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  • LUNAR AND PLANETARY EXPLORATION  (12)
  • ACM6; ACM6_1125; Current direction; Current velocity, east-west; Current velocity, horizontal; Current velocity, north-south; DATE/TIME; DEPTH, water; MOOR; Mooring; Pressure, water; Recording current meter, Aanderaa Data Instruments, RCM5; Salinity; Temperature, water; WOCE; World Ocean Circulation Experiment  (4)
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  • 1
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    PANGAEA
    Publikationsdatum: 2023-02-24
    Schlagwort(e): ACM6; ACM6_1125; Current direction; Current velocity, east-west; Current velocity, horizontal; Current velocity, north-south; DATE/TIME; DEPTH, water; MOOR; Mooring; Pressure, water; Recording current meter, Aanderaa Data Instruments, RCM5; Salinity; Temperature, water; WOCE; World Ocean Circulation Experiment
    Materialart: Dataset
    Format: text/tab-separated-values, 32118 data points
    Standort Signatur Erwartet Verfügbarkeit
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  • 2
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    PANGAEA
    Publikationsdatum: 2023-02-24
    Schlagwort(e): ACM6; ACM6_1125; Current direction; Current velocity, east-west; Current velocity, horizontal; Current velocity, north-south; DATE/TIME; DEPTH, water; MOOR; Mooring; Pressure, water; Recording current meter, Aanderaa Data Instruments, RCM5; Salinity; Temperature, water; WOCE; World Ocean Circulation Experiment
    Materialart: Dataset
    Format: text/tab-separated-values, 32129 data points
    Standort Signatur Erwartet Verfügbarkeit
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  • 3
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    PANGAEA
    Publikationsdatum: 2023-02-24
    Schlagwort(e): ACM6; ACM6_1125; Current direction; Current velocity, east-west; Current velocity, horizontal; Current velocity, north-south; DATE/TIME; DEPTH, water; MOOR; Mooring; Pressure, water; Recording current meter, Aanderaa Data Instruments, RCM5; Salinity; Temperature, water; WOCE; World Ocean Circulation Experiment
    Materialart: Dataset
    Format: text/tab-separated-values, 32207 data points
    Standort Signatur Erwartet Verfügbarkeit
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  • 4
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    PANGAEA
    Publikationsdatum: 2023-02-24
    Schlagwort(e): ACM6; ACM6_1125; Current direction; Current velocity, east-west; Current velocity, horizontal; Current velocity, north-south; DATE/TIME; DEPTH, water; MOOR; Mooring; Pressure, water; Recording current meter, Aanderaa Data Instruments, RCM5; Salinity; Temperature, water; WOCE; World Ocean Circulation Experiment
    Materialart: Dataset
    Format: text/tab-separated-values, 32207 data points
    Standort Signatur Erwartet Verfügbarkeit
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  • 5
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    In:  Other Sources
    Publikationsdatum: 2011-08-19
    Beschreibung: Internal heat flow from radioactive decay in Triton's interior along with absorbed thermal energy from Neptune total 5 to 20 percent of the isolation absorbed by Triton, thus comprising a significant fraction of Triton's surface energy balance. These additional energy inputs can raise Triton's surface temperature between about 0.5 and 1.5 K above that possible with absorbed sunlight alone, resulting in an increase of about a factor of about 1.5 to 2.5 in Triton's basal atmospheric pressure. If Triton's internal heat flow is concentrated in some areas, as is likely, local effects such as enhanced sublimation with subsequent modification of albedo could be quite large. Furthermore, indications of recent global albedo change on Triton suggest that Triton's surface temperature and pressure may not now be in steady state, further suggesting that atmospheric pressure on Triton was as much as ten times higher in the recent past.
    Schlagwort(e): LUNAR AND PLANETARY EXPLORATION
    Materialart: Science (ISSN 0036-8075); 251; 1465-146
    Format: text
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  • 6
    Publikationsdatum: 2011-08-19
    Beschreibung: A global topography is presently calculated for two multilayer Io models in which dissipation occurs in a viscous asthenosphere and a solid mantle: (1) a 'thermal swell' model, in which topography and heat flow are positively correlated, and (2) a 'differentiated lithosphere' model, in which topography and heat flow are negatively correlated. Both the polar topography and the hypsometric distribution of elevations in the differentiated lithosphere model are better matched with observations than the thermal swell model. The shift of the equatorial basin-swell pattern indicates a recent zonal rotation of about 25 deg for Io's lithosphere.
