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  • LUNAR AND PLANETARY EXPLORATION  (3,679)
  • Organic Chemistry  (3,423)
  • Cell & Developmental Biology  (1,486)
  • 1975-1979  (8,588)
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Keywords
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Year
  • 1
    Electronic Resource
    Electronic Resource
    New York, NY : Wiley-Blackwell
    Journal für Praktische Chemie/Chemiker-Zeitung 321 (1979), S. 1000-1006 
    ISSN: 0021-8383
    Keywords: Chemistry ; Organic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Model Calculations on the Counterion Effect in the Cationic Polymerization; Decay of the Mixed Halogenoantimonates SbCl5Br- and SbClBr5-The decay of the halogenoantimonates SbCl5Br- and SbClBr5- according to SbCl5Br- → SbCl5 + Br- resp. SbCl4Br + Cl- and SbClBr5- → SbBr5 + Cl- resp. SbClBr4 + Br- has been investigated by the quantum-chemical CNDO/2 method including geometry optimization. The calculations show that the dissociation of the Sb—Cl bond needs more energy (7,8 kcal/mol) than the dissociation of the Sb—Br bond.Dissociation of the complex anions is facilitated with increasing Br content.
    Additional Material: 4 Ill.
    Type of Medium: Electronic Resource
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  • 2
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    In:  Other Sources
    Publication Date: 2011-08-16
    Description: Classical atmospheric tidal theory is extended to include the effects of large-amplitude planetary-scale variations of the terrain height. Utilizing simple models of the thermotidal forcing, the resulting technique is used to compute the diurnal tide in both the dust-free and the dust-laden Martian atmosphere. The main effect of the Martian variable terrain is to drive topographic tidal modes which can propagate vertically and to excite the possibly resonant diurnal Kelvin mode. The resulting surface wind can exceed 20 m/sec and may determine the preferred location for the initiation of global dust storms. In the middle Martian atmosphere (30-80 km) static and shear instabilities embedded within the tidal fields will generate extensive, though variable, regions of turbulence. Vertical mixing by this turbulence and transport by the tide itself may help to stabilize the middle Martian atmosphere against photolysis.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Journal of the Atmospheric Sciences; 33; Feb. 197
    Format: text
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  • 3
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    In:  CASI
    Publication Date: 2019-06-27
    Description: The complex refractive index in the solar spectral region is estimated. With this index and the size distribution estimated from the UVS data Mie theory is used to compute the radiative parameters required for including radiative scattering in simplified radiative transfer approximations. These approximations then enable the wavelength-integrated solar heating to be computed for various dust-laden Martian atmospheres. The calculations presented in the main body of the paper were computer using the delta-Eddington approximation.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-CR-156696
    Format: application/pdf
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  • 4
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    In:  Other Sources
    Publication Date: 2019-06-27
    Description: This paper examines the solar heating of the Martian atmosphere during the 1971 global dust storm observed by Mariner 9. Radiative scattering as well as absorption is included by utilizing the delta-Eddington approximation to the full radiative transfer equation. The necessary optical parameters are generated by a Mie program which uses a size distribution and a complex refractive index inferred from a number of sources, particularly from recent analyses of Mariner 9 UVS and TV observations. When uniform mixing of the dust is assumed, the solar heating per unit mass during a Martian global dust storm is remarkably uniform with height for small solar zenith angles. Heating rates may reach 80 K/day for overhead sunlight. Overall, 20% of the direct insolation is absorbed by the dust-laden atmosphere. Even optically thin widespread dust hazes may produce heating rates of several degrees Kelvin per day.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Icarus; 35; Aug. 197
    Format: text
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  • 5
    ISSN: 0018-019X
    Keywords: Chemistry ; Organic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: The complexation of 1-methyl-2-hydroxymethyl-imidazole (L) with Cu(I) and Cu(II) has been studied in aqueous acetonitrile (AN). Cu(I) forms three complexes, Cu(AN)L+, CuL2+, and Cu(AN)H-1L, with stability constants logK(Cu(AN)+ + L ⇌ Cu(AN)L+) = 4.60 ± 0.02, logβ2 = 11.31 ± 0.04, and logK(Cu(AN)H-1L+H+ ⇌ Cu(AN)L+) = 10.43 ± 0.08 in 0.15M AN. The main species for Cu(II) are CuL2+, CuH-1L+, CuH-1L2+, and CuH-2L2.The autoxidation of CuL2+ was followed with an oxygen sensor and spectrophotometrically. Competition between the formation of superoxide in a one-electron reduction of O2 and a path leading to H2O2 via binuclear (CuL2)2O22+ was inferred from the rate law \documentclass{article}\pagestyle{empty}\begin{document}$${{ - {\rm d}\left[{{\rm O}_2 } \right]} \mathord{\left/ {\vphantom {{ - {\rm d}\left[{{\rm O}_2 } \right]} {{\rm dt}}}} \right. \kern-\nulldelimiterspace} {{\rm dt}}} = \left[{{\rm CuL}_2^ + } \right]^2 \left[{{\rm O}_2 } \right]\left({\frac{{k_{\rm a} }}{{1 + k_{\rm b} \left[{{\rm CuL}^ + } \right]}} + \frac{{k_{\rm c} \left[{\rm L} \right] + k_{\rm d} + {{\left({{{k_{\rm f} } \mathord{\left/ {\vphantom {{k_{\rm f} } {\left[{\rm L} \right]}}} \right. \kern-\nulldelimiterspace} {\left[{\rm L} \right]}} + k_{\rm g} + k_{\rm h} \left[{\rm L} \right]} \right)} \mathord{\left/ {\vphantom {{\left({{{k_{\rm f} } \mathord{\left/ {\vphantom {{k_{\rm f} } {\left[{\rm L} \right]}}} \right. \kern-\nulldelimiterspace} {\left[{\rm L} \right]}} + k_{\rm g} + k_{\rm h} \left[{\rm L} \right]} \right)} {\left[{{\rm H}^ + } \right]}}} \right. \kern-\nulldelimiterspace} {\left[{{\rm H}^ + } \right]}}}}{{\left[{{\rm CuL}_2 ^ + } \right] + k_{\rm e} \left[{{\rm Cu}\left({{\rm II}} \right)} \right]_{{\rm tot}} }}} \right)$$\end{document} with ka = (2.31 ± 0.12) · 104M-2S-1, kb = (1.0 ± 0.2) · 103M-1, kc = (2.85 ± 0.07) · 102M-2S-1, kd = 3.89 ± 0.14M-1S-1, ke = 0.112 ± 0.004, kf = (2.06 ± 0.24) · 10-10M S-1, kg = (1.35 ± 0.07) · 10-7 S-1, and kh = (6.8 ± 1.4) · 10-7M-1 S-1.
