@article{ca01900k,

title = {Belt-zone variations in the Jovian cloud structure},

author = {B. E. Carlson and A. A. Lacis and W. B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/08/1994_Carlson_ca01900k.pdf, Download file},

doi = {10.1029/94JE01222},

year  = {1994},

date = {1994-01-01},

urldate = {1994-01-01},

journal = {J. Geophys. Res.},

volume = {99},

pages = {14623--14658},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ca07800y,

title = {Tropospheric gas composition and cloud structure of the Jovian North Equatorial Belt},

author = {B. E. Carlson and A. A. Lacis and W. B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/08/1993_Carlson_etal.pdf, Download file},

doi = {10.1029/92JE02737},

year  = {1993},

date = {1993-01-01},

urldate = {1993-01-01},

journal = {J. Geophys. Res.},

volume = {98},

pages = {5251--5290},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ca02800o,

title = {Ortho-para-hydrogen equilibration on Jupiter},

author = {B. E. Carlson and A. A. Lacis and W. B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/08/1992_Carlson_ca02800o.pdf, Download file},

doi = {10.1086/171510},

year  = {1992},

date = {1992-01-01},

urldate = {1992-01-01},

journal = {Astrophys. J.},

volume = {393},

pages = {357--372},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ca05800e,

title = {The abundance and distribution of water vapor in the Jovian troposphere as inferred from Voyager IRIS observations},

author = {B. E. Carlson and A. A. Lacis and W. B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/08/1992_Carlson_ca05800e.pdf, Download file},

doi = {10.1086/171182},

year  = {1992},

date = {1992-01-01},

urldate = {1992-01-01},

journal = {Astrophys. J.},

volume = {388},

pages = {648--668},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ro03400p,

title = {Cloud-tracked winds from Pioneer Venus OCPP images},

author = {W. B. Rossow and A. D. Del Genio and T. Eichler},

url = {https://www.williambrossow.com/wp-content/uploads/2022/08/1990_Rossow_ro03400p.pdf},

doi = {10.1175/1520-0469(1990)047%3C2053%3ACTWFVO%3E2.0.CO;2},

year  = {1990},

date = {1990-01-01},

urldate = {1990-01-01},

journal = {J. Atmos. Sci.},

volume = {47},

pages = {2053--2084},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{de00200p,

title = {Planetary-scale waves and the cyclic nature of cloud top dynamics on Venus},

author = {A. D. Del Genio and W. B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/08/1990_DelGenio_de00200p.pdf, Download file},

doi = {10.1175/1520-0469(1990)047%3C0293%3APSWATC%3E2.0.CO;2},

year  = {1990},

date = {1990-01-01},

urldate = {1990-01-01},

journal = {J. Atmos. Sci.},

volume = {47},

pages = {293--318},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ca05700m,

title = {Cloud microphysics of the giant planets},

author = {B. E. Carlson and W. B. Rossow and G. S. Orton},

url = {https://www.williambrossow.com/wp-content/uploads/2022/08/1988_Carlson_ca05700m.pdf, Download file},

doi = {10.1175/1520-0469(1988)045%3C2066%3ACMOTGP%3E2.0.CO;2},

year  = {1988},

date = {1988-01-01},

urldate = {1988-01-01},

journal = {J. Atmos. Sci.},

volume = {45},

pages = {2066--2081},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ca00700d,

title = {Cloud chemistry on Jupiter},

author = {B. E. Carlson and M. J. Prather and W. B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/08/1987_Carlson_ca00700d.pdf, Download file},

doi = {10.1086/165751},

year  = {1987},

date = {1987-01-01},

urldate = {1987-01-01},

journal = {Astrophys. J.},

volume = {322},

pages = {559--572},

keywords = {CLOUD PROPERTIES, PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ca01700z,

title = {The role of aqueous chemistry in determining the composition and cloud structure of the upper troposphere on Uranus},

author = {B. E. Carlson and M. J. Prather and W. B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/08/1987_Carlson_ca01700z.pdf, Download file},

doi = {10.1086/185013},

year  = {1987},

date = {1987-01-01},

urldate = {1987-01-01},

journal = {Astrophys. J.},

volume = {321},

pages = {L97--L101},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ro06300n,

