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Magnetic and velocity fields in a dynamo operating at extremely small Ekman and magnetic Prandtl numbers

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985530%3A_____%2F17%3A00486241" target="_blank" >RIV/67985530:_____/17:00486241 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1515/congeo-2017-0014" target="_blank" >http://dx.doi.org/10.1515/congeo-2017-0014</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1515/congeo-2017-0014" target="_blank" >10.1515/congeo-2017-0014</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Magnetic and velocity fields in a dynamo operating at extremely small Ekman and magnetic Prandtl numbers

  • Original language description

    Numerical simulations of the geodynamo are becoming more realistic becausenof advances in computer technology. Here, the geodynamo model is investigated numerically at the extremely low Ekman and magnetic Prandtl numbers using the PARODY dynamo code. These parameters are more realistic than those used in previous numerical studies of the geodynamo. Our model is based on the Boussinesq approximation and the temperature gradient between upper and lower boundaries is a source of convection. This study attempts to answer the question how realistic the geodynamo models are. Numerical results show that our dynamo belongs to the strong-field dynamos. The generated magnetic field is dipolar and large-scale while convection is small-scale and sheet-like flows (plumes) are preferred to a columnar convection. Scales of magnetic and velocity fields are separated, which enables hydromagnetic dynamos to maintain the magnetic field atnthe low magnetic Prandtl numbers. The inner core rotation rate is lower than that innprevious geodynamo models. On the other hand, dimensional magnitudes of velocity and magnetic fields and those of the magnetic and viscous dissipation are larger than those expected in the Earth’s core due to our parameter range chosen.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10508 - Physical geography

Result continuities

  • Project

    <a href="/en/project/LG13042" target="_blank" >LG13042: Support of activities in management structures of International Association of Geomagnetism and Aeronomy (IAGA)</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2017

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Contributions to Geophysics & Geodesy

  • ISSN

    1335-2806

  • e-ISSN

  • Volume of the periodical

    47

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    SK - SLOVAKIA

  • Number of pages

    16

  • Pages from-to

    261-276

  • UT code for WoS article

    000425657300001

  • EID of the result in the Scopus database

    2-s2.0-85042107260