Heating of the solar chromosphere through current dissipation
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00569092" target="_blank" >RIV/67985815:_____/22:00569092 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/202243191" target="_blank" >https://doi.org/10.1051/0004-6361/202243191</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202243191" target="_blank" >10.1051/0004-6361/202243191</a>
Alternative languages
Result language
angličtina
Original language name
Heating of the solar chromosphere through current dissipation
Original language description
We aim to investigate the magnetic topology associated with an area of enhanced millimeter (mm) brightness temperatures in a solar active region mapped by the Atacama Large Millimeter/submillimeter Array (ALMA) using spectropolarimetric co-observations with the 1-m Swedish Solar Telescope (SST).
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
—
Continuities
—
Others
Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy & Astrophysics
ISSN
0004-6361
e-ISSN
1432-0746
Volume of the periodical
661
Issue of the periodical within the volume
May
Country of publishing house
FR - FRANCE
Number of pages
17
Pages from-to
A59
UT code for WoS article
000789980900003
EID of the result in the Scopus database
2-s2.0-85129842402