80 results on '"Webber, W. R."'
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2. Voyagers 1 and 2 in a shrunken and squashed heliosphere.
3. What Voyager cosmic ray data in the outer heliosphere tells us about 10Be production in the Earth's polar atmosphere in the recent past.
4. Transient intensity changes of cosmic rays beyond the heliospheric termination shock as observed at Voyager 1.
5. Galactic propagation of cosmic ray nuclei in a model with an increasing diffusion coefficient at low rigidities: A comparison of the new interstellar spectra with Voyager data in the outer heliosphere.
6. Galactic cosmic ray H and He nuclei energy spectra measured by Voyagers 1 and 2 near the heliospheric termination shock in positive and negative solar magnetic polarity cycles.
7. Passage of a large interplanetary shock from the inner heliosphere to the heliospheric termination shock and beyond: Its effects on cosmic rays at Voyagers 1 and 2.
8. Temporal and spectral variations of anomalous oxygen nuclei measured by Voyager 1 and Voyager 2 in the outer heliosphere.
9. Anomalous cosmic rays in the distant heliosphere and the reversal of the Sun's magnetic polarity in Cycle 23.
10. The disappearance of anomalous protons at Voyager 1 and Voyager 2 in the outer heliosphere between 1998 and 2002.
11. Time variations of cosmic ray electrons and nuclei between 1978 and 2004: Evidence for charge-dependent modulation organized by changes in solar magnetic polarity and current sheet tilt.
12. An empirical estimate of the heliospheric termination shock location with time with application to the intensity increases of MeV protons seen at Voyager 1 in 2002-2005.
13. Differences in the spectra of anomalous cosmic ray helium nuclei in two solar magnetic polarity cycles.
14. Intensities of galactic cosmic rays of ∼1.5 GV rigidity at Earth versus the heliospheric current sheet tilt.
15. Heliocentric radial intensity profiles of galactic cosmic rays measured by the IMP, Voyager, and Pioneer spacecraft in solar 11-year modulation cycles of opposite magnetic polarity.
16. Onset and amplitude of the 11-year solar modulation of cosmic ray intensities at the Earth and at Voyagers 1 and 2 during the period from 1997 to 2003.
17. Large global transient decreases of >70 MeV cosmic rays observed at Voyager 1 and Voyager 2 in the outer heliosphere in 2001-2003: The onset of heliospheric 2-3 kHz radio emission and the distance to the heliopause.
18. Modulation of cosmic ray protons in the heliosheath.
19. Production of cosmogenic Be nuclei in the Earth's atmosphere by cosmic rays: Its dependence on solar modulation and the interstellar cosmic ray spectrum.
20. Changes of the outer to inner heliospheric intensity ratios of >70 MeV galactic cosmic rays as a function of solar magnetic polarity.
21. Voyager and Pioneer spacecraft measurements of cosmic ray intensities in the outer heliosphere: Toward a new paradigm for understanding the global solar modulation process: 1. Minimum solar modulation (1987 and 1997).
22. Voyager and Pioneer spacecraft measurements of cosmic ray intensities in the outer heliosphere: Toward a new paradigm for understanding the global modulation process: 2. Maximum solar modulation (1990-1991).
23. Differences in the maximum intensities and the intensity-time profiles of cosmic rays in alternate solar magnetic field polarities.
24. Using transient decreases of cosmic rays observed at Voyagers 1 and 2 to estimate the location of the heliospheric termination shock.
25. A new look at the >70 Mev cosmic ray radial gradients in the heliosphere measured by spacecraft.
26. Cosmic ray modulation during solar activity cycle 20.
27. Spectrum of mean free paths near Earth in the solar cosmic ray event of April 29, 1973.
28. The interplanetary scattering mean free path from 1 to 3 × 10³ MV.
29. A comparison of cosmic ray intensities near the Earth at the sunspot minima in 1976 and 1987 and during 1995 and 1996.
30. Intensities of anomalous and galactic cosmic rays in the outer heliosphere near the heliospheric equator in 1987 and during the period from 1994 to 1996.
31. Comparison of the rigidity dependence of the 11-year cosmic ray variation at the earth in two solar cycles of opposite magnetic polarity.
32. The distance to the solar wind termination shock in 1993 and 1994 from observations of anomalous cosmic rays.
33. Distance to the solar wind termination shock and the source flux of anomalous cosmic rays during 1986-1988.
34. Large cosmic ray transient decreases observed in the heliosphere at the Earth, Voyagers 1 and 2 and Pioneer 10 from 1987 to 1991.
35. Estimate of the distance to the solar wind termination shock from gradients of anomalous cosmic ray oxygen.
36. Giant transient decreases of cosmic rays in the outer heliosphere in September 1991.
37. Absolute spectrum and charge ratio of cosmic ray muons in the energy region from 0.2 GeV to 100 GeV at 600 m above sea level.
38. On the interplanetary cosmic ray latitudinal gradient.
39. An observation of a heliospheric magnetic cycle dependence for the integral radial gradient of E > 60 MeV cosmic rays.
40. Forbush decreases and interplanetary magnetic field disturbances: Association with magnetic clouds.
41. The rigidity dependence of forbush decreases observed at the Earth.
42. Differences in the solar modulation of E > 60 MeV cosmic rays at Earth and 18 AU during a complete 11-year cycle from 1977 to 1988.
43. The onset of the new solar modulation cycle in 1987-1988 as a function of heliocentric radius and latitude.
44. Characteristics of the 22-year modulation of cosmic rays as seen by neutron monitors.
45. Interplanetary cosmic ray latitudinal gradient in 1984 to 1987 using IMP 8 and Voyager data.
46. Characteristics of large Forbush-type decreases in the cosmic radiation: 2. Observations at different heliocentric radial distances.
47. Changes in the energy spectrum of anomalous oxygen during 1977-1985.
48. Characteristic recovery times of Forbush-type decreases in the cosmic radiation: 1. Observations at Earth at different energies.
49. Observations of the dynamics of the cosmic ray modulation.
50. A study of the long-term variation and radial gradient of cosmic rays out to 23 AU.
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