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  • 11
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Journal of Psychosomatic Research 14 (1970), S. 409 
    ISSN: 0022-3999
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Medicine , Psychology
    Type of Medium: Electronic Resource
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  • 12
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 34 (1975), S. 459-465 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The Rayleigh-Taylor instability in a rotating plasma of variable density has been investigated to include simultaneously the effects of viscosity and the finiteness of the ion Larmor radius. It is shown that, for a plasma in which the density is stratified along the vertical, the solution is characterized by a variational principle. Making use of this, proper solutions have been otained for a semiinfinite plasma in which the density varies exponentially. The dispersion relation has been solved numerically and it is found that the influence of the effects of both FLR and viscosity is stabilizing. The Coriolis forces are found to have a dual role, stabilizing for small wave numbers and destabilizing for large wave numbers. The range of the small wave numbers, over which the Coriolis forces have a stabilizing influence, is found to increase with Coriolis forces.
    Type of Medium: Electronic Resource
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  • 13
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 39 (1976), S. 487-494 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We have calculated the spectrum of Cyg X-1 under the assumption that the radiation orginates in a disk around a 11M ⊙ black-hole. Supersonic turbulence prevails in the outer parts of the disk and electron-electron bremsstrahlung appears to be resonsible for the maintenance of the temperature at a level less than 1010 K near the inner edge of the disk. The theoretical spectrum gives the best fit with the observations if the Reynolds number is about 1200.
    Type of Medium: Electronic Resource
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  • 14
    Electronic Resource
    Electronic Resource
    Springer
    Cellular and molecular life sciences 20 (1964), S. 684-685 
    ISSN: 1420-9071
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Summary The bilateral representation of the retina on the visual cortex was investigated by analysing the amplitude, latency and topic distribution of the potentials evoked in the visual cortex by monocular photic stimulation of the retina in the conscious rabbit. The amplitudes of the potentials evoked on both ipsi- and contralateral hemispheres, show a relation 1:4. A small field for bilateral retinal projection of the retina was mapped in the anterolateral part of the visual cortex. These differences in amplitude, latency and topic distribution may be significant for stereoscopic vision.
    Type of Medium: Electronic Resource
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  • 15
    ISSN: 1432-1998
    Source: Springer Online Journal Archives 1860-2000
    Topics: Medicine
    Notes: Abstract We report the results of a 14-year retrospective study of brain MRI abnormalities in 12 pediatric patients presenting with hypomelanosis of Ito (HI). Miscellaneous brain abnormalities were found: one patient had a medulloblastoma, three had cortical malformations, and five demonstrated “minor” abnormalities such as dilated Virchow-Robin spaces or brain atrophy. We emphasize the polymorphism of brain abnormalities associated with HI.
    Type of Medium: Electronic Resource
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  • 16
    Electronic Resource
    Electronic Resource
    Springer
    Bulletin of environmental contamination and toxicology 30 (1983), S. 588-594 
    ISSN: 1432-0800
    Source: Springer Online Journal Archives 1860-2000
    Topics: Energy, Environment Protection, Nuclear Power Engineering , Medicine
    Type of Medium: Electronic Resource
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  • 17
    ISSN: 1432-0967
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Notes: Abstract This investigation describes five Mesozoic dolerite dikes which intrude Paleozoic metamorphic and igneous rocks of the Inner Piedmont of western South Carolina. The dikes are vertical or nearly so and strike approximately N40° W. Three major northeast-trending faults also occur in the study area. Left lateral displacement of one dolerite is documented at a locality near Cleveland, South Carolina. Elsewhere, several of the dolerite dikes appear to terminate at or near the faults. — The dolerite dikes have subophitic to microporphyritic textures and consist principally of plagioclase (generally An70–80), olivine (dominantly Fo80–90) and augite with subordinate pigeonite, titanomagnetite, chromite and brown, partly glassy mesostasis. In one dike pyroxene compositions trend from augite to ferroaugite in contrast to an augite→subcalcic augite→pigeonite trend characteristic of the other dolerites. The contrasting trends primarily result from differences in SiO2 abundance in the dolerite magmas. — Major and trace element analyses indicate the presence of two different olivine-normative dolerite magma types. The two magma types are not related by near surface crystal fractionation. Models for genesis of the olivine-normative dolerite magmas by partial melting of a plagioclase peridotite upper mantle source region are presented. The models require that the source region be enriched in LREE and incompatible elements such as Rb, Ba, Hf and Th relative to Cl chondritic abundances. One magma type appears to represent a primary dolerite magma that ascended from the source region with little subsequent compositional change. The second magma type most likely experienced assimilation of clinopyroxene-garnet (eclogite) during ascent, thereby acquiring a REE pattern with a less steep negative slope for the LREE and a slight positive slope in the HREE.
