Jovian Electrons at SOHO From 1995 - 2002: Indications for Long-term Variations of the Jovian Source Strength

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2116 Energetic Particles, Planetary, 2784 Solar Wind/Magnetosphere Interactions, 5737 Magnetospheres (2756), 6220 Jupiter

Scientific paper

SOHO was launched in December 1995 into the solar minimum between the cycles 22 and 23. Right after launch the COSTEP instrument detected 25 day recurrent periods of enhanced 0.25-15~MeV electron intensity that were not correlated with solar activity. This pattern reoccurred 13 months later, indicating a Jovian origin with the typical Jovian synodic period. However, the systematic 25 day periods present during solar minimum were not seen during solar maximum. Instead, the level of intensity of the 13 month periods increased from minimum to maximum, an observation that is in agreement with Ulysses observations at high latitudes. Possible mechanisms for this behavior will be discussed.

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