関連文書

Nakamura, M., T. Imamura, M. Ueno, N. Iwagami, T. Satoh, S. Watanabe, M.Taguchi, Y. Takahashi, M. Suzuki, T. Abe, G.L. Hashimoto, T. Sakanoi, S.Okano, Y. Kasaba, J. Yoshida, M. Yamada, N. Ishii, T. Yamada, K.-I. Oyama (2007). PLANET-C: Venus Climate Orbiter mission of Japan, Planet. Space Sci., 55, 1831-1842.
Taguchi, M., T. Imamura, M. Nakamura, N. Iwagami, M. Ueno, M. Suzuki, T.Fukuhara, G.L. Hashimoto, and K. Mitsuyama (2007). Longwave Infrared imager onboard the Venus Climate Orbiter, Adv. Space Res., 40, 861-868.

Ueno, M., Ishiguro, M., Kimata, M., Hong, S.S., Otsubo, T., Sato, T.,Usui, F., Yano, H., Nakamura, M. (2005). Observations of zodiacal light during the cruising phase of PLANET-C/VCO mission, Adv. Space Res.

Hashimoto, G.L., M. Roos-Serote, S. Sugita, M.S. Gilmore, L.W. Kamp, R.W. Carlson, and K.H. Baines (2008). Galileo Near Infrared Mapping Spectrometer (NIMS) data suggest felsic highland crust on Venus, J. Geophys. Res., in press.
Iwagami, N., S. Ohtsuki, K. Tokuda, N. Ohira, Y. Kasaba, T. Imamura, H. Sagawa, G.L. Hashimoto, S. Takeuchi, M. Ueno, and S. Okumura (2008). Hemispheric distributions of HCl above and below the Venus' clouds by ground-based 1.7 um spectroscopy, Planet. Space Sci., 56, 1424-1434.
Ohtsuki, S., Iwagami, N., Sagawa, H., Kasaba, Y., Ueno, M., Imamura, T. (2008). Imaging Spectroscopy of the Venus 1.27-um O2 Airglow with Ground-based Telescopes, Adv. Space Res., in press.

Hashimoto, G.L., Y. Abe, and S. Sugita (2007). The chemical composition of the early terrestrial atmosphere: Formation of a reducing atmosphere from CI-like material, J. Geophys. Res., 112, E05010.

Hashimoto, G.L., and Y. Abe (2005). Climate control on Venus: comparison of the carbonate and pyrite models, Planet. Space Sci., 53, 839-848.
Ohtsuki, S., Iwagami, N., Sagawa, H., Kasaba, Y., Ueno, M., Imamura, T. (2005). Ground-based observation of the Venus 1.27um O2 airglow, Adv. Space Res., vol. 36, Issue 11, 2038-2042.

はしもとじょーじ (2004). 金星大気の形成と進化, 日本惑星科学会誌・遊星人, 13, 4-11.
大月祥子、佐川英夫、笠羽康正、今村剛、はしもとじょーじ、岩上直幹 (2004). 地上観測による金星夜側大気へのアプローチ, 日本惑星科学会誌・遊星人、13, 31-37.

Sagawa, H., Kasaba, Y., Imamura, T., Hashimoto, G. L., Ueno, M., Satoh, T., Nakamura, R., Okumura, S., Iwagami, N., Ohtsuki, S., Mihara, F., Nakamura, M. (2003). The nightside of Venus below the cloud layer observed at Okayama Astrophysical Observatory, ISAS Research Note, Vol.765.
Hashimoto, G.L., and S. Sugita (2003). On observing the compositional variability of the surface of Venus using nightside near-infrared thermal radiation, J. Geophys. Res., 108(E9), 5109.

Imamura, T., and G.L. Hashimoto (2002). H2SO4 cycle in the Venusian tropical atmosphere as constrained by a microphysical cloud model, Adv. Space Res., 29(2), 249-254.

Hashimoto, G.L., and T. Imamura (2001). Elucidating the rate of volcanism on Venus: Detection of lava eruptions using near-infrared observations, Icarus, 154, 239-243.
Hashimoto, G.L., and Y. Abe (2001). Predictions of a simple cloud model for water vapor cloud albedo feedback on Venus, J. Geophys. Res., 106, 14675-14690.
Imamura, T., and G.L. Hashimoto (2001). Microphysics of Venusian clouds in rising tropical air, J. Atmos. Sci., 58, 3597-3612.

Hashimoto, G.L., and Y. Abe (2000). Stabilization of Venus' climate by a chemical-albedo feedback, Earth Planets Space, 52, 197-202.
Imamura, T., and G.L. Hashimoto (1998). Venus cloud formation in the meridional circulation, J. Geophys. Res., 103, 31349-31366.
はしもとじょーじ・阿部豊 (1998). 金星の大気・地殻の化学相互作用, 日本惑星科学会誌・遊星人, 7, 109-114.
Hashimoto, G.L., Y. Abe, and S. Sasaki (1997). CO2 amount on Venus constrained by a criterion of topographic-greenhouse instability, Geophys. Res. Lett., 24, 289-292.