Anisotropic avalanche model for solar flares

MORALES, LAURA

Wroclaw

Workshop; F-Chroma Training Workshop, Observations and Modelling of solar flares; 2016

European Comunity - FChroma Project

p { margin-bottom: 0.25cm; direction: ltr; color: rgb(0, 0, 0); line-height: 120%; }p.western { font-family: "Liberation Serif","Times New Roman",serif; font-size: 12pt; }p.cjk { font-family: "Noto Sans CJK SC Regular"; font-size: 12pt; }p.ctl { font-family: "FreeSans"; font-size: 12pt; }For almost three decades solar flares have been modelled under theparadigm of self organized criticality using 2D and 3D cellularautomata. In this work we highlight the possibilities that ouranisotropic model for solar flares has in order to incorporate realdata that is currently being obtained and processed by the FchromaTeam.