Semi-monthly mean sea-level pressure maps for the Mediterranean area     

Werner A. Baum  Lawrence B. Smith 《Meteorology and Atmospheric Physics》1952,5(3):326-345

Summary Semi-monthly mean sea-level pressure maps for the Mediterranean and adjacent areas are presented. Isobars have been drawn at 1-millibar intervals. The most significant features on the maps and the advantages of the mode of presentation are discussed briefly.

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Zusammenfassung Es werden auf das Meeresniveau bezogene halbmonatliche mittlere Luftdruckkarten für das Mittelmeergebiet und die anstoßenden Länder vorgelegt. Die Isobaren wurden für Millibarabstände gezeichnet. Die wichtigsten Resultate der Karten und die Vorzüge der Darstellungsweise werden kurz besprochen.

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Résumé Présentation de cartes de la pression moyenne semi-mensuelle, réduite au niveau de la mer, de la région méditerranéenne et des contrées voisines. Les isobares sont tracées de millibar en millibar. Brève discussion des traits principaux des cartes et des avantages de la méthode de représentation.

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With 25 Figures.

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The work reported in this paper has been supported by the Geophysics Research Division of the Air Force Cambridge Research Center, under Contract AF 19 (122)-466.  相似文献   

A comparative HST imaging study of the host galaxies of radio-quiet quasars, radio-loud quasars and radio galaxies – I     

R. J. McLure  M. J. Kukula  J. S. Dunlop  S. A. Baum  C. P. O'Dea  D. H. Hughes 《Monthly notices of the Royal Astronomical Society》1999,308(2):377-404

We present the first results from a major HST WFPC2 imaging study aimed at providing the first statistically meaningful comparison of the morphologies, luminosities, scalelengths and colours of the host galaxies of radio-quiet quasars, radio-loud quasars and radio galaxies. We describe the design of this study and present the images that have been obtained for the first half of our 33-source sample. We find that the hosts of all three classes of luminous AGN are massive elliptical galaxies, with scalelengths ≃10 kpc, and R − K colours consistent with mature stellar populations. Most importantly, this is first unambiguous evidence that, just like radio-loud quasars, essentially all radio-quiet quasars brighter than M _R =−24 reside in massive ellipticals. This result removes the possibility that radio 'loudness' is directly linked to host galaxy morphology, but is however in excellent accord with the black hole/spheroid mass correlation recently highlighted by Magorrian et al. We apply the relations given by Magorrian et al. to infer the expected Eddington luminosity of the putative black hole at the centre of each of the spheroidal host galaxies we have uncovered. Comparison with the actual nuclear R -band luminosities suggests that the black holes in most of these galaxies are radiating at a few per cent of the Eddington luminosity; the brightest host galaxies in our low- z sample are capable of hosting quasars with M _R ≃− 28, comparable to the most luminous quasars at z ≃3. Finally, we discuss our host-derived black hole masses in the context of the radio luminosity:black hole mass correlation recently uncovered for nearby galaxies by Franceschini et al., and consider the resulting implications for the physical origin of radio loudness.  相似文献   

Basal‐topographic control of stationary ponds on a continuously moving landslide     

Jeffrey A. Coe  Jonathan P. McKenna  Jonathan W. Godt  Rex L. Baum 《地球表面变化过程与地形》2009,34(2):264-279

