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The Quadratic Magnetic Gradient and Complete Geometry of Magnetic Field Lines Deduced from Multiple Spacecraft Measurements
  • +8
  • Chao Shen,
  • Chi Zhang,
  • Zhaojin Rong,
  • Zuyin Pu,
  • Malcolm W Dunlop,
  • Christopher Philippe Escoubet,
  • C. T. Russell,
  • Gang Zeng,
  • Nian Ren,
  • James L Burch,
  • Yufei Zhou
Chao Shen
Harbin Institute of Technology
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Chi Zhang
Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences
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Zhaojin Rong
Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences
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Zuyin Pu
Peking University
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Malcolm W Dunlop
Beihang University
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Christopher Philippe Escoubet
ESA / ESTEC

Corresponding Author:[email protected]

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C. T. Russell
University of California
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Gang Zeng
Jingchu University of Technology
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Nian Ren
School of Science
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James L Burch
Southwest Research Institute
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Yufei Zhou
School of Science
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Abstract

Topological configurations of the magnetic field play key roles in the evolution of space plasmas. This paper presents a novel algorithm that can estimate the quadratic magnetic gradient as well as the complete geometrical features of magnetic field lines, based on magnetic field and current density measurements by a multiple spacecraft constellation at 4 or more points. The explicit estimators for the linear and quadratic gradients, the apparent velocity of the magnetic structure and the curvature and torsion of the magnetic field lines can be obtained with well predicted accuracies. The feasibility and accuracy of the method have been verified with thorough tests. The algorithm has been successfully applied to exhibit the geometrical structure of a flux rope. This algorithm has wide applications for uncovering a variety of magnetic configurations in space plasmas.