‚VD‚QD@’´‚‘¬Õ“ËŽÀŒ±‚̐¬‰ÊƒŠƒXƒg

‚VD‚QD‚PD@¸“ǘ_•¶

[1995”N]

Katayama, M., Kibe, S., and Toda, S. 1995. A numerical simulation method and its validation for debris impact against the whipple bumper shield, Inter. J. Impact Eng. 17, 465-476.

Yamanaka, C., Hosokawa, K., Ikeya, M., Nishijima, S., and Okada, T. 1995. Scanning positron-annihilation microscope, Jpn. J. Appl. Phys. 34, 6528-6529.

 

[1996”N]

Yanagisawa, M., Hasegawa. S., and Shirogane, N. 1996. Momentum and angular momentum transfer in oblique impact: Implications for asteroid rotations. Icarus 123, 192-206.

 

[1997”N]

Murae, T. 1997. Structure of high-molecular carbonaceous compound in carbonaceous chondrites and formation of IR-spectroscopically similar compounds in the laboratory, Adv. Space Res. 19, 1053-1057.

Yamori, A., Kawashima, N. Kohno, M., Minami, S., and Teii, S. 1997. High quality railgun HYPAC for hypervelocity impact experiments, Inter. J. Impact Eng. 20, 829-838.

 

[2000”N]

Miura Y., Fukuyama, S., Kedves, M., Yamori, A., and Okamoto, M. 2000. Chemical separation of Fe-Ni particles after impact. Adv. Space Res. 25, 285-288.

 

[2001”N]

Tanaka, M.,@ Moritaka, Y., Akahoshi, Y.,@ Nakamura, R., Yamori, A., and Sasaki, S. 2001. Development of a Lightweight Space Debris Shield Using High Strength Fibers, Inter. J. Impact Eng. 26, 761-772.

 

[2002”N]

Takano, T., Murotani, Y., Maki, K., Tota, T., Fujiwara, A., Hasegawa, S., Yamori, A. and Yano, H. 2002. Microwave emission due to hypervelocity impacts and its correlation with mechanical destruction, J. Applied Phys. 92, 5550-5554.

 

[2004”N]

Tanaka, M. and Moritaka, Y. 2004. Single bumper shields based on Vectran fibers, Adv. Space Res. 34, 1076-1079.

Maki, K., Takano, T., Fujiwara, A., and Yamori, A. 2004. Radio-wave emission due to hypervelocity impacts in relation to optical observation and projectile speed, Adv. Space Res. 34, 1085-1089.

 

[2005”N]

Maki, K., Soma, E., Takano, T., Fujiwara, A., and Yamori, A. 2005. Dependence of microwave emissions from hypervelocity impacts on the target material, Journal of Applied Physics, 97 104911-104911-6.

 

[2006”N]

Kadono, T., Kameda, J., Saruwatari, K., Tanaka, H., Yamamoto, S., and Fujiwara A. 2006. Surface roughness of alumina fragments caused by hypervelocity impact, Planet.Space Sci. 54, 212-215.

Mieno T. and Yamori A. 2006. Explosion production of fullerenes from carbonaceous bullet in vacuum using rail gun, Jpn. J. Appl. Phys. 45, 1-3.

 

 

Minami, S., Takechi, S., Onishi, T., Kitajima, M., Takahasi, M., Rana. R., and Hasegawa, S. 2006. Detection of Electromagnetic Waves from the Hyper-Velocity Impact of Dust into Piezo Elements, ITE Letters on Battteriies New Tecchnologys and Medicine 7 (5), 434-438.

Yano, H., Kubota, T., Miyamoto, H., Okada, T., Scheeres, D., Takagi, Y., Yoshida, K.,@ Abe, M., Abe, S., Barnouin-Jha, O., Fujiwara, A., Hasegawa, S., Hashimoto, T., Ishiguro, M., Kato, M. ,Kawaguchi, J., Mukai, T., Saito, J., Sasaki, S., and Yoshikawa, M. 2006. Touchdown of the Hayabusa Spacecraft at the Muses Sea on Itokawa, Science 312, 1350-1353.

 

[2007”N]

‰œ•½‹±ŽqA–ìŒû‚–¾A–î–ì‘nA2007DƒGƒAƒƒWƒFƒ‹•ßŠlŽŽ—¿‚ð•]‰¿‚·‚邽‚ß‚Ì’´‚‘¬“xÕ“ËŽÀŒ±A—V¯l 16, 316-321.

’†‘ººŽqAˆ¢•”V•A•½“c¬A2007DƒCƒgƒJƒ-’T¸‹@‚Å‚Ý‚½Õ“ˍďWÏ“V‘̂Ə¬“V‘̂̏ՓˉߒöA—V¯l 16, 216-225.

ŽRŠÝ–¾•FA–î–ì‘nA‰œ•½‹±ŽqA¬—ÑŒ›³A‰¡–xLˆêA“c’[½A‰Í‡GKA‚Q‚O‚O‚VDTANPOPOF—L‹@•¨‚Æ”÷¶•¨‚̉F’ˆ‹óŠÔ”˜˜I‚Æ”÷覐΋y‚Ñ”÷¶•¨‚̕ߏWŽÀŒ±ABiological Sciences in Space 16, 67-75.

Chiba, S., Soma, E., and Takano, T. 2007. Waveform analysis of microwave pulse emitted in association with hyper velocity impacts, IECE Trans. Commun. 55, 2382-2386.

Michikami, T., Moriguchi, K., Hasegawa, S., and Fujiwara, A. 2007. Ejecta velocity distribution for impact cratering experiments on porous and low strength targets, Planet.Space Sci, 55 70-88.

Noguchi, T., Nakamura, T., Okudaira, K., Yano, H., Sugita, S., and Burchell, M. J. 2007. Thermal alternation of hydrated minerals during hypervelocity capture to silica aerogel at the flyby speed of Stardust, Meteorit. Planet. Sci., 42, 357-372.

Ohnishi, H., Chiba, S., Soma, E., Ishii, K., Maki, K., Takano, T., and Hasegawa, S. 2007. Study on microwave emission mechanisms on the basis of hypervelocity impact experiments on various target plates, J. Applied Phys. 101, 124901, 1-8.

 

[2008”N]

‘Š”n‰›—ߎqA–qŒªˆê˜YC‚–ì’‰A²–ì‰ë•qA‚Q‚O‚O‚WDƒ}ƒCƒNƒ”g‚É‚æ‚éƒfƒuƒŠÕ“ËŒŸoŒn‚ÌŒŸ“¢A“ú–{q‹ó‰F’ˆŠw‰ï˜_•¶W Vol.56CNo.650Cpp.105-109.

ŽRŠÝ–¾•FA–î–ì‘nA¬—ÑŒ›³A‰¡–xLˆêA‹´–{”Ž•¶AŽR‰º‰ë“¹A“c’[½A‰Í‡GKA‚Q‚O‚O‚WD‚½‚ñ‚ۂہF‰F’ˆƒXƒe[ƒVƒ‡ƒ“‚Å‚Ì”÷¶•¨—L‹@•¨•ßŠlC”˜˜IŽÀŒ±AViva Origo 16, 72-76.

Hasegawa, S., Mueller, T. G., Kawakami, K., Kasuga, T., Wada, T., Ita, Y., Takato, N., Terada, H., Fujiyoshi, T., and Abe, M. 2008. Albedo, size, and surface characteristics of Hayabusa-2 sample-return target 162173 1999 JU3 from AKARI and Subaru observations, Pub. Astron. Soc. Japan 60, S399-S405.

Mieno, T. and Hasegawa, S. 2008. Production of carbon clusters by collisional explosion using gas gun in experiment modeling asteroid collision, Applied Physics Express, 1, 067006, 1-3.

