Detail publikace

Structural changes in solar corona during total solar eclipses

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

1

Strany od

105

Strany do

105

Strany počet

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"
}