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  • Inorganic Chemistry  (3,512)
  • ASTROPHYSICS  (3,017)
  • 1
    Publication Date: 2019-06-28
    Description: The Giotto Complete Positive ion, Electron and Ram Negative Ion measurements near Comet Halley plasma experiment identified regions in which the solar wind interaction with the cometary plasma displayed characteristic features. Beginning 4.6 million km from the comet there is an upstream region with sporadic connection to the comet. An electron foreshock is present up to 250,000 km away from the bow shock. A bow shock is detected at 1.15 million km. Between the bow shock and the cometopause the outer regions can be divided into three parts. A cometopause is found at 135,000 km, and a density decrease is detected at 45,000 km from the comet. The detailed plasma features associated with these regions are described.
    Keywords: ASTROPHYSICS
    Type: ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 1: Plasma and Gas; p 29-34
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  • 2
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Zeitschrift für anorganische Chemie 502 (1983), S. 199-208 
    ISSN: 0044-2313
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Description / Table of Contents: Untersuchung von CuCl2/SiO2- und Al2O3-Träger-KatalysatorenDie Natur und Stabilität von Oberflächenspezies des CuCl2 auf α-Al2O3, γ-Al2O3 und SiO2 wurden mittels Röntgendiffraktometrie und Reflexionsspektroskopie untersucht. An inertem α-Al2O3-Träger wird keine spezifische chemische Wechselwirkung mit CuCl2 beobachtet im Gegensatz zu den hydratisierten Trägern SiO2 und γ-Al2O3. Bei diesen Trägern besteht die Koordinationssphäre des Cu2+ aus Oberflächengruppen (OH- oder O- nach Trocknung bzw. Aktivierung), H2O und Cl-; mit abnehmender Konzentration an H2O-Liganden im Verlauf von Tränkung, Trocknung und Glühen.γ-Al2O3-Proben, geglüht bei 400°C, zeigen γ-Cu2(OH)3Cl gegenüber CuAl2O4 bei höheren Temperaturen. Das Fehlen von Cu2(OH)3Cl auf SiO2 ist auf die Säure-Base-Eigenschaft der Träger zurückzuführen. Die verschiedenen Träger können in folgender Stabilitätsreihe der gebildeten Oberflächenkomplexe angeordnet werden: γ-Al2O3 〉 SiO2 ≫ -Al2O3.
    Notes: The nature and stability of surface species of CuCl2 supported on α-Al2O3, γ-Al2O3, and SiO2 were investigated by using X-ray diffraction techniques and reflectance spectroscopy. No specific chemical interaction of CuCl2 is observed on an inert α-Al2O3 support, as opposed to hydrated carriers as SiO2 and γ-Al2O3. On these supports the coordination sphere of Cu2+ consists of surface groups (OH- or O- at drying and activation, resp.), H2O and Cl-, with the H2O ligands decreasing in concentration in the process of impregnation, drying and calcination.γ-Al2O3 samples, calcined at 400°C, show γ-Cu2(OH)3Cl as opposed to CuAl2O4 at higher temperatures. The absence of Cu2(OH)3Cl on SiO2-supported samples is related to the acid-base characteristics of the carriers. The various supports can be arranged in the following order of stability of the complexes formed: γ-Al2O3 〉 SiO2 ≫ -Al2O3.
    Additional Material: 6 Ill.
    Type of Medium: Electronic Resource
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  • 3
    ISSN: 0044-2313
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Description / Table of Contents: Untersuchung von spektroskopischen und Bindungseigenschaften von neuen o-, m- und p-Hydroxybenzoid-Komplexen einiger dreiwertiger „open-shell“ Zentralatome mittels experimenteller und HMO-quantenchemischer MethodenNeue Komplexe von Cr(III), Fe(III) und Co(III) mit o-, m- und p-Hydroxydithiobenzoid-Liganden werden dargestellt und charakterisiert. Die Bindungseigenschaften dieser Komplexe werden auf Grund von HMO-quantenchemischen Berechnungen diskutiert. Aus der Abschätzung des Effektes der π-Bindung zwischen Metall und Liganden auf die CT-Energien im Falle der p-Hydroxydithiobenzoid-Komplexe wurden ihre Elektronenübergänge völlig charakterisiert; rationelle Werte werden für den Ligandenfeldparameter (10Dq) erhalten. Die Kristallfeldbanden konnten in den Spektren dieser Komplexe nicht erkannt werden, auf Grund der Überlagerung durch intensive CT-Banden. Aus HMO-Näherungen für die Interpretation elektronischer Spektren konnten wir, im Zusammenhang mit der Ligandenfeldbeschreibung der CT-Spektren, Ligandenfeldspektroskopische Parameter für alle untersuchten Komplexe sowie für die entsprechenden unsubstituierten Dithiobenzoid-Komplexe berechnen. Auf Grund der berechneten Werte von 10Dq können die untersuchten Liganden auf dem oberen Ende der spektrochemischen Reihe eingeordnet werden, was mit dem „low-spin“-Typ dieser Komplexe in Einklang ist.
