Publication detail

Structural changes in solar corona during total solar eclipses

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

1

Pages from

105

Pages to

105

Pages count

1

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"
}