Differences in physical properties of coronal bright points and their ALMA counterparts within and outside coronal holes

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90259%2F23%3A00583585" target="_blank" >RIV/67985815:90259/23:00583585 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/202244160" target="_blank" >https://doi.org/10.1051/0004-6361/202244160</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202244160" target="_blank" >10.1051/0004-6361/202244160</a>

Result language
angličtina
Original language name
Differences in physical properties of coronal bright points and their ALMA counterparts within and outside coronal holes
Original language description
This study investigates and compares the physical properties, such as intensity and area, of coronal bright points (CBPs) inside and outside of coronal holes (CHs) using the Atacama Large Millimeter/submillimeter Array (ALMA) and Solar Dynamics Observatory (SDO) observations.
Czech name
—
Czech description
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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)

Project
<a href="/en/project/LM2023059" target="_blank" >LM2023059: Atacama Large Millimeter /submillimeter Array – participation of the Czech Republic</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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