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Onset of convection in a basally heated spherical shell, application to planets

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F09%3A00206443" target="_blank" >RIV/00216208:11320/09:00206443 - isvavai.cz</a>

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Onset of convection in a basally heated spherical shell, application to planets

  • Original language description

    Onset times of convection in a basally heated spherical shell are investigated in order to obtain scaling relationships for the influences of Rayleigh number, viscosity parameter describing the dependency on the temperature and geometry of spherical shell. The obtained scalings are then applied to the dimensions and plausible initial state of terrestrial planets (Mars, the Earth and Venus

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    DE - Earth magnetism, geodesy, geography

  • OECD FORD branch

Result continuities

  • Project

  • Continuities

    Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2009

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Physics of the Earth and Planetary Interiors

  • ISSN

    0031-9201

  • e-ISSN

  • Volume of the periodical

    176

  • Issue of the periodical within the volume

    3-4

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    17

  • Pages from-to

  • UT code for WoS article

    000270635900002

  • EID of the result in the Scopus database