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  • LUNAR AND PLANETARY EXPLORATION  (10)
  • Analytical Chemistry and Spectroscopy  (4)
  • Coleoptile
  • 1990-1994  (16)
Collection
Publisher
Years
Year
  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Planta 195 (1994), S. 63-69 
    ISSN: 1432-2048
    Keywords: Auxin ; Blue light ; Coleoptile ; Microtubule ; Phototropism ; Transverse polarity ; Zea
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology
    Notes: Abstract In a previous study (Nick and Schäfer 1991, Planta 185, 415–424), unilateral blue light had been shown, in maize coleoptiles, to induce phototropism and a stable transverse polarity, which became detectable as stable curvature if counteracting gravitropic stimulation was removed by rotation on a horizontal clinostat. This response was accompanied by a reorientation of cortical microtubules in the outer epidermis (Nick et al. 1990, Planta 181, 162–168). In the present study, this stable transverse polarity is shown to be correlated with stability of microtubule orientation against blue light and changes of auxin content. The role of auxin in this stabilisation was assessed. Although auxin can induce reorientation of microtubules it fails to induce the stabilisation of microtubule orientation induced by blue light. This was even true for gradients of auxin able to induce a bending response similar to that ellicited by phototropic stimulation. Experiments involving partial irradiation demonstrated different perception sites for phototropism and polarity induction. Phototropism starts from the very coleoptile tip and involves transmission of a signal (auxin) towards the subapical elongation zone. In contrast, polarity induction requires local action of blue light in the elongation zone itself. This blue-light response is independent of auxin.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Planta 185 (1991), S. 415-424 
    ISSN: 1432-2048
    Keywords: Blue light (polarity induction) ; Coleoptile ; Phototropism ; Polarity (transverse) ; Signal transduction ; Zea (phototropism)
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology
    Notes: Abstract Phototropic stimulation induces a spatial memory. This was inferred from experiments with maize (Zea mays L.) coleoptiles involving opposing blue-light pulses, separated by variable time intervals, and rotation on a horizontal clinostat (Nick and Schäfer, 1988b, Planta 175, 380–388). In those experiments, individual seedlings either curved towards the first or towards the second pulse, or they remained straight. Bending, if it occurred, seemed to be an all-or-none response. Intermediates, i.e. plants, bending only weakly, were not observed. In the first part of the present study it was attempted to create such intermediates. For this purpose the strength of the first, inducing, and the second, opposing, pulse was varied. The result was complex: (i) Individual seedlings maintained the all-or-none expression of spatial memory. (ii) However, on the level of the whole population, the time intervals at which a given response type dominated depended on the fluence ratio. (iii) Furthermore, the final curvature was determined by the fluence ratio. These results are discussed in terms of a blue-light-induced transverse polarity. This polarity initiates from a labile precursor, which can be reoriented by an opposing stimulation (indicated by the strong bending towards the second pulse). The strong curvatures towards the first pulse over long time intervals reveal that, eventually, the blue-light-induced transverse polarity becomes stabilised and thus immune to the counterpulse. In the second part of the study, the relation between phototropic transduction and transverse polarity was characterised by a phenomenological approach involving the following points: (i) Sensory adaptation for induction of transverse polarity disappears with a time course similar to that for phototropic sensory adaptataion. (ii) The fluence-response for induction of transverse polarity is a saturation curve and not bell-shaped like the curve for phototropism. (iii) For strong counterpulses and long time intervals the clinostat-elicited nastic response (Nick and Schäfer 1989, Planta 179, 123–131) becomes manifest and causes an “aiming error” towards the caryopsis. (iv) Temperature-sensitivity of polarity induction was high in the first 20 min after induction, then dropped sharply and rose again with the approach of polarity fixation. (v) Stimulus-summation experiments indicated that, for different inducing fluences, the actual fixation of polarity happened at about 2 h after induction. These experiments point towards an early separation of the transduction chains mediating phototropism and transverse polarity, possibly before phototropic asymmetry is formed.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Journal of High Resolution Chromatography 16 (1993), S. 674-676 
    ISSN: 0935-6304
    Keywords: Capillary GC ; Atomic emission detection ; Absolute measurements ; Chemistry ; Analytical Chemistry and Spectroscopy
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Additional Material: 2 Ill.
