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Quasi-periodic Fast-mode Magnetosonic Wave Trains Within Coronal Waveguides Associated with Flares and CMEs

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00472820" target="_blank" >RIV/67985815:_____/16:00472820 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1063/1.4943821" target="_blank" >http://dx.doi.org/10.1063/1.4943821</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1063/1.4943821" target="_blank" >10.1063/1.4943821</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Quasi-periodic Fast-mode Magnetosonic Wave Trains Within Coronal Waveguides Associated with Flares and CMEs

  • Original language description

    Quasi-periodic, fast-mode, propagating wave trains (QFPs) are a new observational phenomenon recently discovered in the solar corona by the Solar 11)ynamics Observatory with extreme ultraviolet (EUV) imaging observations. They originate from flares and propagate at speeds up to similar to 2000 km s(-1) within funnel-shaped waveguides in the wakes of coronal mass ejections (CMEs). QFPs can carry sufficient energy fluxes required for coronal heating during their occurrences. They can provide new diagnostics for the solar corona and their associated flares. We present recent observations of QFPs focusing on their spatio-temporal properties, temperature dependence, and statistical correlation with flares and CMEs. Of particular interest is the 2010-Aug-01 C3.2 flare with correlated QFPs and drifting zebra and fiber radio bursts, which might be different manifestations of the same fast-mode wave trains. We also discuss the potential roles of QFPs in accelerating and/or modulating the solar wind.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GAP209%2F12%2F0103" target="_blank" >GAP209/12/0103: Radio and X-ray diagnostics of primary-energy-release processes in solar flares and their numerical simulations</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2016

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Solar Wind 14: Proceedings of the Fourteenth International Solar Wind Conference

  • ISBN

    9780735413672

  • ISSN

    0094-243X

  • e-ISSN

  • Number of pages

    4

  • Pages from-to

    "040010/1"-"040010/4"

  • Publisher name

    American Institute of Physics

  • Place of publication

    Melville

  • Event location

    Weihai

  • Event date

    Jun 22, 2015

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000392692000021