| Grant number: | 13/04073-2 |
| Support Opportunities: | Research Grants - Young Investigators Grants |
| Start date: | July 01, 2013 |
| End date: | June 30, 2017 |
| Field of knowledge: | Physical Sciences and Mathematics - Astronomy |
| Principal Investigator: | Grzegorz Kowal |
| Grantee: | Grzegorz Kowal |
| Host Institution: | Escola de Artes, Ciências e Humanidades (EACH). Universidade de São Paulo (USP). São Paulo , SP, Brazil |
| City of the host institution: | São Paulo |
| Associated researchers: | Diego Antonio Falceta Gonçalves |
| Associated research grant(s): | 21/06502-4 - Interlink between turbulence, magnetic reconnection, and cosmic-ray production in non-relativistic and relativistic astrophysical plasmas,
AP.JP2 17/04578-8 - Statistics of Reconnection-Driven Turbulence, PUB.ART |
| Associated scholarship(s): | 13/18815-0 - Magnetic reconnection and related processes in collisional and collisionless astrophysical plasmas: from solar flares to extragalactic sources, BP.JP |
Abstract
Nowadays in the astrophysical community, the problem of magnetic reconnection is approached using two different points of view, from the micro-physical scale using collisionless kinetic numerical studies, and from macroscopic magnetohydrodynamical fluid approximation studies, describing well the collisional media. Both approximations have their strong points, but also significant limits, sometimes resulting in separate parameter spaces. There is no real afford taken to understand the bridge between those two approximations applied to the magnetic reconnection problem. The aim of this project is to fill this gap and perform studies which allow to understand the precess of reconnection in both regimes, collisional and collisionless. The collisionless studies, using the Chew-Goldberg-Low magnetohydrodynamics fluid approximation (CGL-MHD) allowing for the presence of the kinetic instabilities, can be directly compared with the Particle-in-Cell (PIC) simulations, using for example a hybrid kinetic-MHD models, which dominate the studies in this regime up to date. As a consequence, the second part of this project will cover the applications of the magnetic reconnection and related processes in both regimes. These applications in plasma physics cover turbulence generation and feedback on the reconnection process, magnetic field amplification mechanism, high energetic particle acceleration. The results have applications in the physics of solar flares, the importance of reconnection in space weather (e.g. interactions with magnetosphere and processes in magnetotail), the interactions of solar magnetic field with the interstellar field in the heliopause, going further up to the scales of active galaxy nuclei and gamma ray burst, where the process of reconnection together with turbulence is expected to be very important in the acceleration of TeV particles. Finally, the properties of turbulence and reconnection in collisionless environments, such intracluster medium, can benefit significantly from our studies. (AU)
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