Variation in the statistical properties of IMF direction fluctuations during the 22-year solar magnetic cycle View Full Text


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Article Info

DATE

2014-12

AUTHORS

D. V. Erofeev

ABSTRACT

The variation in the IMF direction distribution during the 22-year solar magnetic cycle has been studied. Data obtained in near-Earth orbits and measurements in the heliospheric regions located far from the Earth, performed with the Helios and Ulysses spacecraft devices, have been analyzed. It has been found that the correlation between the azimuth and magnetic field fluctuations is statistically significant in the low-latitude heliospheric region at heliocentric distances of 0.3–5.4 AU, and the sign of this correlation reverses at a change in the polar solar magnetic field orientation. In the polar zones of the heliosphere outside the latitudinal extension of the heliospheric current sheet, the angle correlation coefficient rapidly decreases with increasing heliographic latitude. The angle correlation sign reversal during the 22-year cycle is accompanied by a change of the asymmetry sign of the magnetic field inclination distribution. More... »

PAGES

1032-1038

References to SciGraph publications

  • 1979-09. An extended investigation of Helios 1 and 2 observations: The interplanetary magnetic field between 0.3 and 1 AU in SOLAR PHYSICS
  • 2008. The solar wind throughout the solar cycle in THE HELIOSPHERE THROUGH THE SOLAR ACTIVITY CYCLE
  • 2008. The global heliospheric magnetic field in THE HELIOSPHERE THROUGH THE SOLAR ACTIVITY CYCLE
  • 2012-12. Anisotropy and symmetry of fluctuations in the solar wind magnetic field and velocity in GEOMAGNETISM AND AERONOMY
  • Journal

    TITLE

    Geomagnetism and Aeronomy

    ISSUE

    8

    VOLUME

    54

    Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1134/s0016793214080039

    DOI

    http://dx.doi.org/10.1134/s0016793214080039

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1008196471


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