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
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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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