*********************************************************************************** STUDY TITLE: SOLAR MICROFLARES AND NETWORK DYNAMICS - RELEVANCE FOR CORONAL HEATING STUDY TEAM : J. Rybak (choc@astro.sk), P. Gomory, A. veronig, M. Temmer, S. Stoiser *********************************************************************************** Hinode/XRT support: - high cadence of the images using just one selected filter using - no binning - loss-less compression - no compensation of the solar rotation - targets: - an ctive region when located near the disk center (microflares) - quiet Sun near disk center when no activity is present there (solar network) - pointing: specified via e-mail a day in advance Microflare mode: 256x256 px, thin Be filter, exposure max. 1s with AEC, cadence 10s Network mode : 384x384 px, thin-Al/Mesh, exposure max. 15s with AEC, cadence 15s