    Schlagwort(e): LUNAR AND PLANETARY EXPLORATION
    Materialart: Icarus (ISSN 0019-1035); 85; 309-325
    Format: text
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  • 7
    Publikationsdatum: 2019-06-28
    Beschreibung: In order to derive models of the interiors of Uranus, Neptune, Jupiter and Saturn, researchers studied equations of state and electrical conductivities of molecules at high dynamic pressures and temperatures. Results are given for shock temperature measurements of N2 and CH4. Temperature data allowed demonstration of shock induced cooling in the the transition region and the existence of crossing isotherms in P-V space.
    Schlagwort(e): LUNAR AND PLANETARY EXPLORATION
    Materialart: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986; p 141-143
    Format: application/pdf
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  • 8
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    In:  Other Sources
    Publikationsdatum: 2019-01-25
    Beschreibung: A model of Io is presented that consists of an elastic inner core, a low strength asthenosphere, and a thin elastic outer shell. The middle layer is ssumed to posses negligible shear strength and to be characterized by a Newtonian viscosity. The fluid in the viscous layer is forced to circulate mainly by the tidal distortion in the outer shell, modeled here as a variation in the distortion amplitude. As a result, heat is generated in the fluid by viscous dissipation. There are three important unconstrained parameters in the model: the fluid viscosity, the thickness of the fluid layer, and the degree to which the distortion of the outer shell is affected by the fluid viscosity. For a wide range of these model parameters viscous heating can generate just as much or even more heat than does elastic dissipation is the outer shell. The model suggests that much of Io's heat flow may be generated below the outer shell and could provide a source of energy for any silicate volcanism on the satellite.
    Schlagwort(e): LUNAR AND PLANETARY EXPLORATION
    Materialart: Lunar and Planetary Inst. Terrest. Planets: Comp. Planetology; p 12
    Format: text
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  • 9
    Publikationsdatum: 2019-06-28
    Beschreibung: Thermal history of Mercury's interior is examined using the model of Stevenson et al. (1983), extended to include the effects of tidal heating in Mercury's solid inner core. The implications of Mercury's thermal history for the source of the planet's magnetic field are discussed. It is shown that the major results of this model are similar to the results obtained with the Stevenson et al. model, except for the addition of inner-core tidal dissipation. It is concluded that the extended model properly characterizes Mercury's internal structure and thermal history, and that the criteria for dynamo generation are not properly satisfied. Alternative explanations, including the possibility of a weak thermoelectric dynamo, are examined.
    Schlagwort(e): LUNAR AND PLANETARY EXPLORATION
    Format: text
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  • 10
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    In:  Other Sources
    Publikationsdatum: 2019-06-28
    Beschreibung: Thermoluminescence (TL) measurements on Allan Hills A77307 (AH), a carbonaceous chondrite found in Antarctica, are compared with those on other chondrite and applied to its classification. Two lithologically different 250-mg samples were ground, freed of magnetic material, and ground again to pass a 100-micron sieve. Aliquots of 4 mg were heated to 500 C, exposed to beta radiation from a Sr-90 source, and heated at a rate of 7.3 C/sec in N2. TL was measured with a photomultiplier tube fitted with thermal and blue filters. Glow curves for AH and for seven other, established CO-type chondrites area presented, all exhibiting two major peaks of TL sensitivity. The peaks for the seven CO-type chondrites are found at 91 + or - 7 C and at 203 + or - 11 C; those for AH at 170 + or - 17 C and at approximately 250 C. This difference is considered significant and not due to random fluctuation or a typical sampling. From this comparison and from consideration of the weathering, preterrestrial-alteration, petrological and compositional evidence on AH, it is concluded that AH is a unique chondrite, possessing both similarities to and differences from the CO class.
    Schlagwort(e): LUNAR AND PLANETARY EXPLORATION
    Materialart: Meteoritics (ISSN 0026-1114); 18; March 31
    Format: text
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