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- W87207802 abstract "We present the tomography analysis method using MHD simulation code to derive three‐dimensional solar wind structures from IPS observations. By incorporating MHD simulation, this new tomography method, hereafter called MHD tomography, can treat the nonlinear MHD process in solar wind and will improve the result of the reconstruction of global solar wind structure from IPS measurement data. The practical calculation is done as iteration procedure. At the first step of iteration, MHD simulation is carried out with given provisional boundary conditions, and the numerical three‐dimensional solar wind is made. At the next step, the IPS observations are simulated in this three‐dimensional solar wind. The discrepancy between the actual IPS measurement and the numerically reproduced ones are traced back along streamlines onto the inflow boundary surface. Then, the velocity distribution on the boundary surface is modified so that the differences may be reduced. The modified boundary distribution is used in the nex..." @default.
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- W87207802 date "2003-01-01" @default.
- W87207802 modified "2023-09-27" @default.
- W87207802 title "Basic Results of MHD Tomography Analysis Method for IPS Observation" @default.
- W87207802 doi "https://doi.org/10.1063/1.1618562" @default.
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