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  • 1
    Electronic Resource
    Electronic Resource
    New York : Wiley-Blackwell
    Biopolymers 22 (1983), S. 1637-1640 
    ISSN: 0006-3525
    Keywords: Chemistry ; Polymer and Materials Science
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Additional Material: 2 Ill.
    Type of Medium: Electronic Resource
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  • 2
    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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  • 3
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    In:  Other Sources
    Publication Date: 2011-08-18
    Description: Tentative conclusions about the origins of channels and valleys on Mars based on the consensus of investigators who have studied the problem are presented. The morphology of outflow channels is described in detail, and the morphology, distribution, and genesis of Martian valleys are addressed. Secondary modification of channels and valleys by mass-wasting phenomena, eolian processes, cratering, and mantling by lava flows is discussed. The physics of the flows needed to account for the immense volumes of Martian outflow channels is considered in detail, including the possible influence of debris flows and mudflows, glaciers, and ice sheets. It is concluded that Mars once probably possessed an atmosphere with higher temperatures and pressures than at present which played an essential role in an active hydrological cycle.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Geological Society of America, Bulletin (ISSN 0016-7606); 94; 1035-105
    Format: text
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  • 4
    Publication Date: 2011-08-18
    Description: Long-lived upstream energetic ion events at Jupiter appear to be very similar in nearly all respects to upstream ion events at earth. A notable difference between the two planetary systems is the enhanced heavy ion compositional signature reported for the Jovian events. This compositional feature has suggested that ions escaping from the Jovian magnetosphere play an important role in forming upstream ion populations at Jupiter. In contrast, models of energetic upstream ions at earth emphasize in situ acceleration of reflected solar wind ions within the upstream region itself. Using Voyager 1 and 2 energetic ion measurements near the magnetopause, in the magnetosheath, and immediately upstream of the bow shock, the compositional patterns are examined together with typical energy spectra in each of these regions. Characteristic spectral changes are found late in ion events observed upstream of the bow shock at the same time that heavy ion fluxes are enhanced and energetic electrons are present. A model involving upstream Fermi acceleration early in events and emphasizing energetic particle escape in the prenoon part of the Jovian magnetospehre late in events is presented to explain many of the features in the upstream region of Jupiter.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: (ISSN 0273-1177)
    Format: text
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