Planetary extreme ultraviolet spectrometer boarded on Japan's small satellite

Kazuo Yoshioka; Go Murakami; Gentaro Ogawa; Ichiro Yoshikawa; Munetaka Ueno; Atsushi Yamazaki; Kazunori Uemizu; Masato Kagitani; Fuminori Tsuchiya

doi:10.1117/12.825038

Planetary extreme ultraviolet spectrometer boarded on Japan's small satellite

Kazuo Yoshioka, Go Murakami, Gentaro Ogawa, Ichiro Yoshikawa, Munetaka Ueno, Atsushi Yamazaki, Kazunori Uemizu, Masato Kagitani, Fuminori Tsuchiya

SCI - Planetary Plasma and Atmospheric Research Center (PPARC)

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

Abstract

EXtreme ultraviolet spectrosCope for ExosphEric Dynamics (EXCEED) is an earth-orbiting space Extreme Ultraviolet (EUV) telescope mission. The satellite will be launched in 2012 by a Japanese new solid propulsion rocket and injected into the elliptic orbit around the earth. The orbital altitude is 900 to 1200 km for perigee and apogee respectively. EXCEED will make EUV spectroscopic and imaging observations of plasma space around various planets in our solar system. The wavelength range is from 60 to 145 nm and the resolution is 0.2 to 0.5 nm FWHM. It enables us to study Io plasma torus of Jupiter, and interaction of the solar wind with the upper atmosphere of the terrestrial planets and their escape. In this paper, we will introduce the mission overview and its instrument especially for holographic grating which is coated by Chemical vapor deposited silicon carbide.

Original language	English
Title of host publication	UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVI
Volume	7435
DOIs	https://doi.org/10.1117/12.825038
Publication status	Published - 2009 Dec 1
Event	UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVI - San Diego, CA, United States Duration: 2009 Aug 3 → 2009 Aug 3

Other

Other	UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVI
Country/Territory	United States
City	San Diego, CA
Period	09/8/3 → 09/8/3

Keywords

CVD-SiC
EUV
planetary atmosphere
spectrometer

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

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10.1117/12.825038

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Planetary extreme ultraviolet spectrometer boarded on Japan's small satellite. / Yoshioka, Kazuo; Murakami, Go; Ogawa, Gentaro; Yoshikawa, Ichiro; Ueno, Munetaka; Yamazaki, Atsushi; Uemizu, Kazunori; Kagitani, Masato ; Tsuchiya, Fuminori.

UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVI. Vol. 7435 2009. 74350X.

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

Yoshioka, K, Murakami, G, Ogawa, G, Yoshikawa, I, Ueno, M, Yamazaki, A, Uemizu, K, Kagitani, M & Tsuchiya, F 2009, Planetary extreme ultraviolet spectrometer boarded on Japan's small satellite. in UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVI. vol. 7435, 74350X, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVI, San Diego, CA, United States, 09/8/3. https://doi.org/10.1117/12.825038

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abstract = "EXtreme ultraviolet spectrosCope for ExosphEric Dynamics (EXCEED) is an earth-orbiting space Extreme Ultraviolet (EUV) telescope mission. The satellite will be launched in 2012 by a Japanese new solid propulsion rocket and injected into the elliptic orbit around the earth. The orbital altitude is 900 to 1200 km for perigee and apogee respectively. EXCEED will make EUV spectroscopic and imaging observations of plasma space around various planets in our solar system. The wavelength range is from 60 to 145 nm and the resolution is 0.2 to 0.5 nm FWHM. It enables us to study Io plasma torus of Jupiter, and interaction of the solar wind with the upper atmosphere of the terrestrial planets and their escape. In this paper, we will introduce the mission overview and its instrument especially for holographic grating which is coated by Chemical vapor deposited silicon carbide.",

keywords = "CVD-SiC, EUV, planetary atmosphere, spectrometer",

author = "Kazuo Yoshioka and Go Murakami and Gentaro Ogawa and Ichiro Yoshikawa and Munetaka Ueno and Atsushi Yamazaki and Kazunori Uemizu and Masato Kagitani and Fuminori Tsuchiya",

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doi = "10.1117/12.825038",

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AU - Yoshioka, Kazuo

AU - Murakami, Go

AU - Ogawa, Gentaro

AU - Yoshikawa, Ichiro

AU - Ueno, Munetaka

AU - Yamazaki, Atsushi

AU - Uemizu, Kazunori

AU - Kagitani, Masato

AU - Tsuchiya, Fuminori

PY - 2009/12/1

Y1 - 2009/12/1

N2 - EXtreme ultraviolet spectrosCope for ExosphEric Dynamics (EXCEED) is an earth-orbiting space Extreme Ultraviolet (EUV) telescope mission. The satellite will be launched in 2012 by a Japanese new solid propulsion rocket and injected into the elliptic orbit around the earth. The orbital altitude is 900 to 1200 km for perigee and apogee respectively. EXCEED will make EUV spectroscopic and imaging observations of plasma space around various planets in our solar system. The wavelength range is from 60 to 145 nm and the resolution is 0.2 to 0.5 nm FWHM. It enables us to study Io plasma torus of Jupiter, and interaction of the solar wind with the upper atmosphere of the terrestrial planets and their escape. In this paper, we will introduce the mission overview and its instrument especially for holographic grating which is coated by Chemical vapor deposited silicon carbide.

AB - EXtreme ultraviolet spectrosCope for ExosphEric Dynamics (EXCEED) is an earth-orbiting space Extreme Ultraviolet (EUV) telescope mission. The satellite will be launched in 2012 by a Japanese new solid propulsion rocket and injected into the elliptic orbit around the earth. The orbital altitude is 900 to 1200 km for perigee and apogee respectively. EXCEED will make EUV spectroscopic and imaging observations of plasma space around various planets in our solar system. The wavelength range is from 60 to 145 nm and the resolution is 0.2 to 0.5 nm FWHM. It enables us to study Io plasma torus of Jupiter, and interaction of the solar wind with the upper atmosphere of the terrestrial planets and their escape. In this paper, we will introduce the mission overview and its instrument especially for holographic grating which is coated by Chemical vapor deposited silicon carbide.

KW - CVD-SiC

KW - EUV

KW - planetary atmosphere

KW - spectrometer

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BT - UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVI

T2 - UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XVI

Y2 - 3 August 2009 through 3 August 2009

ER -

Planetary extreme ultraviolet spectrometer boarded on Japan's small satellite

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