{ "id": "1105.2157", "version": "v1", "published": "2011-05-11T11:32:24.000Z", "updated": "2011-05-11T11:32:24.000Z", "title": "Observations of the forward scattering Hanle effect in the Ca i 4227 Å line", "authors": [ "M. Bianda", "R. Ramelli", "L. S. Anusha", "J. O. Stenflo", "K. N. Nagendra", "R. Holzreuter", "M. Sampoorna", "H. Frisch", "H. N. Smitha" ], "comment": "4 pages, 5 figures, to be published as a Letter in Astronomy & Astrophysics", "categories": [ "astro-ph.SR" ], "abstract": "Chromospheric magnetic fields are notoriously diffcult to measure. The chromospheric lines are broad, while the fields are producing a minuscule Zeeman-effect polarization. A promising diagnostic alternative is provided by the forward-scattering Hanle effect, which can be recorded in chromospheric lines such as the He i 10830 {\\AA} and the Ca i 4227 {\\AA} lines. We present a set of spectropolarimetric observations of the full Stokes vector obtained near the center of the solar disk in the Ca i 4227 {\\AA} line with the ZIMPOL polarimeter at the IRSOL observatory.We detect a number of interesting forward-scattering Hanle effect signatures, which we model successfully using polarized radiative transfer. Here we focus on the observational aspects, while a separate companion paper deals with the theoretical modeling.", "revisions": [ { "version": "v1", "updated": "2011-05-11T11:32:24.000Z" } ], "analyses": { "keywords": [ "forward scattering hanle effect", "observations", "separate companion paper deals", "chromospheric lines", "interesting forward-scattering hanle effect signatures" ], "tags": [ "journal article" ], "publication": { "doi": "10.1051/0004-6361/201117047", "journal": "Astronomy and Astrophysics", "year": 2011, "month": "Jun", "volume": 530 }, "note": { "typesetting": "TeX", "pages": 4, "language": "en", "license": "arXiv", "status": "editable", "inspire": 899244, "adsabs": "2011A&A...530L..13B" } } }