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Astrophysical Plasmas Group


Introduction

Aims of the group

The main objective of our group is the study of astrophysical phenomena, specially those in which the physics of plasmas is directly relevant. In particular, we are interested in astrophysical problems, such as: heating of the solar corona, propagation of energetic particles, stellar winds, stellar dynamos or accretion disks.

Incidentally, we have also addressed various theoretical problems related the dynamics of magnetofluids or to kinetic plasma processes, such as: numerical simulations of fluids and magnetofluids, stability of stationary solutions of the MHD equations, closure models for MHD turbulence, Fokker-Planck description of electron beams or the development of plasma turbulence. Although these problems have been studied from a purely theoretical point of view, most of them are directly relevant to a number of astrophysical phenomena ( Click here for a more complete description of our research interests).

History of the group

The group was created in 1984 by Dr. Ferro Fontán , who is also the head of the group. In the beginning, the activity was centered in the formation of young researchers in plasma astrophysics. Various master and PhD thesis were completed during this first stage, under the supervision of Dr. Ferro Fontán. In a second stage, some of these doctors held postdoctoral positions abroad and returned to the group. Currently, a third generation of plasma astrophysicists joined the group, either for their graduation thesis or as graduate students of the Department of Physics of the University of Buenos Aires . The group is currently composed by seven researchers and three graduate students. The group activities are performed at the Institute of Astronomy and Space Physics (IAFE) (CONICET-UBA) and the Department of Physics (Facultad de Ciencias Exactas y Naturales, UBA), located at the Ciudad Universitaria (Buenos Aires, Argentina). The researchers of the group regularly teach graduate courses at the Department of Physics, such as: Plasma Physics, Turbulence in Astrophysical Plasmas, General Astrophysics or Dynamical Systems.