On the structure and evolution of a polar crown prominence/filament system

Polar crown prominences are made of chromospheric plasma partially circling the Suns poles between 60 and 70 degree latitude. We aim to diagnose the 3D dynamics of a polar crown prominence using high cadence EUV images from the Solar Dynamics Observatory (SDO)/AIA at 304 and 171A and the Ahead space...

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Veröffentlicht in:	arXiv.org 2014-02
Hauptverfasser:	Panesar, N K, Innes, D E, Schmit, D J, Tiwari, S K
Format:	Artikel
Sprache:	eng
Schlagworte:	Color imagery Columns (structural) Evolution Observatories Physics - Solar and Stellar Astrophysics Prominences Solar activity Solar corona Solar observatories Topology
Online-Zugang:	Volltext
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