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  • 11
    Publikationsdatum: 2013-10-22
    Beschreibung: A method of ultrasound-assisted reduction of a nickel-ammonia complex with borohydride in aqueous solution was used to prepare NiMoB/MCM-41 and NiMoB/SBA-15 supported amorphous alloy catalysts. These catalysts were used to upgrade bio-oil at mild temperatures ranging from 100 to 160 °C and recycling of these two supported catalysts and of unsupported NiMoB was carried out. Then, fresh and third time used catalysts were characterized by X-ray diffraction, X-ray photoelectron spectra, and transmission electron microscopy. Quantitative results were obtained from the analysis of gas chromatography/mass spectrometry. Through mild upgrading, 1-hydroxy-2-propanone, furfural, and 2-methoxy-4-vinylphenol in the bio-oil were converted to relevant alcohols and saturated phenols. The conversion rates were 45.7, 71.5, and 57.1 %, respectively, when crude bio-oil was upgraded using NiMoB/MCM-41 at 160 °C. The two supported catalysts, especially NiMoB/MCM-41, had smaller amorphous NiMoB particles and exhibited more uniform dispersion on mesoporous silica, leading to higher reaction activity and stability than unsupported NiMoB. Deactivation of these catalysts resulted from the reduction of Ni 0 , B 0 , and Mo 4+ species on the surface, the transition from the amorphous to the crystalline state, particle agglomeration, and coke deposition on the surface. The mild hydrogenation of bio-oil is a crucial step in the production of bio fuel. Here, NiMoB catalysts were used to determine the effects of temperature and catalyst recycling on the process. Higher temperature led to smaller concentrations of unsaturated compounds but more serious particle agglomeration and coking. A suitable catalyst support increased catalytic activity and stability.
    Print ISSN: 0930-7516
    Digitale ISSN: 1521-4125
    Thema: Chemie und Pharmazie , Werkstoffwissenschaften, Fertigungsverfahren, Fertigung
    Publiziert von Wiley
    Standort Signatur Erwartet Verfügbarkeit
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  • 12
    Publikationsdatum: 2012-09-20
    Beschreibung: Recent studies have shown that low energy ions constitute a significant part of the total ion population in the Earth's magnetosphere. In this study, we have used a comprehensive data set with measurements of cold (total energy less than 70 eV) ion velocity and density to determine their source. This data set is derived from Cluster satellite measurements combined with solar wind and interplanetary magnetic field measurements and geomagnetic indices. By using the guiding center equation of motion, we were able to calculate the trajectories and thus determine the source region of the cold ions. Our results show that the polar cap region is the primary source for cold ions. We also found that the expansion and contraction of the polar cap as a consequence of changes in solar wind parameters were correlated with the source region size and intensity of the cold ion outflow. Elevated outflow fluxes near the nightside auroral zone and the dayside cusps during disturbed conditions suggest that energy and particle precipitation from the magnetosphere or directly from the solar wind can enhance the outflow of cold ions from the ionosphere.
    Print ISSN: 0094-8276
    Digitale ISSN: 1944-8007
    Thema: Geologie und Paläontologie , Physik
    Publiziert von Wiley im Namen von American Geophysical Union (AGU).
    Standort Signatur Erwartet Verfügbarkeit
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  • 13
    Publikationsdatum: 2014-11-23
    Beschreibung: The Martian ionosphere directly interacts with the solar wind due to lack of a significant intrinsic magnetic field, and an interface is formed in between. The interface is usually recognized by two kinds of indicators: the ionopause identified from ionospheric density profiles and the photoelectron boundary (PEB) determined from the electron energy spectrum at higher energies. However, the difference between them remains unclear. We have determined the locations of crossings of the ionopause and PEB from Mars Express observations during 2005-2013, and found that the average position of the PEB appears to be ~200 km higher than that of the ionopause, which corresponds to 10 3  cm −3 in the electron density profile. The discrepancy can be explained by cross field transport of photoelectrons.
    Print ISSN: 0094-8276
    Digitale ISSN: 1944-8007
    Thema: Geologie und Paläontologie , Physik
    Publiziert von Wiley im Namen von American Geophysical Union (AGU).
