Total Solar Eclipses through Nineteen Years
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216305%3A26210%2F09%3APU81271" target="_blank" >RIV/00216305:26210/09:PU81271 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Total Solar Eclipses through Nineteen Years
Original language description
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 name
Úplná zatmění Slunce v průběhu devatenácti let
Czech description
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.
Classification
Type
O - Miscellaneous
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GA205%2F09%2F1469" target="_blank" >GA205/09/1469: Study of solar coronal structures and their dynamics</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2009
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů