{ "id": "1012.4933", "version": "v1", "published": "2010-12-22T10:46:51.000Z", "updated": "2010-12-22T10:46:51.000Z", "title": "Are short-term variations in solar oscillation frequencies the signature of a second solar dynamo?", "authors": [ "Anne-Marie Broomhall", "Stephen T. Fletcher", "David Salabert", "Sarbani Basu", "William J. Chaplin", "Yvonne Elsworth", "Rafael A. Garcia", "Antonio Jimenez", "Roger New" ], "comment": "6 pages, 2 figures, proceedings for SOHO-24/GONG 2010 conference, to be published in JPCS", "categories": [ "astro-ph.SR" ], "abstract": "In addition to the well-known 11-year solar cycle, the Sun's magnetic activity also shows significant variation on shorter time scales, e.g. between one and two years. We observe a quasi-biennial (2-year) signal in the solar p-mode oscillation frequencies, which are sensitive probes of the solar interior. The signal is visible in Sun-as-a-star data observed by different instruments and here we describe the results obtained using BiSON, GOLF, and VIRGO data. Our results imply that the 2-year signal is susceptible to the influence of the main 11-year solar cycle. However, the source of the signal appears to be separate from that of the 11-year cycle. We speculate as to whether it might be the signature of a second dynamo, located in the region of near-surface rotational shear.", "revisions": [ { "version": "v1", "updated": "2010-12-22T10:46:51.000Z" } ], "analyses": { "keywords": [ "solar oscillation frequencies", "second solar dynamo", "short-term variations", "solar cycle", "solar p-mode oscillation frequencies" ], "tags": [ "conference paper", "journal article" ], "publication": { "doi": "10.1088/1742-6596/271/1/012025", "journal": "Journal of Physics Conference Series", "year": 2011, "month": "Jan", "volume": 271, "number": 1, "pages": "012025" }, "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable", "inspire": 882171, "adsabs": "2011JPhCS.271a2025B" } } }