Steady-state field-aligned currents at Mercury

被引:55
作者
Anderson, Brian J. [1 ]
Johnson, Catherine L. [2 ,3 ]
Korth, Haje [1 ]
Slavin, James A. [4 ]
Winslow, Reka M. [2 ]
Phillips, Roger J. [5 ]
McNutt, Ralph L., Jr. [1 ]
Solomon, Sean C. [6 ,7 ]
机构
[1] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[2] Univ British Columbia, Dept Earth Ocean & Atmospher Sci, Vancouver, BC V5Z 1M9, Canada
[3] Planetary Sci Inst, Tucson, AZ USA
[4] Univ Michigan, Dept Atmospher Ocean & Space Sci, Ann Arbor, MI 48109 USA
[5] SW Res Inst, Boulder, CO USA
[6] Columbia Univ, Lamont Doherty Earth Observ, Palisades, NY USA
[7] Carnegie Inst Sci, Dept Terr Magnetism, Washington, DC USA
基金
加拿大自然科学与工程研究理事会;
关键词
MESSENGER OBSERVATIONS; ELECTRICAL-CONDUCTIVITY; MAGNETOSPHERE; MAGNETOPAUSE; MAGNETOMETER; MODEL; TUTORIAL; SURFACE;
D O I
10.1002/2014GL061677
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Magnetic field observations acquired in orbit about Mercury by the MESSENGER spacecraft demonstrate the presence in the planet's northern hemisphere of Birkeland currents that flow to low altitudes. Currents of density 10-30 nA/m(2) flow downward at dawn and upward at dusk. Total currents are typically 20-40 kA and exceed 200 kA during disturbed conditions. The current density and total current are two orders of magnitude lower than at Earth. An electric potential of similar to 30 kV from dayside magnetopause magnetic reconnection implies a net electrical conductance of similar to 1 S. A spherical-shell conductance model indicates closure of current radially through the low-conductivity layers near the surface and by lateral flow from dawn to dusk through more conductive material at depth.
引用
收藏
页码:7444 / 7452
页数:9
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