Physics – Plasma Physics
Scientific paper
Apr 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989noaa.rept.....d&link_type=abstract
Final Report, 1 Oct. 1986 - 30 Sep. 1988 National Oceanic and Atmospheric Administration, Boulder, CO. Space Environment Lab.
Physics
Plasma Physics
Interplanetary Space, Magnetohydrodynamics, Photosphere, Plasma Physics, Solar Activity, Solar Corona, Solar Physics, Solar Wind, Computerized Simulation, Energy Transfer, Interplanetary Magnetic Fields, Magnetic Storms, Mathematical Models, Momentum Transfer, Three Dimensional Models, Two Dimensional Models
Scientific paper
Magnetohydrodynamic (MHD) numerical modeling and simulations were used as tools to understand the physics of energy and momentum transport from the solar surface through the corona to interplanetary space. Possible physical mechanisms were identified and synthesis calculations were performed using self-consistent MHD theory via numerical and analytical methods. Solar and interplanetary (remote-sensing and in situ) observations play important roles in the synthesis strategy. The models, unique in the field of solar/interplanetary physics, include both 2 1/2-D and 3-D time-dependent codes that could lead to future operational status in geomagnetic storm forecasting procedures. A Bibliography of related papers is included.
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