    Type of Medium: Electronic Resource
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  • 18
    ISSN: 1436-5065
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geography , Physics
    Notes: Summary The movement of cold fronts along the eastern side of the Southern Alps has been studied in detail during the Southerly Change Experiment (SOUCHEX). An enhanced network of surface wind monitoring stations was established in the Canterbury region of the South Island to allow detailed study of meso-scale wind fields during the passage of fronts. Fivesoutherly changes occurred during the experiment, one of which failed to produce a clear wind change over much of the area. The often erratic movement of these fronts along the eastern side of the mountains is illustrated by isochrone maps of the onset of the wind change. Other general characteristics of these events include their shallowness (1000–1500 m deep) and in most cases their abrupt onset. Detailed analysis of anemograph data collected during SOUCHEX indicates great variability in the surface wind field associated with passage of the fronts. Maps of the meso-scale wind field plotted for the first southerly change of the 14 January 1988 illustrate the complexity of the wind changes experienced over the eastern South Island in particular. The arrival of the cold fronts at individual sites provided features of air mass interaction which appear to relate to time of day, and regional and local site factors. Variations, in wind, temperature and relative humidity provide clear examples of both single and double air mass changes. However, nocturnal changes seem to be less distinct due to lower ambient temperatures and increased boundary layer stability.
    Type of Medium: Electronic Resource
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  • 19
    Electronic Resource
    Electronic Resource
    Springer
    International journal of earth sciences 68 (1979), S. 825-831 
    ISSN: 1437-3262
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Description / Table of Contents: Abstract The revised (1975) Phanerozoic time scale incorporates and suggests some systematic regularities at the Period level. If one considers the Cenozoic Era as equivalent to the other geological Periods, and if one combines the Triassic-Permian and Devonian-Silurian Periods, 8 major subdivisions of Phanerozoic time result which group into two distinct populations of 66±3 and 78±1 m. y. duration. Two systematic cycles of 144 m. y. exist back to the Permian-Carboniferous boundary. Extension of the Phanerozoic Eon at both ends and/or one change of a lower Paleozoic, faunally based Period boundary suggests cycles of 288 or 222 m. y. The change of the Lower Paleozoic Period boundary is supported by recent data. Period boundaries which were originally fixed by early 19th century descriptive rock units incorporate distinct regularities. Period boundaries which were based from their inception on fossils do not necessarily do so. The real and possible cycles and subcycles may be related to the periods of the solar, galactic orbit (77, 274 and 220–240 m. y.). A complex galactic periodicity of 1970 m. y. also appears to correlate with the main subdivisions of Precambrian time, namely, the Phanerozoic-Proterozoic boundary, the Proterozoic-Archean boundary, and the age of the earth and solar system. The reason for the above-mentioned possible correlations between the divisions of geological time and all known periodicities of solar galactic dynamics is not understood.
    Abstract: Résumé Une révision de l'échelle du temps du Phanérozoïque montre des régularités systématiques à l'echelle de la Période. Si l'on considère le Génozoïque comme léquivalent des autres formations, et si l'on combine en une unité le Trias et le Permien et aussi le Dévonien et le Silurien il en résulte 8 subdivisions majeures du Phanérozoïque présentant une duree de 66±3 ou 78±1 Millions d'années. Jusqu'à la limite Permien-Carbonifère, apparaissent ainsi 2 cycles systématiques de 144 Millions d'années chacun. Si l'on étend 1'échelle à tout le Phanérozoïque, et si l'on fait une subdivision supplémen taire dans le Paléozoïque inférieur sur la base d'une limitée faunistique démontrable, on obtient des cycles de 288 ou de 222 Millions d'années. Les limites des formations, telles qu'elles ont été fixées au siècle passé à partir des caractéristiques des entités lithologiques, montrent certaines régularités qui n'apparaissent pas si clairement quand on les associe a des limites démontrées par voie de fossiles. Les cycles et sous-cycles réels et vraisemblables peuvent être coordonnés avec les périodes du système solaire (77, 274 et 220–240 Millions d'années). Une périodicité galactique complexe de 1970 Millions d'années correspond avec la subdivision du Précambrien, spécialement avec les grandes limites à l'intérieur du système, ainsi qu'avec 1'âge de la Terre et celui du système solaire. Les raisons de cette coïncidence des cycles géologiques avec les périodes de la dynamique solaire galactique sont encore inconnues.
