Abstract A model study of the solar eclipse induced variations in mesospheric ozone concentrations was undertaken. This study includes, in addition to the Chapman reactions, the chemistry involving hydrogen species (H, OH and HO2) which are found to be important in the destruction of odd oxygen in this altitude region. Coupled time dependent continuity equations are solved for the eclipse duration. The results from the present study are compared with earlier theoretical model and the experimental observations during the 16 February 1980 solar eclipse as well as the results obtained during earlier solar eclipses.


    Zugriff

    Zugriff prüfen

    Verfügbarkeit in meiner Bibliothek prüfen

    Bestellung bei Subito €


    Exportieren, teilen und zitieren



    Titel :

    Solar eclipse induced variations in mesospheric ozone concentrations


    Beteiligte:
    Lal, S. (Autor:in) / Subbaraya, B.H. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1983-01-01


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



    Mesospheric ozone densities deduced from solar occultation measurements

    Ohle, K.H. / Sonnemann, G. / Fichtelmann, B. | Elsevier | 1984


    OSIRIS Retrievals of Daytime Mesospheric Ozone

    Sheese, P.E. / Llewellyn, E.J. / McDade, I.C. et al. | British Library Conference Proceedings | 2009


    A mesospheric ozone profile at sunset

    Yamamoto, H. / Sekiguchi, H. / Makino, T. et al. | Elsevier | 1983


    Mesospheric Ozone: Product Status and Potential Improvements

    Darrell Dolliver / Robbie Manion / Robert Damadeo et al. | NTRS