Articles | Volume 21, issue 2
https://doi.org/10.5194/npg-21-405-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Special issue:
https://doi.org/10.5194/npg-21-405-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Alfvén waves in space and astrophysical dusty plasmas
V. Jatenco-Pereira
Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG/USP), Rua do Matão, 1226, 05508-090 São Paulo, SP, Brazil
A. C.-L. Chian
Paris Observatory, LESIA, CNRS, 92190 Meudon, France
National Institute for Space Research (INPE) and World Institute for Space Environment Research (WISER), P.O. Box 515, 12227-010 São José dos Campos, SP, Brazil
School of Mathematical Sciences, University of Adelaide, Adelaide, SA 5005, Australia
N. Rubab
Department of Space Science, Institute of Space Technology (IST), Islamabad, Pakistan
Related authors
No articles found.
Eugenio E. Vogel, Felipe G. Brevis, Denisse Pastén, Víctor Muñoz, Rodrigo A. Miranda, and Abraham C.-L. Chian
Nat. Hazards Earth Syst. Sci., 20, 2943–2960, https://doi.org/10.5194/nhess-20-2943-2020, https://doi.org/10.5194/nhess-20-2943-2020, 2020
Short summary
Short summary
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.
Eugenio E. Vogel, Felipe G. Brevis, Denisse Pastén, Víctor Muñoz, Rodrigo A. Miranda, and Abraham C.-L. Chian
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
Short summary
Short summary
Earthquakes are natural hazardous phenomena that can bring death, destruction,
economical crisis, migrations and other social implications. This paper aims to understand one of the main causes for seismic activity: subduction of one Earth plate underneath another one in a stochastic way. The time series associated to this activity provides information which we have analyzed it by new techniques. This allows us to estimate where important earthquakes can occur although we cannot yet say when.
Rodrigo A. Miranda, Adriane B. Schelin, Abraham C.-L. Chian, and José L. Ferreira
Ann. Geophys., 36, 497–507, https://doi.org/10.5194/angeo-36-497-2018, https://doi.org/10.5194/angeo-36-497-2018, 2018
Short summary
Short summary
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.
D. Falceta-Gonçalves, G. Kowal, E. Falgarone, and A. C.-L. Chian
Nonlin. Processes Geophys., 21, 587–604, https://doi.org/10.5194/npg-21-587-2014, https://doi.org/10.5194/npg-21-587-2014, 2014
Special issue