    Type of Medium: Electronic Resource
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  • 4
    ISSN: 1052-9306
    Keywords: Chemistry ; Analytical Chemistry and Spectroscopy
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Carvedilol is metabolized via both oxidation and conjugation pathways in dog and rat to more than 12 different products. Several glucuronide conjugates of the parent drug were identified. The drug contains an aliphatic hydroxyl, an aliphatic amine and a carbazole amine, all of which are potential sites for conjugation with glucuronic acid. In order to determine the positions of glucuronidation, a strategy involving acetylation of the metabolites was devised. The metabolites were acetylated using acetic anhydride in either pyridine or aqueous solution, and the products were analyzed by fast atom bombardment mass spectrometry. Carvedilol was acetylated at both the hydroxyl and the aliphatic amine in pyridine and at only the aliphatic amine in aqueous solution. The carbazole nitrogen was unreactive under both conditions. Based on the acetylation patterns observed for the metabolites in pyridine or aqueous solution, the positions of conjugation were determined. Each of the five glucuronide metabolites of carvedilol formed in dog and rat was analyzed and the structures included two diastereomeric carbamoyl glucuronide metabolites formed from addition of CO2 and glcuronic acid to carvedilol, a carbazole-N-linked glucuronide, and two diastereomeric O-linked glucuronides. This approach should be generally applicable in many cases to determine the structures of glucuronide conjugates for compounds which contain more than one potential glucuronidation site.
    Additional Material: 8 Ill.
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  • 5
    ISSN: 0749-1581
    Keywords: REDOR ; Double-cross-polarization ; Solids NMR ; 13C-15N dipolar coupling ; Magic-angle spinning ; Insect cuticle ; Chemistry ; Analytical Chemistry and Spectroscopy
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Insect exoskeleton, multiply labeled with 13C and 15N, was examined by rotational-echo double-resonance (REDOR) and double-cross-polarization (DCP) magic-angle spinning 13C NMR. Low levels of incorporation of label make the analysis of these samples a practical test of the relative advantages of REDOR and DCP for the detection of weak, heteronuclear dipolar coupling between rare spins in solids. The sensitivity of REDOR for the detection of directly bonded 13C-15N pairs is an order of magnitude greater than that of DCP when neither label is involved in homonuclear dipolar coupling of strength comparable to the spinning frequency. However, if either of the 13C or 15N labels undergoes homonuclear spin flips, DCP gains in relative sensitivity and is easier to use for spin counting than REDOR.
    Additional Material: 4 Ill.
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Chichester [u.a.] : Wiley-Blackwell
    Journal of Raman Spectroscopy 24 (1993), S. 637-639 
    ISSN: 0377-0486
    Keywords: Chemistry ; Analytical Chemistry and Spectroscopy
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology , Physics
    Notes: The lattice dynamics of a recently synthesized crystal of (NH4)3-xRbxZnBr5 were studied by Raman spectroscopy. The spectra were found to be in good agreement with the crystal structure. Clear evidence of NH4 group disorder was found. Ordering of these groups at low temperatures was observed.
    Additional Material: 5 Ill.
