Abstract The results of the cross-correlation analysis of the amplitude fluctuations of radio waves of the λ = 32 cm band in seven sessions of radio occultation measurements of the northern polar atmosphere of the planet are presented. The existence of the cross-correlation of fluctuations (b χ ≈ 0.6) is established in the altitude realizations in the interval 61.5–65.0 km for two different sessions of radio occultation. Inner layering is revealed in the upper layer of the clouds of the planet at altitudes of 61.5–65.0 km, which is specified by an enhanced turbulence of the atmosphere. It is found that the “lifetime” of the small-scale layered irregularities is no less than 2 days and that their horizontal extension in the meridional direction can exceed ∼130 km. A possible cause of the emergence of the layered structures inside the upper layer of the polar clouds of Venus is discussed.


    Access

    Check access

    Check availability in my library

    Order at Subito €


    Export, share and cite



    Title :

    Radio Wave Fluctuations and Layered Structure of the Upper Region of Venusian Clouds from Radio Occultation Data


    Contributors:

    Published in:

    Cosmic Research ; 41 , 2 ; 135-140


    Publication date :

    2003-03-01


    Size :

    6 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English





    Aerobots to Explore Venusian Clouds

    Izraelevitz, Jacob S. / Hall, Jeffery L. / Rabinovitch, Jason | NTRS | 2019


    Observation of Wave Structures in the Upper Atmosphere by Means of Radio Holographic Analysis of the Radio Occultation Data

    Igarashi, K. / Pavelyev, A. / Hocke, K. et al. | British Library Conference Proceedings | 2001



    NAVIGATION AND COMMUNICATION THROUGH THE VENUSIAN CLOUDS

    Frazier, William / McElrath, Timothy / Lee, Charles | Springer Verlag | 2024