Motoyashiki, Y., Hasegawa, S., Okudaira, K., and Sato, E. 2008. Micrometeoroid impact on ceramic thin components for interplanetary probe, Inter. J. Impact Eng. 35, 1666-1671.

Nakamura, A. M., Michikami, T., Hirata, N., Fujiwara, A., Nakamura, R., Ishiguro, M., Miyamoto, H., Demura, H., Hiraoka, K., Honda, T., Honda, C., Saito, J., Hashimoto, T., Kubota, T. 2008. Impact process of boulders on the surface of asteroid 25143 Itokawa -Fragments from collisional disruption, Nakamura, Earth Planet. Space 60, 7-12.

 

[2009”N]

Jutzi, M., Michel, P., Hiraoka, K., Nakamura, A, M., and Benmz, W. 2009. Numerical simulations of impacts involving porous bodies. II. Comparison with laboratory experiments, Icarus 201, 802-813.

Kawakita, S., Segami, G., Nitta, K., Kusawake, H., Takahashi, M., Matsumoto, H., and Hasegawa, S. 2009. Discharge of spacecraft solar panels by hypervelocity impact, Trans. JSASS Space Tech. Japan 7, Tr_2_53-Tr_2_56.

Motoyashiki, Y, Shindo, D., K. Okudaira, K. Hasegawa, S., and@ Sato, E. 2009. Micrometeoroid Impact Damage on Thin Ceramic Component for Interplanetary Probe, Trans. JSASS Space Tech. Japan 7, Pc_25-Pc_30.

Nagaoka, Y., Tanaka, K., and Sasaki, S. 2009. Hypervelocity impact experiment on thin film structure, Trans. JSASS Space Tech. Japan 7, Pr_2_31-Pr_2_34.

Ohtsuka, K., Nakamura, T., Nakato, A., Kinoshita, D., Ito, T., Yoshokawa, M., and Hasegawa, S. 2009. Solar Radiation Heating Effects on 3200 Phaethon, Pub. Astron. Soc. Japan 61, 1375-1387.

Shirahata, M., Matsuura, S., Hasegawa, S., Ootsubo, T., Makiuti, S., Yamamura, I., Nakagawa, N., Kawada, M., Kaneda, H., Shibai, H., Doi, Y., Suzuki, T., Mueller, T. G., and Cohen, M. 2009. Calibration and performance of the AKARI far-infrared surveyer (FIS)- Slow scan observation mode for point sources, Pub. Astron. Soc. Japan 61, 737-750.

Tamura, M., Takami, M., Enya, K., Ootsubo, T., Fukagawa, M., Honda, M., Okamoto, Y. K., Sako, K., Yamashita, T., Hasegawa, S., Kataza, H., Doi, Y., Matsuhara, H., and Nakagawa, T. 2009. SPICA Coronagraph Instrument (SCI) for the Direct Imaging and Spectroscopy of Exo-Planets, in SPICA joint European/Japanese Workshop (eds. A. M. Heras, B. M. Swinyard, K. G. Isaak, and J. R. Goicoechea), 02001.

 

[2010”N]

Nogami, K., Fujii, M., Ohashi, H., Miyachi, T., Sasaki, S., Hasegawa, S., Yano, H., Shibata, H., Iwai, T., Minami, S., Takechi, S., Gruen, E., and Srama, R. 2010. Development of the Mercury dust monitor (MDM) onboard the BepiColombo mission, Planet. Space Sci. 58, 108-115.

Setoh, M., Nakamura, A, M., Michel, P., Hiraoka, K., Yamashita, Y., Hasegawa, S., Onose, N., and Okudaira, K. 2010. High and low-velocity impact experiments on porous sintered glass bead targets of different compressive strengths: outcome sensitivity and scaling, Icarus, 205, 702-711.

Katayama, M., Takeba, A., Nitta, K., Kawakita, S., Matsumoto, H., and Kitazawa, Y. 2010. Integrity assessment of the spacecraft subjected to the hypervelocity impact by ceramic and metal projectiles simulating space debris and micrometeoroids, Materials Science and Engineering B, in-press.

 

 

 

‚VD‚QD‚QD@‘ÛŠw‰ïEƒvƒƒV[ƒfƒBƒ“ƒOƒX

[1995”N]

Kawashima, N., Yamori, A., Minami, S., and Rahman, H. 1995. Improvement of Railgun Projectile Using Higher Specific Materials. IEEE Trans. on Magnetics, Vol. 31, p. 189.

Miura Y. 1995. New shock calcite and Fe grains from Noerdlingen Rie imapct crater, Meteoritics 30, 550

Miura Y. 1995. New shock metamorphosed materials - shock calcite, Proc. 28th ISAS Lunar Planet. Symp., 53-56.

Yamori, A., Kawashima, N., and Kohno, M. 1995. Characteristics of high efficinecy 300 kJ railgun, IEEE Trans. on Magnetics, Vol. 31, p. 377.

 

[1996”N]

Miura, Y. and Okamoto, M. 1996. Shocked metamorphosed material from limestone by impacts, Proc. 29th ISAS Lunar Planet. Symp., 293-296.

Murae, T. 1996. Comparison of UV-VIS spectra of shock-metamorphosed carbonaceous matter and carbonaceous chondrites, Proc. 29th ISAS Lunar Planet. Symp., 181-184.

Murae, T. 1996. Structure of high-molevular carbonaceous compound in carbonaceous chondrites, and formation of IR-spectroscopically simillar compound in laboratory,@ 31th Scientific Assembly of COSPAR

 

[1997”N]

Fukuyama, S., Kogayashi, H., and Miura, Y. 1997. Impact metamorphosed compositions of Fe-Si-Ni-S system, Antarctic Meteorites XXII, 41-42.

Minami, S., Yamori, A., and Kawashima, N. 1997. On the railgaun-produced multi-craters for possible new chronological cratering investigation, Proc. 30th ISAS Lunar Planet. Symp., 63-66.

 

[1998”N]

Miura, Y., Fukuyama, S., and Gucsik, A. 1998. Melt or vapor compositions from iron-nickel metals after impact., Antarctic Meteorites XXIII, 86-88.

 

[1999”N]

Miura, Y. and Kedves, M.. 1999. Characteristics of spereules fromes by impact reaction: FE-Ni-Si grains, Proc. 32th ISAS Lunar Planet. Symp., 97-100.

Miura, Y., Fukuyama, S., and Kedves, M.. 1999. Grains formed by impact reaction found at spherules of various impact crater, Meteorite shower and geological boundaries, Lunar Planet Sci. Conf. XXX, #1533.

Miura, Y., Fukuyama, S., Kedves, M., Yamori, A., and Okamoto, M. 1999.@ Chemical separation of Fe-Ni particles after impact. the 32nd COSPAR Scientific Assembly, Nagoya

Murae, T., Mori, Y., and Yamori, A. 1999. The effect of the mixed state of the sample for impact metamorphism of carbonaceous materia1, Intemational Symposium on Planetary Impact Event and their Consequences of Earth, Japan

Yamori, A., Kohno, M., and Kawashima, N. 1999. Preliminary experimental results of A novel induction type railgun, IEEE Trans. on Magnetics, Vol. 35, p. 447

Yamori, A., Kohno, M., and Kawashima, N. 1999. Secondary arc dynamics in a railgun bore, IEEE Trans. on Magnetics, Vol. 35, p. 452.

 

[2000”N]

Miura, Y., Uedo, Y., Kedves, M., and Rampino, R. 2000. Formation of Fe-Ni-Si particles by impact process, Proc. 33th ISAS Lunar Planet. Symp., 193-196.

