Methods and software for cosmic ray scintillation studies

Details Methods and software for cosmic ray scintillation studies Methods and software for cosmic ray scintillation studies

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..518g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 518-520 (SEE N85-34991 23-93)

Physics

Autoregressive Processes, Fourier Transformation, Galactic Cosmic Rays, Scintillation, Statistical Analysis, Time Series Analysis, Forbush Decreases, Solar Flares

Scientific paper

The principal instrument used in cosmic ray scintillation studies is the spectra constructed from intensive observation. This method has its drawbacks in that the statistical characteristics of the process undergo essential reconstruction, i.e., the process becomes nonstationary from the viewpoint of such phenomena as Forbush decrease and during solar flares. The software used to process the above includes the direct Fourier transform and its modifications, autoregressive processes, and instantaneous spectrum methods. Used in various combinations, they prove helpful in handling the time series.

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