MHD heliosphere with boundary conditions from a tomographic reconstruction using interplanetary scintillation data

Observations of interplanetary scintillation (IPS) provide a set of data that is used in estimating the solar wind parameters with reasonably good accuracy. Various tomography techniques have been developed to deconvolve the line‐of‐sight integration effects ingrained in observations of IPS to impro...

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Veröffentlicht in:	Journal of geophysical research. Space physics 2014-10, Vol.119 (10), p.7981-7997
Hauptverfasser:	Kim, T. K., Pogorelov, N. V., Borovikov, S. N., Jackson, B. V., Yu, H.-S., Tokumaru, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accuracy Boundary conditions Charged particles Density Earth Earth orbits heliosphere In situ measurement interplanetary scintillation IPS Kinematics Magnetic fields Magnetohydrodynamics Mathematical models MHD modeling Solar wind Spacecraft Tomography Wind speed
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