The structure and dynamics of a bright point as seen with Hinode, SoHO and TRACE

2008/10/01 by D. Pérez-Suárez, David Pérez–Suárez, R. C. Maclean +2 · 1 citation
Physics and Astronomy · #Astro and Planetary Science #Solar and Space Plasma Dynamics #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809507

10 pages with 11 figures. Accepted in Astronomy and Astrophysics

openalex publication_date 2008/10/01 · arxiv created 2008/10/06 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31

Abstract

Context. Solar coronal bright points have been studied for more than three decades, but some fundamental questions about their formation and evolution still remain unanswered.

Citations

• Coronal plasma flows and magnetic fields in solar active regions

Cited by

• Dynamics of Coronal Bright Points as Seen by Sun Watcher Using Active Pixel System Detector and Image Processing (SWAP), Atmospheric Imaging Assembly (AIA), and Helioseismic and Magnetic Imager (HMI)