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20-125 MeV/nuc cosmic ray carbon nuclei intensities between 2004-2010 in solar cycle #23 as measured near the earth, at voyager 2 and also in the heliosheath at voyager 1 - modulation in a two zone heliospehre

Webber, W. R. and Cummings, A. C. and Stone, E. C. and McDonald, F. B. and Mewaldt, R. A. and Leske, R. and Wiedenbeck, M. and Higbie, P. R. and Heikkila, B. (2012) 20-125 MeV/nuc cosmic ray carbon nuclei intensities between 2004-2010 in solar cycle #23 as measured near the earth, at voyager 2 and also in the heliosheath at voyager 1 - modulation in a two zone heliospehre. . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20200204-101907790

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Abstract

The recovery of cosmic ray Carbon nuclei of energy ~20-125 MeV/nuc in solar cycle #23 from 2004 to 2010 has been followed at three locations, near the Earth using ACE data and at V2 between 74-92 AU and also at V1 beyond the heliospheric termination shock at between 91-113 AU. To describe the observed intensity changes and to predict the absolute intensities measured at all three locations we have used a simple spherically symmetric (no drift) two-zone heliospheric transport model with specific values for the diffusion coefficient in both the inner and outer zones. The diffusion coefficient in the outer zone is determined to be ~5-10 times smaller than that in the inner zone out to 90 AU. For both V1 and V2 the calculated C nuclei intensities agree within an average of ±10% with the observed intensities. Because of this agreement between V1 and V2 observations and predictions there is no need to invoke an asymmetrical squashed heliosphere or other effects to explain the V2 intensities relative to V1 as is the case for He nuclei. The combination of the diffusion parameters used in this model and the interstellar spectrum give an unusually low overall solar modulation parameter Φ = 250 MV to describe the Carbon intensities observed at the Earth in 2009. At all times both the observed and calculated spectra are very closely ~ E^(1.0) as would be expected in the adiabatic energy loss regime of solar modulation.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
https://arxiv.org/abs/1202.2081arXivDiscussion Paper
ORCID:
AuthorORCID
Cummings, A. C.0000-0002-3840-7696
Stone, E. C.0000-0002-2010-5462
Mewaldt, R. A.0000-0003-2178-9111
Leske, R.0000-0002-0156-2414
Wiedenbeck, M.0000-0002-2825-3128
Additional Information:The authors wish to thank the Voyager team (E.C. Stone, P.I.) and the ACE team (Andrew Davis) for making their data available on their web-sites, http://voyager.gsfc.nasa.gov and http://www.srl.caltech.edu/ACE/.
Group:Space Radiation Laboratory
Record Number:CaltechAUTHORS:20200204-101907790
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200204-101907790
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:101110
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:04 Feb 2020 18:47
Last Modified:04 Feb 2020 18:47

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