2008/03/13 by S. Pohjolainen · 13 citations
Physics and Astronomy · #Astronomy #Astrophysics #Coronal mass ejection #Flare #Interplanetary spaceflight #Ionosphere and magnetosphere dynamics #Mechanics #Physics #Plasma #Shock (circulatory) #Shock wave #Solar and Space Plasma Dynamics #Solar flare #Solar radio #Solar wind #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20079155
published in Astronomy and Astrophysics 483(1), 297-300 (EDP Sciences) · 4 pages, 3 figures, accepted by A&A (Research Note)
arxiv created 2008/03/13 · openalex publication_date 2008/03/19 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims. We identify the source of fast-drifting decimetric-metric radio emission that is sometimes observed prior to the so-called flare continuum emission. Fast-drift structures and continuum bursts are also observed in association with coronal mass ejections (CMEs), not only flares.