title = {A general circulation model of a Venus-like atmosphere},

author = {W. B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/03/1983_Rossow_ro06300n.pdf, Download file},

doi = {10.1175/1520-0469(1983)040%3C0273%3AAGCMOA%3E2.0.CO;2},

year  = {1983},

date = {1983-01-01},

urldate = {1983-01-01},

journal = {J. Atmos. Sci.},

volume = {40},

pages = {273--302},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{de08100v,

title = {Temporal variability of ultraviolet cloud features in the Venus stratosphere},

author = {A. D. Del Genio and W. B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/03/1982_DelGenio_de08100v.pdf, Download file},

doi = {10.1016/0019-1035(82)90091-4},

year  = {1982},

date = {1982-01-01},

urldate = {1982-01-01},

journal = {Icarus},

volume = {51},

pages = {391--415},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ro04300u,

title = {Comments on a three-dimensional model of dynamical processes in the Venus atmosphere},

author = {W. B. Rossow and S. B. Fels and P. H. Stone},

url = {https://www.williambrossow.com/wp-content/uploads/2022/08/1980_Rossow_ro04300u.pdf, Download file},

doi = {10.1175/1520-0469(1980)037%3C0250%3ACOTDMO%3E2.0.CO;2},

year  = {1980},

date = {1980-01-01},

urldate = {1980-01-01},

journal = {J. Atmos. Sci.},

volume = {37},

pages = {250--252},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ro03300x,

title = {Cloud morphology and motions from Pioneer Venus images},

author = {W. B. Rossow and A. D. Del Genio and S. S. Limaye and L. D. Travis and P. H. Stone},

url = {https://www.williambrossow.com/wp-content/uploads/2022/03/Cloud_morphology_and_motions_from_Pioneer_Venus_im.pdf, Download file},

doi = {10.1029/JA085iA13p08107},

year  = {1980},

date = {1980-01-01},

urldate = {1980-01-01},

journal = {J. Geophys. Res.},

volume = {85},

pages = {8107--8128},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{tr01000b,

title = {Cloud images from the Pioneer Venus orbiter},

author = {L. D. Travis and D. L. Coffeen and A. D. Del Genio and J. E. Hansen and K. Kawabata and A. A. Lacis and W. A. Lane and S. S. Limaye and W. B. Rossow and P. H. Stone},

url = {https://www.williambrossow.com/wp-content/uploads/2022/03/1979_Travis_tr01000b.pdf, Download file},

doi = {10.1126/science.205.4401.74},

year  = {1979},

date = {1979-01-01},

urldate = {1979-01-01},

journal = {Science},

volume = {205},

pages = {74--76},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ro02300a,

title = {Large-scale motion in the Venus stratosphere},

author = {W. B. Rossow and G. P. Williams},

url = {https://www.williambrossow.com/wp-content/uploads/2022/03/1979_Rossow_ro02300a.pdf, Download file},

doi = {10.1175/1520-0469(1979)036%3C0377%3ALSMITV%3E2.0.CO;2},

year  = {1979},

date = {1979-01-01},

urldate = {1979-01-01},

journal = {J. Atmos. Sci.},

volume = {36},

pages = {377--389},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{nokey,

title = {Cloud microphysics: Analysis of the clouds of Earth, Venus, Mars, and Jupiter. },

author = {W.B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/01/1978_Rossow_ro01300e-2.pdf, Download file},

