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  • 1
    Electronic Resource
    Electronic Resource
    New York, NY [u.a.] : Wiley-Blackwell
    Journal of Cellular Physiology 117 (1983), S. 175-182 
    ISSN: 0021-9541
    Keywords: Life and Medical Sciences ; Cell & Developmental Biology
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Biology , Medicine
    Notes: Four criteria were used to examine serum-free conditioned cell culture medium for protease nexin (PN):(1) formation of SDS-stable ∼77 K Da complexes between a medium component and [125l]thrombin; (2) acceleration by heparin of the rate of formation of these complexes; (3) cellular binding of these complexes; and (4) inhibition by heparin of the cellular binding of complexes. Listed in order of decreasing PN production, PN was detected in media conditioned by the following cell types: human foreskin fibroblasts (0.18 μg/106 cells), rat embryo heart muscle cells (0.13 μg/106 cells), mouse myotubes (0.1 μg/106 cells), monkey kidney epithelial cells, human fibrosarcoma cells, human lung fibroblasts, simian virus 40 (SV-40)-transformed human fibroblasts, human epidermoid carcinoma cells, bovine aortic endothelial cells (only after phorbol ester treatment), and mouse myoblasts. No PN was found in medium conditioned by mouse 3T3 cells, SV40 virus-transformed 3T3 cells, human lymphoblasts, or mouse leukemia cells.Eleven of the cell types examined for secretion of PN were also examined for the presence of cytoplasmic thrombin-binding factors. Lysates from all of these cell types contained a factor that formed ∼60-65 K Da sodium dodecyl sulfate (SDS)-stable complexes with [125l] thrombin. This MW is significantly lower than that of [125l] thrombin-PN complexes, indicating that the factor is distinct from PN. Nevertheless, PN and the cytoplasmic factor share similarities. Production of both PN (by HF cells and WI-26 cells) and the cytoplasmic factor (by HF cells and 3T3 cells) are stimulated by epidermal growth factor and phorbol myristate acetate. Also, both PN and the cytoplasmic factor complex trypsin, plasmin, urokinase, and thrombin, but not pancreatic elastase. Because a number of the cells that produce PN or the cytoplasmic serine protease-binding factor are known to produce plasminogen activators, both PN and the cytoplasmic factor could regulate plasminogen activator activity.
    Additional Material: 5 Ill.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2011-08-18
    Description: Existing models for the genesis of porphyry copper deposits indicate that they formed in granodioritic stocks located in the infrastructure of andesitic stratovolcanoes. It is noted that sites of porphyry-type subvolcanic tin mineralization in the Eastern Cordillera of Bolivia are distinguished by the absence of such andesitic structures. The surface expression of a typical subvolcanic porphyry tin deposit is thought to be an extrusive dome of quartz latite porphyry, sometimes related to a larger caldera structure. Evidence from the El Salvador porphyry copper deposit in the Eocene magmatic belt in Chile indicates that it too may be more closely related to a silicic volcanic structure than to an andesitic stratovolcano. The dome of La Soufriere, Guadeloupe is offered as a modern analog for the surface expression of subvolcanic mineralization processes, with the phreatic eruptions there indicating the formation of hydrothermal breccia bodies in depths. It is pointed out that the occurrence of mineralized porphyries, millions of years after caldera formation, does not necessarily indicate that tin intrusions and mineralization are not genetically related to the subcaldera pluton, but may be a consequence of the long thermal histories (1-10 million years) of the lowermost parts of large plutons.
    Keywords: GEOPHYSICS
    Type: Journal of Volcanology and Geothermal Research (ISSN 0377-0273); 18; 165-190
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  • 3
    Publication Date: 2019-06-28
    Description: The coupling between the solar wind and the geomagnetic disturbances was examined using data from the ISEE-3 spacecraft at an earth-sun libration point and ground-based data. One minute data were used to avoid aliasing in determining the internal magnetospheric response to solar wind conditions. Attention was given to the cross-correlations between the geomagnetic index (AE), the total energy dissipation rate (UT), and the solar wind parameters, as well as the spatial and temporal scales on which the magnetosphere reacts to the solar wind conditions. It was considered necessary to characterize the physics of the solar wind-magnetosphere coupling in order to define the requirements for a spacecraft like the ISEE-3 that could be used as a real time monitoring system for predicting storms and substorms. The correlations among all but one parameter were lower during disturbance intervals; UT was highly correlated with all parameters during the disturbed times. An intrinsic 25-40 min delay was detected between interplanetary activity and magnetospheric response in quite times, diminishing to no more than 15 min during disturbed times.
    Keywords: GEOPHYSICS
    Type: Journal of Geophysical Research (ISSN 0148-0227); 88; Aug. 1
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  • 4
    Publication Date: 2019-06-28
    Description: The spacecraft remained close to or within a previously unexplored part of the distant (60-220 earth radii) geomagnetic tail nearly continuously from January 1 to March 30, 1983. Analysis of the data reveals that all of the plasma regimes identified previously with near-earth measurements (plasma sheet, low-latitude boundary layer, plasma mantle, lobe, and magnetosheath) remain recognizable in the distant tail. These regimes, however, are found to be intermingled in a more chaotic fashion than near the earth. Within the plasma sheet at approximately 200 earth radii, typical flow velocities are about 500 km/s tailward, considerably higher than in the near-earth plasma sheet. Earthward flow within the plasma sheet is observed occasionally, indicating the temporary presence of a neutral line beyond 220 earth radii. Also found are strong bidirectional electron anisotropies throughout much of the distant plasma sheet, boundary layer, and magnetosheath.
    Keywords: GEOPHYSICS
    Type: Geophysical Research Letters (ISSN 0094-8276); 10; Sept
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  • 5
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    In:  Other Sources
    Publication Date: 2019-06-28
    Description: It is thought likely that thermal thinning and/or diapirism can cause the extensional stress required for rifting. The rifting, however, will not occur unless the regional tectonic regime permits the sides of the rift to diverge. Whereas passive plate extension could cause rifting in isolation, the extension and rifting are likely to be localized where the lithosphere is weakest over an existing thermal anomaly. In those cases where asthenospheric diapirism occurs, which is essentially a response to thinning of the lithosphere by thermal thinning or plate extension, the effects of diapirism may completely mask the initiating mechanism. It is believed that anomalous heat transfer into the lithosphere, diapirism, and magmatism must all figure in rifting, along with a deviatoric stress field that will permit extension in a developing rift. Even though the models are useful in permitting idealized processes to be quantified and tested, better knowledge of lithosphere properties is considered necessary, in particular knowledge of mantle viscosity and its temperature dependence.
    Keywords: GEOPHYSICS
    Type: Tectonophysics (ISSN 0040-1951); 94; 1983
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