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W.R. Webber

Identifiers

  • name variant W.R. Webber 0.60 · backfill

Papers (34)

  1. Fitting the Galactic Electron Spectrum Measured by Voyager at Low Energies and also by CALET/AMS-2 at High Energies Using a Monte Carlo Diffusion Model for Electron Propagation - One Spectrum Fits All physics.space-ph · 2018 · author #1
  2. Measurements in Interstellar Space of Galactic Cosmic Ray Isotopes of Li, Be, B and N, Ne Nuclei Between 40-160 MeV/nuc by the CRS Instrument on Voyager 1 physics.space-ph · 2018 · author #1
  3. Cosmic Ray Electrons and Protons ~1 MeV - A 40 Year Study of Their Intensities from the Earth to the Heliopause and Beyond Into Local Interstellar Space by the CRS Experiment on Voyager 1 physics.space-ph · 2018 · author #1
  4. A Comparison of the Galactic Cosmic Ray Electron and Proton Intensities From 1 MeV/nuc to 1 TeV/nuc Using Voyager and Higher Energy Magnetic Spectrometer Measurements Are There Differences in the Source Spectra of These Particles? physics.space-ph · 2018 · author #1
  5. A Comparison of Galactic Cosmic Ray Proton and Helium Nuclei Spectra From ~10 MeV/nuc to 1 TeV/nuc Using New Voyager and Higher Energy Magnetic Spectrometer Measurements - Are There Differences In the Source Spectra of The Two Nuclei physics.space-ph · 2018 · author #1
  6. The Spectra of 2H and 3He Secondary Cosmic Ray Isotopes from ~20-85 MeV/nuc as Measured Using the B-end HET Telescope on Voyager beyond the Heliopause and a Fit to These Interstellar Spectra Using a Leaky Box Propagation Model physics.space-ph · 2018 · author #1
  7. Voyager 1 Measurements Beyond the Heliopause of Galactic Cosmic Ray Helium, Boron, Carbon, Oxygen, Magnesium, Silicon and Iron Nuclei with Energies 0.5 to >1.5 GeV/nuc physics.space-ph · 2017 · author #1
  8. The Different Shapes of the LIS Energy Spectra of Cosmic Ray He and C Nuclei Below ~1 GeV/nuc and The Cosmic Ray He/C Nuclei Ratio vs. Energy -V1 Measurements and LBM Propagation Predictions physics.space-ph · 2017 · author #1
  9. The Cosmic Ray Boron/Carbon Ratio Measured at Voyager and at AMS-2 from 10 MeV/nuc up to ~1 TeV/nuc and a Comparison With Propagation Calculations physics.space-ph · 2017 · author #1
  10. A Galactic Cosmic Ray Electron Intensity Increase of a factor of up to 100 At Energies between 3 and 50 MeV in the Heliosheath between the Termination Shock and the Heliopause Due to Solar Modulation As Measured by Voyager 1 physics.space-ph · 2017 · author #1
  11. The Intensities of Cosmic Ray H and He Nuclei at ~250 MeV/nuc Measured by Voyagers 1 and 2 - Using these Intensities to Determine the Solar Modulation Parameter in the Inner Heliosphere and the Heliosheath Over a 40 Year Time Period physics.space-ph · 2017 · author #1
  12. The Galactic Cosmic Ray Electron Spectrum from 3 to 70 MeV Measured by Voyager 1 Beyond the Heliopause, What This Tells Us About the Propagation of Electrons and Nuclei In and Out of the Galaxy at Low Energies physics.space-ph · 2017 · author #1
  13. Observations of the Abundances of Secondary Galactic Cosmic Rays from Z equals 5 to 28 Between 10 and 200 MeV/nuc Beyond the Heliopause by Voyager, Some Unexpected Anomalies and Their Interpretation Using a LBM for Galactic Propagation physics.space-ph · 2016 · author #1
  14. A Study of the B/C Ratio Between 10 MeV/nuc and 1 TeV/nuc in Cosmic Rays Using New Voyager and AMS-2 Data and a Comparison with the Predictions of Leaky Box Propagation Models physics.space-ph · 2016 · author #1
  15. Determination of the Total Solar Modulation Factors in the Heliosphere For Cosmic Ray Protons and Electrons by Comparing Interstellar Spectra Deduced from Voyager Measurements and PAMELA Spectra of These Particles at the Earth physics.space-ph · 2016 · author #1
  16. Fitting the Low Energy Spectra of Cosmic Ray Primary Nuclei from C to Fe as Measured on Voyager 1 physics.space-ph · 2016 · author #1
  17. The Abundance of Low Energy Cosmic Ray Boron and Nitrogen Nuclei Measured at Voyager 1 Beyond the Heliopause, Where Do They All Come From? An Interpretation Using a Leaky Box Galactic Propagation Model physics.space-ph · 2015 · author #1
  18. The Separation of Secondary Positrons Produced in the Galaxy from the High Energy Positrons that are Observed Recent Space Experiments on PAMELA and AMS2 physics.space-ph · 2015 · author #1
  19. A Galactic Cosmic Ray Electron Spectrum from 2 MeV to 2 TeV That Fits Voyager 5-60 MeV Data at Low Energies and PAMELA and AMS-2 Data at 10 GeV Using an Electron Source Spectrum E^-2.25 A Calculation Using a Monte Carlo Diffusion Model physics.space-ph · 2015 · author #1
  20. Interstellar Spectra of Primary Cosmic Ray Nuclei from H through Fe Measured at Voyager and a Comparison with Higher Energy Measurements, An Interpretation of the Spectra from 10 MeVnuc to Over 100 GeVnuc Using a Leaky Box Model physics.space-ph · 2015 · author #1
  21. The Cosmic Ray Helium and Carbon Nuclei Spectra Measured by Voyager 1 at Low Energies and Earth Based Measurements of these Nuclei up to 200 GeV nuc Concordance at High Energies with a Leaky Box Propagation Model physics.space-ph · 2015 · author #1
  22. A Fit to the Galactic Cosmic Ray Hydrogen and Helium Spectra at Voyager 1 at Low Energies and Earth Based Measurements at Much Higher Energies with Identical Rigidity Independent Source Spectra for the Hydrogen and Helium Nuclei physics.space-ph · 2015 · author #1
  23. A Comparison of Radial Intensity Profiles of Termination Shock Particles and Anomalous Cosmic Rays in the Outer North-South Heliosheaths Using CRS data from V1 and V2 physics.space-ph · 2015 · author #1
  24. A Forecast for a South Heliopause Crossing by Voyager 2 in Late 2014 Using Intensity-time Features of Energetic Particles Observed by V1 and V2 in the North and South Heliosheaths physics.space-ph · 2014 · author #1
  25. Voyager 1 and 2 Observations of Cosmic Ray Intensities in the North-South Heliosheaths-Implications for the Latitude Extent of the Heliospheric Current Sheet and Radial Structure in the Heliosheath physics.space-ph · 2014 · author #1
  26. Calculations of the Propagated LIS Electron Spectrum Which Describe the Cosmic Ray Electron Spectrum below ~100 MeV Measured Beyond 122 AU at Voyager 1 and its Relationship to the PAMELA Electron Spectrum above 200 MeV physics.space-ph · 2013 · author #1
  27. A Comparison of the Galactic Cosmic Ray H, He and C/O Nuclei Spectra Measured Between ~5 and 500 MeV/nuc Beyond 122 AU at Voyager 1 with the Predictions of a Diffusion Model for Propagation in the Galaxy physics.space-ph · 2013 · author #1
  28. The Unfolding of the Spectra of Low Energy Galactic Cosmic Ray H and He Nuclei as the Voyager 1 Spacecraft Exits the Region of Heliospheric Modulation physics.space-ph · 2013 · author #1
  29. 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 physics.geo-ph · 2012 · author #1
  30. Recovery of 150-250 MeV/nuc Cosmic Ray Helium Nuclei Intensities Between 2004-2010 Near the Earth, at Voyager 2 and Voyager 1 in the Heliosheath - A Two Zone Helioshpere physics.geo-ph · 2011 · author #1
  31. Voyagers 1 and 2 in a Shrunken and Squashed Heliosphere astro-ph.SR · 2011 · author #1
  32. A Comparison Of New Calculations Of The Yearly 10Be Production In The Earths Polar Atmosphere By Cosmic Rays With Yearly 10Be Measurements In Multiple Greenland Ice Cores Between 1939 And 1994 - A Troubling Lack Of Concordance Paper #2 physics.geo-ph · 2010 · author #1
  33. A comparison of new calculations of 10be production in the earths polar atmosphere by cosmic rays with 10be concentration measurements in polar ice cores between 1939-2005 - a troubling lack of concordance paper #1 physics.geo-ph · 2010 · author #1
  34. Two recent kHz outer heliospheric radio emissions seen at Voyager 1-What are the interplanetary events that trigger them and where are these events when the radio emissions start? physics.space-ph · 2009 · author #1

