On the Visibility of Prominence Fine Structures at Radio Millimeter Wavelengths
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00450489" target="_blank" >RIV/67985815:_____/15:00450489 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1007/s11207-015-0719-7" target="_blank" >http://dx.doi.org/10.1007/s11207-015-0719-7</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11207-015-0719-7" target="_blank" >10.1007/s11207-015-0719-7</a>
Alternative languages
Result language
angličtina
Original language name
On the Visibility of Prominence Fine Structures at Radio Millimeter Wavelengths
Original language description
The aim of this article is to predict the visibility of prominence fine structures in the submillimeter/millimeter (SMM) domain, to estimate their brightness temperatures at various wavelengths, and to demonstrate the feasibility and usefulness of futurehigh-resolution radio observations of solar prominences with ALMA (Atacama Large Millimeter-submillimeter Array). Our novel approach is the conversion of H coronagraphic images into microwave spectral images. We show that the spatial variations of the prominence brightness both in the H line and in the SMM domain predominantly depend on the line-of-sight emission measure of the cool plasma, which we derive from the integrated intensities of the observed H line. We also describe how we determine the prominence kinetic temperature from SMM spectral images. Finally, we apply the ALMA image-processing software Common Astronomy Software Applications (CASA) to our simulated images to assess what ALMA would detect at a resolution level that i
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Solar Physics
ISSN
0038-0938
e-ISSN
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Volume of the periodical
290
Issue of the periodical within the volume
7
Country of publishing house
NL - THE KINGDOM OF THE NETHERLANDS
Number of pages
20
Pages from-to
1981-2000
UT code for WoS article
000359738800008
EID of the result in the Scopus database
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