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Voyager 2 Observations of MeV Ions in the Outer Heliosphere Over the Solar Maximum Period of Cycle 23

Authors :
Acharya, B.
Gupta, S.
Jain, Atul
Karthikeyan, S.
Morris, S.
Tonwar, S.
McDonald, F. B.
Stone, E. C.
Burlaga, L. F.
Cummings, A. C.
Heikkila, B. C.
Lal, N.
Ness, N. F.
Richardson, J. D.
Webber, W. R.
Acharya, B.
Gupta, S.
Jain, Atul
Karthikeyan, S.
Morris, S.
Tonwar, S.
McDonald, F. B.
Stone, E. C.
Burlaga, L. F.
Cummings, A. C.
Heikkila, B. C.
Lal, N.
Ness, N. F.
Richardson, J. D.
Webber, W. R.
Publication Year :
2005

Abstract

Over the period 2001.0 - 2005.4, (63 - 74 AU) Voyager 2 observed a series of 9 energetic particle increases that persist over some 3 - 4 solar rotations, occur with a quasi-periodicity of some 145 days and are generally associated with the passage of a merged interaction region. With the onset of GCR recovery from solar maximum levels in 2004.6 there is a marked change in the nature of the V2 energetic particle increases that suggest these new events originated at the termination shock.

Details

Database :
OAIster
Notes :
application/pdf, Voyager 2 Observations of MeV Ions in the Outer Heliosphere Over the Solar Maximum Period of Cycle 23, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1005055632
Document Type :
Electronic Resource