TRANSACTIONS OF THE JAPAN SOCIETY FOR AERONAUTICAL AND SPACE SCIENCES, SPACE TECHNOLOGY JAPAN
Online ISSN : 1347-3840
ISSN-L : 1347-3840
k) Solar System Exploration and Scientific Research
Observation of the Near-Earth Plasmas by Telescope of Extreme Ultraviolet (TEX) Onboard SELENE: Science from the Moon
Ichiro YOSHIKAWAAtsushi YAMAZAKIGo MURAKAMIFukuhiro EZAWAKazuo YOSHIOKAShingo KAMEDAWataru MIYAKEMakoto TAGUCHIMasayuki KIKUCHIMasato NAKAMURATakeshi SAKANOIShoichi OKANO
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2009 Volume 7 Issue ists26 Pages Tk_27-Tk_32

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Abstract

The Upper Atmosphere and Plasma Imager (UPI) was launched in 2007, and went to the moon. From the lunar orbit, two telescopes direct toward the Earth. The moon has no atmosphere, which leads no active emission near the spacecraft, thus we have a high quality image of the near-Earth environment. Moreover the moon orbits the Earth once a month and the Earth is observed from many different directions. This is called a "science from the Moon". The two telescopes are mounted on 2-axis gimbal system, Telescope of Extreme ultraviolet (TEX) and Telescope of Visible light (TVIS). TEX detects the O II (83.4nm) and He II (30.4nm) emissions scattered by ionized oxygen and helium, respectively. The targets of EUV imaging are the polar ionosphere, the polar wind, and the plasmasphere and the inner magnetosphere. The maximum spatial and time resolutions are 0.09 Re and 1 minute, respectively.

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© 2009 The Japan Society for Aeronautical and Space Sciences
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