日本地球惑星科学連合2018年大会

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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-EM16] Dynamics of Earth's Inner Magnetosphere and Initial Results from Arase

2018年5月22日(火) 13:45 〜 15:15 303 (幕張メッセ国際会議場 3F)

コンビーナ:Danny Summers(Memorial University of Newfoundland)、三好 由純(名古屋大学宇宙地球環境研究所)、細川 敬祐(電気通信大学大学院情報理工学研究科、共同)、海老原 祐輔(京都大学生存圏研究所)、座長:海老原 祐輔(京都大学生存圏研究所)

14:15 〜 14:30

[PEM16-33] Hectometric Line Radiation found by the Arase (ERG) satellite

*橋本 弘藏1熊本 篤志2土屋 史紀2笠原 禎也3 (1.京都大学、2.東北大学、3.金沢大学)

キーワード:あらせ、ヘクトメーター波

Nonthermal terrestrial continuum at frequencies below ~100 kHz was characterized by Gurnett and Shaw (1973) and Gurnett (1975). These emissions are found to originate at the plasma frequency at steep density gradients at the plasma pause and magnetopause regions of the Earth's magnetosphere. A higher frequency component of terrestrial continuum that appears to be generated inside the Earth’s plasmasphere was detected by the Geotail satellite at a frequency of 100 to 800 kHz, corresponding to the plasma frequency inside the plasmasphere at an altitude extending down to only a few thousand kilometers in the topside equatorial region of the Earth's ionosphere (Hashimoto et al., 1999 and 2006). They named this component as 'kilometric continuum' (KC), which is found to consist of multiple narrowband emissions sometimes lasting for 5 hours or more at a constant or slowly drifting frequency.

We reports newly observed line radiations with even higher frequencies in hectometric wavelengths of 600 to 1,700 kHz found by the Arase (ERG) satellite. Since they are composed of line spectra, we have named this as ‘hectometric line radiation’ (HLR). Although they look like extension of kilometric continuum, they are generally line emissions with long durations different from KC. This has the following characteristics.

1. This is composed of line emissions.
2. This sometimes continues more than five hours.
3. Their frequencies occasionally change.
4. The frequency rage is from 600 kHz to 1,700 kHz.
5. This terminates before the local plasma frequencies or UHR frequencies become close to the frequencies of emission lines.
6. It is not possible for medium frequency broadcasting signals to pass the ionosphere since foF2s are higher the signal frequencies.

In conclusion, the HLR is believed to be new radio emissions generated in the topside ionosphere.

References
Gurnett, D. A. (1975), The Earth as a radio source: The nonthermal continuum, J. Geophys. Res., 80, 2751-2763.

Gurnett, D. A., and R. R. Shaw (1973), Electromagnetic radiation trapped in the magnetosphere above the plasma frequency, J. Geophys. Res., 78, 8136-8149.

Hashimoto, K., W. Calvert, and H. Matsumoto (1999), Kilometric continuum detected by Geotail, J. Geophys. Res., 104, 28,645? 28,656.

Hashimoto, K., J. L. Green, R. R. Anderson, and H. Matsumoto (2006), Review of kilometric continuum, in geospace, Electromagnetic Waves and Radiation, Lect. Not. in Phys., vol. 687, edited by J. W. LaBelle and R. A. Treumann, pp. 37?54, Springer, New York.