    Standort Signatur Erwartet Verfügbarkeit
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  • 14
    Publikationsdatum: 2014-08-08
    Beschreibung: Measurements of inner radiation belt protons have been made by the Van Allen Probes Relativistic Electron-Proton Telescopes as a function of kinetic energy (24 to 76 MeV), equatorial pitch angle, and magnetic L shell, during late-2013 and early-2014. A probabilistic data analysis method reduces background from contamination by higher energy protons. Resulting proton intensities are compared to predictions of a theoretical radiation belt model. Then trapped protons originating both from cosmic ray albedo neutron decay (CRAND) and from trapping of solar protons are evident in the measured distributions. An observed double-peaked distribution in L is attributed, based on the model comparison, to a gap in the occurrence of solar proton events during the 2007 to 2011 solar minimum. Equatorial pitch angle distributions show that trapped solar protons are confined near the magnetic equator, but that CRAND protons can reach low-altitudes. Narrow pitch angle distributions near the outer edge of the inner belt are characteristic of proton trapping limits.
    Print ISSN: 0148-0227
    Thema: Geologie und Paläontologie , Physik
    Publiziert von Wiley im Namen von American Geophysical Union (AGU).
    Standort Signatur Erwartet Verfügbarkeit
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  • 15
    Publikationsdatum: 2018
    Beschreibung: Abstract The feasibility of Pb immobilization via bioapatite (BAp) and CO2 in the acidic red soil (RS) and saline‐alkaline soil (SS) was compared in this study. The elevated CO2 (10% in air) significantly promoted the dissolution of BAp in water, that is, the concentrations of released P were enhanced from 2 to 20 ppm as pH decreased from 6.9 to 5.6. Then, it was shown that 30–40% TCLP leached Pb was removed from RS and SS, with the combination of BAp addition and CO2 elevation. In RS, the addition of BAp (even without CO2) could significantly increase water‐soluble P. Moreover, some Pb cations were adsorbed onto iron (hydr)oxides within RS. In contrast, CO2 elevation is essential for enhancing P release in SS as it dramatically increased the dissolution of phosphates. The released P then reacted with Pb cations to form insoluble pyromorphite. Therefore, this combination is effective for Pb immobilization in saline‐alkaline soil whereas adding solely BAp is feasible for acid soil.
    Print ISSN: 0266-0032
    Digitale ISSN: 1475-2743
    Thema: Geologie und Paläontologie , Land- und Forstwirtschaft, Gartenbau, Fischereiwirtschaft, Hauswirtschaft
    Publiziert von Wiley
    Standort Signatur Erwartet Verfügbarkeit
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  • 16
    Publikationsdatum: 2016-02-12
    Beschreibung: Radiation belt protons in the kinetic energy range 24 to 76 MeV are being measured by the Relativistic Electron Proton Telescope (REPT) on each of the two Van Allen Probes. Data have been processed for the purpose of studying variability in the trapped proton intensity during October 2013 to August 2015. For the lower energies ( 32 MeV), equatorial proton intensity near L = 2 showed a steady increase that is consistent with inward diffusion of trapped solar protons, as shown by positive radial gradients in phase space density at fixed values of the first two adiabatic invariants. It is postulated that these protons were trapped with enhanced efficiency during the March 7, 2012 solar proton event. A model that includes radial diffusion, along with known trapped proton source and loss processes, shows that the observed average rate of increase near L = 2 is predicted by the same model diffusion coefficient that is required to form the entire proton radiation belt, down to low L , over an extended (∼10 3 -year) interval. A slower intensity decrease for lower energies near L = 1.5 may also be caused by inward diffusion, though it is faster than predicted by the model. Higher energy ( 40 MeV) protons near the L = 1.5 intensity maximum are from cosmic ray albedo neutron decay (CRAND). Their observed intensity is lower than expected by a factor ∼2, but the discrepancy is resolved by adding an unspecified loss process to the model with a mean lifetime ∼120 years.
    Print ISSN: 0148-0227
    Thema: Geologie und Paläontologie , Physik
    Publiziert von Wiley im Namen von American Geophysical Union (AGU).
    Standort Signatur Erwartet Verfügbarkeit
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  • 17
    Publikationsdatum: 2013-06-04
    Beschreibung: [1]  Several cases of short-time durational large amplitude 3-dimensional electrostatic solitary waves (ESWs) are observed within the transition layer of the terrestrial bow-shock by THEMIS/E. Their pulse-width is small (0.8 ~ 2 milliseconds) but the amplitude is large (greater than 100 mV/m), suggesting much strong potential drop. Two character angles ( θ 1 and θ 2 ) are defined to describe the 3-D characteristics of the ESWs, and it returns results as 76 0  〉  θ 1  〉 27 0 and 70 0  〉  θ 2  〉 20 0 , suggesting that the electron potential holes are mainly in 3-D ellipsoid-sphere-shaped structure, including “pancake-shaped” structure and “sphere-shaped” structure. None of the theories commonly used to describe ESWs adequately address these pancake-shaped and sphere-shaped 3-dimentional structure observed in the terrestrial bow-shock where ω ce  〈 〈  ω pe in a weak magnetized plasma. The observation of large 3-dimensional ESWs with different spatial structure during small time interval suggests anisotropic distribution of electric potentials and presents evidence of complex wave fluctuation within the bow-shock.
