33RD INTERNATIONAL COSMIC RAY CONFERENCE, RIO DE JANEIRO 2013 THE ASTROPARTICLE PHYSICS CONFERENCE Realization of the global survey method in real-time

Abstract: The global survey method was developed at ShICRA of SB RAS more than 40 years ago. It is a powerful and useful instrument for studying of the interplanetary medium. The essence of method is that the world neutron monitor network is used as the unified omnidirectional device. It allows to receive information on a spatial distribution of cosmic rays (CR) with a high accuracy for each hour of measurements. The notion of accepting vectors is a basis for this method. The influence of atmosphere and geomagnetic field on the measured cosmic ray intensity at each point of observation is taken into consideration. At present, realization of global survey method in real-time became possible with a creation and development of database of neutron monitor measurements (NMDB). This report is a continuation of work by authors on development of methods for the space weather forecast by means of CR measurements. The first results of determination of CR daily anisotropy parameters by means of the global survey method in real-time and their connections with solar wind large-scale disturbances are given