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  • LUNAR AND PLANETARY EXPLORATION  (8)
  • COMPOSITE MATERIALS  (5)
  • Cell & Developmental Biology  (3)
  • 1980-1984  (15)
  • 1950-1954  (1)
Collection
Publisher
Years
Year
  • 1
    Electronic Resource
    Electronic Resource
    New York, NY [u.a.] : Wiley-Blackwell
    Journal of Cellular Physiology 112 (1982), S. 291-297 
    ISSN: 0021-9541
    Keywords: Life and Medical Sciences ; Cell & Developmental Biology
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Biology , Medicine
    Notes: Protease nexin (PN) is a cell-secreted protein that links to thrombin (Th) and certain other serine proteases. PN mediates the binding, internalization, and degradation of these proteases by cells (Baker et al., 1980; Low et al., 1981). Here we show that binding of Th-PN complexes to human foreskin fibroblasts (HF cells) accounted for 90% of the specific cellular Th binding at certain mitogenic doses of the protease. However, cell-associated Th-PN complexes were likely to be inactive mitogenically because heparin (170 units/ml) inhibited cellular binding of 125-Th-PN by about 95% (a reduction from 1.3 × 105 to 6 × 103 125I-Th-PN complexes per cell) but did not influence Th-mediated mitogenic stimulation. In experiments with mouse embryo cells, heparin also markedly decreased cellular binding of 125I-Th-PN without changing the mitogenic response to Th. The lack of mitogenic activity of cell-associated Th-PN complexes suggested that PN might inhibit the mitogenically essential proteolytic activity of Th. This possibility is supported by the following findings. First, amounts of serum-free conditioned culture medium that contained enough PN to complex a large fraction of added Th inhibited the clotting activity of Th. Second, heparin increased the formation of 125I-Th-PN complexes and also increased this inhibitory effect of conditioned medium. We conclude that PN acts as a negative modulator of thrombin mitogenic activity.It is shown that like other fibroblastic cells HF cells bound free 125I-Th specifically (although with relatively low affinity, Kass 〈 108 M-1). Specific binding of free 125I-Th to HF cells increased fourfold in the presence of heparin (50 IU/ml).
    Additional Material: 8 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
    Electronic Resource
    Electronic Resource
    Philadelphia : Wiley-Blackwell
    Journal of Cellular and Comparative Physiology 43 (1954), S. 257-269 
    ISSN: 0095-9898
    Keywords: Life and Medical Sciences ; Cell & Developmental Biology
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Biology , Medicine
    Additional Material: 2 Ill.
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  • 4
    facet.materialart.
    Unknown
    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
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  • 5
    Publication Date: 2011-08-17
    Description: Results of Pioneer 11 imaging photopolarimeter observations of Saturn, its rings, and Titan are presented. The imaging photopolarimeter is a pointable telescope with an aperture of 2.5 cm and passbands of 390 to 500 to 720 nm which uses the spin of the spacecraft to scan across an object. Images of the Saturn system and of the rings are presented, and the absence of a D ring, structures in the C, B and A rings and the Cassini division and the discoveries of the F ring and the provisionally named Pioneer division separating it from the A ring are reported. A mean particle size less than 15 meters is estimated from estimates of total ring mass and the optical depth of the B ring. The discovery of the satellite 1979 S 1 at 2.53 Saturn radii is also noted. Models of the vertical aerosol structure of Saturn's atmosphere are compared with the polarization data, and it is indicated that the density of cloud particles decreases with altitude with a scale height about one fourth that of the gas, and that an optical depth of one is to be found at 750 mbar.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Science; 207; Jan. 25
    Format: text
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  • 6
    facet.materialart.
    Unknown
    In:  Other Sources
    Publication Date: 2011-08-19
    Description: Residual strength results are presented on four composite material systems that were exposed for three years at locations on the North American Continent. The exposure locations are near the areas where Bell Model 206L Helicopters, that are in a NSA/U.S. Army sponsored flight service program, are flying in daily commercial service. The composite systems are: (1) Kevlar-49 fabric/F-185 epoxy; (2) Kevlar-49 fabric/LRF-277 epoxy; (3) Kevlar-49 fabric/CE-306 epoxy; and (4) T-300 Graphite/E-788 epoxy. All material systems exhibited good strength retention in compression and short beam shear. The Kevlar-49/LRF-277 epoxy retained 88 to 93 percent of the baseline strength while the other material systems exceeded 95 percent of baseline strength. Residual tensile strength of all materials did not show a significant reduction. The available moisture absorption data is also presented.
    Keywords: COMPOSITE MATERIALS
    Format: text
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  • 7
    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)
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  • 8
    Publication Date: 2016-06-07
    Description: The long-term durability of those advanced composite materials which are applicable to aircraft structures was discussed. The composite components of various military and commercial aircraft and helicopters were reviewed. Both ground exposure and flight service were assessed in terms of their impact upon composite structure durability. The ACEE Program is mentioned briefly.
    Keywords: COMPOSITE MATERIALS
    Type: ACEE Composite Struct. Technol.; p 17-50
    Format: application/pdf
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  • 9
    Publication Date: 2014-09-27
    Description: In an analog to the great landslides of the Vales Marineris, Mars, a detailed study was made of the Corfu Landslide in south-central Washington. This prehistoric slide is located on the northern flank of the Saddle Mountains, southwest of Othello, Washington. The slide covers a 13 square km area centered on section 11 of T.15N., R.27E., Willamette Meridian, adjacent to the Corfu townsite. Approximately 1 cubic km of material is involved in sliding that was probably initiated by Missoula flooding through the Channeled Scabland. It is concluded that there were four primary factors involved in the initiation of the Corfu landsliding: (1) A slip surface was present at the right orientation; (2) Glacial flooding undercut the slope; (3) Wetter climatic conditions prevailed during that time period; and (4) Some seismic vibrations, known to occur locally, probably acted as a trigger. These factors show that special conditions were required in conjunction to produce landsliding. Studies in progress of the Vales Marieneris suggest that the same factors probably contributed to landsliding there.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA. Washington Rept. of Planetary Geology Program, 1983; p 230
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  • 10
    facet.materialart.
    Unknown
    In:  Other Sources
    Publication Date: 2019-06-28
    Description: Early observations of Mars conducted by means of telescopes are considered. Secchi introduced the Italian word 'canale' ('channel') in 1869 to describe apparent lines on the planet's surface. Between 1877 and 1888 Schiaparelli mapped a profusion of 'canali'. Schiaparelli's work led to famous controversies about Mars. This book attempts to investigate the puzzle posed by the Martian channels, taking into account also the results of the studies conducted with the aid of the two orbiting Viking spacecraft which have produced a total number of nearly 60,000 pictures. The channel types are discussed along with questions regarding the distribution, the ages, and the proposed origins of the channels. Attention is given to the geomorphology of Mars, the patterns and networks of Martian valleys, ice and the Martian surface, the outflow channels, catastrophic flood processes, questions of analogy between terrestrial and Martian geographic features, and Martian phenomena associated with water liquid or water ice.
    Keywords: LUNAR AND PLANETARY EXPLORATION
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