- Pravděpodobně máte vypnutý JavaScript. Některé funkce portálu nebudou funkční.
Výsledky výzkumu a vývoje
Detail publikace
| Originální název: | Total Solar Eclipses in Mathematical Processing Epoch |
|---|---|
| Český název: | Úplná zatmění Slunce v epoše matematického zpracování |
| Anglický název: | Total Solar Eclipses in Mathematical Processing Epoch |
| Autor(ři): | BĚLÍK, M.; MARKOVÁ, E.; KŘIVSKÝ, L.; DRUCKMÜLLEROVÁ, H.; DRUCKMÜLLER, M. |
| Typ: | konferenční sborník, ne článek |
| Jazyk: | en |
| Originální abstrakt: | 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 solar radii. 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. |
| Český abstrakt: | 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 solar radii. 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. |
| Anglický abstrakt: | 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 solar radii. 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. |
| Klíčová slova: | zatmění, koronální sturktury |
| Vydáno: | 23.07.2009 |
| Nakladatel: | Nanjing University |
| Místo: | Nanjing, Čína |
| Strany od: | 8 |
| Strany do: | 8 |
| Strany počet: | 1 |
