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- W1974834437 abstract "We present a kinetic model of the stationary solar wind based on the equation for two-particle (electron–proton) velocity distribution. The influence of collisions and the magnetic field is neglected. The approximation of the quasi-neutral plasma is applied to close the model, which results in excluding a Coulomb potential of plasma polarization field from consideration. The kinetic equation is solved using the method of characteristics. Solar wind density and speed are evaluated by integrating the two-particle distribution function over its domain of definition formed by related characteristics. The obtained dependences of the density and velocity on heliocentric distance agree with observational data of the in-ecliptic slow solar wind." @default.
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- W1974834437 date "2003-05-23" @default.
- W1974834437 modified "2023-09-27" @default.
- W1974834437 title "Two-particle quasi-neutral kinetic model of collisionless solar wind" @default.
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- W1974834437 doi "https://doi.org/10.1088/0305-4470/36/22/350" @default.
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