Articles | Volume 35, issue 3
https://doi.org/10.5194/angeo-35-365-2017
© Author(s) 2017. 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-35-365-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Non-triggered auroral substorms and long-period (1–4 mHz) geomagnetic and auroral luminosity pulsations in the polar cap
Nadezda Yagova
CORRESPONDING AUTHOR
Schmidt Institute of Physics of the Earth, Moscow, Russia
Natalia Nosikova
Schmidt Institute of Physics of the Earth, Moscow, Russia
National Research Nuclear University “MEPhI”, Moscow, Russia
Lisa Baddeley
University Centre in Svalbard, Svalbard, Norway
Birkeland Centre for Space Science (BCSS), University of Bergen, Bergen, Norway
British Antarctic Survey, Cambridge, UK
Olga Kozyreva
Schmidt Institute of Physics of the Earth, Moscow, Russia
Dag A. Lorentzen
University Centre in Svalbard, Svalbard, Norway
Birkeland Centre for Space Science (BCSS), University of Bergen, Bergen, Norway
British Antarctic Survey, Cambridge, UK
Vyacheslav Pilipenko
Schmidt Institute of Physics of the Earth, Moscow, Russia
Space Research Institute of the Russian Academy of Sciences, Moscow, Russia
Magnar G. Johnsen
Tromsø Geophysical Observatory, UiT – the Arctic University of Norway, Tromsø, Norway
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A substorm is a dramatic phenomenon in the near-Earth space that is visualized as an aurora. Mostly substorms are caused by changes in the solar wind, but some of them can develop without any evident trigger. Such substorms together with undisturbed days were investigated using magnetometer and photometer data from Svalbard. Substorm precursors, i.e., specific features in 1–4 mHz geomagnetic and auroral luminosity pulsations, have been found at high geomagnetic latitudes.
A substorm is a dramatic phenomenon in the near-Earth space that is visualized as an aurora....