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  • 1
    Publication Date: 2011-08-16
    Description: Venus atmosphere and surface conditions, describing temperature, accumulation of carbon dioxide and runaway greenhouse effect
    Keywords: SPACE SCIENCES
    Type: ; 17 (
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  • 2
    Publication Date: 2011-08-16
    Description: The basic elements of the physical ephemeris of Mars are reexamined, and the new values adopted for the Mariner 9 mapping are specified, in particular, for the direction of the spin axis and the first meridian.
    Keywords: SPACE SCIENCES
    Type: Journal of Geophysical Research; 78; July 10
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  • 3
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    In:  Other Sources
    Publication Date: 2019-06-27
    Description: The most important feature of the extended sources is the double structure characterized in an ideal model by two extended radio-emitting regions situated symmetrically about the nucleus of an optical galaxy or QSO, with a characteristic overall size of about 100 kpc. Not all extended radio sources show this double structure. It has been found that at moderate resolutions about 20% of the well-resolved sources have a core-halo structure. Theoretical proposals for the containment of extended double sources have so far relied either upon self-gravitation of the ejected material or upon assuming the existence of a gaseous intergalactic medium. The advantages and the problems of a model proposed by Burbidge (1967) are discussed, together with the nuclear event serving to release the energy required to make an extended radio source.
    Keywords: SPACE SCIENCES
    Type: Comments on Modern Physics; vol. 5
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  • 4
    Publication Date: 2019-06-27
    Description: Studies of sudden disintegrations of filaments in solar cycles 19 and 20 (to 1969) indicate that such events occur frequently. Approximately 30% of all large filaments in these cycles disintegrated in the course of their transit across the solar disk. 'Major' flares occurred with above average frequency on the last day on which 141 large disappearing filaments were observed. Relationships between a disintegrating filament on July 10-11, 1959, a prior major flare, a newly formed spot, and concomitant growth of H-alpha plage are presented. Observation of prior descending prominence material apparently directed towards the location of the flare of July 15, 1959 is reported. The development of the filament-associated flare of Feb. 13, 1967 is described.
    Keywords: SPACE SCIENCES
    Type: Solar Physics; 23; Apr. 197
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  • 5
    Publication Date: 2019-06-27
    Description: It is shown that a precursor type IIIb burst is really associated with a type III burst. The broad longitude distribution of the occurrence of type IIIb bursts also suggests that these bursts are emitted at a large angle to the open magnetic field in the corona.
    Keywords: SPACE SCIENCES
    Type: Solar Physics; 37; July 197
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  • 6
    Publication Date: 2019-06-27
    Description: Venus atmospheric turbulence from Venera 4, 5, 6 and Mariner 5 observations, discussing scaling laws and normalized signal-amplitude standard deviation
    Keywords: SPACE SCIENCES
    Type: ; YSICA STATUS SOLIDI
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  • 7
    Publication Date: 2019-06-27
    Description: Microwave signal fading in Venus atmosphere due to turbulence, discussing atmospheric dielectric permittivity variance
    Keywords: SPACE SCIENCES
    Type: ; ADEMIE DES SCIENCES
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  • 8
    Publication Date: 2019-06-27
    Description: The observed strengths of interstellar absorption lines of Fe II and Mn II in the spectra of alpha Vir, beta Cen, pi Sco, and zeta Oph along with laboratory f values of some of these lines between 2343 and 2606 A have been used to determine curves of growth for these ions and the f-values of ten lines of Fe II and three lines of Mn II between 1055 and 1261 A. The Fe and Mn abundances are derived.
    Keywords: SPACE SCIENCES
    Type: Astronomy and Astrophysics; 31; 4, Ap; Apr. 197
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  • 9
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    In:  Other Sources
    Publication Date: 2019-06-27
    Description: In attempts to reconstruct the environment of condensation of solar system materials, particularly exemplified by certain meteorite components, the relative temperatures of the gas and the solid are of critical importance. The relationships that determine the heat balance in a circumsolar grain-gas system are examined. Fundamental considerations show that regardless of opacity or gas density, the gas will always be at a higher temperature than the solid in such regions of the system where condensation is possible. Implications of the characteristic temperature differential between the gas and the condensing solid are discussed.
    Keywords: SPACE SCIENCES
    Type: Meteorities; 8; Dec. 31
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  • 10
    Publication Date: 2019-07-13
    Description: Theoretical studies and observations of interstellar dust are described in papers dealing with the passive properties of dust grains, their physical and chemical activities in the interstellar medium, and their interactions in association with stars. The papers are grouped according to the principal topics of (1) extinction and polarization, (2) diffuse interstellar features, (3) dust around and in close association with stars, (4) reflection nebulae and other aspects of dust scattering properties, (5) alignment mechanisms, (6) distribution of molecules and processes of molecule formation, (7) radiation effects on dust, (8) physical and chemical interactions of dust with the ambient medium, and (9) gas and dust in H II regions. Individual items are announced in this issue.
    Keywords: SPACE SCIENCES
    Type: Symposium on Interstellar Dust and Related Topics; May 29, 1972 - Jun 02, 1972; Albany, NY; US
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