Paper included in the Appendix:
A. F. Rappazzo, M. Velli, G. Einaudi & R. B. Dahlburg
"Diamagnetic and Expansion Effects on the Observable Properties of the
Slow Solar Wind in a Coronal Streamer"
ApJ, 2005, volume 633, part 1, pages 474-488
DOI: 10.1086/431916
ArXiv e-print: arXiv:1002.3325v1 [astro-ph.SR]
Stemming from this work we have also published:
A. F. Rappazzo, M. Velli, G. Einaudi & R. B. Dahlburg
"Coronal Heating, Weak MHD Turbulence, and Scaling Laws"
ApJ, 2007, volume 657, part 2, pages L47-L51
DOI: 10.1086/512975
ArXiv e-print: arXiv:astro-ph/0701872v2
A. F. Rappazzo, M. Velli, G. Einaudi & R. B. Dahlburg
"Nonlinear Dynamics of the Parker Scenario for Coronal Heating"
ApJ, 2008, volume 677, issue 2, pages 1348-1366
DOI: 10.1086/528786
ArXiv e-print: arXiv:0709.3687v2 [astro-ph]
For my publication list see the arXiv --->
http://arxiv.org/a/rappazzo_a_1
Movies (animated gifs):
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run 7: 512x512x200 grid points, vA=1000, Hyperdiffusion R4=1.e19
jhyp.gif (10M) Current in the midplane
jflhyp.gif (12M) Same as above but with fieldlines of the orthogonal magnetic field.
whyp.gif (3M) Vorticity in the midplane
j2hyp3Dt.gif (3M) 3D view (from the top) of two isosurfaces of j squared
j2hyp3Ds.gif (5M) 3D view (from the side) of two isosurfaces of j squared
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run 1: 512x512x200 grid points, vA=200, normal diffusion R=800
j.gif (6M) Current in the midplane
jfl.gif (8M) Current with fieldlines of the orthogonal magnetic field
w.gif (5M) Vorticity in the midplane
wfl.gif (6M) Vorticity with fieldlines of the orthogonal magnetic field
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Last modified Feb 18 2010
rappazzoATdf.unipi.it (AT ---> @)