Computer Science – Numerical Analysis
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sici.symp...33h&link_type=abstract
In Alabama Univ., Huntsville. STIP Symposium on Physical Interpretation of Solar/Interplanetary and Cometary Intervals p 33 (SEE
Computer Science
Numerical Analysis
Interplanetary Medium, Intervals, Numerical Analysis, Solar Wind, Surges, Thermal Conductivity, Hydrodynamic Equations, Models, Plasma Density, Simulation, Solar Wind Velocity, Steady State, Unsteady State
Scientific paper
A numerical analysis of transient solar wind starting at the solar surface and arriving at 1 AU is performed by an implicit numerical method. The model hydrodynamic equations include thermal conduction terms for both steady and unsteady simulations. Simulation results show significant influence of thermal conduction on both steady and time-dependent solar wind. Higher thermal conduction results in higher solar wind speed, higher temperature, but lower plasma density at 1 AU. Higher base temperature at the solar surface gives lower plasma speed, lower temperature, but higher density at 1 AU. Higher base density, on the other hand, gives lower velocity, lower temperature, but higher density at 1 AU.
Dryer Murray
Han Ming Sheng
Wu Shi Tsan
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