Detail publikace

Úplná zatmění Slunce v průběhu devatenácti let

MARKOVÁ, E. BĚLÍK, M. KŘIVSKÝ, L. DRUCKMÜLLEROVÁ, H. DRUCKMÜLLER, M.

Český název

Úplná zatmění Slunce v průběhu devatenácti let

Anglický název

Total Solar Eclipses through Nineteen Years

Typ

konferenční sborník (ne článek)

Jazyk

en

Originální abstrakt

Observatory Upice in Czech Republic starts the observations of total solar eclipses in the epoch of phenomenal progress of satellite observation of the Sun. In this epoch the interest in terrestrial observations of solar eclipses temporary fallen down. This situation changed after applying of new mathematical methods of coronal picture processing. These methods allow us to detect very faint structures in solar corona, especially in the lowest part of it. This low layer of solar atmosphere, directly connected with chromosphere and often hidden for space and terrestrial coronagraphs, plays key role in transferring of energy from the Sun and other processes. We present development of observational and processing methods used by authors, as well as some examples of coronal pictures processed by traditional and mathematical methods.

Český abstrakt

Observatory Upice in Czech Republic starts the observations of total solar eclipses in the epoch of phenomenal progress of satellite observation of the Sun. In this epoch the interest in terrestrial observations of solar eclipses temporary fallen down. This situation changed after applying of new mathematical methods of coronal picture processing. These methods allow us to detect very faint structures in solar corona, especially in the lowest part of it. This low layer of solar atmosphere, directly connected with chromosphere and often hidden for space and terrestrial coronagraphs, plays key role in transferring of energy from the Sun and other processes. We present development of observational and processing methods used by authors, as well as some examples of coronal pictures processed by traditional and mathematical methods.

Anglický abstrakt

Observatory Upice in Czech Republic starts the observations of total solar eclipses in the epoch of phenomenal progress of satellite observation of the Sun. In this epoch the interest in terrestrial observations of solar eclipses temporary fallen down. This situation changed after applying of new mathematical methods of coronal picture processing. These methods allow us to detect very faint structures in solar corona, especially in the lowest part of it. This low layer of solar atmosphere, directly connected with chromosphere and often hidden for space and terrestrial coronagraphs, plays key role in transferring of energy from the Sun and other processes. We present development of observational and processing methods used by authors, as well as some examples of coronal pictures processed by traditional and mathematical methods.

Klíčová slova česky

zatmění, korńa

Klíčová slova anglicky

eclipse, corona

Vydáno

23.07.2009

Nakladatel

Nanjing University

Místo

Nanjing, Čína

Kniha

The Dynamic Solar Corona

Číslo edice

1

Strany od–do

56–56

Počet stran

1

BIBTEX


@proceedings{BUT65511,
  author="Eva {Marková} and Marcel {Bělík} and Ladislav {Křivský} and Hana {Druckmüllerová} and Miloslav {Druckmüller},
  title="Total Solar Eclipses through Nineteen Years",
  booktitle="The Dynamic Solar Corona",
  year="2009",
  month="July",
  pages="56--56",
  publisher="Nanjing University",
  address="Nanjing, Čína"
}