Detail publikace

Total Solar Eclipses in Mathematical Processing Epoch

BĚLÍK, M. MARKOVÁ, E. KŘIVSKÝ, L. DRUCKMÜLLEROVÁ, H. DRUCKMÜLLER, M.

Originální název

Total Solar Eclipses in Mathematical Processing Epoch

Typ

konferenční sborník (ne článek)

Jazyk

angličtina

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

eclipse, coronal structures

Autoři

BĚLÍK, M.; MARKOVÁ, E.; KŘIVSKÝ, L.; DRUCKMÜLLEROVÁ, H.; DRUCKMÜLLER, M.

Vydáno

23. 7. 2009

Nakladatel

Nanjing University

Místo

Nanjing, Čína

Strany od

8

Strany do

8

Strany počet

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"
}