Detail publikace

3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006

AMBROŽ, P. DRUCKMÜLLER, M. GALAL, A. HAMID, R.

Anglický název

3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006

Typ

Článek recenzovaný mimo WoS a Scopus

Jazyk

en

Originální abstrakt

The good quality of the observing sequence of about 60 photographs of the white-light corona taken during the total solar eclipse observations on 29 March 2006, in Al Sallum, Egypt, enable us to use a new method of image processing for enhancement of the fine structure of coronal phenomena. We present selected magnetic-field lines derived for different parameters of the extrapolation model. The coincidence of the observed coronal white-light fine structures and the computed field-line positions provides a 3D causal relationship between coronal structures and the coronal magnetic field.

Klíčová slova anglicky

Eclipse observations – Corona, structures – Magnetic fields, corona

Vydáno

2009-07-23

ISSN

0038-0938

Časopis

SOLAR PHYSICS

Ročník

2009(258)

Číslo

2

Strany od–do

243–270

Počet stran

27

BIBTEX


@article{BUT48357,
  author="Pavel {Ambrož} and Miloslav {Druckmüller} and A.A. {Galal} and R.H. {Hamid}",
  title="3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006",
  journal="SOLAR PHYSICS",
  year="2009",
  volume="2009(258)",
  number="2",
  pages="243--270",
  issn="0038-0938"
}