Is Solar Wind Turbulence a Driver of Geomagnetic Activity at Mid-Low Latitudes?

Abstract

The coupling of solar wind to the magnetosphere is one of the widely studied dynamical processes that characterize the Sun-Earth coupled system. In this work, the effects of solar wind magnetohydrodynamic (MHD) turbulence on geomagnetic field at the mid-low latitudes during the year 2009 when the Sun nearly plunged into the Maunder minimum was studied statistically. We characterized the MHD Alfvénic turbulence by means of 2-D histograms and related these histograms to the behaviour of geomagnetic activity at mid-low latitudes as measured by ASY-D, ASY-H, SYM-D, and SYM-H indices. We discovered that geomagnetic activity at mid-low latitudes is not driven by solar wind Alfvénic turbulence during period of low solar activity.

Authors and Affiliations

E. B. I. Ugwu , F. N. Okeke , O. J. Ugonabo

Keywords

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  • EP ID EP152343
  • DOI -
  • Views 133
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How To Cite

E. B. I. Ugwu, F. N. Okeke, O. J. Ugonabo (2014). Is Solar Wind Turbulence a Driver of Geomagnetic Activity at Mid-Low Latitudes?. INTERNATIONAL JOURNAL OF RECENT TRENDS IN SCIENCE AND TECHNOLOGY, 9(2), 230-232. https://europub.co.uk/articles/-A-152343