Intermittency of magnetic turbulence in slow solar wind

Details Intermittency of magnetic turbulence in slow solar wind Intermittency of magnetic turbulence in slow solar wind

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004p%26ss...52..953c&link_type=abstract

Planetary and Space Science, Volume 52, Issue 10, p. 953-956.

Computer Science

5

Magnetohydrodynamic, Isotropic Turbulence

Scientific paper

We investigate the properties of intermittency of magnetic turbulence by using magnetic field data collected by the Helios spacecraft in the inner heliosphere. Clear scaling laws for magnetic structure functions are visible in periods where the velocity of the bulk plasma is low. Within these periods we found that intermittency of magnetic turbulence is high with respect to velocity field. A comparison with fluid flows where passive scalars are more intermittent than velocity, yields to consider the magnetic field like a ``passive vector''.

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