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  • 1
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    In:  Phil. Trans. Roy. Soc. London, Hannover, Dt. Geophys. Ges. e. V., vol. A211, no. B11, pp. 163-198, pp. L06304, (ISBN: 0534351875, 2nd edition)
    Publication Date: 1920
    Keywords: Review article ; Rock mechanics ; Rheology ; Fracture ; cracks and fractures (.NE. fracturing)
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  • 2
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    In:  Phil. Trans. Roy. Soc., London, Dt. Geophys. Ges. e. V., vol. A221, no. B11, pp. 163-198, pp. L06304, (ISBN: 0534351875, 2nd edition)
    Publication Date: 1921
    Keywords: Rock mechanics ; cracks and fractures (.NE. fracturing) ; Fracture ; Rheology
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  • 3
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    In:  Bull. Seism. Soc. Am., London, Dt. Geophys. Ges. e. V., vol. 95, no. 4, pp. 1263-1275, pp. L06304, (ISBN: 0534351875, 2nd edition)
    Publication Date: 2005
    Keywords: Seismology ; Strain ; Geodesy ; Crustal deformation (cf. Earthquake precursor: deformation or strain) ; Fault zone ; Structural geology ; BSSA
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  • 4
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    In:  Proc. 1st. Int. Congr. Appl. Mech., Zurich and Glattbrugg, Electrowatt Eng. & GeoSys (Switzerland), vol. 10, no. GL-TR-89-0157, pp. 54-63, (ISBN 3-933346-037)
    Publication Date: 1924
    Keywords: Rock mechanics ; Fracture ; cracks and fractures (.NE. fracturing)
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  • 5
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    Society of Petroleum Engineers
    In:  Paper 24050 presented at the Western Regional Meeting of SPE, Bakersfield, Society of Petroleum Engineers, vol. 10, no. 421, pp. 1-24, (ISBN 3-933346-037)
    Publication Date: 1992
    Keywords: Borehole geophys. ; Borehole Compensated Sonic log
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  • 6
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    Society of Petroleum Engineers
    In:  Technical Paper presented at the SPE Asia Pacific Oil and Gas Conf., Melbourne, Society of Petroleum Engineers, vol. 1, no. paper SPWLA 90-C, pp. M1-M4, (ISBN 3-933346-037)
    Publication Date: 1994
    Keywords: Applied geophysics ; Borehole geophys. ; Data analysis / ~ processing
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  • 7
    Publication Date: 2011-08-24
    Description: It is often argued that substantially more carbon dioxide and water were degassed from the martian interior than can be found at present in the atmosphere, polar caps and regolith. Calculations have shown that atmospheric escape cannot account for all of the missing volatiles. Suggestions that carbon dioxide is stored as marine or lacustrine deposits, are challenged by Earth-based and spacecraft remote-sensing data. Moreover, recent modelling of the martian atmosphere suggests that rainfall or open bodies of water are in any case unlikely to have persisted for extended periods of time. Hydrothermal carbonates therefore provide a possible solution to this dilemma. Using an accessible terrestrial system (Iceland) as a guide to the underlying processes, and a host rock composition inferred from the least-altered martian meteorite, we present a geochemical model for the formation of carbonates in possible martian hydrothermal systems. Our results suggest that an extensive reservoir of carbonate minerals--equivalent to an atmospheric pressure of carbon dioxide of at least one bar--could have been sequestered beneath the surface by widespread hydrothermal activity in the martian past.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Nature (ISSN 0028-0836); Volume 377; 6548; 406-8
    Format: text
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  • 8
    Publication Date: 2011-08-24
    Description: The National Aeronautics and Space Administration (NASA) Infrared Telescope Facility was used to investigate the collision of comet Shoemaker-Levy 9 with Jupiter from 12 July to 7 August 1994. Strong thermal infrared emission lasting several minutes was observed after the impacts of fragments C, G, and R. All impacts warmed the stratosphere and some the troposphere up to several degrees. The abundance of stratospheric ammonia increased by more than 50 times. Impact-related particles extended up to a level where the atmospheric pressure measured several millibars. The north polar near-infrared aurora brightened by nearly a factor of 5 a week after the impacts.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Science (ISSN 0036-8075); Volume 267; 5202; 1277-82
    Format: text
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  • 9
    Publication Date: 2011-08-24
    Description: We have reanalyzed the Voyager radio occultation data for Titan, examining two alternative approaches to methane condensation. In one approach, methane condensation is facilitated by the presence of nitrogen because nitrogen lowers the condensation level of a methane/nitrogen mixture. The resulting enhancement in methane condensation lowers the upper limit on surface relative humidity of methane obtained from the Voyager occultation data from 0.7 to 0.6. We conclude that in this case the surface relative humidity of methane lies between 0.08 and 0.6, with values close to 0.6 indicated. In the other approach, methane is allowed to become supersaturated and reaches 1.4 times saturation in the troposphere. In this case, surface humidities up to 100% are allowed by the Voyager occultation data, and thus the upper limit must be set by other considerations. We conclude that if supersaturation is included, then the surface relative humidity of methane can be any value greater than 0.08--unless a deep ocean is present, in which case the surface relative humidity is limited to less than 0.85. Again, values close to 0.6 are indicated. Overall, the tropospheric lapse rate on Titan appears to be determined by radiative equilibrium. The lapse rate is everywhere stable against dry convection, but is unstable to moist convection. This finding is consistent with a supersaturated atmosphere in which condensation-and hence moist convection-is inhibited.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Icarus (ISSN 0019-1035); Volume 129; 2; 498-505
    Format: text
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  • 10
    Publication Date: 2011-08-24
    Description: A study was conducted to (1) determine the feasibility of design and fabrication of a low pass filter with a relatively sharp cut-on at higher wavelengths (i.e. 30-40 microns), using metallic mesh technique; and (2) investigate whether the combination of this filter and a suitable IR detector, as a part of a Lunar Observer (LO) horizon sensor, is capable of detecting radiation emanating from two blackbody sources kept at temperatures simulating space and the surface temperature of dark or lit sides of the moon. Various designs of multilayer metallic mesh filters with different mesh parameters and substrate thicknesses were simulated. Using mesh parameters corresponding to the optimum four-layer filter design, a filter was fabricated on a 6.35 micron thick mylar substrate. The transmission curve of the fabricated filter is very close to what the simulation predicted. Room temperature signal level tests were performed on the combination of filter-detector assemblies. The data obtained from these tests indicate that the assembly can detect temperature differences as low as few degrees K between two black bodies.
    Keywords: SPACECRAFT INSTRUMENTATION
    Type: In: Infrared technology XVII; Proceedings of the Meeting, San Diego, CA, July 22-26, 1991 (A93-38376 15-35); p. 764-774.
    Format: text
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