Cloud microphysics: Analysis of the clouds of Earth, Venus, Mars and Jupiter

Icarus

Volumn 36, Issue 1, 1978, Pages 1-50

  Rossow, William B ^a  

^a PRINCETON UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0011591598     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/0019-1035(78)90072-6     Document Type: Article

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111. A numerical investigation of the efficiency with which simple columnar ice crystals collide with supercooled water drops
112. A comparison of formulations of stochastic collection
113. Poisson statistics in distributions of coalescing droplets
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115. The “soil” of Mars
116. The upper Jovian atmosphere aerosol content determined from a satellite eclipse observation
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118. Size distribution of raindrops generated by their breakup and coalescence
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127. Recent thinking on the chemical formation of aerosols in the air by gas phase reactions
128. Stability of submicron aqueous solution droplets in the atmosphere
129. Coagulation and size distribution of condensation aerosols
130. The microstructure of cumulus cloud Part I General features of the droplet spectrum
131. Relaxation time and steady evaporation rate of freely falling rain drops
132. Atmospheric and cloud structures of the Jovian planets
133. Efficiency of natural rain
134. Venus cloud models
135. Experimental determination of collision efficiencies for small water droplets in air
136. Are the clouds of Venus sulfuric acid?
137. The clouds of Venus
138. An improved Venus cloud model
139. The evolution of drop spectra due to condensation, coalescence and breakup