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- W1664219864 abstract "A realistic and time‐varying termination shock position is studied by using three‐dimensional MHD simulation. The effect of heliospheric disturbances on the position of the termination shock (TS) is examined in some detail by using model of (1) rectangular‐type periodic change and (2) triangle‐type pulse of the solar‐wind ram‐pressure. Comparing study of our forecasting simulation (Washimi et al. 2007B) with observed V2‐TS crossing enables us a new prospect of the heliospheric structure. It is discussed that the heliosphere can be skewed not only by N‐S asymmetry, which is produced by obliquely oriented interstellar magnetic field, but also by some TS‐depression in lower latitudes." @default.
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- W1664219864 date "2008-01-01" @default.
- W1664219864 modified "2023-09-26" @default.
- W1664219864 title "MHD analysis of the time-varying termination-shock position" @default.
- W1664219864 doi "https://doi.org/10.1063/1.2982461" @default.
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