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  • 7
    Publication Date: 2013-08-31
    Description: The chemical evolution of the early Martian hydrosphere is discussed. The early Martian ocean can be modeled as a body of relatively pure water in equilibrium with a dense carbon dioxide atmosphere. The chemical weathering of lavas, pyroclastic deposits, and impact melt sheets would have the effect of neutralizing the acidity of the juvenile water. As calcium and other cations are added to the water by chemical weathering, they are quickly removed by the precipitation of calcium carbonate and other minerals, forming a deposit of limestone beneath the surface of the ocean. As the atmospheric carbon dioxide pressure and the temperature decrease, the Martian ocean would be completely frozen. Given the scenario for the chemical evolution of the northern lowland plains of Mars, it should be possible to draw a few conclusions about the expected mineralogy and geomorphology of this regions.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Inst., Scientific Results of the NASA-Sponsored Study Project on Mars: Evolution of Volcanism, Tectonics, and Volatiles; p 255-256
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  • 8
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    In:  CASI
    Publication Date: 2013-08-29
    Description: One question of great interest to those who study the evolution of the Martian atmosphere is: if there was an early, dense atmosphere that was removed, is there any mechanism that could restore it? In the case of an atmosphere removed largely by the formation of carbonates, the only obvious means of restoring it is by the thermal decomposition of the carbonates. Decomposition of carbonates under turbulently flowing lava holds great promise as a means of resupplying the atmosphere with CO2. Huppert and colleagues have modeled the emplacement of terrestrial komatiite flows and found that komatiites, even when flowing over previously emplaced and cooled komatiite flows, could melt and erode this rock to a significant depth. Based on this work, I have begun modeling the erosion of Martian carbonate deposits under turbulently flowing, komatiitic lava. Initial results from this modeling indicate that a high-volume lava flow, emerging at a temperature of, say, 1600 degrees, is capable of eroding several meters of carbonate deposits per day. If such a flow is active for a hundred days, several hundreds of meters of carbonate could be decomposed. If this process occurred over a large area, a bar or more of CO2 could be injected back into the atmosphere over an extremely short period of time. The implications of such an occurrence are intriguing. For instance, if a relatively late pulse of volcanism (such as is suggested by Frey) were to cause a large flow of lava over carbonate deposits in the northern lowlands, the resulting pulse of CO2 into the atmosphere could conceivably restore the climate to one in which liquid water could exist on the surface, or ice could flow.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Inst., Papers Presented to the Workshop on the Evolution of the Martian Atmosphere; p 26
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  • 9
    Publication Date: 2013-08-29
    Description: A model for the carbonate-silicate geochemical cycle of an early, wet Mars is under development. The results of this study will be used to constrain models of the geochemical history of Mars and the likely mineralogy of its present surface. Although Mars today is a cold, dry planet, it may once have been much warmer and wetter. Values of total outgassed CO2 from several to about 10 bars are consistent with present knowledge (Pollack et al. 1987), and this amount of CO2 implies an amount of water outgassed at least equal to an equivalent depth of 500-1000 meters (Carr 1986). Pollack et al. (1987), in addition, estimate that a thick CO2 atmosphere may have existed for an extended period of time, perhaps as long as a billion years. The greenhouse effect of such an atmosphere would permit the presence of liquid water on the surface, most likely in the form of a shallow sea in the lowest regions of the planet, such as the northern plains (Schaefer 1990). The treatment of geochemical cycles as complex kinetic chemical reactions has been undertaken for terrestrial systems in recent years with much success (Lasaga 1980, 1981; Berner et al. 1983; Lasaga et al. 1985). Although the Martian system is vastly less well understood, and hence less well-constrained, it is also a much simpler system, due to the lack of biogenic reactions that make the terrestrial system so complex. It should be possible, therefore, to use the same techniques to model the Martian system as have been used for terrestrial systems, and to produce useful results. A diagram of the carbonate-silicate cycle for Mars (simplified from the terrestrial system) is given.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Inst., Workshop on the Martian Surface and Atmosphere Through Time; p 130-131
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  • 10
    Publication Date: 2019-01-25
    Description: There is a growing body of evidence in favor of the importance of aqueous sedimentary processes on Mars. It is important to understand the role that surface weathering processes have played in the development of the present morphology of the Martian surface. Such an understanding is important not only for its relevance to the study of volatile sources and sinks on Mars through time, but also for its relevance to Martian geologic and tectonic history. Starting in the fall of this year, the Mars Observer Laser Altimeter will begin sending back to Earth data on the topography of Mars that is of a higher quality than most of the topography data available for the Earth. This data will be invaluable, not only for understanding global and large-scale regional processes and landforms on Mars, but also for the study of local and smaller-scale regional processes and landforms. Digital topography is an important part of geologic and geomorphic studies, useful in distinguishing between different lithologies and between different types of weathering. Digital topography data may be used to study a wide variety of local and regional-scale landforms, including valleys, sand dunes, lava flows, landslides, and slopes. Topography data are also essential to the analysis of spectral response patterns, especially in areas of high topographic relief. Geomorphic classification can be significantly improved by the addition of topographic information.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 3: N-Z; p 1243-1244
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