The solar-flare induced earth's environment

Details The solar-flare induced earth's environment The solar-flare induced earth's environment

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985asdy.conf.....w&link_type=abstract

AAS and AIAA, Astrodynamics Specialist Conference, Vail, CO, Aug. 12-15, 1985. 19 p. USAF-supported research.

Astronomy and Astrophysics

Astronomy

Earth Environment, Energy Transfer, Interplanetary Space, Magnetic Storms, Polar Regions, Solar Flares, Astronomical Models, Atmospheric Density, Boundary Value Problems, Geomagnetism, Interplanetary Magnetic Fields, Solar Wind

Scientific paper

A composite numerical simulation model developed from a series of MHD models was used to compute the solar-flare-generated disturbances of physical parameters, such as density, temperature, velocity, and magnetic field from the solar surface (i.e., the photospheric level) to the earth's environment. It is shown that the disturbed earth's environment at high latitudes can be approximated by starting with the knowledge of the occurrence and the strength of a solar flare, then simulating the evolutionary consequences of the solar disturbance through interplanetary space up to and through the magnetosphere.

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