Are short-term variations in solar oscillation frequencies the signature of a second solar dynamo?

Anne-Marie Broomhall, Stephen T. Fletcher, David Salabert, Sarbani Basu, William J. Chaplin, Yvonne Elsworth, Rafael A. Garcia, Antonio Jimenez, Roger New

Published 2010-12-22Version 1

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.