Identification of Solar Coronal Mass Ejections in Cosmic Ray Flux Using Flicker Noise Spectroscopy

In this article, we examine the possibility of applying the method of flicker noise spectroscopy to identification of anomalies in flux of cosmic rays (CR). Typically, such anomalies appears after intense solar outbursts, when the Sun emits into space giant blobs of plasma also called coronal mass ejection (CME). Identification of such anomalies in the CR flux allows us to detect CME, approaching to Earth. CMEs, powerful enough, can cause significant damage to electrical appliances. The present paper describes basic concepts of the flicker noise spectroscopy and principles of cosmic rays data processing algorithms.