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BĚLÍK, M. DRUCKMÜLLER, M. MARKOVÁ, E.
Originální název
Structural changes in solar corona during total solar eclipses
Typ
článek ve sborníku ve WoS nebo Scopus
Jazyk
angličtina
Originální abstrakt
Total solar eclipses observed on the long baseline allow obtaining the pictures of solar corona with the long temporal distance. New mathematical methods of picture processing allow visualizing very faint coronal structures, which enable to compare their position in corona with very high accuracy. We can detect the moving of these faint structures by comparing of pictures obtained on the different places. Some techniques and results are described in this paper.
Klíčová slova
solar eclipse, image processing
Autoři
BĚLÍK, M.; DRUCKMÜLLER, M.; MARKOVÁ, E.
Rok RIV
2006
Vydáno
4. 3. 2006
Nakladatel
Cambridge University Press
Místo
Cairo, Egypt
ISBN
978-05-2186-342-1
Kniha
Contributions for IAUS 233 Solar Activity and its Magnetic Origin
Edice
1
Číslo edice
Strany od
105
Strany do
Strany počet
URL
http://www.iaus233.edu.eg/Final%20Abstract%20Book.pdf
BibTex
@inproceedings{BUT18431, author="Marcel {Bělík} and Miloslav {Druckmüller} and Eva {Marková}", title="Structural changes in solar corona during total solar eclipses", booktitle="Contributions for IAUS 233 Solar Activity and its Magnetic Origin", year="2006", series="1", number="1", pages="1", publisher="Cambridge University Press", address="Cairo, Egypt", isbn="978-05-2186-342-1", url="http://www.iaus233.edu.eg/Final%20Abstract%20Book.pdf" }