The formation and disappearance of filament barbs observed by SDO
Abstract
Employing six-day (August 16-21, 2010) SDO/AIA observations, we systematically investigate the formation and disappearance of 58 barbs of a northern (~N60) polar crown filament. Three different ways of barb formation are discovered, including (1) the convergence of surrounding moving materials (55.2%), (2) the flows of materials from the filament (37.9%), and (3) the material injections from neighboring brightening regions (6.9%). We also find three different types of barb disappearance, involving: (i) the bi-lateral movements (44.8%), and (ii) the outflowing (27.6%) of barb material resulting in the barb disappearance, as well as (iii) the barb disappearance associated with neighboring brightenings (27.6%). We propose that barbs exchange materials with the filament, surrounding atmosphere, and nearby brightening regions, causing the barb formation and disappearance.
- Publication:
-
Nature of Prominences and their Role in Space Weather
- Pub Date:
- January 2014
- DOI:
- 10.1017/S1743921313010727
- Bibcode:
- 2014IAUS..300...44L
- Keywords:
-
- Sun: filaments;
- Sun: prominences;
- Sun: evolution;
- Sun: corona