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Density profile in a fluid approximation

It is important to note that it is not necessary to assume that the velocity distributions are Kappa functions in order to derive such a density profile. One may adopt instead the usual fluid description and solve the corresponding equations along tex2html_wrap_inline1829 , assuming isotropic pressures and a polytrope law of index tex2html_wrap_inline2119 . These equations read

  eqnarray628

where tex2html_wrap_inline2175 is the tex2html_wrap_inline1829 -aligned electric field. Here, the electron and ion (isotropic) pressures are tex2html_wrap_inline2179 , and we consider the simplest case where electrons and ions obey the same polytrope law tex2html_wrap_inline2181 . Then tex2html_wrap_inline2183 , so that

  eqnarray650

One gets

eqnarray663

Substituting in Eq.(26) and using (28) with tex2html_wrap_inline2185 , one finds

eqnarray675

Inserting the expression (3) of tex2html_wrap_inline1909 and integrating, one obtains

  eqnarray688

with H given in (25). This is equivalent to Eq.( 23) if tex2html_wrap_inline1861 and tex2html_wrap_inline1663 are related by (18).

Hence a profile of the form (23) can be deduced either from Liouville's theorem - assuming Kappa distribution functions (10) at z = 0, or from fluid equations - assuming isotropic polytrope laws of index tex2html_wrap_inline2119 , for both electrons and ions. Note that polytropes with exponent tex2html_wrap_inline2199 would give negative densities farther than some finite distance z, which is unphysical. This is not surprising since, as we have seen, physical velocity distributions generally produce anticorrelated density and temperature along z, which is not compatible with polytropic exponents tex2html_wrap_inline2199 .

Finally, we note that the classical Gaussian density profile corresponding to statistical equilibrium can be recovered as a particular case of the above derivations, either microscopic (Liouville) - by assuming a Maxwellian velocity distribution at z = 0, or fluid - by taking the limit tex2html_wrap_inline2209 in the polytrope law. Indeed, Maxwellians of temperatures tex2html_wrap_inline2211 are the limits for tex2html_wrap_inline2045 of the Kappa functions (10) and (20), for the electrons and ions, respectively. So that the density profile is obtained by taking the same limit tex2html_wrap_inline2045 in Eq.(23), i.e., referring to (11)

  eqnarray710

with the scale height given in (25). This is just the result of the traditional isothermal torus models in the particular case of one isotropic ion species ([Bagenal and Sullivan 1981]). Similarly, in the fluid description, this Gaussian profile can be recovered by taking the limit tex2html_wrap_inline2209 in Eq.( 29).


next up previous
Next: Comparison with the Up: PLASMA DENSITY PROFILE Previous: Density profile with

Michel Moncuquet
Mon Feb 2 16:12:15 MET 1998