    Print ISSN: 0094-8276
    Digitale ISSN: 1944-8007
    Thema: Geologie und Paläontologie , Physik
    Publiziert von Wiley im Namen von American Geophysical Union (AGU).
    Standort Signatur Erwartet Verfügbarkeit
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  • 18
    Publikationsdatum: 2012-12-05
    Beschreibung: ABSTRACT Temporal trends (1971–2007) in 10-m wind speeds from homogeneous observational data sets from 540 weather stations and reanalysis data sets are quantified and compared. Also, possible physical cause of inconsistencies between the data sets and temporal trends and variability in wind speeds are investigated. Annual mean wind speeds from the observational data exhibit pronounced downward trends especially in the upper percentiles and during spring. The NCEP/NCAR reanalysis reproduces the observed wind speeds, seasonality and temporal trends better than the ERA-40 even though it shows larger interannual fluctuations. The warm and cold AO and ENSO phases have significant influence on probability distribution of wind speeds, thus internal climate variability is a major source of both interannual and long-term variability.
    Print ISSN: 0899-8418
    Digitale ISSN: 1097-0088
    Thema: Geologie und Paläontologie , Physik
    Publiziert von Wiley
    Standort Signatur Erwartet Verfügbarkeit
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  • 19
    Publikationsdatum: 2013-08-20
    Beschreibung: [1]  Ionospheric outflow is believed to be a significant contribution to the magnetospheric plasma population. Ions are extracted from the ionosphere and transported downtail by the large scale convection motion driven by dayside reconnection. In this paper, we use a comprehensive data set of cold ion (total energy less than 70 eV) measurements combined with simultaneous observations from the solar wind to investigate the fate of these ions. By tracing the trajectories of the ions, we are able to find out where in the magnetotail ions end up. By sorting the observation according to geomagnetic activity and solar wind parameters, we then generate maps of the fate regions in the magnetotail and investigate the effects of these drivers. Our results suggest that, on overall, for about 85% of the cases, the outflowing ions are transported to the plasma sheet. The region where the ions are deposited into the plasma sheet is larger during geomagnetic quiet time than during disturbed conditions. A persistent dawn-dusk asymmetry in the plasma sheet deposition is also observed.
    Print ISSN: 0148-0227
    Thema: Geologie und Paläontologie , Physik
    Publiziert von Wiley im Namen von American Geophysical Union (AGU).
    Standort Signatur Erwartet Verfügbarkeit
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  • 20
    Publikationsdatum: 2019
    Beschreibung: Abstract The evolution of planetary boundary‐layer (PBL) was investigated using observations from laser ceilometer, eddy covariance system and automatic meteorological station in the north of Nanjing city during an air pollution episode in 2016‐2017 winter. Based on 7‐day observation under clean to polluted day, we recorded the temporal variations of backscatter signals observed by the ceilometer, and then inter‐compare planetary boundary‐layer height (PBLH) retrieved from individual methods. The results show that backscatter signal gradient, standard deviation, and wavelet transform analysis methods generated similar PBLH values and PBL diurnal variation patterns. Moreover, the PBL structure varied diurnally, with distinct patterns corresponding to clean and polluted days. Based on these measurements, the relationships between PBLH, weather conditions, and contaminants were analyzed. Results show that: on clean days, strong surface turbulence exchange makes the PBL fully developed and makes the PBLH increased sharply after sunrise, with a maximum of 1483 m; on polluted days, stable synoptic conditions and the weaker wind speeds facilitated the accumulation of air pollutants, leading to smaller net surface radiation and weaker turbulence. Consequently, these conditions during polluted days led to lower PBLH values, which were typically less than 900 m.
    Print ISSN: 2169-897X
    Digitale ISSN: 2169-8996
    Thema: Geologie und Paläontologie , Physik
    Publiziert von Wiley im Namen von American Geophysical Union (AGU).
    Standort Signatur Erwartet Verfügbarkeit
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