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Record Search Query:
ServiceParameters>MODELS>SOLAR-ATMOSPHERE/SPACE-WEATHER MODELS
Exospheric Solar Wind Model
Entry ID: Exospheric
Summary
Abstract:
This is an exospheric model of the solar wind with only protons and electrons
(we defer the inclusion of heavy ions to upcoming versions of the code), with a non-monotonic total potential for the protons and with a Lorentzian (kappa) velocity distribution function (VDF) for the electrons. This code is developed for the coronal holes. Exospheric kinetic models assume that there is a sharp level called the exobase, separating a collision dominated region (where a fluid approximation is valid) from a region fully collisionless. In fact, there is a transition region where collisions between particles become less and less numerous when the distance to the Sun increases.
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