The Slumgullion landslide in the San Juan Mountains of southwestern Colorado has been moving for at least the last few hundred years and has multiple ponds on its surface. We have studied eight ponds during 30 trips to the landslide between July 1998 and July 2007. During each trip, we have made observations on the variability in pond locations and water levels, taken ground‐based photographs to document pond water with respect to moving landslide material and vegetation, conducted Global Positioning System surveys of the elevations of water levels and mapped pond sediments on the landslide surface. Additionally, we have used stereo aerial photographs taken in October 1939, October 1940 and July 2000 to measure topographic profiles of the eight pond locations, as well as a longitudinal profile along the approximate centerline of the landslide, to examine topographic changes over a 60‐ to 61‐year period of time. Results from field observations, analyses of photographs, mapping and measurements indicate that all pond locations have remained spatially stationary for 60–300 years while landslide material moves through these locations. Water levels during the observation period were sensitive to changes in the local, spring‐fed, stream network, and to periodic filling of pond locations by sediment from floods, hyperconcentrated flows, mud flows and debris flows. For pond locations to remain stationary, the locations must mimic depressions along the basal surface of the landslide. The existence of such depressions indicates that the topography of the basal landslide surface is irregular. These results suggest that, for translational landslides that have moved distances larger than the dimensions of the largest basal topographic irregularities (about 200 m at Slumgullion), landslide surface morphology can be used as a guide to the morphology of the basal slip surface. Because basal slip surface morphology can affect landslide stability, kinematic models and stability analyses of translational landslides should attempt to incorporate irregular basal surface topography. Additional implications for moving landslides where basal topography controls surface morphology include the following: dateable sediments or organic material from basal layers of stationary ponds will yield ages that are younger than the date of landslide initiation, and it is probable that other landslide surface features such as faults, streams, springs and sinks are also controlled by basal topography. The longitudinal topographic profile indicated that the upper part of the Slumgullion landslide was depleted at a mean vertical lowering rate of 5.6 cm/yr between 1939 and 2000, while the toe advanced at an average rate of 1.5 m/yr during the same period. Therefore, during this 61‐year period, neither the depletion of material at the head of the landslide nor continued growth of the landslide toe has decreased the overall movement rate of the landslide. Continued depletion of the upper part of the landslide, and growth of the toe, should eventually result in stabilization of the landslide. Published in 2008 by John Wiley & Sons, Ltd.  相似文献   

Magnetic properties of the clinopyroxenes aegirine and hedenbergite: a magnetic susceptibility study on single crystals     

E. Baum  W. Treutmann  W. Lottermoser  G. Amthauer 《Physics and Chemistry of Minerals》1997,24(4):294-300

Two natural clinopyroxene single crystals were investigated, an aegirine-augite (AEG) and a magnesian hedenbergite (HED). Both samples were carefully characterized by electron microprobe, X-ray diffraction, and Mössbauer spectroscopy. Magnetic susceptibility measurements of powdered samples reveal low temperature antiferromagnetic coupling and Curie-Weiss behaviour with T _N =7.5(5)?K, Θ _P =?19(1)?K for AEG, and T _N =31(1)?K, Θ _P =+21(1)?K for HED, respectively. Low temperature Mössbauer spectra exhibit relaxation phenomena. Magnetic susceptibility measurements of the single crystals show the direction of the magnetic moments to be lying within the a/c plane for both samples: 50(±2)° from a and 57(±2)° from c in AEG, and 45(±2)° from a and 60(±2)° from c in HED, respectively. The antiferromagnetic interchain interaction competes with the ferromagnetic intrachain interaction in both pyroxenes. In the magnesian hedenbergite a field induced magnetic transition is found. Its dependence on temperature, magnetic field and crystallographic direction is investigated and described.  相似文献   

Privacy and Ethics in Undergraduate GIS Curricula     

Peter Scull  Adam Burnett  Emmalee Dolfi  Ali Goldfarb  Peter Baum 《The Journal of geography》2016,115(1):24-34

The development of location-aware technologies, such as smartphones, raises serious questions regarding locational privacy and the ethical use of geographic data. The degree to which these concepts are taught in undergraduate geographic information science (GISci) courses is unknown. A survey of GISci educators shows that issues of privacy and ethics are important in a GISci education. However, a large proportion of GISci educators are not concerned about the loss of locational privacy and many do not devote classes to the subject. Those not teaching the subject cite lack of course time and the need for more information.  相似文献   

The ability of the Space Telescope to detect extra-solar planetary systems     

W. A. Baum 《Celestial Mechanics and Dynamical Astronomy》1980,22(2):183-190

The Space Telescope can play a key role in searching for and investigating the contents of extra-solar planetary systems. For about 90 nearby stars, positional variations due to major planets would be well within the astrometric capability of the Wide-Field/Planetary Camera system. Since the centroids of star images will be determined to within a milliarcsecond down to 22nd magnitude, there will be an abundance of reference stars at very small angular distances from each planetary system candidate, and they will have small enough motions of their own to provide a reference frame of the stability required.Presented at the Symposium Star Catalogues, Positional Astronomy and Celestial Mechanics, held in honor of Paul Herget at the U.S. Naval Observatory, Washington, November 30, 1978.  相似文献   

Regional Population and Employment Change in Australia 1991–2001: Inertia in the Face of Rapid Change?     

