On the application of numerical models to the inverse mapping of solar wind flow structures

Details On the application of numerical models to the inverse mapping of solar wind flow structures On the application of numerical models to the inverse mapping of solar wind flow structures

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jgr....86.6685p&link_type=abstract

Journal of Geophysical Research, vol. 86, Aug. 1, 1981, p. 6685-6690.

Statistics

Computation

11

Flow Characteristics, Magnetohydrodynamic Flow, Mapping, Mathematical Models, Plasma Diffusion, Solar Wind, Boundary Value Problems, Conservation Laws, Inviscid Flow, Plasma Heating, Rotating Fluids, Steady Flow, Supersonic Flow

Scientific paper

It is pointed out that sophisticated MHD numerical models can be applied to the inverse mapping problem of solar wind structures seen near 1.0 AU back to the vicinity of the sun, with greater accuracy than that of the widely used, constant velocity technique. Within the restrictions outlined, it is shown that researchers will be able to choose a more complete data set as the origin of the mapping, increasing the total number of spacecraft alignments that can be employed as a basis for computation.

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