Wavelet analysis of solar wind ion flux fluctuations.

Details Wavelet analysis of solar wind ion flux fluctuations. Wavelet analysis of solar wind ion flux fluctuations.

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996kosis..34..407a&link_type=abstract

Kosmicheskie Issledovaniia, Tom 34, No. 4, p. 407 - 413

Physics

1

Solar Wind: Ions, Solar Wind: Solar Corona

Scientific paper

The authors analyse solar wind ion flux data measured by Monitor instrument at satellite Prognoz-8: the set about 30 - 70 h duration with 10, 24 s time-resolution and the set about 3 - 10 h with 1.28 s resolution. They present power spectra and results of wavelet analysis. They determine the set of temporal (from 11 h to 20 s) or spatial (from 17×106 to 10×103km) scales which may be typical for two processes: Alfvén waves and convective structures moving from upper corona of the Sun.

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