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(154) %9%%:;1<=>?@A BA9CDEF GH I 7 %-) *+JKBG45-6 3 LM*+123. 15) 16) 17) 18) 19) 20) 21) 22) 23). Miyagoshi T., Yokoyama T., 2004, ApJ 614, 1042 Kosugi T., et al., 2007, Sol. Phys. 243, 3 Golub L., et al., 2007, Sol. Phys. 243, 63 Kano R., et al., 2007, Sol. Phys. in press Cirtain J., et al., 2007, Science 318, 1519 Savcheva A., et al., 2007, PASJ 59. S771 Shimojo M., et al., 2007, PASJ 59, S745 Kamio, S., et al., 2007, PASJ 59, S757 Culhane L., et al., 2007, PASJ 59, S751. 4 5 N O P Q R 6 D G S T 9 MHD UV WXYZ

(155) -7[% 3 LM *+%\]^_5 à%b cd%-Refg h<=1ijE45 k@PQR$ l5mjCD ST9 à%b cd%no pqrlHk. ῎῍῏ῌ 1) 2) 3) 4) 5) 6) 7) 8) 9) 10) 11) 12) 13) 14). Ogawara Y., et al., 1991, Sol. Phys. 136, 1 Tsuneta S., et al., 1992, Sol. Phys. 136, 37 Shibata K., et al., 1992, PASJ 44, L173 Strong K. T., et al., 1992, PASJ 44, L161 Shimojo M., et al., 1996, PASJ 48, 123 Shibata K., et al., 1994, ApJ 431, L51 Canfield R., et al., 1996, ApJ 464, 1016 Kundu M. R., et al., 1998, Sol. Phys. 178, 173 Shimojo M., Shibata K., Harvey K. L., 1998, Sol. Phys. 178, 379 Yokoyama T., Shibata K., 1995, Nature 375, 6526, 42 Yokoyama T., Shibata K., 1996, PASJ 48, 353 Shimojo M., Shibata K., 2000, ApJ 542, 1100 Shimojo M., et al., 2001, ApJ 550, 1051 Miyagoshi T., Yokoyama T., 2003, ApJ 593, L133. s 101 t. s6u. Solar X-ray Jets Observed with the X-ray Telescope aboard Hinode Masumi SHIMOJO Nobeyama Solar Radio Observatory, National Astronomical Observatory of Japan, Nobeyama, Minamimaki, Minamisaku, Nagano 384ῌ1305, Japan Abstract : A solar X-ray jet is the jet phenomenon of coronal plasma and it was discovered by the Soft X-ray Telescope aboard Yohkoh. Since the X-ray telescope (XRT) aboard Hinode has the high-resolution and the wider temperature response, we found that the X-ray jets frequently occur even in the polar coronal hole. And, XRT also revealed that the jets generate MHD wave. Based on the XRT results, we suggest that the X-ray jets in coronal hole provide the energy for the acceleration of fast solar wind.. 317.

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