Publication detail
Total Solar Eclipses through Nineteen Years
MARKOVÁ, E. BĚLÍK, M. KŘIVSKÝ, L. DRUCKMÜLLEROVÁ, H. DRUCKMÜLLER, M.
Czech title
Úplná zatmění Slunce v průběhu devatenácti let
English title
Total Solar Eclipses through Nineteen Years
Type
conference proceedings
Language
en
Original abstract
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.
Czech abstract
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.
English abstract
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.
Keywords in Czech
zatmění, korńa
Keywords in English
eclipse, corona
Released
23.07.2009
Publisher
Nanjing University
Location
Nanjing, Čína
Book
The Dynamic Solar Corona
Edition number
1
Pages from–to
56–56
Pages count
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"
}