JpGU-AGU Joint Meeting 2017

講演情報

[EE] ポスター発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM14] [EE] Dynamics in magnetosphere and ionosphere

2017年5月20日(土) 10:45 〜 12:15 ポスター会場 (国際展示場 7ホール)

コンビーナ:堀 智昭(東京大学大学院理学系研究科)、田中 良昌(国立極地研究所)、中溝 葵(情報通信研究機構 電磁波計測研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)

[PEM14-P29] The estimation of spatial structures of magnetospheric plasma by using the data observed by LEO satelites.

*横山 佳弘1家森 俊彦2青山 忠司1 (1.京都大学大学院理学研究科地球惑星科学専攻、2.京都大学大学院理学研究科附属地磁気世界資料解析センター)

キーワード:SWARM satellite, magnetospheric plasma

In the regions of high-beta plasma such as the plasma sheet or the boundary layer in the magnetosphere, it can be expected that the plasma behaves as turbulence due to the effects of various plasma instabilities, non-linear development of Alfven waves, and so on. Satellites in the plasmasheet also have observed the fluctuations in velocity and magnetic field that have the characteristics of fluid turbulence (Borovsky et al. 1997). If the plasmas usually behave as turbulence, the spectrum and their distribution are important for understanding phenomena in the magnetosphere. However, it is almost impossible to have sufficient simultaneous satellite observations that cover the huge magnetospheric domain.

On the other hand, we confirmed that the magnetic fluctuations having period longer than 2s observed by low Earth orbit (LEO) satellites can be regarded as the manifestation of the spatial structure of the field-aligned currents by using the magnetic data obtained by Swarm satellites during December, 2013 when the satellites flew on nearly the same orbits with slight time separations. In addition, the LEO satellites fly through wide range of magnetic latitudes in a short period of time, so, by project- ing their orbits into the magnetosphere, they can scan wide range on the equatorial plane of the magnetosphere. therefore, by projecting these fluctuations onto the equatorial plane of the magnetosphere, i.e., the source regions of field-aligned currents, we try to estimate the distribution of turbulent region and their characteristics there.

We made statical maps of the amplitude of magnetic fluctuations for both quiet(AE<50nT) and disturbed(AE>50nT) conditions. We also made spectral analysis of magnetic fluctuations by MEM and found that there are many peaks in wide frequency range in every spectrum regardless of the geomagnetic conditions, MLTs, and so on.

This result suggests that the magnetospheric plasmas usually behave as turbulence.
In this paper, in addition to the result above, we also discuss the wave-number spectrum in the magnetosphere.