Takano, T., Murotani, Y., Maki, K., Tota, T., Fujiwara, A., Hasegawa, S., Yamori, A. and Yano, H. 2000. Microwave generation due to hypervelocity impact", 51th IAF Congress, IAA-00-IAA.6.5.07

Tanaka, M., Moritaka, Y., Akahoshi, Y., Nakamura, R., Yamori, A., and Sasaki, S. 2000. Development of a lightweight space debris shield using high dtrength fibers, Hypervelocity Impact Symposium 2000, Galveston, USA

 

[2001”N]

Moritaka, Y., Ogawa, Y., Tanaka, M., Akahoshi, Y., Nakamura, R., Watanabe, D., Yamori, A., and Sasaki, S. 2001. A lightweight debris shield using high strength fibers, Proceedings of the Third European Conference on Space Debris, 687 - 690, ESA SP-473.

Murae, T., Ikeda, E., and Yamori, A. 2001. Effect of shock wave on glysine and a mixture of glysine and alanine, Proc. 34th ISAS Lunar Planet. Symp., 1, 41-44.

Takano, T., Murotani, Y., Tota, T., Fujiwara, A., Hasegawa, S., and Yamori, A. 2001. Microwave emission experiment with hypervelocity impacts and applications of its results, Proceedings of the Meteoroids 2001 Conference, 569-575, ESA SP-495.

Yamori, A., Ono, Y., Kubo, H., Kohno, M.@ and Kawashima, K. 2001. Development of an induction type railgun, IEEE Trans. on Magentics, Vol. 37, p. 470.

 

[2002”N]

Maki, K., Takano, T., Yamori, A. and Kawashima, N. 2002. Detection of microwave emission in hypervelocity impact on aluminum, 2002 Asia-Pacific Microwave Conference, Kyoto.

Maki, K., Takano, T., Fujiwara, A., and Yamori, A. 2002. Radio-wave emission due to hypervelocity impacts in relation to optical observation and projectile Speed, 34 th COSPAR-2nd World Space Congress.

Mieno, T. and Yamori, A. 2002. Fullerene Production in Vacuum by Use of the Carbon-Pellet Injection of the Rail-Gun, Proc. 22nd Fullerene General Sympo

Tanaka, M. and Moritaka, Y. 2002. Debris Mitigation Using Two Hemispheric Deployable Space Structures, The World Space Congress, Houston, USA.

 

[2003”N]

Miura Y., Nakamura A. and Yamori A. 2003. Chemical evolution of active organic compounds by railgun experiments, International Symposium on Impact Events in Japan, Southeast Asia and @Pacific Rim (IEJSAP'03), 64-65.

Yamanaka, C., Hisatomi O., and Yomori, A. 2003 Shock effects on frozen DNA samples. Geochim. Cosmochim. Acta, 67 A554.

Yamori, A., Kohno, M., and Kawashima, N. 2003. Experimental results of a two-stage plasma armature railgun, IEEE Trans. on Magnetics, Vol. 39, p. 476

 

[2004”N]

Kaneko, T., Kobayashi, K., and Yamori, A. 2004. Formation and transformation of amino acids and amino acid precursors by high-velocity impacts, 35th COSPAR Scientific Assembly., p.4162

Miura Y., Nakamura A., and Yamori A. 2004. Water role for active organic and inorganic compounds as life precursor materials and circular system on the solar system. Proc. Inter. Workshop on Water Dynamics, Tohoku University COE, 123-124.

Soma, E., Ishii, K., Maki, K., Takano, T., and Yamori, A. 2004. Proposal of an impact detector of apace debris via maicrowave, Intertaional Symposium on Space Technology and Science, 2004-r-09, Japan

 

[2005”N]

Ishida, Y., Ninagawa, K., Sakamoto, K., Toyoda, S., Nishido, H., and Gucsik, A. 2005. Thermoluminescene study of shocked Standstone, Meteoritics & Planetary Science, Vol. 40, Supplement, A74.

Ishida, Y., Ninagawa, K., Sakamoto, K., Toyoda, S., Nishido, H., and Gucsik, A. 2005. Thermoluminescene studies of shocked minerals and rocks. 29th symposium on Antarctic Meteorites, pp. 25-26

Michikami, T., Moriguchi, K., and Nakamura, R. 2005. Application to large blocks on asteroid 25143 Itokawa: Ejecta mass distribution with low velocity for impact cratering experiment on porous target, Lunar and Planetary Science Conference XXXV, #1729.

Ohnishi, H., Maki, K., Soma, E., Ishii, K., Chiba, S., Takano, T., and Yamori, A. 2005. Study on microwave emission due to hypervelocity impact destruction, Union Radio-Scientfique intrtnational, A01

Takagi, Y., Hasegawa, S., Teramoto, K., Yano, H., Yamamoto, S., Sugita, S., and Abe, M. 2005. Impact cratering experiments in microgravity enviroment, Lunar and Planetary Science Conference XXXV, #1627.

 

 

Takano, T., Maki, K., Soma, E., Ohnishi, H., Ishii, K., Chiba, S., Fujiwara, A., and Yamori, A. 2005. Material dependence of microwave emission due to a hypervelocity impact, Proceedings of the 4th European Conference on Space Debris, 501.

 

[2006”N]

Chiba, S., Soma, E., and Takano, T. 2006. Waveform analysis of microwave pulse emitted in association with hyper velocity impacts, Intertaional Symposium on Antennas and Propagation, Shingapore

Kobayashi, Taniuchi, Y., Kaneko, T., Al-hanbki, H., Yamori, A., Miyakawa, S., and Takano, Y. 2006. Possible formation of amino acid precursors in the lower atmosphere of Titan, 36th COSPAR Scientific Assembly, #2927.

Mieno T., Hasegawa S., and Yamori A. 2006. Synthesis of fullerenes by shooting and explosion of a carbonic bullet by using a rail-gun, Proc. 6th Int. Conf. Reactive Plasmas,791-792.

Okudaira, K., Yano, H., Noguchi, T., Burchell, M. J., Hasegawa, S., Onose, N., Nakamura, T., and Cole, M. J. 2006. Assessment of micrometeoroid analog particlesÕ survivability captured in the laboratory by silica aerogel, International Symposium on Sample Returns from Solar System Minor Bodies-The Second HAYABUSA Symposium, Tokyo,

Onose, N. and Fujiwara, A. 2006. Mass - cumulative number distributions of fragments produced in impact craterings on gypsum targets, Impact craters as indicators for planetary environmental evolution and astrobiology, Ostersund, Sweden

Onose, N. and Fujiwara, A. 2006. Elastic ejection of late fragments produced in impact craterings on gypsum targets, Impact craters as indicators for planetary environmental evolution and astrobiology, Ostersund, Sweden

Onose, N., Hasegawa, S., and Fujiwara, A. 2006. Shapes and dimensions of craters produced by impact cratering on gypsum, International Symposium on Sample Returns from Solar System Minor Bodies-The Second HAYABUSA Symposium, Tokyo, Japan

Soma, E., Ishii, K., Ohnishi, Chiba, S., Takano, T., and Hasegawa, S. 2006. Destruction and microwave emission due to hypervelocity impacts onto external wall of spececraft, Intertaional Symposium on Space Technology and Science, 2006-r-2-09, Japan

Soma, E., Ishii, K., Chiba, S., Hasegawa, S.,Takano, T., and Sano, M. 2006. Study on pistion determination of space debris impact via micrawave, Intertaional Symposium on Antennas and Propagation, Shingapore

Takagi, Y., Hasegawa, S., Yano, H., Yamamoto, S., Sugita, S., Teramoto, K., Honda, C., Kurosawa, K., Nakada, T., and Abe, M.@ 2006. Impact cratering experiments in microgravity environment, International Symposium on Sample Returns from Solar System Minor Bodies-The Second HAYABUSA Symposium, Tokyo, Japan

Tanaka, K., Saitoh, Y., Kosyo, S., and Sasaki, S. 2006. Measurement of the ejector generated by the hypervelocity impact experiment on the thin film materials, 24th Int. Symp. Space Tech. Sci., 2006-r-2-02g

Yano, H., Kubota, T.,@ Miyamoto, H., Okada, T., Scheeres, D., Takagi, Y., Yoshida, K.,@ Abe, M., Abe, S., Barnouin-Jha, O., Fujiwara, A., Hasegawa, S., Hashimoto, T., Ishiguro, M., Kato, M. ,Kawaguchi, J., Mukai, T., Saito, J., Sasaki, S., and Yoshikawa, M. 2006. Hayabusa touch down sites at the smooth terrain on asteroid 25143 Itokawa: Initial investigation, Lunar and Planetary Science Conference XXXVII, #2463.

