Heliospheric Modulation of Cosmic Rays in the Era of Neutron Monitoring

The heliospheric modulation potential of galactic cosmic rays (CRs) is reconstructed for the era of neutron monitoring. It is based on using a modern model of the interstellar spectrum of galactic CRs and the spectrum of CR density variations. The spectrum of CR variations is obtained via global spectrographic processing of continuous monitoring data from the world network of detectors and is calibrated using data from direct measurements of the particle spectrum on the PAMELA magnetic spectrometer in base year 2009.