Magnetism of Solar Flares and Prominences

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00386872" target="_blank" >RIV/67985815:_____/12:00386872 - 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
Magnetism of Solar Flares and Prominences
Original language description
We give an overview of magnetic fields in solar flares and prominences. Magnetic fields related to flares play a crucial role in the process of energy release and transport to the lower atmosphere, and thus magnetometry under the coronal and chromospheric conditions is extremely challenging. Magnetic fields in prominences are supposed to keep the prominence plasma at coronal heights against the gravity. Their measurements have been numerous, but high-resolution mapping is still missing. We discuss various flare and prominence models in connection to current and future high-resolution observations.
Czech name
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Czech description
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Project
<a href="/en/project/GAP209%2F10%2F1680" target="_blank" >GAP209/10/1680: Energetic Processes In Solar Atmosphere: Relations of Simulations to Observations</a><br>
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)

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

Article name in the collection
The Second ATST-EAST Meeting: Magnetic Fields from the Photosphere to the Corona
ISBN
9781583818084
ISSN
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e-ISSN
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Number of pages
12
Pages from-to
121-132
Publisher name
Astronomical Society otf the Pacific
Place of publication
San Francisco
Event location
Washington
Event date
Nov 9, 2011
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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