Bright Points in the Internetwork Quiet Sun
Author(s) -
J. Sánchez Alméida,
I. Márquez,
José Bonet,
I. Domínguez Cerdeña,
R. Müller
Publication year - 2004
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/422752
Subject(s) - physics , quiet , astrophysics , magnetism , resolution (logic) , astronomy , condensed matter physics , computer science , artificial intelligence
High resolution G-band images of the interior of a supergranulation cell showubiquitous Bright Points (some 0.3 BPs per Mm^2). They are located inintergranular lanes and often form chains of elongated blobs whose smallestdimension is at the resolution limit (135 km on the Sun). Most of them live fora few minutes, having peak intensities from 0.8 to 1.8 times the meanphotospheric intensity. These BPs are probably tracing intense magneticconcentrations, whose existence has been inferred in spectro-polarimetricmeasurements. Our finding provides a new convenient tool for the study of theinter-network magnetism, so far restricted to the interpretation weakpolarimetric signals.Comment: To appear in ApJL. 4 pages, 4 figure
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom