Wavelet analysis of the 26 days recurrent component in the outer heliosphere

Details Wavelet analysis of the 26 days recurrent component in the outer heliosphere Wavelet analysis of the 26 days recurrent component in the outer heliosphere

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3592k&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

It has been reported in previous studies that the 26-day recurrent phenomena exist in the data of intensity variations of solar wind, interplanetary magnetic field and cosmic rays observed in the outer Heliosphere. In recent paper by Zhang (1994), a liner correlation between mean amplitude of those recurrent phenomena and latitudinal gradient of cosmic rays has been reported based on the data from Ulysses. We analyse this phenomena at larger heliospheric distances using observations from the cycle 21 solar minimum period by applying a wavelet transform technique to the data from Voyager-1 &-2 and Pioneer-11. The average amplitudes as derived for Ions (>70 MeV/n) or H (>80 MeV), are 1.78+0.47 (%), 0.69+0.25 (%) and 5.64+1.05 (%) at the location of Voyager-1, -2 and Pioneer-11, respectively.

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