Scott Baum  Kevin O’Connor 《GeoJournal》2005,62(1):85-94

Analyses of the patterns of national population change have been influenced by the US experience where major differences between a older north and a newer south are prominent in many studies. The current paper argues that these perspectives overlook some inertia in the pattern of population and jobs. Drawing upon US and European experience the paper explores the pattern of change in Australia. There it finds that population has favoured newer locations but that gains in share of national population have not been large. At the same time some of the older regions have maintained population share, or at worst recorded small declines. That broad insight is enriched by sectoral analysis where it is clear that only the retail sector has experienced the large gains in new regions; employment change in other sectors showed the links with population change are weak. The paper concludes that simple notions of new region population and employment gains are oversimplified and overlook the substantial development around established centres. In particular it is possible that the old regions are re-structuring their spatial form and spilling over statistical boundaries and so actually maintaining established role in national networks.  相似文献   

Modeling regional initiation of rainfall-induced shallow landslides in the eastern Umbria Region of central Italy   总被引：3，自引：6，他引：3  

Diana Salciarini  Jonathan W. Godt  William Z. Savage  Pietro Conversini  Rex L. Baum  John A. Michael 《Landslides》2006,3(3):181-194

We model the rainfall-induced initiation of shallow landslides over a broad region using a deterministic approach, the Transient Rainfall Infiltration and Grid-based Slope-stability (TRIGRS) model that couples an infinite-slope stability analysis with a one-dimensional analytical solution for transient pore pressure response to rainfall infiltration. This model permits the evaluation of regional shallow landslide susceptibility in a Geographic Information System framework, and we use it to analyze susceptibility to shallow landslides in an area in the eastern Umbria Region of central Italy. As shown on a landslide inventory map produced by the Italian National Research Council, the area has been affected in the past by shallow landslides, many of which have transformed into debris flows. Input data for the TRIGRS model include time-varying rainfall, topographic slope, colluvial thickness, initial water table depth, and material strength and hydraulic properties. Because of a paucity of input data, we focus on parametric analyses to calibrate and test the model and show the effect of variation in material properties and initial water table conditions on the distribution of simulated instability in the study area in response to realistic rainfall. Comparing the results with the shallow landslide inventory map, we find more than 80% agreement between predicted shallow landslide susceptibility and the inventory, despite the paucity of input data.  相似文献   

Saturn satellite observations and orbits from the 1980 ring plane crossing     

P.K. Seidelmann  R.S. Harrington  D. Pascu  W.A. Baum  D.G. Currie  J.A. Westphal  G.E. Danielson 《Icarus》1981,47(2):282-287

The ground-based observations of the recently discovered Saturnian satellites, obtained during the 1980 apparition, have been collected from the IAU Circulars and identified with and fit to four orbital groups: (1) the inner pair of coorbital librating satellites, (2) the satellite known as “Dione B” near the L₄ point of Dione-Saturn, (3) the satellites associated with the L₄ and L₅ points of Tethys-Saturn or, alternatively, one satellite unconfortably near the orbit of Tethys, and (4) the F-ring satellites observed by Voyager I.  相似文献   

Report on the solar physics-plasma physics workshop     

P. A. Sturrock  P. J. Baum  J. M. Beckers  C. E. Newman  E. R. Priest  H. Rosenberg  D. F. Smith  D. G. Wentzel 《Solar physics》1976,46(2):411-431

This report summarizes the proceedings of a meeting held on 17–20 September 1974, at Stanford University. The purpose was to explore plasma physics problems which arise in the study of solar physics. Sessions were concerned with specific questions including the following: Is the solar plasma thermal or non-thermal? What spectroscopic data are required? What types of magnetic field structures exist? Do MHD instabilities occur? Do resistive or non-MHD instabilities occur? What mechanisms of particle acceleration have been proposed? What information do we have concerning shock waves? Very few questions were answered categorically but, for each question, there was discussion concerning the observational evidence, theoretical analyses, and existing or potential laboratory and numerical experiments.  相似文献