An Application of the Random Walk Model to Proper Motions of Coronal Bright Points from SDO Data
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00470316" target="_blank" >RIV/67985815:_____/16:00470316 - isvavai.cz</a>
Alternative codes found
RIV/67985815:_____/16:00488875
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
An Application of the Random Walk Model to Proper Motions of Coronal Bright Points from SDO Data
Original language description
Atmospheric Imaging Assembly (AIA) images from the Solar Dynamics Observatory (SDO) were used to follow the motions of coronal bright points (CBPs) in the period 1 January - 19 May 2011 with a cadence of 10 minutes. This resulted in a data set of 80966 CBPs with measured lifetimes and mean velocities which were used in a random walk model to calculate the diffusion coefficient, D.
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
<a href="/en/project/7E13003" target="_blank" >7E13003: High-Resolution Solar Physics Network</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Central European Astrophysical Bulletin
ISSN
1845-8319
e-ISSN
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Volume of the periodical
40
Issue of the periodical within the volume
1
Country of publishing house
HR - CROATIA
Number of pages
6
Pages from-to
23-28
UT code for WoS article
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EID of the result in the Scopus database
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