Articles | Volume 33, issue 10
https://doi.org/10.5194/angeo-33-1301-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-33-1301-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
A physical explanation for the magnetic decrease ahead of dipolarization fronts
Z. H. Yao
CORRESPONDING AUTHOR
UCL Mullard Space Science Laboratory, Dorking, RH5 6NT, UK
Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA 90095-1567, USA
C. J. Owen
UCL Mullard Space Science Laboratory, Dorking, RH5 6NT, UK
C. Forsyth
UCL Mullard Space Science Laboratory, Dorking, RH5 6NT, UK
I. J. Rae
UCL Mullard Space Science Laboratory, Dorking, RH5 6NT, UK
Z. Y. Pu
School of Earth and Space Sciences, Peking University, Beijing 100871, China
H. S. Fu
Space Science Institute, School of Astronautics, Beihang University, Beijing 100191, China
X.-Z. Zhou
School of Earth and Space Sciences, Peking University, Beijing 100871, China
Q. Q. Shi
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University, Weihai 264209, China
A. M. Du
Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China
R. L. Guo
School of Earth and Space Sciences, Peking University, Beijing 100871, China
X. N. Chu
Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA 90095-1567, USA
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Cited
38 citations as recorded by crossref.
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Latest update: 23 Nov 2024
Short summary
We use THEMIS large data set of dipolarization front events to build a 2-D pressure distribution in XZ plane, and thus derive the current system around the dipolarization front. Our results show that a banana current loop is formed around the dipolarization front. This current is also suggested to be the reason for the magnetic dip observed ahead of the dipolarization front. In addition, the current density is too small to contribute a substorm current wedge.
We use THEMIS large data set of dipolarization front events to build a 2-D pressure distribution...