Search Results - "Tomasko, M.G."

Limits on the size of aerosols from measurements of linear polarization in Titan’s atmosphere by Tomasko, M.G., Doose, L.R., Dafoe, L.E., See, C.

“…The Descent Imager/Spectral Radiometer (DISR) instrument on the Huygens probe into the atmosphere of Titan yielded information on the size, shape, optical…”
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A model of Titan's aerosols based on measurements made inside the atmosphere by Tomasko, M.G., Doose, L., Engel, S., Dafoe, L.E., West, R., Lemmon, M., Karkoschka, E., See, C.

“…The descent imager/spectral radiometer (DISR) instrument aboard the Huygens probe into the atmosphere of Titan measured the brightness of sunlight using a…”
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Heat balance in Titan's atmosphere by Tomasko, M.G., Bézard, B., Doose, L., Engel, S., Karkoschka, E., Vinatier, S.

“…The recent measurements of the vertical distribution and optical properties of haze aerosols as well as of the absorption coefficients for methane at long…”
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Measurements of methane absorption by the descent imager/spectral radiometer (DISR) during its descent through Titan's atmosphere by Tomasko, M.G., Bézard, B., Doose, L., Engel, S., Karkoschka, E.

“…New low-temperature methane absorption coefficients pertinent to the Titan environment are presented as derived from the Huygens DISR spectral measurements…”
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Latitudinal variations in Titan’s methane and haze from Cassini VIMS observations by Penteado, Paulo F., Griffith, Caitlin A., Tomasko, Martin G., Engel, Steffi, See, Charles, Doose, Lyn, Baines, Kevin H., Brown, Robert H., Buratti, Bonnie J., Clark, Roger, Nicholson, Phillip, Sotin, Christophe

“…We analyze observations taken with Cassini’s Visual and Infrared Mapping Spectrometer (VIMS), to determine the current methane and haze latitudinal…”
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The properties of Titan's surface at the Huygens landing site from DISR observations by Keller, H.U., Grieger, B., Küppers, M., Schröder, S.E., Skorov, Y.V., Tomasko, M.G.

“…The descent imager/spectral radiometer (DISR) onboard the Huygens probe investigated the radiation balance inside Titan's atmosphere and took hundreds of…”
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Results from the Mars Pathfinder Camera by Smith, P. H., Bell, J. F., Bridges, N. T., Britt, D. T., Gaddis, L., Greeley, R., Keller, H. U., Herkenhoff, K. E., Jaumann, R., Johnson, J. R., Kirk, R. L., Lemmon, M., Maki, J. N., Malin, M. C., Murchie, S. L., Oberst, J., Parker, T. J., Reid, R. J., Sablotny, R., Soderblom, L. A., Stoker, C., Sullivan, R., Thomas, N., Tomasko, M. G., Ward, W., Wegryn, E.

“…Images of the martian surface returned by the Imager for Mars Pathfinder (IMP) show a complex surface of ridges and troughs covered by rocks that have been…”
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Solar and Thermal Radiation in Jupiter's Atmosphere: Initial Results of the Galileo Probe Net Flux Radiometer by Sromovsky, L. A., Best, F. A., Collard, A. D., Fry, P. M., Revercomb, H. E., Freedman, R. S., Orton, G. S., Hayden, J. L., Tomasko, M. G., Lemmon, M. T.

“…The Galileo probe net flux radiometer measured radiation within Jupiter's atmosphere over the 125-kilometer altitude range between pressures of 0.44 bar and 14…”
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On the optical studies of the atmospheric water vapour from the surface of Mars by Titov, D.V, Markiewicz, W.J, Thomas, N, Keller, H.U, Tomasko, M.G, Lemmon, M, Smith, P.H

“…Remote observations of the atmospheric water vapour from the Mars orbit were usually carried out to study its global distribution and variability. Measurements…”
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