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Introductory Comments on Venuss Lower Atmosphere
Multiple Light Scattering in Planetary Atmospheres
9 other sections not shown
absorption albedo altitude angle approximately assumed atmos atmosphere of Mars band Brandt/McElroy calculated Chamberlain 1965 Chamberlain and McElroy circulation cloud cloud albedo coefficient computed Coriolis force curve diffusion discussed Doppler broadening Earth electron density energy loss equation errors Eshleman estimates exospheric exospheric temperature Figure Fjeldbo flux Geophys Goody heat indicated infrared ionization ionosphere isotropic Kitt Peak Kliore Kuiper loss rate lower atmosphere Mariner Martian atmosphere measurements mesopause method mosphere motions neutral number density observed obtained occultation optical depth optical thickness parameters particles peak phase effect phase function phere photoelectrons planet potential temperature problem pure C02 radiation radiative Rasool ratio recombination refractivity region Rossby rotation Sagan scale height scattering shown in Fig solar wind Space Sci specific amount spectra spectrum Spinrad studies surface pressure temperature gradient thermal thermopause thermosphere tion vertical water vapor wave wavelength