The structure of helical interplanetary magnetic fields

Details The structure of helical interplanetary magnetic fields The structure of helical interplanetary magnetic fields

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991georl..18.1505g&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 18, Aug. 1991, p. 1505-1508.

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Interplanetary Magnetic Fields, Magnetic Field Configurations, Astronomical Models, Power Spectra

Scientific paper

The interplanetary magnetic field is known to be highly helical. Although the detailed spatial structure of the fields has yet to be elucidated, the helicity spectrum has been conjectured to result from a random walk in the direction of a constant magnitude magnetic field vector. A model using three-dimensional fluctuations with variations in B is demonstrated giving a good fit to the helicity spectrum as well as to other properties of the interplanetary magnetic field.

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