{ "id": "1206.4545", "version": "v1", "published": "2012-06-20T16:08:35.000Z", "updated": "2012-06-20T16:08:35.000Z", "title": "Dead calm areas in the very quiet Sun", "authors": [ "M. J. Martínez González", "R. Manso Sainz", "A. Asensio Ramos", "E. Hijano" ], "comment": "accepted in ApJ", "categories": [ "astro-ph.SR" ], "abstract": "We analyze two regions of the quiet Sun (35.6 x 35.6 Mm^2) observed at high spatial resolution (~100 km) in polarized light by the IMaX spectropolarimeter onboard the Sunrise balloon. We identify 497 small-scale (~400 km) magnetic loops, appearing at an effective rate of 0.25 loop h^{-1} arcsec^{-2}; further, we argue that this number and rate are underestimated by ~30%. However, we find that these small dipoles do not appear uniformly on the solar surface: their spatial distribution is rather filamentary and clumpy, creating dead calm areas, characterized by a very low magnetic signal and a lack of organized loop-like structures at the detection level of our instruments, that cannot be explained as just statistical fluctuations of a Poisson spatial process. We argue that this is an intrinsic characteristic of the mechanism that generates the magnetic fields in the very quiet Sun. The spatio-temporal coherences and the clumpy structure of the phenomenon suggest a recurrent, intermittent mechanism for the generation of magnetic fields in the quietest areas of the Sun.", "revisions": [ { "version": "v1", "updated": "2012-06-20T16:08:35.000Z" } ], "analyses": { "keywords": [ "quiet sun", "magnetic fields", "imax spectropolarimeter onboard", "poisson spatial process", "low magnetic signal" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/755/2/175", "journal": "The Astrophysical Journal", "year": 2012, "month": "Aug", "volume": 755, "number": 2, "pages": 175 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1118816, "adsabs": "2012ApJ...755..175M" } } }