Modeling the quiet Sun cell and network emission with ALMA
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00539664" target="_blank" >RIV/67985815:_____/20:00539664 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/202038461" target="_blank" >https://doi.org/10.1051/0004-6361/202038461</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202038461" target="_blank" >10.1051/0004-6361/202038461</a>
Alternative languages
Result language
angličtina
Original language name
Modeling the quiet Sun cell and network emission with ALMA
Original language description
Observations of the Sun at millimeter wavelengths with the Atacama Large Millimeter/submillimeter Array (ALMA) offer a unique opportunity to investigate the temperature structure of the solar chromosphere. In this article we expand our previous work on modeling the chromospheric temperature of the quiet Sun, by including measurements of the brightness temperature in the network and cell interiors, from high-resolution ALMA images at 3 mm (Band 3) and 1.26 mm (Band 6). We also examine the absolute calibration of ALMA full-disk images.
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
2020
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
1432-0746
e-ISSN
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Volume of the periodical
640
Issue of the periodical within the volume
August
Country of publishing house
FR - FRANCE
Number of pages
10
Pages from-to
A57
UT code for WoS article
000560449600001
EID of the result in the Scopus database
2-s2.0-85089775668