Úplná zatmění Slunce v průběhu devatenácti let

Kód výsledku v 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>

Výsledek na webu

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DOI - Digital Object Identifier

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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.

Druh

O - Ostatní výsledky

CEP obor

BN - Astronomie a nebeská mechanika, astrofyzika

OECD FORD obor

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Projekt

<a href="/cs/project/GA205%2F09%2F1469" target="_blank" >GA205/09/1469: Studium slunečních koronálních struktur a jejich dynamiky</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2009

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů