Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
High Altitude Observatory, National Center for Atmospheric Research, Boulder CO
High Altitude Observatory, Boulder, CO
Chicago, University, Chicago, IL
High Altitude Observatory, National Center for Atmospheric Research, 3450 Mitchell Lane, Boulder, CO 80301
High Altitude Observatory
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, Colorado 80307-3000
MIT, Cambridge, Mass.
HAO - NCAR
HAO / NCAR
National Center for Atmospheric Research, Boulder, CO, US
HAO, NCAR
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000
Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass; Chicago, University, Chicago, Ill.
High Altitude Observatory, National Center for Atmospheric Research, PO Box 3000, Boulder, Colorado 80307, USA
National Center for Atmospheric Research, Boulder, CO.
Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.
High Altitude Observatory, NCAR Boulder, CO 80301, USA
NCAR
High Altitude Observatory, National Center for Atmospheric Research, P. O. Box 3000, Boulder, CO 80307
High Altitude Observatory, National Center for Atmospheric Research, 3450 Mitchell Lane, Boulder, CO 80301 Altitude Observatory, NCAR, P.O. Box 3000, Boulder, CO 80307
High Altitude Observatory, National Center for Atmospheric Research, 3080 Center Green, Boulder, CO 80301 National Center for Atmospheric Research, P.O, Box 3000, Boulder, Colorado 80307
A Non-Radial Radiation Force in Hot Star Winds
A Numerical Simulation of Two-Dimensional Radiative Equilibrium in Magnetostatic Flux Tubes
A Numerical Simulation of Two-Dimensional Radiative Equilibrium in Magnetostatic Flux Tubes
A numerical simulation of two-dimensional radiative equilibrium in magnetostatic flux tubes. I - The model
A numerical simulation of two-dimensional radiative equilibrium in magnetostatic flux tubes. II - Computational results
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