Francois Colas, Jeremie vaubaillon, Praksh Atreya, Frederique vachier, IMCCE, Paris, France

ÊÊ Generaly video observations are made to count meteores and to measure radians, not to measure accurates orbits. In an other hand fireball observations made with large photographic plates produce good orbits but for a few events. The use of large CCD can chage this status as we can reach fainter magnitude with low noise CCD cameras and accurates orbits with large formats. Our goal is to install at least two cameras in two stations to investigate the field.