Further indications of a ∼140 day recurrence in energetic particle fluxes at 1 and 5 AU from the Sun

Author:

Dalla S.,Balogh A.,Heber B.,Lopate C.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference15 articles.

1. A 154-day periodicity in the occurrence rate of proton flares;Bai;Astrophys. J.,1990

2. The role of interplanetary shocks in the longitude distribution of solar energetic particles;Cane;J. Geophys. Res.,1988

3. Interplanetary magnetic field periodicity of 153 days;Cane;Geophys. Res. Lett.,1998

4. Recurrence in MeV proton fluxes and anisotropies at 5 AU from the Sun;Dalla;Geophys. Res. Lett.,2000

5. Spatial evolution of 26-day recurrent galactic cosmic ray decreases: Correlated ULYSSES COSPIN KET and SOHO COSTEP observations;Heber;Proc. ESLAB Symp. 31st,1997

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