Technical FAQs 4

Why is pressure so high in the Solar System?

Out at the boundary of our solar system, pressure runs high. This pressure, the force plasma, magnetic fields and particles like ions, cosmic rays and electrons exert on one another when they flow and collide, was recently measured by scientists in totality for the first time — and it was found to be greater than expected.

What are solar wind dynamic pressure pulses (DPPs)?

Solar wind dynamic pressure pulses (DPPs) are small-scale plasma structures with abrupt and large-amplitude plasma dynamic pressure changes on timescales of seconds to several minutes.

What is the dynamic pressure change of a solar wind transient?

The main results of this investigation are as follows: 1) The absolute dynamic pressure changes of most DPP events, both in the undisturbed solar wind and solar wind transients, are 1.0–2.0 nPa. Statistically, the most probable values of the relative dynamic pressure change are 0.2–0.4 for all DPPs.

What is the relative pressure of a solar wind transient?

The most probable relative pressure changes are 0.2–0.4 in the undisturbed solar wind and solar wind transients. The value of d relative for all cases in the undisturbed solar wind varies from 0.20 to 1.97 with an average value of 0.47, and 3.00% of the events have values greater than 1.0.

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Pressure-type solar system

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