Mentions

  • 1508.06237 #1 · backfill · confidence 0.70 W.R. Webber
  • 1508.01542 #1 · backfill · confidence 0.70 W.R. Webber
  • 1503.05891 #1 · backfill · confidence 0.70 W.R. Webber
  • 1503.01035 #1 · backfill · confidence 0.70 W.R. Webber
  • 1502.01307 #1 · backfill · confidence 0.70 W.R. Webber
  • 1409.7402 #1 · backfill · confidence 0.70 W.R. Webber
  • 1403.3322 #1 · backfill · confidence 0.70 W.R. Webber
  • 1308.6598 #1 · backfill · confidence 0.70 W.R. Webber
  • 1308.4426 #1 · backfill · confidence 0.70 W.R. Webber
  • 1308.1895 #1 · backfill · confidence 0.70 W.R. Webber
  • 1202.2081 #1 · backfill · confidence 0.70 W.R. Webber
  • 1109.1810 #1 · backfill · confidence 0.70 W.R. Webber
  • 1101.3533 #1 · backfill · confidence 0.70 W.R. Webber
  • 1004.2675 #1 · backfill · confidence 0.70 W.R. Webber
  • 1003.4989 #1 · backfill · confidence 0.70 W.R. Webber
  • 0906.2746 #1 · backfill · confidence 0.70 W.R. Webber

Frequent Coauthors