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D. K. Lilly

590 JOURNAL OF APPLIED METEOROLOGY VOLUME10NOTES AND CORRESPONDENCEComments on "Case Studies of a Convective Plume and a Dust Devil" D. K. L~LLY National Cen~er for Atmospheric Research,~ Boulder, Colo. 26 October 1970 The paper by Kaimal and Businger (1970) is an important contribution to our observational knowledge ofplumes and dust devils in the planetary

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Todd A. Cerni and Thomas R. Parish

atmospheric water vapor in the 8-12 ~m window. App!. Opt., 15, 2085-2090.Rodgers, C. D., and C. D. Walshaw, 1966: The computation ofinfrared cooling rate in planetary atmospheres. Quart. J. Roy.Meteor. Soc., 93, 43-54.Roewe, D., and K. Liou, 1978: Influence of cirrus clouds on theinfrared cooling rate in the troposphere and lower stratosphere.J. App!. Meteor., 17, 92-106.Sasamori, T., 1968: The radiative cooling calculation for applicationto general circulation experiments. J. App!. Meteor., 7, 721

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George Ohring and Dina Goldberg

Av6vsT1977 GEORGE OHRING AND DINA GOLDBERG 855A Direct Method for Obtaining Ballistic Densities from Satellite Radiance Observations GEORGE OI-IRING AND DINA GOLDBE,RGDepartment of Geophysics and Planetary Sciences, Tel-Avlv University, Ramat Avlv, Israel(Manuscript received 26 February 1977, in revised form I0 June 1977)ABSTRACT A nonstatistical method for obtaining ballistic densities

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J. A. Weinman and P. J. Guetter

of near ultraviolet irradiances through smog over Los Angeles. Preprlnts of Papers Conf. Air Pollution Meteorology. Raleigh, N. C. Amer. Meteor. Soc., 121-125.van de Hulst, H. C., 1971: The spectrum of the anisotropic transfer equation. Astron. Astrophys. (in press). , and K. Grossman, 1968: Multiple scattering in planetary atmospheres. The Atmospheres of Venus and Mars, New York, Gordon and Breach, 35-55.

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Wen-Yih Sun and Chiao-Zen Chang

boundary layer. For instance, all of the secondmoments and the dissipation term are integrated frompartial differential equations in Wyngaard and Cot6's(1974) model. The second-order model developed byZeman and Lumley (1976) requires 12 prognostic differential equations for the higher-order moments, inaddition to the differential equations for the first moments in a dry atmosphere, and the third-order modelfor a moist planetary boundary proposed by Andr~ etal. (1976a, 1978) consists of 33 prognostic

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Frank Haurwitz and William R. Kuhn

.1-1.8 km. These thicknesses agree well with thosereported by Tverskoi (1965). The distribution of cloudlayers is shown in Fig. 2.3. Resultsa. Outgoing planetary radiation Zonal averages of the annual outgoing planetaryradiation at the top of the atmosphere from this as wellas from other investigations are shown in Fig. 3.Since our calculations only extended to 137.5 mb andtherefore did not include the contribution to the outward flux from the stratosphere, we have added theoutgoing stratospheric

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N. A. Scott and A. Chedin

satellites, like interferometers. This is mainly the case for studies on thestratosphere and on planetary atmospheres forwhich atmospheric conditions (temperature and/orcomposition) are not very well known or are unknown and must be constantly varied by oftenlarge amounts when adjusting theory to experiment. The approach used in this paper for obtaining acomputationally fast and general line-by-line methodconsists, at first, in using a standard line-by-lineprocedure to derive the transmittances

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Freeman F. Hall Jr.

answer thisquestion we need to know how variable the wind is inthe free atmosphere and then determine what constitutes a representative wind value. Previous investigations of wind variability have usedtheodolite tracking of sequential pilot balloons (Singer1956 ), radar tracking of sequential $imspheres ($ohnson and Vaughan 1978), sequential tracking ofMETRAC (Meteorological Tracking) balloons (Gageand Jasperson 1979), and both aircraft and radar windprofiler data analyses (Gage and Nastrom 1985

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Stanley A. Changnon Jr.

: Atmospheric Diffusion. London, D. Van Nos trand Co., 297 pp.Peng, L., 1965: Stratospheric wind temperature and isobaric height conditions during the IG- period: Part III. Rept. No. 15, Planetary Circulations Project, Dept. of Meteorology, M. I. T., 201 pp,Prabhakara, C., 1963: Effects of non-photochemical processes on the meridional distribution and total amount of ozone in the atmosphere. Mon. Wea. Re'v, 91,441-431.Reed, R. J., and K. E. German, 1965: A contribution to the prob lem of

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S. SethuRaman

-192.Kitaigorodskii, S. A., 1973: The Physics of Air-Sea Interaction.Israel Program for Scientific Translations, Jerusalem, 237 pp.Kondo, J., Y. Fujinawa and G. Naito, 1972: Wave-induced windfluctuations over the sea. J. Fluid Mech., 51, 751-711.Keuttner, J., 1959: The band structure of the atmosphere. Tellus,11,267-294.1971: Cloud bands in the earth's atmosphere. Observationsand theory. Tellus, 23, 404-425.Lemone, M. A., 1973: The structure and dynamics of horizontalroll vortices in the planetary boundary layer

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