Cosmic ray fluctuations parameter as indicator of interplanetary "magnetic cork"

Abstract. It is established, that the main contribution into dynamics of galactic cosmic ray intensity fluctuations (GCR) in a vicinity of magnetic "cork" from a shock gives a nonrandom, non-Gauss component of GCR intensity. An occurrence of correlated fluctuations is caused by following circumstance: due to laws of conservation the probability that the cosmic ray particles reflected from a magnetic cork (in the expanding magnetic field) will undergo collimations, becomes considerable. The collimation will be manifested in focusing of particles into the anisotropic beams. In this case, observations should show "scintillations" of celestial sphere in cosmic rays i.e. the" HALO" effect .Similar scintillations are the indicator of interplanetary magnetic cork. The algorithm of detection of GCR scintillations is realized in real time using "Cyber-FORSHOCK" robotized system. Introduction It is known, that in diffusive approach the individual casual trajectories are attributed to particles. At the same time, during short periods of time (small spatial-temporal scales) a correlation of trajectories should be essential owing to which the groups of particles (near in phase space) are conserved rather long like compact formations or cluster