    Notes: Zusammenfassung Eine revidierte Zeitskala des Phanerozoikums zeigt einige systematische Abfolgen im Bereich der Formationen. Betrachtet man das Känozoikum als Äquivalent zu den anderen Formationen und verbindet Trias und Perm sowie Devon und Silur zu einer Einheit, so ergeben sich 8 größere Unterteilungen des Phanerozoikums, die entweder eine Länge von 66±3 Millionen Jahre oder 78±1 Million Jahre aufweisen. Bis zur Perm-Karbon-Grenze zurück kann man 2 Zyklen zu je 144 Millionen Jahre nachweisen. Erweitert man die Skala auf das gesamte Phanerozoikum und zieht im Altpaläozoikum eine faunistisch nachweisbare zusätzliche Grenze, so erhält man Zyklen von 288 bzw. 222 Millionen Jahre. Formationsgrenzen, so wie sie im vorigen Jahrhundert aus der Charakteristik von Gesteinseinheiten festgelegt wurden, zeigen bestimmte Regelmäßigkeiten, die nicht so klar hervortreten, wenn man die durch Fossilien nachgwiesenen Grenzen mit hinzunimmt. Wirkliche und wahrscheinliche Zyklen und Subzyklen können den Perioden des Solarsystems zugeordnet werden (77, 274 und 220–240 Mill. Jahre). Eine komplexe galaktische Periodizität von 1970 Mill. Jahren korrespondiert mit der Untergliederung des Prä-Kambriums, speziell mit den großen Grenzen innerhalb des Systems, sowie mit dem Alter der Erde und dem des Sonnensystems. Die Gründe für das Zusammentreffen geologischer Zyklen mit Perioden solar-galaktischer Dynamik sind noch unbekannt.
    Type of Medium: Electronic Resource
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  • 20
    ISSN: 1432-2072
    Keywords: Electroconvulsive shock ; Corticosterone ; Muscarinic agonists ; Serotoninergic agonists ; α-Adrenoceptor agonists ; Rats
    Source: Springer Online Journal Archives 1860-2000
    Topics: Medicine
    Notes: Abstract The effect of repeated and single electroconvulsive shocks (ECS) on the corticosterone response to pharmacological stimuli has been studied in male rats. Plasma corticosterone concentrations are elevated by oxotremorine, a muscarinic agonist, and by 5-hydroxy-l-tryptophan, a precursor of serotonin. Both these agonists probably stimulate corticotrophinreleasing-factor release from the hypothalamus. The log dose-response curves of the corticosterone response to oxotremorine and to 5-hydroxy-l-tryptophan are shifted to the left after a single ECS given daily for 10 days compared with sham-shocked controls. Plasma corticosterone concentrations are elevated by treatment with α-methyl-p-tyrosine methyl ester (400 mg/kg IP). This rise is suppressed by clonidine. The log dose-response curve for the corticosterone response to clonidine after α-methyl-p-tyrosine methyl ester is also shifted to the left by repeated ECS, compared with controls. There is no difference in the corticosterone response of ECS and sham-treated groups given vasopressin, which is thought to act directly on the pituitary to release ACTH. A single ECS produces a slight enhancement of the response to 5-hydroxy-l-tryptophan, a slight decrease in the response to oxotremorine and no change in the response to clonidine after α-methyl-p-tyrosine. The disappearance of the difference in response between ECS and sham-treated animals was also studied 1,3, and 6 days after a series of ten ECS or sham procedures. Significant differences in the corticosterone responses to oxotremorine, 5-hydroxy-l-tryptophan and clonidine after α-methyl-p-tyrosine between ECS and sham-treated animas were found 24 h after the last ECS or sham shock. These differences were in decline 3 days after the last procedure and had completely disappeared by day 6. The decline was largely due to an increase in plasma corticosterone responsiveness to pharmacological stimuli of the shamshocked controls. Responses in the ECS-treated groups remained constant. It is apparent that the anaesthetic procedure suppresses the effect of oxotremorine, 5-hydroxy-l-tryptophan and clonidine after α-methyl-p-tyrosine on corticosterone concentrations in plasma. This effect is spontaneously reversible. Repeated ECS reverses the effect of the anaesthetic procedure but produces no reversible enhancement of its own.
    Type of Medium: Electronic Resource
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