NASA Technical TranslationNational Aeronautics and Space Administration, 1970 |
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according albedo APPENDIX cont'd Astrometry Astron Band 12 Band Dark Band Band Light Band Barabashov brightness coefficient brightness distribution Bugayenko calculations caps of Mars central meridian Characteristics of Details CONTINUATION OF TABLE craters curve Dark Band Dark Dark Band Light Dark Detail Dark Region decrease Details Identification determined disk Earth's atmosphere Equatorial equivalent width error Following Dark Band Following Light Band Formations formula I.K. Koval Identification with Constant intensity equator interval Jupiter kOhm Light Band 13 Light Band Dark Light Band Light Light Region longitude luminous fluxes lunar lunar surface maria Mars atmosphere Mars observations measured methane absorption Moon N-Polar Region obtained optical optical thickness Overlapping of Dark Overlapping of Light phase angle photographic photometric photomultiplier polar cap pulse ridges Section Sharp Band signal slopes spectral region spectrograms spherical tion Tropical Dark Band Ukrainian S.S.R. values
Populære passager
Side 60 - the 70-cm reflector of the Main Astronomical Observatory of the Academy of Sciences of the Ukrainian SSR was
Side 91 - The effect of the width of the slit used in determining the vibrational disk on the atmospheric vibration (instrumental function) is estimated for the case when the latter is a Gaussian function. It is shown that a rather narrow slit does not effect the instrumental function.
Side 76 - This assumes that the layer of snow occupies approximately 25% of the area of the cap. Using a value of 2 cm for the thickness of the snow layer, the amount of precipitable water is found to be equal to
Side 76 - long-term photometric investigations. The amount of water on Mars is estimated. The substance forming the polar caps is assumed to be concentrated on the Mars surface, and seems to be a discontinuous layer of snow with neutral albedo equal to
Side 119 - of the 6190 A band are smaller for the edge zones of the Jupiter disk than for the center. The difference between the equivalent widths is 5-6 A. The variations change substantially from the edges to the center.
Side 119 - It is shown that the value of the methane absorption for the center of the disk of Jupiter changed during different periods of observations. The greatest variations in intensity of absorption are found for longitudes of 190-320°.
Side 56 - Photometric data on the contrasts between the highlands and maria of Mars, measured in different spectral regions, are analyzed. The optical parameters of the Mars atmosphere are determined. Some assumptions on the behavior of the true
Side 75 - the Book: Rezul'taty nablyudeniy Marsa vo vremya velikogo protivostoyaniya 1956 g. v SSSR (Results of
Side 119 - The results of measurements of the methane absorption in the 6190 A band along the disk of Jupiter are given. The data were taken from 52 spectrograms, which were obtained in
Side 153 - It is shown that, during the period of observations, the absorption in the 6190 'A methane band was stable at the center of the Saturn disk, and equal to 25-27