Saturn's E ring: I. CCD observations of March 1980     

W.A. Baum  T. Kreidl  J.A. Westphal  G.E. Danielson  P.K. Seidelmann  D. Pascu  D.G. Currie 《Icarus》1981,47(1):84-96

The tenuous E ring of Saturn is found to commence abruptly at 3 Saturn radii, to peak sharply in the vicinity of the orbit of the satellite Enceladus (about 4 radii), and to spread out thinly to more than 8 radii. This distribution strongly suggests it to be associated with Enceladus and perhaps to be material ejected from Enceladus. The spread of E-ring material above and below the ring plane is greater in its tenuous outskirts than in its denser inner region, suggesting that the E ring may be at an early stage in its evolution. Thus far, our analysis reveals only a marginal variation of the ring with time or Enceladus azimuth. In this paper we describe the special instrumentation used for photometric observations of the E ring, and we present some of the data obtained in March 1980. In Paper II we shall derive the three-dimensional distribution of material in the E ring and discuss its cosmogonic implications.  相似文献   

Scale‐Dependent Variability of As and Heavy Metals in a River Elbe Floodplain     

Dana Zimmer  Kristian Kiersch  Christel Baum  Ralph Meissner  Robert Müller  Gerald Jandl  Peter Leinweber 《洁净——土壤、空气、水》2011,39(4):328-337

  相似文献   

Quasars, their host galaxies and their central black holes     

J. S. Dunlop  R. J. McLure  M. J. Kukula  S. A. Baum  C. P. O'Dea  D. H. Hughes 《Monthly notices of the Royal Astronomical Society》2003,340(4):1095-1135

  相似文献   

Weather cycles: Real or imaginary?: William J. Burroughs, Cambridge University Press, Cambridge, UK, paperback, XIII + 207 pp., US $20.00, ISBN 0-521-47869-3     

Steven K. Baum 《Dynamics of Atmospheres and Oceans》1996,25(1):57-59

  相似文献   

The host galaxies of luminous quasars   总被引：1，自引：0，他引：1  

David J. E. Floyd  Marek J. Kukula  James S. Dunlop  Ross J. McLure  Lance Miller  Will J. Percival  Stefi A. Baum  Christopher P. O'Dea 《Monthly notices of the Royal Astronomical Society》2004,355(1):196-220

  相似文献   

A three‐dimensional stratigraphic model for the Messinian crisis in the Pannonian Basin,eastern Hungary     

I. Csato  D. Granjeon  O. Catuneanu  G. R. Baum 《Basin Research》2013,25(2):121-148

A three‐dimensional quantitative stratigraphic forward model is employed to investigate the controls leading to the Messinian events in the lacustrine Pannonian Basin of Central Paratethys, and the link between the Messinian salinity crisis in the Mediterranean and the late Miocene‐Pliocene stratigraphy of the Pannonian Basin. Subsurface geological data show that a prominent unconformity surface formed during Messinian time in the Pannonian Basin associated with a sudden forced regression, abrupt basinward shift of facies and a subsequent, prolonged lowstand normal regression. The lowstand prograding series filled up the shallow basin fast, while, at the same time, the marginal areas of the basin were subject to tectonic inversion. The Dionisos program used in this research is built on a nonlinear water‐driven sediment diffusion process, and it employs multiple sediment classes, basin flexure and compaction. Four different scenarios were built in the experiments to test possible basin histories with different rates and timing of tectonic inversion. Each scenario was modelled in two versions: including and not including a lake‐level fall in the Messinian. The results confirm that the Pannonian Basin in the study area has undergone a tectonic inversion since the Messinian, although the exact rates of uplift at different locations remain uncertain. The unconformity and the observed stratigraphic architecture and facies pattern could be modelled adequately only in the versions that applied a Messinian lake‐level fall. Our research concludes that the Messinian unconformity in the Pannonian Basin was caused by an absolute lake‐level drop, likely linked to the desiccation of the Mediterranean, followed by subsidence and normal regression in the basin centre and concomitant tectonic inversion and uplift along the basin margins.  相似文献   

The international planetary patrol program: An assessment of the first three years     

