Intensity variations of >70‐Mev cosmic rays measured by Pioneer 10, Voyager 1 & 2 and IMP in the heliosphere during the recovery period from 1992–1995

Geophysical Research Letters

Volumn 22, Issue 19, 1995, Pages 2669-2672

  Webber, W R ^a   Lockwood, J A ^b  

^a NEW MEXICO STATE UNIVERSITY   (United States)

^b UNIVERSITY OF NEW HAMPSHIRE   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0043176605     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/95GL02636     Document Type: Article

References (7)

1. Anomalous cosmic ray gradients throughout the heliosphere
2. Differences in the solar modulation of >70‐MeV cosmic‐rays at the Earth and at 18 AU during a complete 11‐year cycle from 1977 to 1988
3. Re‐analysis and confirmation of positive latitudinal gradients for anomalous Helium and galactic cosmic‐rays measured in 1975–1976 with Pioneer 11
4. The role of merged interaction regions and drifts in the heliospheric modulation of cosmic‐rays beyond 20 AU: A computer simulation
5. A drift model for the modulation of galactic cosmic‐rays
6. The latitude gradients of galactic cosmic‐ray and anomalous Helium fluxes measured on Ulysses from the Sun's south polar regions to the Equator
7. An estimate of the location of the modulation boundary for >70‐MeV galactic cosmic rays using Voyager and Pioneer spacecraft data