Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...488..482c&link_type=abstract
Astrophysical Journal v.488, p.482
Astronomy and Astrophysics
Astronomy
14
Magnetohydrodynamics: Mhd, Sun: Solar Wind, Turbulence
Scientific paper
Some turbulent signed measures show a singularity related to extreme oscillations in sign, the scaling behavior of cancellations between positive and negative contributions being characterized by the cancellation exponent kappa . Using in situ observations of magnetic fluctuations in the solar wind, we show that magnetic helicity is sign singular, a property that underlies the dominance of a single sign of polarization of fluctuations at small scales. We recover a statistical correlation between kappa and the bulk solar wind speed when any correlation has been found between kappa and the distance from the Sun. Even if the usual models of magnetic fluctuations based on random phases are able to reproduce (in a statistical sense) the gross features of helicity fluctuations, they cannot reproduce the behavior of sign singularity.
Bruno Roberto
Carbone Vincenzo
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