Universidad de Alcalá

Descripción: The study of Space Plasmas covers a wide range of Heliospheric and Astrophysical phenomena and processes in most of the cosmic media. Space Plasmas are generally organized by magnetic fields, though in some places plasmas organize magnetic fields as in the case of the Convective zone of the Sun. Plasmas prevail at: the solar interior, the Sun environment, sunspots, solar flares, solar wind, coronal mass ejections, interplanetary medium, collisionless shocks, planetary environments, magnetospheres, magnetic storms radiation belts, auroras, as well as in the intergalactic space, galaxies, accretion disks, galactic winds, galactic jets, supernova, radio filaments, interstellar space, stellar atmospheres, stellar winds, stellar flares and so on. Space Plasmas also generate radio waves, X-rays and cosmic energetic particles: among the later, extragalactic and galactic cosmic rays, energetic particles generated at the Sun in a wide range of energy, mass and charge.

Fecha inicio: 13/05/2013 - Fecha fin: 17/05/2013

Lugar del evento: Mexico

Convocante: Grupo de Plasmas EspAciales y Astropartículas. SpAce Plasmas and AStroparticle (SPAS) Group

Más Información: El plazo de presentación de Abstract para contribuir a este workshop finaliza el 6 de febrero de 2013.
Contacto: Convener Dr. Luis del Peral luis.delperal@gmail.com

Consultar en: http://spas.uah.es http://spas.uah.es:81/hom...