Detail publikace
Total Solar Eclipses in Mathematical Processing Epoch
BĚLÍK, M. MARKOVÁ, E. KŘIVSKÝ, L. DRUCKMÜLLEROVÁ, H. DRUCKMÜLLER, M.
Anglický název
Total Solar Eclipses in Mathematical Processing Epoch
Typ
Konferenční sborník (ne stať)
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.
Klíčová slova anglicky
eclipse, coronal structures
Vydáno
2009-07-23
Nakladatel
Nanjing University
Místo
Nanjing, Čína
Kniha
The Dynamic Solar Corona
Strany od–do
8–8
Počet stran
1
BIBTEX
@proceedings{BUT65510,
editor="Marcel {Bělík} and Eva {Marková} and Ladislav {Křivský} and Hana {Druckmüllerová} and Miloslav {Druckmüller}",
title="Total Solar Eclipses in Mathematical Processing Epoch",
year="2009",
number="1",
pages="8--8",
publisher="Nanjing University",
address="Nanjing, Čína"
}