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Statistical characteristics of field-aligned currents in Saturn's nightside magnetosphere

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posted on 2012-10-24, 09:08 authored by D. L. Talboys, E. J. Bunce, S. W. H. Cowley, C. S. Arridge, A. J. Coates, M. K. Dougherty
[1] During 2008, the Cassini spacecraft traversed Saturn's high-latitude field-aligned current systems on sequential north–south periapsis passes in the nightside magnetosphere. Two types of current systems have previously been identified, associated with antisymmetric azimuthal field signatures in the northern and southern hemispheres. The first exhibits exclusively “lagging” field morphology, while the second also includes an equatorward interval of “leading” field. Here we report the statistical characteristics of these currents, their strength, ionospheric location, and relationship to plasma boundaries. From high to low latitude, the first type comprises a downward current followed by an upward current, whose strengths are ∼0.5–3.5 MA per radian of azimuth. The downward current maps to ionospheric colatitudes of ∼13.5° and ∼16° in the north and south, respectively, usually centered in the outer magnetosphere, while the upward current maps to ∼16.5° and ∼19° in the north and south, located within the ring current region. The second type comprises a distributed downward current of ∼1–2 MA rad−1 flowing in the open field and outer magnetosphere regions, followed by an upward current of ∼2.5–5 MA rad−1 mapping to ∼15.5° and ∼18° in the north and south, corresponding to the outer magnetosphere and outer ring current, and a further downward current of ∼1–2.5 MA rad−1 mapping to ∼17.5° and ∼20° in the north and south, corresponding to the inner ring current.

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Citation

Journal of Geophysical Research A: SPACE PHYSICS, 2011, 116 (4)

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  • VoR (Version of Record)

Published in

Journal of Geophysical Research A: SPACE PHYSICS

Publisher

American Geophysical Union (AGU); Wiley

issn

0148-0227

Copyright date

2011

Available date

2012-10-24

Publisher version

http://onlinelibrary.wiley.com/doi/10.1029/2010JA016102/abstract

Language

en

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