On the Nature of Prominence Bubbles and Plumes

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00386695" target="_blank" >RIV/67985815:_____/12:00386695 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
On the Nature of Prominence Bubbles and Plumes
Original language description
An example of bubble and related plume, using time series in selected SDO/AIA channels and co-temporal MSDP observations in the Ha line obtained at Wroclaw-Bialkow observatory on April 20, 2011 is presented. The formation of bubbles may be due to emerging arcades in the filament channel, below the prominence. After discussing on MHD modeling, we conclude that bubbles and plumes are parts of the corona observed through gaps/windows in the prominence.
Czech name
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Czech description
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Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
The Fifth Hinode Science Meeting: Exploring the active Sun
ISBN
9781583817940
ISSN
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e-ISSN
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Number of pages
2
Pages from-to
77-78
Publisher name
Astronomical Society otf the Pacific
Place of publication
San Francisco
Event location
Cambridge
Event date
Oct 10, 2011
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000308615700016

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