Spectroscopic Observations of Coronal Rain Formation and Evolution following an X2 Solar Flare

A significant impediment to solving the coronal heating problem is that we currently only observe active region (AR) loops in their cooling phase. Previous studies showed that the evolution of cooling loop densities and apex temperatures are insensitive to the magnitude, duration, and location of en...

Ausführliche Beschreibung

Bibliographische Detailangaben

Hauptverfasser:	Brooks, David H, Reep, Jeffrey W, Ugarte-Urra, Ignacio, Unverferth, John E, Warren, Harry P
Format:	Artikel
Sprache:	eng
Schlagworte:	Physics - Solar and Stellar Astrophysics
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!