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  • 1965-1969  (3)
Material
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  • 1965-1969  (3)
Year
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Subjects(RVK)
  • 1
    Online Resource
    Online Resource
    Ausscheidungsverhalten von Nickel-Vanadium-Legierungen
    Walter de Gruyter GmbH ; 1969
    In:  International Journal of Materials Research Vol. 60, No. 11 ( 1969-11-01), p. 835-839
    Details
    In: International Journal of Materials Research, Walter de Gruyter GmbH, Vol. 60, No. 11 ( 1969-11-01), p. 835-839
    Type of Medium: Online Resource
    ISSN: 2195-8556 , 1862-5282
    URL: Article
    DOI: 10.1515/ijmr-1969-601103
    RVK:
    ZG 1100
    Language: English
    Publisher: Walter de Gruyter GmbH
    Publication Date: 1969
    detail.hit.zdb_id: 2232675-3
    detail.hit.zdb_id: 2128058-7
    detail.hit.zdb_id: 203021-4
    Location Call Number Limitation Availability
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    Online Resource
  • 2
    Online Resource
    Online Resource
    ZUM MOZART-STIL
    Brill Osterreich GmbH ; 1969
    In:  Österreichische Musikzeitschrift Vol. 24, No. JG ( 1969-01)
    Details
    In: Österreichische Musikzeitschrift, Brill Osterreich GmbH, Vol. 24, No. JG ( 1969-01)
    Type of Medium: Online Resource
    ISSN: 2307-2970 , 0029-9316
    URL: Article
    DOI: 10.7767/omz.1969.24.jg.433
    RVK:
    LD 8700
    Language: Unknown
    Publisher: Brill Osterreich GmbH
    Publication Date: 1969
    detail.hit.zdb_id: 2558595-2
    detail.hit.zdb_id: 206605-1
    SSG: 9,2
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  • 3
    Online Resource
    Online Resource
    B. The Solar Atmospheric Convection Zone
    Cambridge University Press (CUP) ; 1967
    In:  Symposium - International Astronomical Union Vol. 28 ( 1967), p. 347-404
    Details
    In: Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 28 ( 1967), p. 347-404
    Abstract: Observational progress has, in the last decade, greatly surpassed theoretical progress in our study of the non-thermal velocity fields in the solar photosphere and chromosphere. This differential progress has not been simply a matter of filling in details. Attempted formulation of the theoretical problem of the velocity fields arising from convective instability in stellar atmospheres has resulted in no really new conceptual developments, nor large clarifications in approach, to match the observational ones just summarized by Noyes. Discussion of the problem at Varenna consisted mainly in the expression by aerodynamicists of severe reservations on the likelihood of gaining deep physical insight, or reliable numerical results, from the mixing-length approach generally used in astrophysics, with essentially no suggestions of a better approach. What progress that has been made in the general area of convective problems similar to those of interest in stellar atmospheres lies in the exploration of the physical structure of simplified convective configurations, often by exploration of various intuitive approaches.
    Type of Medium: Online Resource
    ISSN: 0074-1809
    URL: Article
    DOI: 10.1017/S0074180900019057
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 1967
    SSG: 16,12
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