W.A. Baum 《Planetary and Space Science》1973,21(9):1511-1519

Day-to-day and hour-to-hour changes in the large-scale atmospheric and surface features of the planets can now be studied more effectively than previously possible. Since 1969 a network of observatories has obtained almost uninterrupted photographic coverage during all apparitions of Jupiter and Mars, plus some of Venus. Patrol films and catalogues are available to the scientific community. Recent or current analyses include the distribution and motion of clouds on Mars, the development and decay of Martian dust storms, the seasonal, diurnal and random fluctuations in contrast between adjacent light and dark regions on Mars, the detection of vertical shear in the Jovian atmosphere, the longitudinal oscillation of the Red Spot, the dependence of rotation period on xenographic latitude and on time, the eruption and spread of SEB disturbances, and the retrograde circulation of the Venus cloud deck.  相似文献   

Unemployment in Non-Metropolitan Australia: integrating geography,social and individual contexts     

Scott Baum  Anthea Bill  William Mitchell 《The Australian geographer》2008,39(2):193-210

Despite a significant period of strong economic and jobs growth nationally, there is well-established evidence in Australia that the proceeds of this growth have not been shared equally, either between places or between individuals. Empirically, it is well known that particular socioeconomic groups have a higher risk of unemployment and it has become equally well established that there are particular geographic patterns of labour market disadvantage that suggest that local geographic context is also important. What is not well understood are the ways in which phenomena at the geographic level are associated with individual-level characteristics and other social contexts in ways that negatively impact on a range of social outcomes, including unemployment. The present paper specifically addresses this issue by using a multi-scalar approach and using survey data from the Housing, Income and Labour Force Dynamics Australia (HILDA) survey and aggregate level census data to model unemployment risk. The paper argues that to better understand unemployment and to add to sound policy development, approaches that incorporate a variety of contexts, including the impact of local geographies, are important.  相似文献   

Theoretical interpretation of photometric properties of the Martian surface and atmosphere     

Kari Lumme  Leonard J. Martin  William A. Baum 《Icarus》1981,45(2):379-397

Earth-based UBV photometry, high-quality photographs from the Lowell Observatory collection, and Mariner 9 data have been combined with a new radiative transfer theory to derive physical parameters for the Martian surface and atmosphere, both before and during the 1971 dust storm. We find that the dust particles of the storm had a single-scattering albedo of 0.84 ± 0.02 and an asymmetry factor of 0.35 ± 0.10 in green (V) light. The geometric albedo of Mars was 0.15 and the phase integral 1.83, which yield 0.27 for the Bond albedo. The mean optical thickness of the “clear” atmosphere averaged over the whole planet was 0.15 ± 0.05 and was not detectably dependent on wavelength. Geometric albedos for the surface are 0.25 (light areas) and 0.17 (dark areas) in V, 0.095 in B (both areas), and 0.060 in U (both areas). The soil particles are moderately backward scattering with an asymmetry factor of ?0.20, indicating them to be rather opaque. The mean surface roughness, on a scale larger than that of individual dust particles and therefore large compared with the wavelength, is 0.57. This represents the depth/radius ratio of an average hole and it is only one-half as large as values typical for the Moon and asteroids.  相似文献   

Saturn's Rings: Azimuthal variations,phase curves,and radial profiles in four colors     

W.T. Thompson  K. Lumme  W.M. Irvine  W.A. Baum  L.W. Esposito 《Icarus》1981,46(2):187-200

Four-color photographic photometry of Saturn for the 1977–1979 apparitions has been analyzed to determine the dependence of ring brightness on wavelength, solar phase angle, ring particle orbital phase angle (azimuthal effect), declination of the Earth relative to the ring plane (tilt angle), and radial distance from Saturn. Azimuthal brightness variations up to ±20% relative to the ansae are clearly apparent for the maximum of ring A, but are not detectable for ring B or the outer portion of ring A. The shape of the intensity (I) versus orbital phase angle (θ) curve varies with ring tilt (B) and probably with wavelength, and shows 180° symmetry. As characterized by its slope near the ansae, this curve suggests that the azimuthal effect increases as B decreases from 26 to ≈11°. The phase curves l(α) for the ansae show very little dependence on ring tilt (26° > B > 6°), on wavelength, or on radial distance from Saturn; possibly the curves are somewhat steeper at the smallest tilt angles and for ring A relative to ring B. The radial profile of both rings becomes flatter with decreasing tilt angle and with decreasing wavelength. The latter effect is a natural result of the classical, many-particle-thick ring model.  相似文献