next up previous
: Two dimensional anelastic model : 6 地表面熱収支モデル


Carr, M. H. 1996: Water on Mars, Oxfird Univ. Press, 229pp.

Conrath, B. J., 1975: Thermal structure of the Martian atmosphere during the dissipation of the dust storm of 1971, Icarus, 24, 36-46.

Forget, F., 1998: Improved optical properties of the Martian atmospheric dust for radiative transfer calculations in the infrared, Geopys. Res. Lett., 25, 1105-1108.

Forget, F., F. Hourdin, R. Fournier, C. Hourdin, O. Talagrand, M. Collins, S. R. Lewis, P. L. Read, and J. P. Huot, 1999: Improved general circulation models of the Martian atmosphere from the surface to above 80 km, J. Geophys. Res., 104, 24155-24175.

Goody, R. M., and Y. L. Yung, 1989: Atmospheric Radiation (Theoritcal basis), 2'nd ed., Oxford Univ. Press, 519pp.

Houghton, J. T., 1986: The Physiscs of Atmospheres, 2'nd ed., Cambridge Univ. Press, 271pp.

国立天文台編, 2000: 理科年表 2000 年版, 丸善.

Kieffer, H. H., T. Z. Martin, A. R. Peterfreund, B. M. Jakosky, E. D. Miner, and F. D. Palluconi, 1977: Thermal and albedo mapping of Mars during the Viking primary mission, J. Geophys. Res., 82, 4249-4291.

Klemp, J. B., and R. B. Wilhelmson, 1978: The simulation of three-dimensional convective storm dynamics. J. Atmos. Sci., 35, 1070-1096.

Liou, K-N. 1980: An Introduction to Atmosphric Radiation, Academic Press, 392pp.

Louis, J. 1979: A parametric model of vertical eddy fluxes in the atmosphere. Bound.-Layer Meteor., 17, 187-202.

Nakajima, K. 1994: Direct numerical experiments on the large-scale organizations of cumulus convection, Ph.D thesis, Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo, Tokyo, Japan(in Japanese).

Ockert-Bell, M. E., J. F. Bell III, J. B. Pollack, C. P. McKay, and F. Forget, 1997: Absorption and scattering properties of the Martian dust in the solar wavelengths, J. Geophys. Res., 102, 9039-9050.

小倉 義光, 1999: 一般気象学 第2版, 東京大学出版会.

Ogura, Y., and N. A. Phillips, 1962: Scale analysis of deep and shallow convection in the atmosphere, J. Atmos. Sci., 19, 173-179.

小高正嗣, 中島健介, 石渡正樹, 林祥介, 2001: 2 次元非弾性系を用いた火星大気放射対流の数値計算, ながれマルチメディア 2001, http:www.nagare.or.jpmm2001 odaka

Pollack, J. B., D. S. Colburn, F. M. Flasar, R. Kahn, C. E. Carlston, and D. Pidek, 1979: Properties and effects of dust particles suspended in the Martian atmosphere, J. Geophys. Res., 84, 2929-2945.

Savijärvi, H. 1991a: Radiative fluxes on dustfree Mars, Contr. Atmosph. Phys., 64, 103-112.

柴田清孝, 1999: 光の気象学, 応用気象学シリーズ1, 朝倉書店

Sutton, J. L., C. B. Leovy, and J. E. Tillman, 1978: Diurnal variations of the Martian surface layer meteorological parameters during the first 45 sols at two Viking lander sites, J. Atmos. Sci., 35, 2346-2355.

Toon, O. B., J. B. Pollack, and C. Sagan, 1977: Physical properties of the particles composing the Martian dust storm of 1971-1972, Icarus, 30, 663-693.

White, B. R., B. M. Lacchia, R. Greeley, and R. N. Leach, 1997: Aeolian behavior of dust in a simulated Martian environment, J. Geophys. Res., 102, 25629-25640.

next up previous
: Two dimensional anelastic model : 6 地表面熱収支モデル
Odaka Masatsugu 平成19年4月25日