Yano, H., Noguchi, T., Matsunaga, S., Mori, O., Habu, H., Hasegawa, S., Kato, K., Kunota, S., Miura, Y., Nakaya, K., Nozoe, K., Ogata, Y., Tsuchiyama, A., Wada, Y., and the Minor Body Exploration Working Group Sampling Sub-Group. 2006 Development of the sampling device for undifferentiated asteroid surface and sub-surface materials, Intertaional Symposium on Space Technology and Science, 2006-K-28, Japan

 

[2007”N]

Mieno T. and Yamori A. 2007. Production of carbon clusters by colllisonal bullet-target explosion using a rail-gun, 8th Asia-Pacific Conf. Plasma Sci. & Technol., Cairns.

Setoh, M., Nakamura, A. M., Hiraoka, K., Hasegawa, S., Onose, N., Okudaira, K., Yamashita, Y., and Michel, P., 2007. Experimental Study of Stress Wave Attenuation in Porous Small Bodies, Proc. 40th ISAS Lunar and Planet. Symp., 112-117.

Setoh, M., Nakamura, A. M., Hiraoka, K., Onose, N., and Hasegawa, S. and Michel, P. 2007. Impact Experiments of sintered glass beads targets at low and high velocities, Lunar Planet Sci. Conf. XXXVIII, #1263.

Takagi, Y., Hasegawa, S., Yano, H., Yamamoto, S., Sugita, S., Teramoto, K., Honda, C., Kurosawa, K., Abe, M., and Fujiwara, A. 2007. Impact cratering experiments in microgravity enviroment, Lunar Planet Sci. Conf. XXXVIII, #1634.

 

[2008”N]

Gavin, P., Chevrier, V., and Ninagawa. K. 2008. Effects of impact and heating on the spectral properties of clays on Mars, Lunar Planet Sci. Conf. XXXIX, #7012.

Gavin, P., Chevrier, V., and Ninagawa. K., Hasegawa, S., and Gucsik, A. 2008.@ Effects of impact and heating on the properties of clays on Mars. Workshop on Martian Phyllosilicates: Recorders of Aqueous Processes?, CNES Paris, France

Kawakita, S., Segami, G., Nitta, K., Kusawake, H., Takahashi, M., Matsumoto, H., and Hasegawa, S. 2008. Discharge of spacecraft solar panels by hypervelocity impact, 26th Int. Symp. Space Tech. Sci., 2008-r-2-41p, Hamamatsu, Japan

Makabe, T. amd Yano, H. 2008. The effective projectile shape for asteroid impact sampling, 26th Int. Symp. Space Tech. Sci., 2008-k-08, Hamamatsu, Japan

Mieno, T., and Hasegawa, S.@ 2008. Taitan satellite would be a carbon cluster factory from light gas gun experiment, 26th Int. Symp. Space Tech. Sci., 2008-r-2-27, Hamamatsu, Japan

Miura, Y.,@ Takatori, Y. ,Sueyoshi, Y.,@ Sasaki, S., and Hasegawa, S. 2008. Formation of micro-textures with carbon and chlorine on the Moon asteroids and Mars, Proc. 41th ISAS Lunar and Planet. Symp., 169-172.

Michikami, T., Miura, S., Haruyama, J., and Lykawka, P. S. 2008. Impact cratering experiments to targets with cavity: Application to cave skylight on Mars, Lunar Planet Sci. Conf. XXXIX, #1391.

Motoyashiki, Y, Shindo, D., K. Okudaira, K. Hasegawa, S., and@ Sato, E. 2008. Micrometeoroid Impact Damage on Thin Ceramic Component for Interplanetary Probe, 26th Int. Symp. Space Tech. Sci., 2008-c-27, Hamamatsu, Japan

Nagaoka, Y., Tanaka, K., and Sasaki, S. 2008. Hypervelocity impact experiment on thin film structure, 26th Int. Symp. Space Tech. Sci., 2008-r-2-38, Hamamatsu, Japan

Nakamura, A. M., 2008, Laboratory impact disruption experiments -Towards understanding the impact process of porous bodies, The seventh international workshop on catastrophic disruption in the solar system, Alicante, Spain

Noritake, K., Ninagawa, K., Usami, T., and Toyoda, S. 2008. Thermoluminescence and ESR study of shocked minerals, Seminar on Solar System Cosmochemistry and Planetary Science Studies; 3rd Planetology Seminar-Planetology and its application to education, Budapest, Hungary

Onose, N., Okudaira, K. and Hasegawa, S. 2008. Ejection Velocities of Late Fragments Produced in Impact Craterings on Gypsum Targets: Empirical Measurements and an Elastic Ejection Model, Proc. 41th ISAS Lunar and Planet. Symp., 9-12.

Onose, N., Okudaira, K. and Hasegawa, S. 2008. Energy Partition into Compaction of a Target in Impact Cratering on a Gypsum Target, Proc. 41th ISAS Lunar and Planet. Symp., 13-22.

Setoh, M., Yamashita, Y., Nakamura, A. M., and Michel, P. 2008. Attenuation rate of stress wave in sintered and non-sintered glass beads targets, Workshop on simulations and experiments of impact processes, Meudon Observatory, September, 2008.

Setoh, M., Yamashita, Y., Nakamura, A. M., and Michel, P. 2008. Impact experiments of rubble pile, Asteroids, Comets, Meteors, Baltimore, July, 2008.

Setoh, M., Nakamura, A. M., Hiraoka, K., Yamashita, Y., Hasegawa, S., Onose, N., Okudaira, K., and Michel, P. 2008. Experimental study of stress wave attenuation in porous sintered glass beads targets, Lunar Planet Sci. Conf. XXXIX, #1797.

Yano, H., Noguchi, T., Matsunaga, S., Watanabe, T., Fujii, H., Makane, T., Hasegawa, S.,@ Miura, Y., Tsuchiyama, A., Miyamoto, H., Kato, Y., and the Minor Body Exploration Working Group Sampling Sub-Group. 2008. Sampling system of asteroid and comet nucleus samples for primitive body exploration program, 26th Int. Symp. Space Tech. Sci., 2008-k-07, Hamamatsu, Japan

Yamagishi, A., Yano, H., Okudaira, K., Kobayashi, K., Yokobori, S., Tabata, M., Kawai, H., Yamashita, M., Hashimoto, H., Naraoka, H., and Mita, H. 2008. Tanpopo: Astrobiology exposure and micrometeoroid capture experiments, The 26th International Symposium on Space Technology and Science, ISTS 2008-K-05

 

[2009”N]

Gavin, P., Chevrier, V., Ninagawa, K., Gucsik, A., and Hasegawa, S. 2009. Experimental investigation of the effect of meteoritic impacts on clays on Mars, Lunar Planet Sci. Conf. XXXX, #2069.

