2006/09/20 by D. Salabert, W. J. Chaplin, Y. Elsworth +3
Earth and Planetary Sciences · Physics and Astronomy · #Amplitude #Degree (music) #Distribution (mathematics) #Geophysics and Gravity Measurements #Range (aeronautics) #Solar and Space Plasma Dynamics #Solar cycle #Solar physics #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:20066419
8 pages, 3 figures, 2 tables; Submitted to A&A
arxiv created 2006/09/20 · openalex publication_date 2006/12/18 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Aims.We use 9.5-yr of BiSON Sun-as-a-star data to search for dependence of solar-cycle parameter changes on the angular degree, , of the data. The nature of the Sun-as-a-star observations is such that for changes measured at fixed frequency, or for changes averaged across the same range in frequency, any dependence present carries information on the latitudinal distribution of the agent (i.e., the activity) responsible for those changes.