Articles | Volume 34, issue 10
https://doi.org/10.5194/angeo-34-901-2016
© Author(s) 2016. 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-34-901-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Filamentary field-aligned currents at the polar cap region during northward interplanetary magnetic field derived with the Swarm constellation
GFZ, German Research Centre for Geosciences, Section 2.3 “Earth's
Magnetic Field”, 14473 Potsdam, Germany
Tao Huang
GFZ, German Research Centre for Geosciences, Section 2.3 “Earth's
Magnetic Field”, 14473 Potsdam, Germany
Department of Space Physics, College of Electronic Information, Wuhan
University, 430072 Wuhan, China
Simon Wing
The Johns Hopkins University, Applied Physics Laboratory, Laurel, MD
20723, USA
Guram Kervalishvili
GFZ, German Research Centre for Geosciences, Section 2.3 “Earth's
Magnetic Field”, 14473 Potsdam, Germany
Jan Rauberg
GFZ, German Research Centre for Geosciences, Section 2.3 “Earth's
Magnetic Field”, 14473 Potsdam, Germany
Haje Korth
The Johns Hopkins University, Applied Physics Laboratory, Laurel, MD
20723, USA
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Y. L. Zhou, S. Y. Ma, R. S. Liu, H. Luehr, and E. Doornbos
Ann. Geophys., 31, 15–30, https://doi.org/10.5194/angeo-31-15-2013, https://doi.org/10.5194/angeo-31-15-2013, 2013
Short summary
ESA's constellation mission Swarm makes it possible for the first time to determine field-aligned currents (FACs) reliably in the ionosphere. FACs are able to transport energy from the solar wind to the Earth and heat the upper atmosphere. Here we investigate FAC structures that have been missed by previous satellite missions. Most of them are found poleward of the northern light zone. The energy sources seem to be located on the nightside of Earth about 100 000 km away.
ESA's constellation mission Swarm makes it possible for the first time to determine...