Hasegawa, S., Miyasaka, S., Tokimasa, N., Sogame, A., Ibrahimov, M. A., Yoshida, F., Abe, M., and Kuroda, D. 2009. BRz' phase function of asteroid 4 Vesta during the 2006 opposition, Lunar and Planetary Science Conference XXXX, #1503.

Katsura, T., Nakamura, A., Setoh, M., Takabe, A., Hasegawa, S., and Sangen, K., 2009. Experimental Study on Collisional Destruction of Iron-meteorite Parent Bodies, AOGS2009, Suntec, Singapore, August 11-15.

Kitazawa, Y., Sakurai, A., Yasaka, T., Funakoshi, F., Hanada, T., and Matsumoto, H. 2009. Development of a New Type Sensor for Micrometeoroid and Space Debris In-Situ Measurement at JAXA European Geosciences Union@General Assembly 2009,Vienna, Austria, 19 - 24 April 2009, (EGU2009-1598)

Kitazawa, Y., Sakurai, A., Yasaka, T., Funakoshi, F., Hanada, T., and Matsumoto, H. 2009. Development of a New Type Sensor for Micrometeoroid and Space Debris In-Situ Measurement at JAXA 27th ISTS, 2009-r-2-37p, July 9, 2009.

Kitazawa, Y., Sakurai, A., Yasaka, T., Kunakoshi, F., Hanada, T., Hasegawa, S., and Matsumoto, H. 2009. Development of a new type sensor for micrometeoroid and space debris in-situ measurement at JAXA, European Geosciences Union General Assembly 2009, Vienna, Austria

Kitazawa, Y., Sakurai, A., Yasaka, T., Kunakoshi, F., Hanada, T., Hasegawa, S., and Matsumoto, H. 2009. Development of a new type sensor for in-site space debris measurement, 60th International Astronautical Congress 2009, Daejeon, Korea

Matsumoto, H., Sakurai, A., Yasaka, T., Kunakoshi, F., Hanada, T., Hasegawa, S., and Kitazawa, Y. 2009. Development of a new type sensor for in-site space debris measurement, Proceedings of the Advanced Maui Optical and Space Surveillance Technologies Conference, p.E78

Takabe, A., Nakamura, A.M., Setoh, M., Katsura, T., Hasegawa, S. 2009. Collision experiment on dehydration of hydrated asteroids, AOGS2009, Suntec, Singapore, August 11-15.

 

 

 

‚VD‚QD‚RD@ŠwˆÊ˜_•¶

‚VD‚QD‚RD‚PD@”ŽŽm˜_•¶

[2002”N]

–îŽçÍA‚Q‚O‚O‚QA’´‚‘¬E‚ˆÀ’背[ƒ‹ƒKƒ“i‚g‚x‚o‚`‚bj‚ÌŠJ”­A”ŽŽm˜_•¶A‹ß‹E‘åŠw

[2004”N]

–qŒªˆê˜YA‚Q‚O‚O‚SA’´‚‘¬Õ“Ë‚É”º‚¤ƒ}ƒCƒNƒ”g•úŽË‚ÌŠÏ‘ª‹y‚Ñ•úŽËƒƒJƒjƒYƒ€‚̍lŽ@A”ŽŽm˜_•¶A“Œ‹ž‘åŠw

 

[2006”N]

Okudaira, K. 2006. Evaluation of Micrometeoroid Analogs Alteration on Capturing by Aerogel, Ph.D. thesis, The Graduate University for Advanced Studies, Kanagawa, Japan.

[2007”N]

¬–쐣’¼”üA‚Q‚O‚O‚VAÎp‚ɑ΂·‚éŽÎ‚ߏՓ˃NƒŒ[ƒ^[Œ`¬‚É‚¨‚¢‚Ä”­¶‚·‚é”j•Ð‚Ì‘¬“xŽ¿—Ê•ª•zF‚Q‚‚̔j•ÐŒQ‚Ì’è‹`‚Æ‚»‚Ì•úo‹@\A”ŽŽm˜_•¶A“Œ‹ž‘åŠw

[2008”N]

‘Š”n‰›—ߎqA‚Q‚O‚O‚WA’´‚‘¬Õ“Ë‚É”º‚¤ƒ}ƒCƒNƒ”g•úŽË‚Ì“Á«‚¨‚æ‚щF’ˆƒfƒuƒŠÕ“ËŒŸoŒn‚ÌŒŸ“¢A”ŽŽm˜_•¶A“Œ‹ž—‰È‘åŠw

Hiraoka, K. 2008. Experimental Study of the Impact Cratering Process in the Strength Regime, Ph.D. thesis, Kobe University, hyogo, Japan.

[2009”N]

Jutzi, M. 2009. Studies of collisions involving porous bodies, These de Doctorat, Universite de Nice Sophia Antipolis, France and Universite de Berne, Switzerland.

Tabata, M. 2009. Study of Transparent Silica Aerogel over the Wide Range of Densities, Ph.D. thesis, Chiba University, Chiba, Japan.

 

‚VD‚QD‚RD‚QD@CŽm˜_•¶

[1997”N]

“àŽR‹M”ŽA‚P‚X‚X‚VAƒfƒuƒŠÕ“Ë‚É‚æ‚éƒ}ƒCƒNƒ”g•úŽË‚ÌŒŸo‚ÉŠÖ‚·‚錤‹†ACŽm˜_•¶A“d‹C’ʐM‘åŠwi‚–ì’‰j

[1998”N]

•ŸŽR½“ñ˜YA‚P‚X‚X‚WAÕŒ‚•Ï¬ì—p‚É‚æ‚é‹…—±ó¬‡•¨Ž¿‚ÌŒ¤‹†ACŽm˜_•¶AŽRŒû‘åŠwiŽO‰Y•Û”́j

[2000”N]

Žº’J‰ÀGA‚Q‚O‚O‚OA’´‚‘¬Õ“Ë‚É‚æ‚éƒ}ƒCƒNƒ”g•úŽË‚ÌŒŸoE‰ž“š“Á«ACŽm˜_•¶A“Œ‹ž‘åŠwi‚–ì’‰j

[2002”N]

’r“c‰p“ñA‚Q‚O‚O‚QAƒAƒ~ƒmŽ_‚̏Ռ‚ŽÀŒ±ACŽm˜_•¶A‹ãB‘åŠwi‘º]’BŽmj

ŽODâM‹vA‚Q‚O‚O‚QAƒŒ[ƒ‹ƒKƒ“‚©‚ç‚̍‚‘¬”òãđ̂̏Փ˂ɂæ‚Á‚ж‚¸‚é“dŽ¥”g‚ÌŒv‘ªACŽm˜_•¶A‹ß‹E‘åŠwi‰Í“‡MŽ÷j

[2005”N]

‘Š”n‰›—ߎqA‚Q‚O‚O‚TA’´‚‘¬Õ“Ë‚É‚¨‚¯‚éƒCƒNƒ”g•úŽËŒ»Û‚̉𖾋y‚Ñ‚»‚̉ž—pACŽm˜_•¶A“Œ‹ž—‰È‘åŠwi‚–ì’‰j

[2006”N]

‰Á”[ŠwA‚Q‚O‚O‚UA‚•ªŽqŒnÞ—¿‚ð—˜—p‚µ‚½ƒfƒuƒŠƒV[ƒ‹ƒh‚̐«”\•]‰¿ACŽm˜_•¶A–@­‘åŠwiVˆä˜a‹gj

