On Io, all that flickers is not cold

The 4.8 micron flux from the Galilean satellite Io was shown to fluctuate with an amplitude of approximately 10 percent on time scales of every 28 seconds, 40 minutes, night-to-night, and perhaps year-to-year. Such behavior was found to be the result of random fluctuations for which the mean square fluctuation varies inversely with frequency for constant bandwidth measurement. The theory developed for thermionic emission from barium oxide cathodes in vacuum tubes might be applicable to this situation. If so, the fluctuations in the flux from Io's volcanoes may be caused by diffusion of hot convective cells onto the surface of Io. Long term fluctuations may furnish a means by which the Io volcanism can shut down and conserve energy. Thus the discrepancy that exists between measurements of the current heat flow from Io and calculations of tidal dissipation may be resolved. Tests for rapid flickering at 10 microns showed no fluctuations greater than one percent. This agrees with the prediction of the flow model theory in which the 10 microns volcanic thermal emission arises from cooling of old flows

Determination of the Io heat flow. 1: Eclipse observations

The thermal emission from Io during eclipse by Jupiter yields data from which the total thermal flux from the volcanoes on the satellite surface can be estimated. Thermal infrared observations in spectral bands between 3.5 and 30 microns of five Io eclipse reappearances and one eclipse disappearance are reported and discussed. The thermal emission of the volcanoes which occurs almost all of the time was determined from the Io heat flux data. The thermal observations of Io are discussed with respect to previous thermophysical theories

High resolution imaging of the Venus night side using a Rockwell 128x128 HgCdTe array

The University of Hawaii operates an infrared camera with a 128x128 HgCdTe detector array on loan from JPL's High Resolution Imaging Spectrometer (HIRIS) project. The characteristics of this camera system are discussed. The infrared camera was used to obtain images of the night side of Venus prior to and after inferior conjunction in 1988. The images confirm Allen and Crawford's (1984) discovery of bright features on the dark hemisphere of Venus visible in the H and K bands. Our images of these features are the best obtained to date. Researchers derive a pseudo rotation period of 6.5 days for these features and 1.74 microns brightness temperatures between 425 K and 480 K. The features are produced by nonuniform absorption in the middle cloud layer (47 to 57 Km altitude) of thermal radiation from the lower Venus atmosphere (20 to 30 Km altitude). A more detailed analysis of the data is in progress

Age Progressive Volcanism Opposite Nazca Plate Motion: Insights from Seamounts and Drowned Islands on the Northeastern Margin of the Galápagos Platform

Highlights • Four of the seven seamounts northeast of the Galápagos Platform are drowned islands • The ages of the seamounts range from 5.2 Ma to 0.5 Ma • Seamount morphology changes from conical to elongate at ~1.5 Ma • The locus of volcanism appears to migrate eastward at the rate of Nazca plate motion Abstract We present new geochemical and 40Ar/39Ar analyses from seven seamounts located off the northeastern margin of the shallow Galápagos Platform. Initial volcanism at 5.2 Ma created a small island (Pico) over the current location of the hotspot with geochemically enriched lavas. There is no further record of magmatism in the study area until 3.8 to 2.5 Ma, during which four roughly conical volcanoes (Sunray, Grande, Fitzroy, and Beagle) formed through eruption of lavas derived from a depleted mantle source. Sunray, Fitzroy, and Grande were islands that existed for ~3 m.y. ending with the submergence of Fitzroy at ~0.5 Ma. The youngest seamounts, Largo and Iguana, do not appear to have been subaerial and were active at 1.3 Ma and 0.5 Ma, respectively, with the style of edifice changing from the previous large cones to E-W elongate, composite structures. The progression of magmatism suggests that Pico erupted near 91.5°W near the location of the Galápagos plume while the others formed well east of the plume center. If the locations of initial volcanism are calculated using the eastward velocity of the Nazca plate, there appears to be a progression of younger volcanism toward the east, opposite what would be expected from a fixed mantle plume source. The rate that initial volcanism moves eastward is close to the plate velocity. A combination of higher temperature and geochemical enrichment of the thickened lithosphere of the Galápagos platform could have provided a viscosity gradient at the boundary between the thick lithosphere and the thinner oceanic lithosphere to the northeast. As this boundary moved eastward with the Nazca plate, it progressively triggered shear-driven mantle upwelling and volcanism

5-micron photometry of late-type dwarfs

We present narrowband-M photometry of nine low-mass dwarfs with spectral types ranging from M2.5 to L0.5. Combining the (L'-M') colours derived from our observations with data from the literature, we find colours consistent with a Rayleigh-Jeans flux distribution for spectral types earlier than M5, but enhanced F_3.8/F_4.7 flux ratios (negative (L'-M') colours) at later spectral types. This probably reflects increased absorption at M' due to the CO fundamental band. We compare our results against recent model predictions and briefly discuss the implications.Comment: accepted for the Astronomical Journa