    Notes: New complexes of Cr(III), Fe(III) and Co(III) with the o-, m- and p-hydroxydithiobenzoato ligands have been prepared and characterized. The bonding properties in these complexes are discussed in the light of HMO quantum-chemical calculations. By estimation of the effect of metal-ligand π-bonding on the electronic transition energies in the case of the p-hydroxydithiobenzoate complexes their electronic transitions have been fully characterized and reasonable values for the ligand field parameter, 10Dq, have been obtained. Crystal field bands could not be detected in the electronic spectra of these complexes, as they are obscured by the more intense charge transfer bands. Using the HMO approach for the interpretation of the electronic spectra in combination with the ligand field description of the charge transfer spectra we were able to calculate reasonable ligand field spectral parameters for all the complexes studied, as well as for the corresponding unsubstituted dithiobenzoate complexes. The calculated 10Dq values place the ligands under investigation at the upper end in the spectrochemical series of chelating dithio-ligands, a fact which is consistent with the low-spin type of these complexes.
    Additional Material: 2 Ill.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Berichte der deutschen chemischen Gesellschaft 28 (1895), S. 922-927 
    ISSN: 0365-9496
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Weinheim : Wiley-Blackwell
    Berichte der deutschen chemischen Gesellschaft 27 (1894), S. 470-471 
    ISSN: 0365-9496
    Keywords: Chemistry ; Inorganic Chemistry
    Source: Wiley InterScience Backfile Collection 1832-2000
    Topics: Chemistry and Pharmacology
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  • 6
    Publication Date: 2011-08-18
    Description: The first detection of interference fringes by VLBI at a wavelength of 3.4 mm during observations of 3C84 are reported. The compact source in the nucleus of 3C84 was observed for a 9-hr period on the 485 km baseline between the Owens Valley Radio Observatory and the Hat Creek Observatory. The fringe data are given and the derivation of the correlated flux densities is described. The findings are discused in the context of previous obervations. The results demonstrate that there are no unforeseen technical difficulties associated with millimeter VLBI, and that the sensitivity of existing systems is sufficient to observe objects brighter than a few Jy. The observations are consistent with the millimeter wavelength radio structure of 3C84 being more compact than its centimeter wavelength structure.
    Keywords: ASTROPHYSICS
    Type: Nature (ISSN 0028-0836); 303; June 9
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  • 7
    Publication Date: 2019-06-28
    Description: Data from the Vega 1 permitted the determination of the total neutral gas density profile along the spacecraft trajectory. Discounting small fluctuations, the field ionization source instrument measured a density profile which varied approximately as the inverse radial distance squared. Data from the electron impact ionization instrument yielded a series of calibration points; e.g., the neutral density at 100,000 km is 10,000/cc. The combined data provide a calibrated total density profile, and imply a neutral production rate of 10 to the 30th power molecules/sec.
    Keywords: ASTROPHYSICS
    Type: ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 1: Plasma and Gas; p 391-395
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  • 8
    Publication Date: 2019-06-28
    Description: The ultraviolet spectrum of comet P/Halley was monitored with the IUE between 12 September 1985 and 8 July 1986 (r 〈2.6 AU pre and post-perihelion) at regular time intervals except for a two-month period around the time of perihelion. A complete characterization of the UV spectrum of the comet was obtained to derive coma abundances and to study the light emission mechanisms of the observed species. The Fine Error Sensor (FES) camera of the IUE was used to photometrically investigate the coma brightness variation on time scales of the order of hours. Spectroscopic observations as well as FES measurements show that the activity of the nucleus is highly variable, particularly at the end of December 1985 and during March and April 1986. The production rates of OH, CS and dust are derived for the entire period of the observations. The total water loss rate for this period is estimated to be 150 million metric tons.
    Keywords: ASTROPHYSICS
    Type: ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 1: Plasma and Gas; p 325-328
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  • 9
    Publication Date: 2019-06-28
    Description: The UV spectrum of comet P/Halley (1982 i) was monitored with the IUE at regular time intervals. A complete characterization of the UV spectrum of the comet was obtained to derive coma abundances and to study the light emission mechanisms of the observed species. The Fine Error Sensor (FES) camera of the IUE was used to investigate the coma brightness variability on short time scales. Spectroscopic observations as well as FES measurements show that the comet nucleus activity was highly variable.
    Keywords: ASTROPHYSICS
    Type: ESA Proceedings of an International Symposium on New Insights in Astrophysics. Eight Years of UV Astronomy with IUE; p 39-42
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  • 10
    Publication Date: 2019-06-28
    Description: Contemporaneous IUE ultraviolet spectra and visible photoelectric data of the eclipsing binary V471 Tauri (K2V + DA) between 1979 and 1985 was analyzed. The combined data detail the three-dimensional structure of atmospheric loops and their associated starspots on the K dwarf. The distribution of starspot regions on the surface of the K star was inferred from the visible photometry. When spots are located near the limb of the K dwarf prior to and shortly after the total eclipse of the white dwarf, absorption lines such as C II, C III, c IV, and Si IV appear superimposed on the continuum of the white dwarf. These absorption lines are likely caused by cool coronal loops overlying the spots in the atmosphere of the K dwarf. The loops can extend nearly one stellar radius above the surface of the K2V star.
    Keywords: ASTROPHYSICS
    Type: ESA Proceedings of an International Symposium on New Insights in Astrophysics. Eight Years of UV Astronomy with IUE; p 197-200
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