Úplná zatmění Slunce v průběhu devatenácti let
Popis výsledku
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
Identifikátory výsledku
Kód výsledku v IS VaVaI
Výsledek na webu
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DOI - Digital Object Identifier
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Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Total Solar Eclipses through Nineteen Years
Popis výsledku v původním jazyce
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.
Název v anglickém jazyce
Total Solar Eclipses through Nineteen Years
Popis výsledku anglicky
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.
Klasifikace
Druh
O - Ostatní výsledky
CEP obor
BN - Astronomie a nebeská mechanika, astrofyzika
OECD FORD obor
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Návaznosti výsledku
Projekt
GA205/09/1469: Studium slunečních koronálních struktur a jejich dynamiky
Návaznosti
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Ostatní
Rok uplatnění
2009
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Druh výsledku
O - Ostatní výsledky
CEP
BN - Astronomie a nebeská mechanika, astrofyzika
Rok uplatnění
2009