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NASA NTRS · 19720045454

Three-dimensional plasma diffusion in a very strong magnetic field.

Abstract

The thermal equilibrium coefficient of spatial diffusion transverse to a strong uniform dc magnetic field is calculated for a fully ionized plasma. The particles are assumed to move transverse to the field only as a consequence of the E x B drift, but to move freely parallel to it. The particles interact only electrostatically. The calculation is done at large, but fixed and finite, plasma volume. It is shown that, as magnetic field density approaches infinity, the leading term of the coefficient of transverse spatial diffusion falls off in a prescribed manner, but contains a multiplicative factor which goes to zero as the plasma volume becomes infinite. The method of calculation fails for unbounded plasmas.

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BibTeXRIS

Montgomery, D., Vahala, G., Liu, C.-S.. 1972-05-01. Three-dimensional plasma diffusion in a very strong magnetic field.. https://ntrs.nasa.gov/citations/19720045454

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