Sentence examples for evolution of the solar wind from inspiring English sources

We model the evolution of the solar wind with distance, using inner heliosphere data to predict plasma parameters at Voyager.

Particular emphasis is placed on the evolution of the solar wind stream structure, and its effect on the energetic particle fluxes observed at Ulysses.

We use solar wind data at Earth as input to numerical models which include the effect of pickup ions to model the radial evolution of the solar wind.

The inclusion of the spherical grids into HALFSHEL was a complicated and major step in the evolution toward more accurate simulations of the solar wind interaction with Mars' ionosphere.

In this report, we summarize our recent advances in modeling the properties and evolution of CMEs in the solar wind.

As an initial effort to study the evolution of the Venus atmosphere, the influence of the solar wind density and the interplanetary magnetic field (IMF) x component (the x-axis points from Venus towards the Sun) on the O+ ion escape rate from Venus is investigated using a three-dimensional quasi-neutral hybrid (HYB-Venus) model.

The resulting three-dimensional structure of the solar wind and the evolution of the inner heliosphere over the solar cycle are discussed.

Heliosphere, the region surrounding the Sun and the solar system that is filled with the solar magnetic field and the protons and electrons of the solar wind.

Eventually the pressure of the solar wind becomes comparable to that of the interstellar medium.

Shielded from the buffeting of the solar wind, ions quietly leak out of the atmosphere.

Fifth panel: number density of the solar wind.