Inferring Energetic Particle Mean-free Paths from Observations of Anomalous Cosmic rays in the Outer Heliosphere at Solar Maximum

Details Inferring Energetic Particle Mean-free Paths from Observations of Anomalous Cosmic rays in the Outer Heliosphere at Solar Maximum Inferring Energetic Particle Mean-free Paths from Observations of Anomalous Cosmic rays in the Outer Heliosphere at Solar Maximum

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc...10.4243c&link_type=abstract

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

Physics

3

Scientific paper

We find that the mean free pathlength is higher by a factor of 10 or more at solar minimum than at the last solar maximum in 1900-1991, consistent with previous findings. In 2000-2001, the mean free pathlength has declined by a factor of ¡ 10, but is still larger by a factor of ¡ 3.6 than its value of ¡ 0.15 AU in 1990-1991. As solar maximum conditions become durably established in the outer heliosphere over the next few months, it may be possible to deduce the radial dependence of the mean free pathlength.

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