Comparing Simulations of Rising Flux Tubes Through the Solar Convection Zone with Observations of Solar Active Regions: Constraining the Dynamo Field Strength

Solar Physics

Volumn 287, Issue 1-2, 2013, Pages 239-263

  Weber, M A ^a,b   Fan, Y ^a   Miesch, M S ^a  

^a NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^b Veterinary Dentistry and Oral Surgery   (United States)

Author keywords

Interior, convection zone; Magnetic fields, models

Indexed keywords

EID: 84883653143     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/s11207-012-0093-7     Document Type: Article

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