Ö“¡—z—ºA‚Q‚O‚O‚UA’´‚‘¬Õ“Ë”j‰ó‚É‚¨‚¯‚éƒCƒWƒFƒNƒ^ŒŸoŽÀŒ±ACŽm˜_•¶A“Œ‹ž—‰È‘åŠwi²X–ؐij

ÎˆäŒ’‘¾˜Y A‚Q‚O‚O‚UAÕ“Ë‚âÃˆ³‚É‚æ‚é”j‰ó‚É”º‚¤ƒ}ƒCƒNƒ”g•úŽËŒ»Û‚Ì“Á«‹y‚Ñ‚»‚̉ž—p‚ÉŠÖ‚·‚錤‹†ACŽm˜_•¶A“Œ‹ž—‰È‘åŠwi‚–ì’‰j

‘吼—TŽqA‚Q‚O‚O‚UA’´‚‘¬Õ“Ë‚É‚æ‚éƒ}ƒCƒNƒ”g•úŽËƒƒJƒjƒYƒ€‚ÉŠÖ‚·‚錤‹†ACŽm˜_•¶A“Œ‹ž‘åŠwi‚–ì’‰j

Î“cN«A‚Q‚O‚O‚UA”Mƒ‹ƒ~ƒlƒbƒZƒ“ƒXEƒJƒ\[ƒhƒ‹ƒ~ƒlƒbƒZƒ“ƒX‚É‚æ‚éÕŒ‚‚ðŽó‚¯‚½z•¨‚ÌŒ¤‹†ACŽm˜_•¶A‰ªŽR—‰È‘åŠwi吐쐴—²j

[2007”N]

ç—t–ΐ¶A‚Q‚O‚O‚VA’´‚‘¬Õ“Ë‚É”º‚¤ƒ}ƒCƒNƒ”g•úŽË‚Ì“Á«‚Æ”gŒ`‰ðÍACŽm˜_•¶A“Œ‹ž‘åŠwi‚–ì’‰j

’†_³’qA‚Q‚O‚O‚VAƒXƒy[ƒXƒfƒuƒŠƒV[ƒ‹ƒh\¬Þ—¿‚̐ϑw\‘¢‚ÌŒŸ“¢ACŽm˜_•¶A–@­‘åŠwiVˆä˜a‹gj

[2008”N]

¬ŽRClA‚Q‚O‚O‚WACFRP‚¨‚æ‚э‚•ªŽqÞ—¿‚ð—p‚¢‚½ƒV[ƒ‹ƒh‚̃Xƒy[ƒXƒfƒuƒŠ–hŒä«”\ACŽm˜_•¶A–@­‘åŠwiVˆä˜a‹gj

²“¡N”VA‚Q‚O‚O‚WA–Í‹[¯ŠÔ•¡ŽG—L‹@•¨‚̏Փˋy‚Ñ‚wü‚ɑ΂·‚éˆÀ’萫ACŽm˜_•¶A‰¡•l‘—§‘åŠwi¬—ÑŒ›³j

åM‰º‚³‚â‚©A‚Q‚O‚O‚WA’n‹…Žü‰ñ‹O“¹ã‚ł̉F’ˆo•ßŠl‚¨‚æ‚Ñ—L‹@•¨•ªÍ‚ÉŠÖ‚·‚éŠî‘bŒ¤‹†ACŽm˜_•¶A‰¡•l‘—§‘åŠwi¬—ÑŒ›³j

i“¡‘å“TA‚Q‚O‚O‚WAƒZƒ‰ƒ~ƒbƒNƒXƒ‰ƒXƒ^—pSi3N4‚Ì’´‚‘¬Õ“ˉº‚É‚æ‚鑹‹““®•]‰¿ACŽm˜_•¶A“ŒŠC‘åŠwi²“¡‰pˆêj

ŽO–Ø—mŽiA‚Q‚O‚O‚WAHHACŽm˜_•¶A“Œ‹ž—‰È‘åŠwi‚–ì’‰j

¬‘q®–çA‚Q‚O‚O‚WAŠÜ…Îp‚¨‚æ‚Ñ–³…Îp‚̏Փ˔j‰óŽÀŒ±F¬˜f¯Õ“Ë‚É‚æ‚é‰Á”ME’E…‚ªoŒ`¬‚É—^‚¦‚é‰e‹¿ACŽm˜_•¶A_ŒË‘åŠwi’†‘ººŽqj

Makabe, T. 2008. The Determination of Projectile Shape for Asteroid Impact Sampling System, Master thesis, University of Tokyo, Hyogo, Japan.

[2009”N]

’·’Jì½•vA‚Q‚O‚O‚XAƒzƒCƒbƒvƒ‹ƒV[ƒ‹ƒh‚̃Xƒy[ƒXƒfƒuƒŠ–hŒä«”\‚̐”’l‰ðÍACŽm˜_•¶A–@­‘åŠwiVˆä˜a‹gj

“¡èŒ’‘¾A‚Q‚O‚O‚XA–Í‹[‰F’ˆŠÂ‹«‰º‚Å‚Ì”÷¶•¨‚̐¶‘¶‰Â”\«‚Æ‚»‚ÌŒŸo–@‚ÌŒŸ“¢ACŽm˜_•¶A‰¡•l‘—§‘åŠwi¬—ÑŒ›³j

‘¥•Oˆê˜YA‚Q‚O‚O‚XA”Mƒ‹ƒ~ƒlƒbƒZƒ“ƒXEESR‚É‚æ‚éÕŒ‚‚ðŽó‚¯‚½z•¨‚ÌŒ¤‹†ACŽm˜_•¶A‰ªŽR—‰È‘åŠwi吐쐴—²j

 

‚VD‚QD‚RD‚RD@ŠwŽm˜_•¶

[1995”N]

ÍŒ‹ÎA‚P‚X‚X‚TA‰ÈŠwŽÀŒ±—pƒŒ[ƒ‹ƒKƒ“‚ÌŠJ”­AŠwŽm˜_•¶A’·è‘‡‰ÈŠw‘åŠwi‰Í“‡MŽ÷j

’†‘ºâMA‚P‚X‚X‚TAƒŒ[ƒ‹ƒKƒ“‚É‚¨‚¯‚鍂‘¬ƒvƒ‰ƒYƒ}‚̐U‚é•‘‚¢AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi‰Í“‡MŽ÷j

‹{Œ´‘åA‚P‚X‚X‚TAŠO•”Ž¥ê‚É‚æ‚郌[ƒ‹ƒKƒ“‚Ì“®ì“Á«AŠwŽm˜_•¶A•‘ H‹Æ‘åŠwi‰Í“‡MŽ÷j

[1996”N]

’·]ŒcˆêA‚P‚X‚X‚UAƒŒ[ƒ‹ƒKƒ“‚É‚¨‚¯‚é“®ìŒø—¦‚̉ðÍAŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi‰Í“‡MŽ÷j

[1997]

‰–Œ´Š²A‚P‚X‚X‚VAƒŒ[ƒ‹ƒKƒ“‚Ì“dˆ³‚Æ‚QŽžƒA[ƒN‚Æ‚ÌŠÖ˜AAŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi‰Í“‡MŽ÷j

Ö“¡—FŠîA‚P‚X‚X‚VAŠO•”Ž¥êƒŒ[ƒ‹ƒKƒ“‚Ì“®ì“Á«AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi‰Í“‡MŽ÷j

[1998”N]

‹àˆä—SŽjA‚P‚X‚X‚WAƒŒ[ƒ‹ƒKƒ“‚̏eg‚É‚¨‚¯‚éƒvƒ‰ƒYƒ}ƒA[ƒN‚Ì‹““®AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

