Univ, Grad Sch Sci, Kyoto, JapanKyoto Univ, Grad Sch Sci, Kyoto, Japan
Aoyama, Tadashi
[1
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Yokoyama, Yoshihiro
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Kyoto Univ, Grad Sch Sci, Kyoto, JapanKyoto Univ, Grad Sch Sci, Kyoto, Japan
Yokoyama, Yoshihiro
[1
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Koyama, Yukinobu
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Kyoto Univ, Grad Sch Sci, Kyoto, JapanKyoto Univ, Grad Sch Sci, Kyoto, Japan
Koyama, Yukinobu
[1
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Luehr, Hermann
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GFZ German Res Ctr Geosci, Helmholtz Ctr Potsdam, Potsdam, GermanyKyoto Univ, Grad Sch Sci, Kyoto, Japan
Luehr, Hermann
[2
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机构:
[1] Kyoto Univ, Grad Sch Sci, Kyoto, Japan
[2] GFZ German Res Ctr Geosci, Helmholtz Ctr Potsdam, Potsdam, Germany
magnetic field;
field-aligned current;
acoustic gravity wave;
middle latitudes;
atmospheric wave;
ionospheric dynamo;
SUMATRA EARTHQUAKE;
CHAMP;
D O I:
10.1002/2014GL062555
中图分类号:
P [天文学、地球科学];
学科分类号:
07 ;
摘要:
The magnetic data obtained by the SWARM (the Earth's Magnetic Field and Environment Explorers) satellites in middle or low latitudes during the initial 2months after launch were analyzed, when they flew nearly on the same orbit with variable time separation ranging from 5 to 100s. It was confirmed that the small-scale magnetic fluctuations having period around 10-30s are the manifestation of spatial structure of small-scale field-aligned currents along the orbits. From the statistical relation between correlation coefficients and two satellite separation in time, the typical time scale of temporal variation of the field-aligned current system is estimated to be around 200s for meridional component and 340s for zonal components of the magnetic fluctuations, respectively. Existence of shorter time scale around 30-50s was also found. These results suggest that the main source of current generation is the acoustic mode of atmospheric gravity waves.
机构:
Univ Colombo, Dept Phys, Astron & Space Sci Unit, Colombo 00300, Sri LankaUniv Colombo, Dept Phys, Astron & Space Sci Unit, Colombo 00300, Sri Lanka
Ranasinghe, Manjula
Fujimoto, Akiko
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Kyushu Inst Technol, Fac Comp Sci & Syst Engn, 680-4 Kawazu, Fukuoka 8208502, JapanUniv Colombo, Dept Phys, Astron & Space Sci Unit, Colombo 00300, Sri Lanka
Fujimoto, Akiko
Yoshikawa, Akimasa
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机构:
Kyushu Univ, Int Ctr Space Weather Sci & Educ ICSWSE, Nishi Ku, 744 Motooka, Fukuoka 8190395, JapanUniv Colombo, Dept Phys, Astron & Space Sci Unit, Colombo 00300, Sri Lanka
Yoshikawa, Akimasa
Jayaratne, Chandana
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机构:
Univ Colombo, Dept Phys, Astron & Space Sci Unit, Colombo 00300, Sri LankaUniv Colombo, Dept Phys, Astron & Space Sci Unit, Colombo 00300, Sri Lanka