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(168) D 10 kg 6xs8" >cd 6ῑ2 l ῒ"}~8" 7pp* ;0 X H CCD ¡ 1 ¢£l ¤¥¦J§¨ῐ X H©ª«¬«~® )8" k +=8" ῒ" X HXY¯°±. ῎῍῏ῌ 1) 2) 3) 4) 5) 6) 7) 8) 9). 624. Metzger A. E., et al., 1983, J. Geophys. Res. 88, 7731 Snowden S. L., et al., 1994, ApJ 424, 714 Gladstone G. R., et al., 2002, Nature 415, 1000 Wargelin B. J., et al., 2004, ApJ 607, 596 Dennerl K., et al., 2002, A&A 386, 319 Dennerl K., 2002, A&A 394, 1119 Ness J.-U., et al., 2004, A&A 418, 337 Branduardi-Raymont G., et al., 2004, A&A 424, 331 Snowden S. L., et al., 2004, ApJ 610, 1182. Planets Observed with the X-Ray Observatory Suzaku Yuichiro EZOE Department of Physics Tokyo Metropolitan University, 1ῌ1 Minami-Osawa, Hachioji, Tokyo 192ῌ0397, Japan Abstract : In spite of their proximity, there remain many puzzles on atmospheric and magnetospheric environments of planets in the solar system. Thanks to advances in space X-ray observations, X-ray emission from planets is now becoming a new scientific field. These remote X-ray observations can be complementary to in situ exploration missions, in order to investigate the planetary environments. We have been studying Jovian magnetosphere, and Earth’s and Martian exospheres, using the Suzaku satellite which is best to study di#use X-ray emission.. ¶·¸U. 2010 5 10 ¸.
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