doi = {10.1016/0019-1035(78)90072-6},

year  = {1978},

date = {1978-10-01},

urldate = {1978-10-01},

journal = {Icarus},

volume = {36},

number = {1},

pages = {1-10},

abstract = {A simple method of deducing the probable microphysics of a cloud is developed that uses only information about cloud particle mean size, composition, number density, and atmospheric structure. This analysis is applied to the sulfuric acid clouds of Venus, the water ice and dust clouds of Mars, and the ammonia-water and ammonia ice clouds of Jupiter. The Venus cloud layer most closely resembles smog and haze layers on Earth with no sharp concentration gradients. The cloud microphysics is dominated by coagulation, sedimentation, and turbulent mixing. No precipitation is formed. The water ice clouds on Mars resemble tenuous, nonprecipitating cirrus clouds on Earth. Deposition of condensed water on Mars only occurs from surface fogs or direct condensation on the surface. These fogs can provide a very efficient dust deposition mechanism. The observed settling behavior of the great dust storm of 1971 suggests sedimentation at the surface from a turbulent cloud with coagulation growth of large particles to replace those lost by sedimentation, analogous to the nighttime evolution of submicron tropospheric aerosols on Earth. The ammonia-water and ammonia ice clouds on Jupiter produce precipitation on time scales \<104 sec. The vertical structure of all clouds is significantly altered. The activity of the lower ammonia-water cloud has significant effects on the vertical distribution of other gases and aerosols, on the vertical transport of heat, and on the dynamics in this portion of the atmosphere.},

keywords = {AEROSOLS, CLOUD PROPERTIES, PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ro09200l,

title = {The clouds of Venus: II. An investigation of the influence of coagulation on the observed droplet size distribution},

author = {W. B. Rossow},

url = {https://www.williambrossow.com/wp-content/uploads/2022/03/1977_Rossow_ro09200l.pdf, Download file},

doi = {10.1175/1520-0469(1977)034%3C0417%3ATCOVIA%3E2.0.CO;2},

year  = {1977},

date = {1977-01-01},

urldate = {1977-01-01},

journal = {J. Atmos. Sci.},

volume = {34},

pages = {417--431},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{ro00300h,

title = {The clouds of Venus: I. An approximate technique for treating the effects of coagulation, sedimentation and turbulent mixing on an aerosol},

author = {W. B. Rossow and P. J. Gierasch},

url = {https://www.williambrossow.com/wp-content/uploads/2022/03/1977_Clouds0fVenus...Rossow_ro00300h.pdf, Download File},

doi = {10.1175/1520-0469(1977)034%3C0405%3ATCOVIA%3E2.0.CO;2},

year  = {1977},

date = {1977-01-01},

urldate = {1977-01-01},

journal = {J. Atmos. Sci.},

volume = {34},

pages = {405--416},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}

@article{nokey,

title = {Microwave boundary conditions on the atmosphere and clouds of Venus},

author = {W.B. Rossow and C. Sagan},

url = {https://www.williambrossow.com/wp-content/uploads/2022/01/1975_Rossow_ro08200o-1.pdf, Download file},

doi = {10.1175/1520-0469(1975)032%3C1164%3AMBCOTA%3E2.0.CO;2},

year  = {1975},

date = {1975-06-01},

urldate = {1975-06-01},

journal = { Journal of the Atmospheric Sciences},

volume = {32},

number = {6},

pages = {1164-1176.},

abstract = {The dielectric properties of H2O and H2SO4 at microwave frequencies have been calculated from the Debye equations. The derived frequency and temperature dependence agrees wed with existing data. The dielectric properties of H2O/H2SO4 mixtures are deduced and, for a well-mixed atmosphere, the structure of H2O and H2O/H2SO4 clouds is calculated. With the COSPAR model atmosphere and the calculated cloud models, the microwave properties of the atmosphere and clouds are determined. The 3.8 cm radar reflectivity of the planet, the Mariner 5 S-band occultation profile, and the passive microwave emission spectrum of the planet together set an upper limit on the mixing ratio by number of H2O of ∼102 in the lower Venus atmosphere, and of H2SO4 of ∼10−5. The polarization value of the real part of the refractive index of the clouds, the spectroscope limits on the abundance of water vapor above the clouds, and the microwave data together set corresponding upper limits on H2O of ∼2 × 10−4 and on H2SO4 of ∼9 × 10−6. Upper limits on the surface density of total cloud constituents and of cloud liquid water are, respectively, ∼0.1 g cm−2 and ∼0.01 g cm−2. The infrared opacities of 90 bars of CO2, together with the derived upper limits to the amounts of water vapor and liquid H2O/H2SO4, may be sufficient to explain the high surface temperatures through the greenhouse effect.},

keywords = {PLANETARY ATMOSPHERES},

pubstate = {published},

tppubtype = {article}

}