Publication detail
Total Solar Eclipses in Mathematical Processing Epoch
BĚLÍK, M. MARKOVÁ, E. KŘIVSKÝ, L. DRUCKMÜLLEROVÁ, H. DRUCKMÜLLER, M.
English title
Total Solar Eclipses in Mathematical Processing Epoch
Type
Conference proceedings
Language
en
Original abstract
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.
Keywords in English
eclipse, coronal structures
Released
2009-07-23
Publisher
Nanjing University
Location
Nanjing, Čína
Book
The Dynamic Solar Corona
Pages from–to
8–8
Pages count
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"
}