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In addition, the shock speed σ does not vanish, i.e., there is not a stationary shock.
In addition, the IP shock speed is found to be slightly higher than the ICME speed.
Right: Percentage of initial total grain mass lost because of dust destruction in the shock vs. shock speed.
Results for the Sod shock tube comparison show that the shock speed and profile are captured accurately.
The SC/SI rise time decreases with the increase in the orientation angle and IP shock speed.
Also, we found that the IP shock speed and the average ICME speed measured at 1 AU are well correlated.
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The shock speeds up blood supply, drawing oxygen to muscles and thereby accelerating recovery.
The new primitive preconditioner can handle both strong and weak shocks, providing highly resolved shock solutions together with correct shock speeds.
The RL associated IP shock speeds show a better correlation than RQ shocks with SC/SI rise time irrespective of the orientation angle.
They also found that predictions based on kilometric type II bursts improved significantly when the ENLIL model density was used rather than the average solar wind plasma density in deriving shock speeds from the type II drift rate.
But numerical examples in one dimension demonstrate that if the switching strategy is cautious (e.g., if switching is prohibited too close to shocks), then high accuracy can be achieved for both shock speeds and smooth regions.
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