An EUV spectrometer on earth-orbiting satellite for planetary science

Hiroaki Ishii; Kouichi Sakai; Tatsuro Homma; Ichiro Yoshikawa; Kazuo Yoshioka; Go Murakami; Munetaka Ueno; Atsushi Yamazaki; Kazunori Uemizu; Masato Kagitani; Fuminori Tsuchiya; Naoki Terada

doi:10.1117/12.892085

An EUV spectrometer on earth-orbiting satellite for planetary science

Hiroaki Ishii, Kouichi Sakai, Tatsuro Homma, Ichiro Yoshikawa, Kazuo Yoshioka, Go Murakami, Munetaka Ueno, Atsushi Yamazaki, Kazunori Uemizu, Masato Kagitani, Fuminori Tsuchiya, Naoki Terada

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

Abstract

EXtreme ultraviolet spectrosCope for ExosphEric Dynamics (EXCEED) will carry out the extreme ultraviolet (EUV) spectroscopic imaging observations from earth orbit. It clarifies the plasma distributions and compositions around the various planets and examines the interactions with the solar wind. Observations should be carried out at high altitude so that the earth's atmospheric absorption is free. Our spectral range is from 60 to 145 nm and the spectral resolution is 0.3 to 1 nm (FWHM). The mission is planned to be launched in 2013, beginning of the next period of solar maximum. In this paper, we will introduce the general mission overview, scientific objectives and development of instrument.

Original language	English
Title of host publication	UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVII
DOIs	https://doi.org/10.1117/12.892085
Publication status	Published - 2011
Event	UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVII - San Diego, CA, United States Duration: 2011 Aug 21 → 2011 Aug 24

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	8145
ISSN (Print)	0277-786X

Conference

Conference	UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVII
Country/Territory	United States
City	San Diego, CA
Period	11/8/21 → 11/8/24

Keywords

EUV
Jupiter
Mars
Venus
planetary plasma
small satellite series
spectroscope

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10.1117/12.892085

Cite this

Ishii, H., Sakai, K., Homma, T., Yoshikawa, I., Yoshioka, K., Murakami, G., Ueno, M., Yamazaki, A., Uemizu, K., Kagitani, M., Tsuchiya, F., & Terada, N. (2011). An EUV spectrometer on earth-orbiting satellite for planetary science. In UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVII Article 81450O (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8145). https://doi.org/10.1117/12.892085

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title = "An EUV spectrometer on earth-orbiting satellite for planetary science",

abstract = "EXtreme ultraviolet spectrosCope for ExosphEric Dynamics (EXCEED) will carry out the extreme ultraviolet (EUV) spectroscopic imaging observations from earth orbit. It clarifies the plasma distributions and compositions around the various planets and examines the interactions with the solar wind. Observations should be carried out at high altitude so that the earth's atmospheric absorption is free. Our spectral range is from 60 to 145 nm and the spectral resolution is 0.3 to 1 nm (FWHM). The mission is planned to be launched in 2013, beginning of the next period of solar maximum. In this paper, we will introduce the general mission overview, scientific objectives and development of instrument.",

keywords = "EUV, Jupiter, Mars, Venus, planetary plasma, small satellite series, spectroscope",

author = "Hiroaki Ishii and Kouichi Sakai and Tatsuro Homma and Ichiro Yoshikawa and Kazuo Yoshioka and Go Murakami and Munetaka Ueno and Atsushi Yamazaki and Kazunori Uemizu and Masato Kagitani and Fuminori Tsuchiya and Naoki Terada",

year = "2011",

doi = "10.1117/12.892085",

language = "English",

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series = "Proceedings of SPIE - The International Society for Optical Engineering",

booktitle = "UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVII",

note = "UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVII ; Conference date: 21-08-2011 Through 24-08-2011",

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Ishii, H, Sakai, K, Homma, T, Yoshikawa, I, Yoshioka, K, Murakami, G, Ueno, M, Yamazaki, A, Uemizu, K, Kagitani, M , Tsuchiya, F & Terada, N 2011, An EUV spectrometer on earth-orbiting satellite for planetary science. in UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVII., 81450O, Proceedings of SPIE - The International Society for Optical Engineering, vol. 8145, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVII, San Diego, CA, United States, 11/8/21. https://doi.org/10.1117/12.892085

An EUV spectrometer on earth-orbiting satellite for planetary science. / Ishii, Hiroaki; Sakai, Kouichi; Homma, Tatsuro et al.
UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVII. 2011. 81450O (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8145).

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

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AU - Ishii, Hiroaki

AU - Sakai, Kouichi

AU - Homma, Tatsuro

AU - Yoshikawa, Ichiro

AU - Yoshioka, Kazuo

AU - Murakami, Go

AU - Ueno, Munetaka

AU - Yamazaki, Atsushi

AU - Uemizu, Kazunori

AU - Kagitani, Masato

AU - Tsuchiya, Fuminori

AU - Terada, Naoki

PY - 2011

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N2 - EXtreme ultraviolet spectrosCope for ExosphEric Dynamics (EXCEED) will carry out the extreme ultraviolet (EUV) spectroscopic imaging observations from earth orbit. It clarifies the plasma distributions and compositions around the various planets and examines the interactions with the solar wind. Observations should be carried out at high altitude so that the earth's atmospheric absorption is free. Our spectral range is from 60 to 145 nm and the spectral resolution is 0.3 to 1 nm (FWHM). The mission is planned to be launched in 2013, beginning of the next period of solar maximum. In this paper, we will introduce the general mission overview, scientific objectives and development of instrument.

AB - EXtreme ultraviolet spectrosCope for ExosphEric Dynamics (EXCEED) will carry out the extreme ultraviolet (EUV) spectroscopic imaging observations from earth orbit. It clarifies the plasma distributions and compositions around the various planets and examines the interactions with the solar wind. Observations should be carried out at high altitude so that the earth's atmospheric absorption is free. Our spectral range is from 60 to 145 nm and the spectral resolution is 0.3 to 1 nm (FWHM). The mission is planned to be launched in 2013, beginning of the next period of solar maximum. In this paper, we will introduce the general mission overview, scientific objectives and development of instrument.

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KW - Jupiter

KW - Mars

KW - Venus

KW - planetary plasma

KW - small satellite series

KW - spectroscope

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An EUV spectrometer on earth-orbiting satellite for planetary science

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