VìrŽkA‚P‚X‚X‚WA—U“±Œ^ƒŒ[ƒ‹ƒKƒ“‚Ì“®ì“Á«AŠwŽm˜_•¶A•‘ H‹Æ‘åŠwi–îŽçÍj

‘ë‹{ŒOA‚P‚X‚X‚WA—U“±Œ^ƒŒ[ƒ‹ƒKƒ“‚ÌŠJ”­AŠwŽm˜_•¶A“Œ‹žH‰È‘åŠwi–îŽçÍj

’|“à’¼ÆA‚P‚X‚X‚WA—U“±Œ^ƒŒ[ƒ‹ƒKƒ“‚ÌŠJ”­AŠwŽm˜_•¶A“Œ‹žH‰È‘åŠwi–îŽçÍj

“y‰ª³Ž¡A‚P‚X‚X‚WA—U“±Œ^ƒŒ[ƒ‹ƒKƒ“‚ÌŠJ”­AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

ˆ¢‘]Œ“ŽŸA‚P‚X‚X‚WA—U“±Œ^ƒŒ[ƒ‹ƒKƒ“‚ÌŠJ”­AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

[1999”N]

’†–ìÉ‰„BA‚P‚X‚X‚XA‚Q’iŽ®ƒŒ[ƒ‹ƒKƒ“‚ÌŠJ”­‚ÉŠÖ‚·‚錤‹†AŠwŽm˜_•¶A•‘ H‹Æ‘åŠwi–îŽçÍj

’|“à^‹KŽqA‚P‚X‚X‚XA‚g‚x‚o‚`‚bƒŒ[ƒ‹ƒKƒ“‚Ì‘¬“x•Ï‘JAŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

•—ŠÔ–qA‚P‚X‚X‚XA‚g‚x‚o‚`‚bƒŒ[ƒ‹ƒKƒ“‚É‚¨‚¯‚鑬“xŒv‘ª‚Æ—U“±Œ^ƒŒ[ƒ‹ƒKƒ“‚̃Vƒ~ƒ…ƒŒ[ƒVƒ‡ƒ“ŒvŽZAŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

¬–x‹v’jA‚P‚X‚X‚XA“ñ’iŽ®ƒŒ[ƒ‹ƒKƒ“‚ÌŠJ”­AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

‘º“c—YˆêA‚P‚X‚X‚XA—U“±Œ^“dŽ¥”òãđ̉Á‘¬‘•’uŠJ”­‚ׂ̗̈\”õŽÀŒ±Œ‹‰ÊAŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

[2000”N]

—L“c—LŽiA‚Q‚O‚O‚OA—U“±Œ^ƒŒ[ƒ‹ƒKƒ“‚ÌŠJ”­‚ׂ̗̈\”õŽÀŒ±AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

ìè ”üA‚Q‚O‚O‚OA“dŽ¥”òãđ̉Á‘¬‘•’u‚ð覐΂̏ՓˎÀŒ±ƒVƒ~ƒ…ƒŒ[ƒVƒ‡ƒ“—p‰Á‘¬‘•’u‚Æ‚µ‚Ä—p‚¢‚½”òãđ̂̌¤‹†ŠJ”­AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

’†“ÚŒ’A‚Q‚O‚O‚OA“ñ’iŽ®ƒŒ[ƒ‹ƒKƒ“ŠJ”­‚ÌŒ¤‹†AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

[2001”N]

’r“cŒb”üA‚Q‚O‚O‚PA—U“±Œ^ƒŒ[ƒ‹ƒKƒ“ŠJ”­‚ׂ̗̈\”õŽÀŒ±AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

´…ŒbŽqA‚Q‚O‚O‚PAƒ~ƒjƒŒ[ƒ‹ƒKƒ“‚ÌŒ¤‹†‚ÆŠJ”­AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

“ñ‹{‰ÀŽÀA‚Q‚O‚O‚PA“ñ’iŽ®ƒŒ[ƒ‹ƒKƒ“‚ÌŠJ”­‚ÌŒ¤‹†AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

[2002”N]

Vˆä—WA‚Q‚O‚O‚QAƒŒ[ƒ‹ƒKƒ“‚̐^‹óƒV[ƒ‹‚É‚æ‚é‰e‹¿AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

Š}Œ´“NA‚Q‚O‚O‚QA—U“±Œ^ƒŒ[ƒ‹ƒKƒ“‚ÌŒ¤‹†AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

»”‘—²ŒõA‚Q‚O‚O‚QA“ñ’iŽ®ƒŒ[ƒ‹ƒKƒ“‚ÌŒ¤‹†‚ÆŠJ”­AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj@@@

¼‰iŠx•FA‚Q‚O‚O‚QA“ñ’iŽ®ƒŒ[ƒ‹ƒKƒ“‚ÌŠJ”­‚ÉŠÖ‚·‚錤‹†AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

[2003”N]

²“¡r–çA‚Q‚O‚O‚RA‚Q‚V‚U‚‹‚i‚É‚¨‚¯‚é”òãđ̉Á‘¬‚Ì”äŠrŒŸ“¢AŠwŽm˜_•¶AÃ“ìH‰È‘åŠwi–îŽçÍj

[2004”N]

‹àŽq‘nA‚Q‚O‚O‚SAƒŒ[ƒ‹ƒKƒ“”­ŽËŽž‚É‚¨‚¯‚éƒvƒ‰ƒYƒ}ƒA[ƒ}ƒ`ƒƒ[‚Ì‹““®‰ðÍAŠwŽm˜_•¶A“ŒŠC‘åŠwi–îŽçÍj

’|“c¹•½A‚Q‚O‚O‚SA‚c‚d‚rƒŒ[ƒ‹ƒKƒ“‚ÌŒ¤‹†AŠwŽm˜_•¶A“ŒŠC‘åŠwi–îŽçÍj

[2005”N]

‘½“cãĈê˜YA‚Q‚O‚O‚TA’´‚‘¬Õ“Ë‚É‚¨‚¯‚é”––Œ‚Ì”j‰óŒ»Û‚Æ‚»‚ÌŒõ‘¬ðŒ‚ւ̈ˑ¶«AŠwŽm˜_•¶A“ŒŠC‘åŠwi²X–ؐij

ŽO‰Y“ÖŽjA‚Q‚O‚O‚TA”––Œ\‘¢•¨‚ւ̃Xƒy[ƒXƒfƒuƒŠÕ“Ë‚ð–Í‹[‚µ‚½’´‚‘¬Õ“ËŽÀŒ±AŠwŽm˜_•¶A“ŒŠC‘åŠwi²X–ؐij

²“¡’¼A’†_³’qA‚Q‚O‚O‚TAƒXƒy[ƒXƒfƒuƒŠ—pŒy—Ê¥¬Œ^ƒoƒ“ƒp‚ÌŠJ”­A ŠwŽm˜_•¶A–@­‘åŠwiVˆä˜a‹gj

[2006”N]

ìã‚Ž÷A¬ŽRClA‚Q‚O‚O‚UA‚•ªŽqŒnÞ—¿‚ð—˜—p‚µ‚½ƒXƒy[ƒXƒfƒuƒŠÕ“Ë–hŒäƒV[ƒ‹ƒh‚ÌŽŽìAŠwŽm˜_•¶A–@­‘åŠwiVˆä˜a‹gj

ŒÃ«rŒcA‚Q‚O‚O‚UA’´‚‘¬”òãđ̂̔––Œ\‘¢•¨‚ɑ΂·‚éÕ“ËŽÀŒ±AŠwŽm˜_•¶A“ŒŠC‘åŠwi²X–ؐij

[2007”N]

