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Bright Points in the Internetwork Quiet Sun

2004/05/26 by J. Sanchez Almeida, J. Sánchez Alméida, I. Marquez +7 · 3 citations
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #Artificial intelligence #Astronomy #Astrophysics #Computer science #Condensed matter physics #Geomagnetism and Paleomagnetism Studies #Magnetism #Physics #QUIET #Resolution (logic) #Solar and Space Plasma Dynamics #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1086/422752

published as Astrophys.J. 609 (2004) L91-L94 · To appear in ApJL. 4 pages, 4 figures

arxiv created 2004/05/26 · openalex publication_date 2004/06/09 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

High-resolution G-band images of the interior of a supergranulation cell show ubiquitous bright points (BPs; some 0.3 BPs per Mm 2 ). They are located in intergranular lanes and often form chains of elongated blobs whose smallest dimension is at the resolution limit (135 km on the Sun). Most of them live for a few minutes, having peak intensities from 0.8 to 1.8 times the mean photospheric intensity. These BPs are probably tracing intense magnetic concentrations, whose existence has been inferred in spectropolarimetric measurements. Our finding provides a new convenient tool for the study of the internetwork magnetism, so far restricted to the interpretation of weak polarimetric signals.

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