Numerical Simulations of Solar Magneto-Convection

ePAPER READ

DOWNLOAD ePAPER

nso.edu

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

START NOW

Simple model: Flows around obstacle in CZCylinderHeat fluxBlockageCone15 degCone30 degNSO Workshop 27 May 7-10, 2013

Helioseismology in Space Weather - National Solar Observatory

NSO FY11 AR & FY12 APP - National Solar Observatory

Curriculum Vitae - NSO - National Solar Observatory

Statement of Work and Specifications for the Optical Design ... - ATST

Section 7 - ATST - National Solar Observatory

NSO Workshop # 27 - National Solar Observatory

Comparing Magnetic Fields in the Solar Photosphere and ... - NSO

Observational Aspects of Waves in the Chromosphere - NSO

Section 10 - ATST - National Solar Observatory

Bidder's Quote/ Proposal for Fixed Price Contract with Cost ... - ATST

Simple model: Flows around obstacle in CZCylinderHeat fluxBlockageCone15 degCone30 degNSO Workshop 27 May 7-10, 2013

Sunspot fine structure: highestresolution• Domain size– 49x49x6 Mm 3• Resolution– 16x16x12 km 3– 3072x3072x512• Sunspot finestructure– Umbral dots– Penumbra– 4km/s Evershed flowNSO Workshop 27 May 7-10, 2013

Page 1: Numerical Simulations of SolarMagne
Page 5 and 6: Sun at 2 km resolution• Simulatio
Page 8 and 9: Field strength of quiet sun?• Dep
Page 10 and 11: From granulation to supergranulatio
Page 12 and 13: Power spectrum from 2km to 100Mm•
Page 14 and 15: Spontaneous pore formationStein 201
Page 16 and 17: The imagecannot bedisplayed.Yourcom
Page 18 and 19: Subsurface field structure?Monolith
Page 22 and 23: Sunspot fine structure (at tau=1)NS
Page 24 and 25: MHD simulations and helioseismology

Numerical Simulations of Solar Magneto-Convection

Create successful ePaper yourself

Delete template?

Save as template?