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AMBROŽ, P. DRUCKMÜLLER, M. GALAL, A. HAMID, R.
Originální název
3D Coronal Structures and Magnetic Field During the Total Solar Eclipse of 29 March 2006
Typ
článek v časopise - ostatní, Jost
Jazyk
angličtina
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
Eclipse observations - Corona, structures - Magnetic fields, corona
Autoři
AMBROŽ, P.; DRUCKMÜLLER, M.; GALAL, A.; HAMID, R.
Rok RIV
2009
Vydáno
23. 7. 2009
ISSN
0038-0938
Periodikum
Solar Physics
Ročník
2009(258)
Číslo
2
Stát
Nizozemsko
Strany od
243
Strany do
270
Strany počet
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" }