Results of cosmic ray monitoring with a multichannel complex

This paper presents a method for monitoring geophysical parameters (atmospheric and magnetospheric) using cosmic rays (CR). This method rests on the principle of synchronous multichannel recording of all secondary CR components in the energy region from units to 200 GeV. The geophysical parameters can be estimated from the system of CR variation equations. We have analyzed results of CR monitoring over the period from January 2004, using the multichannel observation complex.