Articles | Volume 36, issue 2
https://doi.org/10.5194/angeo-36-497-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Special issue:
https://doi.org/10.5194/angeo-36-497-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Non-Gaussianity and cross-scale coupling in interplanetary magnetic field turbulence during a rope–rope magnetic reconnection event
UnB-Gama Campus, University of Brasília (UnB), Brasília DF 70910-900, Brazil
Plasma Physics Laboratory, Institute of Physics, University of Brasília (UnB), Brasília DF 70910-900, Brazil
Adriane B. Schelin
Plasma Physics Laboratory, Institute of Physics, University of Brasília (UnB), Brasília DF 70910-900, Brazil
Abraham C.-L. Chian
School of Mathematical Sciences, University of Adelaide, Adelaide SA 5005, Australia
Institute of Aeronautical Technology (ITA), São José dos Campos, SP 12228-900, Brazil
National Institute for Space Research (INPE), P.O. Box 515, São José dos Campos, SP 12227-010, Brazil
José L. Ferreira
Plasma Physics Laboratory, Institute of Physics, University of Brasília (UnB), Brasília DF 70910-900, Brazil
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The Nazca–South American subduction front is one of the most active in the world. We have chosen four zones along this front to do a comparative study on possible different dynamics. Data are public and well tested in the last decades. The methods are original since mutability and Shannon entropy are not always used in this kind of problem, and, to our knowledge, this is the first time they are combined. The north of Chile could be a zone with greater chances of a large earthquake.
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The Nazca–South American subduction front is one of the most active in the world. We have chosen four zones along this front to do a comparative study on possible different dynamics. Data are public and well tested in the last decades. The methods are original since mutability and Shannon entropy are not always used in this kind of problem, and, to our knowledge, this is the first time they are combined. The north of Chile could be a zone with greater chances of a large earthquake.
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Nat. Hazards Earth Syst. Sci. Discuss., https://doi.org/10.5194/nhess-2019-309, https://doi.org/10.5194/nhess-2019-309, 2019
Manuscript not accepted for further review
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Earthquakes are natural hazardous phenomena that can bring death, destruction,
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The solar wind is a tenuous turbulent plasma permeating the interplanetary space and is not well understood. A complex process called magnetic reconnection can act as a source of solar wind turbulence. Here we study this process using statistics. We demonstrate that high-order statistics of the magnetic field display a parabolic relation that is enhanced when magnetic reconnection occurs. Our results can help us understand the nature of solar wind turbulence.
The solar wind is a tenuous turbulent plasma permeating the interplanetary space and is not well...
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