Detail publikace

Structural changes in solar corona during total solar eclipses

BĚLÍK, M. DRUCKMÜLLER, M. MARKOVÁ, E.

Anglický název

Structural changes in solar corona during total solar eclipses

Typ

Stať ve sborníku v databázi WoS či Scopus

Jazyk

en

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 anglicky

solar eclipse, image processing

Vydáno

2006-03-04

Nakladatel

Cambridge University Press

Místo

Cairo, Egypt

ISBN

978-05-2186-342-1

Kniha

Contributions for IAUS 233 Solar Activity and its Magnetic Origin

Strany od–do

105–

Počet stran

1

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"
}