Compressive turbulent cascade and heating in solar wind

Details Compressive turbulent cascade and heating in solar wind Compressive turbulent cascade and heating in solar wind

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009eguga..11.1536s&link_type=abstract

"EGU General Assembly 2009, held 19-24 April, 2009 in Vienna, Austria http://meetings.copernicus.org/egu2009, p.1536"

Computer Science

Scientific paper

Incompressible and isotropic magnetohydrodynamic turbulence in plasmas
can be described by an exact relation for the energy flux through the
scales. This Yaglom-like scaling law has been recently observed in
the solar wind above the solar poles observed by the Ulysses
spacecraft, where the turbulence is in an Alfv

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