Study on plasma waves and electron density profile around the moon observed by KAGUYA in the solar wind

Yoshiya Kasahara; Kazuya Kanatani; Yoshitaka Goto; Kozo Hashimoto; Yoshiharu Omura; Masaki N. Nishino; Hideo Tsunakawa; Takayuki Ono

doi:10.1109/URSIGASS.2014.6929918

Study on plasma waves and electron density profile around the moon observed by KAGUYA in the solar wind

Yoshiya Kasahara, Kazuya Kanatani, Yoshitaka Goto, Kozo Hashimoto, Yoshiharu Omura, Masaki N. Nishino, Hideo Tsunakawa, Takayuki Ono

SCI - Geophysics

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

The moon has basically no intrinsic magnetic field and atmosphere, and plasma cavity called 'Lunar Wake'' is created just behind the moon in the solar wind. Electrons which collided with moon surface are supposed to be carried toward downstream region of solar wind forming unique electron density distribution around the moon. In the present paper, we study electron density profile around the moon at nominal altitude of KAGUYA (∼100km) in the solar wind controlled by the parameters such as IMF direction and solar wind velocity.

Original language	English
Title of host publication	2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014
Publisher	Institute of Electrical and Electronics Engineers Inc.
ISBN (Electronic)	9781467352253
DOIs	https://doi.org/10.1109/URSIGASS.2014.6929918
Publication status	Published - 2014 Oct 17
Event	31st General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2014 - Beijing, China Duration: 2014 Aug 16 → 2014 Aug 23

Publication series

Name	2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014

Other

Other	31st General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2014
Country/Territory	China
City	Beijing
Period	14/8/16 → 14/8/23

ASJC Scopus subject areas

Electrical and Electronic Engineering
Computer Networks and Communications

Access to Document

10.1109/URSIGASS.2014.6929918

Cite this

Kasahara, Y., Kanatani, K., Goto, Y., Hashimoto, K., Omura, Y., Nishino, M. N., Tsunakawa, H., & Ono, T. (2014). Study on plasma waves and electron density profile around the moon observed by KAGUYA in the solar wind. In 2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014 [6929918] (2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014). Institute of Electrical and Electronics Engineers Inc.. https://doi.org/10.1109/URSIGASS.2014.6929918

Study on plasma waves and electron density profile around the moon observed by KAGUYA in the solar wind. / Kasahara, Yoshiya; Kanatani, Kazuya; Goto, Yoshitaka et al.

2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014. Institute of Electrical and Electronics Engineers Inc., 2014. 6929918 (2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Kasahara, Y, Kanatani, K, Goto, Y, Hashimoto, K, Omura, Y, Nishino, MN, Tsunakawa, H & Ono, T 2014, Study on plasma waves and electron density profile around the moon observed by KAGUYA in the solar wind. in 2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014., 6929918, 2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014, Institute of Electrical and Electronics Engineers Inc., 31st General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2014, Beijing, China, 14/8/16. https://doi.org/10.1109/URSIGASS.2014.6929918

Kasahara Y, Kanatani K, Goto Y, Hashimoto K, Omura Y, Nishino MN et al. Study on plasma waves and electron density profile around the moon observed by KAGUYA in the solar wind. In 2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014. Institute of Electrical and Electronics Engineers Inc. 2014. 6929918. (2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014). doi: 10.1109/URSIGASS.2014.6929918

Kasahara, Yoshiya ; Kanatani, Kazuya ; Goto, Yoshitaka et al. / Study on plasma waves and electron density profile around the moon observed by KAGUYA in the solar wind. 2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014. Institute of Electrical and Electronics Engineers Inc., 2014. (2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014).

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title = "Study on plasma waves and electron density profile around the moon observed by KAGUYA in the solar wind",

abstract = "The moon has basically no intrinsic magnetic field and atmosphere, and plasma cavity called 'Lunar Wake'' is created just behind the moon in the solar wind. Electrons which collided with moon surface are supposed to be carried toward downstream region of solar wind forming unique electron density distribution around the moon. In the present paper, we study electron density profile around the moon at nominal altitude of KAGUYA (∼100km) in the solar wind controlled by the parameters such as IMF direction and solar wind velocity.",

author = "Yoshiya Kasahara and Kazuya Kanatani and Yoshitaka Goto and Kozo Hashimoto and Yoshiharu Omura and Nishino, {Masaki N.} and Hideo Tsunakawa and Takayuki Ono",

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doi = "10.1109/URSIGASS.2014.6929918",

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AU - Kasahara, Yoshiya

AU - Kanatani, Kazuya

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AU - Hashimoto, Kozo

AU - Omura, Yoshiharu

AU - Nishino, Masaki N.

AU - Tsunakawa, Hideo

AU - Ono, Takayuki

PY - 2014/10/17

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N2 - The moon has basically no intrinsic magnetic field and atmosphere, and plasma cavity called 'Lunar Wake'' is created just behind the moon in the solar wind. Electrons which collided with moon surface are supposed to be carried toward downstream region of solar wind forming unique electron density distribution around the moon. In the present paper, we study electron density profile around the moon at nominal altitude of KAGUYA (∼100km) in the solar wind controlled by the parameters such as IMF direction and solar wind velocity.

AB - The moon has basically no intrinsic magnetic field and atmosphere, and plasma cavity called 'Lunar Wake'' is created just behind the moon in the solar wind. Electrons which collided with moon surface are supposed to be carried toward downstream region of solar wind forming unique electron density distribution around the moon. In the present paper, we study electron density profile around the moon at nominal altitude of KAGUYA (∼100km) in the solar wind controlled by the parameters such as IMF direction and solar wind velocity.

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Study on plasma waves and electron density profile around the moon observed by KAGUYA in the solar wind

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