NMR imaging and hydrodynamic analysis of neutrally buoyant non-Newtonian slurry flows

The flow of solids loaded suspension in cylindrical pipes has been the object of intense experimental and theoretical investigations in recent years. These types of flows are of great interest in chemical engineering because of their important use in many industrial manufacturing processes. Such flows are for example encountered in the manufacture of solid-rocket propellants, advanced ceramics, reinforced polymer composites, in heterogenous catalytic reactors, and in the pipeline transport of liquid-solids suspensions. In most cases, the suspension microstructure and the degree of solids dispersion greatly affect the final performance of the manufactured product. For example, solid propellant pellets need to be extremely-well dispersed in gel matrices for use as rocket engine solid fuels. The homogeneity of pellet dispersion is critical to allow good uniformity of the burn rate, which in turn affects the final mechanical performance of the engine. Today`s manufacturing of such fuels uses continuous flow processes rather than batch processes. Unfortunately, the hydrodynamics of such flow processes is poorly understood and is difficult to assess because it requires the simultaneous measurements of liquid/solids phase velocities and volume fractions. Due to the recent development in pulsed Fourier Transform NMR imaging, NMR imaging is now becoming a powerful technique for the non intrusive investigation of multi-phase flows. This paper reports and exposes a state-of-the-art experimental and theoretical methodology that can be used to study such flows. The hydrodynamic model developed for this study is a two-phase flow shear thinning model with standard constitutive fluid/solids interphase drag and solids compaction stresses. this model shows good agreement with experimental data and the limitations of this model are discussed

24. GEOMAGNETIC-FIELD VARIATIONS RECORDED WITHIN DRILL PIPE AT SITE 865: IMPLICATIONS FOR PALEOMAGNETIC STUDIES 1

ABSTRACT In this study, we measured the magnetic field within the drill string with a wireline magnetometer log and estimated the effect that this magnetic-field might have on paleomagnetic core samples. Sharp decreases in the vertical magnetic-field component and sharp increases in the horizontal component were observed at approximately 10-m intervals, corresponding to the pipe joints. Induced magnetization by the greater thicknesses of iron at these connection points apparently causes the magnetic-field variations. The bottom-hole assembly of the drill string was dominated by induced magnetization and possibly was affected by permanent magnetization. In general, the magnetic-field throughout most of the drill pipe and bottom-hole assembly is only two to five times greater than the Earth's magnetic field at Site 865 and so is not likely to affect paleomagnetic samples. However, the magnetometers vertical sensor became saturated in a downward direction between 344 and 356 m below the rig floor at Site 865, suggesting negative inclination of a strong permanent magnetization of two pipes within this zone. Such a strong magnetic field is a likely cause of remagnetization of core samples

28. STRUCTURAL IMPLICATIONS OF GRAVITY ANOMALIES, RESOLUTION AND HEEZEN GUYOTS, MID-PACIFIC MOUNTAINS 1

ABSTRACT Drilling showed that carbonate rocks make up most of Resolution Guyot, located in the western Mid-Pacific Mountains. Density data from Hole 866A, in the top of the guyot, were used to calculate a forward model of the gravity anomaly caused by the guyot's topography. After this anomaly was subtracted from the observed free-air anomaly, a significant positive residual, 35 mGal in amplitude, remained. The same densities were used for nearby Heezen Guyot, which yielded a similar, 45 mGal residual. Inverse models of the Resolution Guyot residual indicate that most of the mass excess can be attributed to the contrast between surrounding sediments and the dolomites at the bottom of the guyot's limestone section and the basalt pedestal beneath the guyot. Nevertheless, models with a central mass concentration fit the residual significantly better than those without, suggesting that there may be either a buried, conical, seamount remanent in the center of the guyot or a central conduit with dense intrusive rocks. The latter seems more plausible because seismic reflection profiles show no evidence of a buried conical structure. In addition, models with bottoms below the predicted top of the underlying basaltic plateau give more plausible density contrasts, suggesting that either a dense zone exists within the plateau beneath the guyot or that the extrapolated depth to the plateau top is incorrect by 500 m to 1000 m. The Resolution Guyot models imply that the carbonate bank buried a small seamount or igneous pedestal and retained nearly the same shape and width. Although the Heezen Guyot residual anomaly was not explicitly modeled, it is similar to that of Resolution Guyot and implies an analogous subsurface structure. In contrast, the Heezen Guyot residual is located to the west side of that edifice and does not have the same elongated shape as the guyot. Thus, it appears that the carbonate bank of Heezen Guyot expanded eastward from its pedestal