PHASE-CORRELATION BASED MEASUREMENT OF SOLAR ROTATION RATE
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216305%3A26210%2F13%3APU104249" target="_blank" >RIV/00216305:26210/13:PU104249 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
PHASE-CORRELATION BASED MEASUREMENT OF SOLAR ROTATION RATE
Original language description
The presented paper deals with a new method for measurement of the differential rotation rate of the solar photosphere. This method is based on shift measurement using the phase correlation, which does not require any tracing points and long observationover many days and weeks. The method was applied on images taken at 1700- A by the Atmospheric Imaging Assembly (AIA), a part of the Solar Dynamics Observatory (SDO) mission. The results of our measurements are latitudinal dependences of the sidereal rotation period determined from couples of images.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
S - Specificky vyzkum na vysokych skolach
Others
Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
MENDEL 2013
ISBN
978-80-214-4755-4
ISSN
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e-ISSN
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Number of pages
6
Pages from-to
331-336
Publisher name
Brno Univesity of Technology, Faculty of Mechanical Engineering
Place of publication
Brno
Event location
Brno University of Technology
Event date
Jun 26, 2013
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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