Expansion of magnetic flux concentrations: A comparison of Hinode SOT data and models

Astronomy and Astrophysics

Volumn 518, Issue 19, 2010, Pages

  Pietarila, A ^a   Cameron, R ^a   Solanki, S K ^a,b  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b Kyung Hee University   (South Korea)

Author keywords

Sun: magnetic topology; Sun: photosphere

Indexed keywords

EXPANSION PROPERTIES; EXPANSION RATE; FLUX TUBES; FUNDAMENTAL PROPERTIES; HIGH RESOLUTION; MAGNETIC CANOPY; MAGNETIC FEATURES; MAGNETIC FLUX CONCENTRATION; MAGNETIC NETWORKS; MAGNETIC TOPOLOGIES; MAGNETOCONVECTION; NUMERICAL SIMULATION; POTENTIAL FIELD; RAPID EXPANSION; SOLAR DISK; SPECTROPOLARIMETERS; SUN: PHOTOSPHERE; TUBE MODEL; VERTICAL FIELDS;

BOUNDARY CONDITIONS; CIRCULAR POLARIZATION; DISKS (STRUCTURAL COMPONENTS); EXPANSION; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETIC STRUCTURE; POLARIZATION; SUN; TOPOLOGY; TUBES (COMPONENTS);

COMPUTER SIMULATION;

EID: 77956324174     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913887     Document Type: Article

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