Total Solar Eclipses in Mathematical Processing Epoch

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216305%3A26210%2F09%3APU81270" target="_blank" >RIV/00216305:26210/09:PU81270 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Total Solar Eclipses in Mathematical Processing Epoch
Original language description
Observation of total solar eclipses, processed by new mathematical methods, allow us to study very faint structures never seen before during eclipse. These structures are visible practically continuously from solar chromosphere to several dozens of solarradii. Moreover, coordinate observation of solar eclipse from different places of totality path allow us to observe dynamic of coronal plasma. We present interesting examples of detected dynamic of coronal structures, as well as reflections concerning of some commonly used parameters of solar corona.
Czech name
Úplná zatmění Slunce v epoše matematického zpracování
Czech description
Observation of total solar eclipses, processed by new mathematical methods, allow us to study very faint structures never seen before during eclipse. These structures are visible practically continuously from solar chromosphere to several dozens of solarradii. Moreover, coordinate observation of solar eclipse from different places of totality path allow us to observe dynamic of coronal plasma. We present interesting examples of detected dynamic of coronal structures, as well as reflections concerning of some commonly used parameters of solar corona.

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)

Publication year
2009
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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