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P-mode induced convective collapse in vertical expanding magnetic flux tubes?

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00485019" target="_blank" >RIV/67985815:_____/17:00485019 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1017/S174392131700401X" target="_blank" >http://dx.doi.org/10.1017/S174392131700401X</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S174392131700401X" target="_blank" >10.1017/S174392131700401X</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    P-mode induced convective collapse in vertical expanding magnetic flux tubes?

  • Original language description

    Small-scale kG strong magnetic field elements in the solar photosphere are often identified as so-called magnetic bright points (MBPs). In principle these MBPs represent the cross-section of a vertical, strong, magnetic flux tube which is expanding with height in thensolar atmosphere. As these magnetic elements re present possible MHD wave guides, a significant interest has been already paid to them from the viewpoint of observations and simulations. In this work we would like to shed more light on a possible scenario for the creation of such strong magnetic field concentrations. The accepted standard scenario involves the convective collapse process. In this ongoing work we will show indications that this convective collapse process maybecome triggered by sufficiently strong pressure disturbances. However, it is highly unlikely that p-mode waves can be of such a strength.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • 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

  • Article name in the collection

    Fine Structure and Dynamics of the Solar Atmosphere

  • ISBN

    9781107170049

  • ISSN

    1743-9213

  • e-ISSN

  • Number of pages

    8

  • Pages from-to

    86-93

  • Publisher name

    Cambridge University Press

  • Place of publication

    Cambridge

  • Event location

    Cartagena de Indias

  • Event date

    Oct 9, 2016

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000455235900014