’‡“c“NiA‚Q‚O‚O‚VA”÷¬d—͉º‚̃NƒŒ[ƒ^[Œ`¬ŽÀŒ±AŠwŽm˜_•¶A–@­‘åŠwiVˆä˜a‹gj

‘“cŒ˜ŒáA‚Q‚O‚O‚VAŽŽìƒXƒy[ƒXƒfƒuƒŠƒV[ƒ‹ƒh‚ÌŒy—ʉ»‚ÌŒŸ“¢AŠwŽm˜_•¶A–@­‘åŠwiVˆä˜a‹gj

{‰iFˆêA‚Q‚O‚O‚VAƒŒ[ƒ‹ƒKƒ“‚ð—p‚¢‚½‹à‘®”––Œ‚ւ̃fƒuƒŠÕ“ˁAŠwŽm˜_•¶A“Œ‹ž—‰È‘åŠwi²X–ؐij

ŠÝNOA‚Q‚O‚O‚VA•¨‘Ì‚Ì”j‰ó‚É”º‚¤“dŽ¥”g•úŽË‚Ì•¨«’lE•¨—’l‚É’…–Ú‚µ‚½Œ¤‹†AŠwŽm˜_•¶A“Œ‹ž—‰È‘åŠwi‚–ì’‰j

ìŒûŽõ‘¾˜YA‚Q‚O‚O‚VA‰F’ˆ‹óŠÔ‚É‚¨‚¯‚é”÷¶•¨‘¶Ý‚̉”\«AŠwŽm˜_•¶A“Œ‹ž–ò‰È‘åŠwiŽRŠÝ–¾•Fj

H“¡Œ’—TA‚Q‚O‚O‚VC’´‚‘¬‚ð–ÚŽw‚µ‚½2’iŽ®ƒŒ[ƒ‹ƒKƒ“‚ÌŒ¤‹†AŠwŽm˜_•¶A”ªŒËH‹Æ‚“™ê–åŠwZi–îŽçÍj

’·‰ª—mˆêA‚Q‚O‚O‚VCƒŒ[ƒ‹ƒKƒ““à•”‚É‚¨‚¯‚é2ŽŸƒA[ƒN‚Ì”­¶AŠwŽm˜_•¶A”ªŒËH‹Æ‚“™ê–åŠwZi–îŽçÍj

[2008”N]

ˆÉ“¡—²Š°A–q–ì—YìA‚Q‚O‚O‚WACFRP‚ð—p‚¢‚½ƒzƒCƒbƒvƒ‹ƒV[ƒ‹ƒh‚Ì‘¹•]‰¿AŠwŽm˜_•¶A–@­‘åŠwiVˆä˜a‹gj

¬ì–õ”ŽA¬—Ñ—SãāA‚Q‚O‚O‚WAƒAƒ‹ƒ~ƒi‚¨‚æ‚Ñ’‚‰»Œ]‘f‚Ì”÷—±Žq‚‘¬Õ“Ë‘¹AŠwŽm˜_•¶A–@­‘åŠwiVˆä˜a‹gj

‹´‹à‘¾˜YA‚Q‚O‚O‚WA‰„«EÆ«Þ—¿‚Ì’´‚‘¬Õ“Ë”j‰ó‹““®‚̈ႢAŠwŽm˜_•¶A“Œ‹ž“s—§‰ÈŠw‹Zp‘åŠwi²“¡‰pˆêj

ÎžÒ—E‰îA‚Q‚O‚O‚WAŽ¥Î‚ƃRƒCƒ‹‚É‚æ‚é”òãđ̂̌Ÿo‚Æ‘¬“xŒv‘ªAŠwŽm˜_•¶A“d‹C’ʐM‘åŠwi–öàV³‹vj

“c’†Tˆê˜YA‚Q‚O‚O‚WAŽ¥Î‚ƃRƒCƒ‹‚É‚æ‚é”òãđ̂̌Ÿo‚Æ‘¬“xŒv‘ªAŠwŽm˜_•¶A“d‹C’ʐM‘åŠwi–öàV³‹vj

 

ƒ_ƒkƒJEƒTƒ}ƒ‰ƒi[ƒ„ƒJA‚Q‚O‚O‚WAƒtƒHƒgƒ_ƒCƒI[ƒh‚É‚æ‚éŒõ—Ê‚Ì‘ª’èAŠwŽm˜_•¶A“d‹C’ʐM‘åŠwi–öàV³‹vj

[2009”N]

ꎓ¡—mA‚Q‚O‚O‚XAVŒ^“ñ’iŽ®ŒyƒKƒXe‚ð—p‚¢‚½˜f¯’T¸‹@ƒXƒ‰ƒXƒ^—pSi3N4‚Ì’´‚‘¬Õ“Ë”j‰ó‹““®AŠwŽm˜_•¶A–@­‘åŠwi²“¡‰pˆêj

Œj•–MA‚Q‚O‚O‚XA“SŽ¿¬“V‘Ì‚ð–Í‹[‚µ‚½Õ“Ë”j‰óŽÀŒ±AŠwŽmŒ¤‹†A_ŒË‘åŠwi’†‘ººŽqj

‚•”Ê“ށA‚Q‚O‚O‚XA_ŒË‘åŠw—Šw•”’n‹…˜f¯‰ÈŠw‰È‘²‹ÆŒ¤‹†AŠwŽmŒ¤‹†A_ŒË‘åŠwi’†‘ººŽqj

ÂˆäGŽ÷A‚Q‚O‚O‚XA‚Q’iŽ®ŒyƒKƒXe‚É‚æ‚éÕ“Ë‘MŒõŽÀŒ±AŠwŽm˜_•¶A“d‹C’ʐM‘åŠwi–öàV³‹vj

‰|–{¹Ž÷A‚Q‚O‚O‚XAƒtƒ‰ƒbƒVƒ…Xü‚É‚æ‚é”òãđ̂̎B‰eAŠwŽm˜_•¶A“d‹C’ʐM‘åŠwi–öàV³‹vj

—é–ØŒ[—SA‚Q‚O‚O‚XAŒõƒtƒFƒ“ƒX‚É‚æ‚é”òãđ̂̌ŸoAŠwŽm˜_•¶A“d‹C’ʐM‘åŠwi–öàV³‹vj

 

 

‚VD‚QD‚SD@Žg—p‚µ‚½ƒvƒƒWƒFƒNƒg

‚i‚`‚w‚`‰q¯ÝŒv•W€i‚v‚f3FƒfƒuƒŠ–hŒäj F‚Q‚O‚O‚T`

Deep Impact iƒCƒWƒFƒNƒ^•úo‰ß’öŠÏŽ@j@@F‚Q‚O‚O‚T

StardustiƒGƒAƒƒWƒFƒ‹ŠÑ“üŠÏŽ@j@@@@@F‚Q‚O‚O‚U

‚ ‚©‚‚«iƒXƒ‰ƒXƒ^‘̐§ŽŽŒ±j@@@@@@@F‚Q‚O‚O‚U`

Ikarosi–Œ‘̐§ŽŽŒ±•ƒ_ƒXƒgŒŸoŠíŠJ”­j@@F‚Q‚O‚O‚T`

‚½‚ñ‚ۂہiƒGƒAƒƒWƒFƒ‹ŠJ”­j@@@@@@@F‚Q‚O‚O‚V`

ƒyƒsƒRƒƒ“ƒ{iƒ_ƒXƒgŒŸoŠíŠJ”­j@@@@@F‚Q‚O‚O‚X`

‚f‚b‚n‚liƒfƒuƒŠ–hŒä‘΍ôj@@@@@@@@F‚Q‚O‚O‚X