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APPENDIX

Consider a distribution made of a sum of Maxwellians of temperatures tex2html_wrap_inline1755 and densities tex2html_wrap_inline2329 , at z = 0. Eq.(4) shows that the distribution at distance z is a sum of Maxwellians of temperatures tex2html_wrap_inline1755 and densities

eqnarray812

The temperature of each individual Maxwellian (which, as seen in Sect.4, is independent of q and z) is related to its moment tex2html_wrap_inline2341 by Eq.(6), i.e.

eqnarray821

where, by definition, tex2html_wrap_inline2343 . The temperature tex2html_wrap_inline1969 of the whole distribution at distance z is obtained by substituting in (6) its moment tex2html_wrap_inline2349 with the above expressions of tex2html_wrap_inline2341 . This gives

eqnarray837

To find the sense of variation of tex2html_wrap_inline1969 , we have to calculate the sign of the derivative tex2html_wrap_inline2355 :

eqnarray849

where

eqnarray869

Thus

eqnarray878

eqnarray883

  eqnarray895

The bracket can be rearranged by dropping the terms that cancel out in the summations, and symmetrizing over the dummy indices. This gives:

eqnarray906

which is a sum of positive terms, so that the bracket in Eq.( 31) is positive. Hence, with a monotonic attractive potential ( tex2html_wrap_inline1917 ), the temperatures tex2html_wrap_inline1969 all increase with z. This holds for a velocity distribution which can be modelled by a sum of several Maxwellians (a single Maxwellian giving tex2html_wrap_inline2379 ).

Acknowledgements
The Ulysses URAP experiment, whose Principal Investigator is R.G. Stone, is a joint project of NASA/GSFC, Observatoire de Paris, CRPE and University of Minnesota. The French contribution was mainly financed by the CNES. We are very grateful to the team at the Département de Recherche Spatiale (Observatoire de Paris), who designed, built and tested the radio astronomy receivers, whose great performances allowed us to obtain these results. We thank our colleagues at GSFC for the successful operation of the experiment during the flyby and their help in the data reduction. We thank D. F. Strobel for his critical reading of an earlier version of this paper and useful suggestions, the referees for their helpful comments, and J. L. Steinberg for his suggestions which made this paper easier to understand.


next up previous
Next: References Up: Temperature inversion in the Previous: SUMMARY AND FINAL

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