Transforming a turbulent corona into a turbulent wind

Details Transforming a turbulent corona into a turbulent wind Transforming a turbulent corona into a turbulent wind

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..333g&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 333-336 (1999).

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Particle Emission, Solar Wind, Magnetohydrodynamics And Plasmas

Scientific paper

We illustrate the possibility that the accelerating region of the solar wind is the birthplace of both jet-like phenomena and of the quasi-incompressible turbulence observed in situ at largest distances. We consider axisymetric, time-dependent isothermal MHD simulations in a shell containing the sonic point, within an external dipolar magnetic field, with β about unity or larger. We use as boundary conditions an ad hoc model of turbulent corona which leads to a) the quasi-periodic ejection of compressive blobs in the current sheet region b) an eddy circulation advected by the wind.

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