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<p>Recordamos el coloquio de hoy,<br>
<br>
<br>
COLOQUIOS DEL DEPARTAMENTO DE FÍSICA FCEYN - UBA<br>
<br>
En el Aula Seminario, 2do piso, Pab. I, <br>
<br>
Jueves 22/8, 14hs:<br>
<br>
WILLIAM MATTHAEUS<br>
<br>
BARTOL RESEARCH INSTITUTE AND DEPARTMENT OF PHYSICS AND ASTRONOMY,<br>
UNIVERSITY OF DELAWARE<br>
<br>
<br>
Structures, heating and particle acceleration in the turbulent solar wind<br>
plasma <br>
<br>
Abstract:<br>
<br>
Turbulent behavior has been observed in the solar wind for many years, as<br>
magnetic field, plasma velocity and density fluctuations recorded by<br>
spacecraft instruments have been analyzed from perspective of the<br>
hydrodynamic and magnetohydrodynamic turbulence theory. However only<br>
recently both instrumentation and simulations have advanced to the point<br>
that turbulence properties in a fully kinetic plasma can be investigated.<br>
Several aspects of fluid and kinetic plasma turbulence are explored in this<br>
talk. <br>
<br>
<br>
<br>
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