Solar turbulent magnetic fields: Surprisingly homogeneous distribution during the solar minimum

Astronomy and Astrophysics

Volumn 524, Issue 5, 2010, Pages

  Kleint, L ^a,b   Berdyugina, S V ^c   Shapiro, A I ^d   Bianda, M ^b  

^a ETH ZURICH   (Switzerland)

^b Istituto Ricerche Solari Locarno   (Switzerland)

^c KIEPENHEUER INSTITUT FÜR SONNENPHYSIK   (Germany)

^d WORLD RADIATION CENTER   (Switzerland)

Author keywords

magnetic fields; molecular processes; polarization; scattering; Sun: photosphere

Indexed keywords

ENERGY BUDGETS; FLUX DENSITIES; FORMATION MODEL; HANLE EFFECTS; HOMOGENEOUS DISTRIBUTION; HORIZONTAL FLUXES; LINE RATIOS; LINEAR POLARIZATION; MOLECULAR PROCESS; SMALL VARIATIONS; SOLAR ATMOSPHERE; SOLAR CYCLE; SOLAR MAXIMA; SOLAR MINIMA; SPATIAL DISTRIBUTION; SPECTRAL LINE; STATISTICAL ANALYSIS; SUN: PHOTOSPHERE; TEMPORAL AND SPATIAL VARIATION; TURBULENT FIELDS; TURBULENT MAGNETIC FIELDS; WEAK MAGNETIC FIELDS;

MAGNETIC FIELDS; POLARIZATION; SCATTERING; SPECTROSCOPY;

SOLAR ENERGY;

EID: 78651278826     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015285     Document Type: Article

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