SOHO/SUMER observations of prominence oscillation before eruption

2008/02/14 by P. F. Chen, D. E. Innes, S. K. Solanki · 92 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Coronal mass ejection #Ionosphere and magnetosphere dynamics #Oscillation (cell signaling) #Protein filament #Solar and Space Plasma Dynamics #Solar prominence #Space (punctuation) #Space weather #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809544

published in Astronomy and Astrophysics 484(2), 487-493 (EDP Sciences) · 14 pages, 8 figures, submitted for publication in A&A

arxiv created 2008/02/14 · openalex publication_date 2008/03/11 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Coronal mass ejections (CMEs), as a large-scale eruptive phenomenon, often reveal some precursors in the initiation phase, e.g., X-ray brightening, filament darkening, etc., which are useful for CME modelling and space weather forecasting.

Citations

• The Large Angle Spectroscopic Coronagraph (LASCO)
• A Practical Guide to Wavelet Analysis

Cited by

• Large-amplitude Longitudinal Oscillations Triggered by the Merging of Two Solar Filaments: Observations and Magnetic Field Analysis
• Hemispheric Preference and Cyclic Variation of Solar Filament Chirality from 2000 to 2016
• Some interesting topics provoked by the solar filament research in the past decade