    Additional Material: 6 Ill.
    Type of Medium: Electronic Resource
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  • 6
    ISSN: 0362-2525
    Keywords: Life and Medical Sciences ; Cell & Developmental Biology
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Biology , Medicine
    Notes: Fifty-one cadavers of human adults of both sexes were examined for the raminfications and site of opening of the cervical segment of the thoracic duct. It was found that the duct opened into veins of the neck through either one (84.31%) or two branches (15.69%). The most frequent site of opening was in the junction of the left internal jugular vein with the subclavian vein (18 individuals), but another frequent site (15 individuals) was in the internal jugular vein. The duct opened at the angle formed by the internal jugular vein and the internal posterior jugular vein in five individuals, and at a variety of the other locations in the remaining cadavers. These results are compared with the findings of previous investigators.
    Additional Material: 8 Ill.
    Type of Medium: Electronic Resource
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  • 7
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    In:  CASI
    Publication Date: 2019-06-27
    Description: A thin membrane covering the open side of a meteoroid capture cell causes an impacting meteoroid to disintegrate as it penetrates the membrane. The capture cell then contains and holds the meteoroid particles for later analysis.
    Keywords: LUNAR AND PLANETARY EXPLORATION
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  • 8
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    In:  Other Sources
    Publication Date: 2019-07-13
    Description: Velocity distributions obtained from earth-based meteor observations and corrected to constant meteoroid mass are transformed to meteoroid impact velocity distributions at the moon. Average velocities at the moon thus obtained range from 13 to 18 km/sec. This information is then combined with impact heating estimates to determine the amounts of resident lunar material and incoming meteoritic material that is melted or vaporized. It is found that about 5% of the resulting melt and about 25% of the impact generated vapor should be of meteoritic content. The uncertainties in these estimates are rather large, however, because of uncertainties in the various experimental results required to establish the parameters used in this analysis. The impact generated melts and impact generated vapor deposits, if the latter can be found, should provide additional means for chemically separating out the meteoritic component in the lunar soil.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Science Conference; Mar 17, 1975 - Mar 21, 1975; Houston, TX
    Format: text
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  • 9
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    In:  Other Sources
    Publication Date: 2019-07-13
    Description: The large variation in the areal density of meteoroid impact pits observed over the face of lunar rock chip 12054,54 was previously attributed to variable amounts of shielding of this chip by loosely bound dust. However, an examination of the directionality of flow of the disk and splash accreta on this chip now suggests that the regions with low areal densities of pits and disk accreta were geometrically shielded by a formerly overhanging part of the rock. The 'overhang' is postulated to have broken off during the return of this rock to earth. There remains, nevertheless, considerable evidence for shielding of rock and grain surfaces on the lunar surface by loosely bound dust. The areal extent and depth of deposition of dust is still poorly understood, however. Populations of disk (or pancake) accreta and 'solid' accreta that show evidence of melting are shown to be correlated with impact pit densities. The population of solid angular accreta with exteriors that exhibit little evidence of melting shows no correlation with impact pit densities.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Science Conference; Mar 13, 1978 - Mar 17, 1978; Houston, TX
    Format: text
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  • 10
    Electronic Resource
    Electronic Resource
    New York, NY : Wiley-Blackwell
    Helvetica Chimica Acta 60 (1977), S. 1845-1860 
    ISSN: 0018-019X
    Keywords: Chemistry ; Organic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Notes: Thallium compounds as catalysts for transesterifications and ester exchange reactionsThe transesterification of di-, tri- and tetracarboxylic alkyl esters with 2,3-epoxy-propanol was investigated in the presence of various metal compounds as catalysts. It was found that only thallium compounds catalyse the reactions under mild conditions without decomposition of 2,3-epoxypropanol. Many thallium compounds also proved to be very good catalysts for the reactions of 2,3-epoxypropanol with alkoxysilanes and the ester exchange reactions of di-, tri- and tetracarboxylic alkyl esters with 2,3-epoxypropyl-acetate.
    Additional Material: 5 Tab.
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