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- W1490659991 abstract "A preliminary analysis of the dynamic heliosphere to estimate the termination shock (TS) distance from the sun around the time when Voyager 1 passed the termination shock at December 16, 2004 is performed by using MHD simulations. For input to this simulation, we use the Voyager 2 solar‐wind data. We first find a stationary solution of the 3‐D outer heliosphere by assigning a set of LISM parameters as our outer boundary conditions and then the dynamical analysis is performed. The model TS crossing is within 6 months of the observed date. The TS is pushed outward every time a high ram‐pressure solar wind pulse arrives. After the end of the high ram‐pressure wind, the TS shock shrinks inward. When the last Halloween event passed through the TS at DOY 250, 2004, the TS began to shrink inward very quickly and the TS crossed V1. The highest inward speed of the TS is over 400 km/s. The high ram‐pressure solar wind transmitted through the TS becomes a high thermal‐pressure plasma in the heliosheath, acting to pu..." @default.
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- W1490659991 date "2006-01-01" @default.
- W1490659991 modified "2023-09-24" @default.
- W1490659991 title "Preliminary analysis of the dynamic heliosphere by MHD simulations" @default.
- W1490659991 doi "https://doi.org/10.1063/1.2359306" @default.
- W1490659991 hasPublicationYear "2006" @default.
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