Seismic tomography shows that upwelling beneath Iceland is confined to the upper mantle   总被引：3，自引：0，他引：3  

G. R. Foulger  M. J. Pritchard  B. R. Julian  J. R. Evans  R. M. Allen  G. Nolet  W. J. Morgan  B. H. Bergsson  P. Erlendsson  S. Jakobsdottir  S. Ragnarsson  R. Stefansson  K. Vogfjörd 《Geophysical Journal International》2001,146(2):504-530

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Applied geography and a place for passion     

Morgan Sant 《Applied geography (Sevenoaks, England)》1992,12(4)

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The relation between the concentration of atmospheric condensation nuclei and other meteorological elements at valentia observatory     

S. McWilliams B. Sc.  W. A. Morgan M. Sc. 《Pure and Applied Geophysics》1955,31(1):129-146

Summary Measurements of the concentration of condensation nuclei made twice daily (0h and 12h GMT) with aNolan-Pollak photo-electric counter at Valentia Observatory, in the extreme Southwest of Ireland, over the 4 years 1951–1954, are analysed to show relation with other meteorological elements. It is found that concentration at 12h is generally higher than at (h and that precipitation at the time of observation or in the preceding hour reduces concentration by between 40% and 50%. From measurements made when there was no precipitation at the time or in the previous hour it is found that concentration decreases with increasing wind speed but does not vary appreciably with wind direction apart from a sector from which pollution could be expected. High concentrations are found with visibility below 7 miles, with inversion of temperature, when free from the effects of pollution, follows fairly closely that of duration of bright sunshine.

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Zusammenfassung Es werden Messungen der Konzentration von Kondensationskernen, welche zweimal täglich (um 0 ^h und 12 ^h G.M.T.) mit einem photo-elektrischen Kernzähler nachNolan undPollak am Observatorium in Valentia (im äussersten Südwesten von Irland) in den Jahren 1951 bis 1954 durchgeführt wurden, auf Beziehungen zu anderen meteorologischen Elementen hin untersucht. Die Resultate zeigen, dass die Konzentration um 12 Uhr im allgemeinen grösser ist als um 0 Uhr und, dass die Niederschlag zur Zeit der Beobachtung oder in der der Beobachtung vorausgehenden Stunde die Konzentration um 40 bis 50% herabsetzt. Wenn kein Niederschlag zur Zeit der Messung oder in der vorangehenden Stunde verzeichnet wurde, nimmt die Konzentration mit zunehmender Windgeschwindigkeit ab; sie ändert sich jedoch nicht nennenswert mit der Windrichtung, abgesehen von einem Sektor, aus welchem Verunreinigung zu erwarten war. Hohe Konzentration wurde bei Sichtweiten unterhalb 7 Meilen gefunden, ferner bei Temperaturinversion, und, um 12 Uhr, bei geringer Bewölkung. Der jährliche Gang der Konzentration der Kerne folgt ziemlich genau jenem der Sonnenscheindauer, wenn die Fälle, wo Verunreinigung der Luft stattfindet, ausgeschlossen werden.

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Absence of whistlers at the equator reaffirmed     

M.G. Morgan 《Planetary and Space Science》1980,28(4):359-361

Synoptic observations made on magnetic recording tape at Huancayo, Peru, at the magnetic dip equator, during the International Geophysical Year 1957–1958, were aurally reviewed at that time and no whistlers, hiss, or other emissions were heard. In view of the more recent observation of whistlers at geomagnetic latitudes as low as 12°, and in conjunction with a study of equatorial hiss observed in the topside ionosphere, these recordings have recently been reassessed by reducing them with modern real-time, digital spectrographic equipment. Although the observations were found to be of high quality, and to show the classical features of ground-wave and sky-wave propagation of sferics and VLF transmissions, again no evidence whatsoever of whistlers, hiss, or other emissions is found. Thus it is concluded that the whistlers observed at very low latitudes do not propagate subionospherically to the equator and it is confirmed that “hybrid” whistlers must be due to subionospheric propagation across the equator of the causative sferic rather than of the short whistler.  相似文献   

First Results from Viper: Detection of Small-scale Anisotropy at 40 GHz     

Peterson JB  Griffin GS  Newcomb MG  Alvarez DL  Cantalupo CM  Morgan D  Miller KW  Ganga K  Pernic D  Thoma M 《The Astrophysical journal》2000,535(2):L83-L86

