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BĚLÍK, M. DRUCKMÜLLER, M. MARKOVÁ, E.
Original Title
Structural changes in solar corona during total solar eclipses
Type
conference paper
Language
English
Original Abstract
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.
Keywords
solar eclipse, image processing
Authors
BĚLÍK, M.; DRUCKMÜLLER, M.; MARKOVÁ, E.
RIV year
2006
Released
4. 3. 2006
Publisher
Cambridge University Press
Location
Cairo, Egypt
ISBN
978-05-2186-342-1
Book
Contributions for IAUS 233 Solar Activity and its Magnetic Origin
Edition
1
Edition number
Pages from
105
Pages to
Pages count
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" }