2008/07/31 by F. Berrilli, D. Del Moro, B. Viticchie +1
Physics and Astronomy · #Astrophysics and Star Formation Studies #Ionosphere and magnetosphere dynamics #Solar and Space Plasma Dynamics #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809683
6 pages, 5 figures, accepted for publication on Astronomy & Astrophysics
openalex publication_date 2008/08/01 · arxiv created 2008/08/03 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/04
Context. The quiet Sun presents magnetized plasma whose field strengths vary from zero to about 2 kG. The probability density function of the magnetic field strength B efficaciously describes the statistical properties of the quiet Sun magnetic field.