Using all available major samples of Seyfert galaxies and their corresponding closely matched control samples of nonactive galaxies, we find that the bar ellipticities (or axial ratios) in Seyfert galaxies are systematically different from those in nonactive galaxies. Overall, there is a deficiency of bars with large ellipticities (i.e., "thin" or "strong" bars) in Seyfert galaxies compared to nonactive galaxies. Accompanied with a large dispersion due to small number statistics, this effect is strictly speaking at the 2 sigma level. To obtain this result, the active galaxy samples of near-infrared surface photometry were matched to those of normal galaxies in type, host galaxy ellipticity, absolute magnitude, and, to some extent, redshift. We discuss possible theoretical explanations of this phenomenon within the framework of galactic evolution, and, in particular, of radial gas redistribution in barred galaxies. Our conclusions provide further evidence that Seyfert hosts differ systematically from their nonactive counterparts on scales of a few kiloparsecs.  相似文献   

Book reviews     

W. Manshard  W. B. Morgan  Philip Tilley  Atsushi Otomo  G. Kunkel  W. Lauer  K. Kunkel  David Rickard  Joan M. Kenworthy  A. Grotewold  C. Chr Liebmann 《GeoJournal》1981,5(3):291-296

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Economic development,technological change,and the new international economic order     

Morgan D. Thomas 《Geoforum》1979,10(2):129-140

This paper examines dimensions of technological change and selected relationships between new technology and the process of economic development within the general framework of the New International Economic Order. Concepts discussed include economic growth and development, structural change, technological change, innovations, the transfer of technology, and appropriate technology. The relationships between these concepts are described and their significance with regard to the economic development of lesser-developed countries is assessed.  相似文献   

Comment on “The Fossil Coleoptera of the Two Creeks Forest Bed, Wisconsin”, by Alan V. Morgan and Anne Morgan     

Edward B. Evenson  Donald F. Eschman  William R. Farrand  Louis J. Maher  David M. Mickelson  Alan V. Morgan  Anne Morgan   《Quaternary Research》1980,14(3):377-378

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Kimberlites: Their relation to mantle hotspots     

S. Thomas Crough  W. Jason Morgan  Robert B. Hargraves 《Earth and Planetary Science Letters》1980,50(1):260-274

Available age data support the hypothesis that kimberlite intrusions are formed by mantle hotspots. The hypothesis has been tested by inverting the volcanic traces formed by three hotspots to determine the post-Triassic motions of Africa, South America, and North America relative to these hotspots. Then, using these motions, the kimberlites intruded on these continents within the last 150 m.y. are relocated to their place of origin in the present hotspot reference frame. The result indicates that a majority of the kimberlites formed within 5° of a mantle hotspot. Statistical analysis shows that this kimberlite/hotspot correlation is significant at above the 90% level.  相似文献   

Rare earth element distribution in some hydrothermal minerals: evidence for crystallographic control   总被引：1，自引：0，他引：1  

John W. Morgan  Gregory A. Wandless 《Geochimica et cosmochimica acta》1980,44(7):973-980

Rare earth element (REE) abundances were measured by neutron activation analysis in anhydrite (CaSO₄), barite (BaSO₄), siderite (FeCO₃) and galena (PbS). A simple crystal-chemical model qualitatively describes the relative affinities for REE substitution in anhydrite, barite, and siderite. When normalized to ‘crustal’ abundances (as an approximation to the hydrothermal fluid REE pattern), log REE abundance is a surprisingly linear function of (ionic radius of major cation—ionic radius of REE)² for the three hydrothermal minerals, individually and collectively. An important exception, however, is Eu, which is anomalously enriched in barite and depleted in siderite relative to REE of neighboring atomic number and trivalent ionic radius. In principle, REE analyses of suitable pairs of co-existing hydrothermal minerals, combined with appropriate experimental data, could yield both the REE content and the temperature of the parental hydrothermal fluid.The REE have only very weak chalcophilic tendencies, and this is reflected by the very low abundances in galena—La, 0.6 ppb; Sm, 0.06 ppb; the remainder are below detection limits.  相似文献