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  • 1
    Publikationsdatum: 2019-06-27
    Beschreibung: IUE observations indicate that the spectrum of 3C 273 is similar to that of other large-redshift quasars. There is a large excess of flux in the range 2400 A to 5300 A, which encompasses the Balmer jump region but which does not appear to be explainable by Balmer emission. The intensity ratio of Lyman-alpha to H-beta is 5.5, in agreement with other measures and a factor 6 smaller than the recombination value. The only absorption lines in the spectrum are due to our Galaxy. There is marginal evidence for a depression of the continuum shortward of the Lyman-alpha emission line, but the errors are too large to warrant any conclusion that 3C 273 has a rich absorption-line spectrum such as that seen in large-redshift quasars. The absence of emission and absorption lines of Fe II leads to the conclusion that resonance fluorescence probably produces the visual Fe II emission lines.
    Schlagwort(e): ASTRONOMY
    Materialart: Astrophysical Journal; vol. 230
    Format: text
    Standort Signatur Erwartet Verfügbarkeit
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  • 2
    Publikationsdatum: 2019-07-13
    Beschreibung: The model consists of four phases: single electron dynamics, single electron avalanche, negative streamer development, and tree formation. Numerical algorithms and computer code implementations are presented for the first three phases. An approach to developing a code description of fourth phase is discussed. Numerical results are presented for a crude material model of Teflon.
    Schlagwort(e): ELECTRONICS AND ELECTRICAL ENGINEERING
    Materialart: NASA-CR-159560 , SAI-102-79-002
    Format: application/pdf
    Standort Signatur Erwartet Verfügbarkeit
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  • 3
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    Academy of Science of South Africa
    In:  South African Journal of Science, 97 (5-6). pp. 199-208.
    Publikationsdatum: 2020-05-26
    Beschreibung: A multidisciplinary survey on board R.V. Poseidon off Angola and northern Namibia in April 1999 allowed a large-scale view of the South-East Atlantic boundary current system. The data set comprises meteorological, hydrographical, biological and chemical data. Sequences of satellite images of sea-surface temperature and wind stress provided additional synoptic information. Several mesoscale cyclonic gyres were observed embedded in a larger area of low dynamic height, known as the Angola Gyre. The most developed mesoscale feature was the subthermoclinal Angola Dome detected at 9 degreesS, 8.5 degreesE. At the beginning of April, the Angola-Benguela Frontal Zone (ABFZ) was found at an unusually southerly position near 19 degreesS. During the time of the cruise, the zone moved rapidly northward. The dynamics of this event are discussed in detail. The high-frequency temporal variations of the front were closely related to local wind forcing. Below the thermocline the conditions were more persistent. The ABFZ was represented as a front between different types of Central Water. The existence of a poleward undercurrent below the ABFZ, reported in recent publications, was not verified from direct current measurements. However, water mass distribution suggests overall poleward transport below the thermocline.
    Materialart: Article , PeerReviewed
    Format: text
    Standort Signatur Erwartet Verfügbarkeit
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