10-14 October 2016
Milan Hotel
Europe/Moscow timezone

Method of flicker-noise spectroscopy of cosmic rays muon flux variations caused by non-stationary processes

12 Oct 2016, 15:30
30m
Hall of the 2nd floor (Milan Hotel)

Hall of the 2nd floor

Milan Hotel

Shipilovskaya Street, 28A, Moscow, Russia, 115563
Poster Cosmic rays Poster session - III

Speaker

Dr. Vladimir Borog (National Research Nuclear University MEPhI (Moscow Engineering Physics Institute))

Description

The paper presents a new method of identifying signals in a statistically noisy non-stationary time series. In difference from Fourier and wavelet analysis in the processing of data does not make any assumptions about the structure of the signal-analyzer. The proposed method of flicker-noise spectroscopy is demonstrated on simulated and real time series related to monitoring solar activity registration flow of solar and cosmic radiation using ground level muon hodoscope. The method is applicable for analysis of a wide range of different helio - and geophysical processes. This work was supported by RFBR grant 16-05-00997.

Primary author

Dr. Vladimir Borog (National Research Nuclear University MEPhI (Moscow Engineering Physics Institute))

Co-authors

Dr. Anna Dmitrieva (National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)) Ms. Anna Kovylyaeva (National Research Nuclear University MEPhI)

Presentation Materials

There are no materials yet.
Your browser is out of date!

Update your browser to view this website correctly. Update my browser now

×