Determination of magnetic helicity in the solar wind and implications for cosmic ray propagation

Details Determination of magnetic helicity in the solar wind and implications for cosmic ray propagation Determination of magnetic helicity in the solar wind and implications for cosmic ray propagation

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981cicc.conf....2m&link_type=abstract

In its Contrib. to the 17th Intern. Cosmic Ray Conf. p 2-4 (SEE N81-25029 15-93)

Physics

Cosmic Rays, Magnetic Fields, Magnetohydrodynamic Flow, Solar Wind, Magnetometers, Solar Corpuscular Radiation

Scientific paper

The mean value of the correlation between local magnetic field and vector potential, known as the magnetic helicity, is a measure of the lack of mirror reflection symmetry of magnetic covariances in a turbulent medium. A method is presented for extraction of helicity spectra from magnetometer data, and applied to an evaluation of the magnetic helicity of interplanetary magnetic fluctuations.

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