Combined helioseismic inversions for 3D vector flows and sound-speed perturbations
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00511458" target="_blank" >RIV/67985815:_____/19:00511458 - isvavai.cz</a>
Alternative codes found
RIV/00216208:11320/19:10405016
Result on the web
<a href="http://hdl.handle.net/11104/0301724" target="_blank" >http://hdl.handle.net/11104/0301724</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201833000" target="_blank" >10.1051/0004-6361/201833000</a>
Alternative languages
Result language
angličtina
Original language name
Combined helioseismic inversions for 3D vector flows and sound-speed perturbations
Original language description
We introduce an improved methodology of the time-distance helioseismology which allows us to invert for a full 3D vector of plasma flows and the sound-speed perturbations at once. Using this methodology one can also derive the mean value of the vertical component of plasma flows and the cross-talk between the plasma flows and the sound-speed perturbations.n
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
<a href="/en/project/GA18-06319S" target="_blank" >GA18-06319S: Evolution of sunspots and active regions</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2019
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
—
Volume of the periodical
622
Issue of the periodical within the volume
February
Country of publishing house
FR - FRANCE
Number of pages
12
Pages from-to
A163
UT code for WoS article
000458599600002
EID of the result in the Scopus database
2-s2.0-85061772879