Moraal, H. (1990) Cosmic Ray Perpendicular Diffusion Coefficient and Drift Velocity Calculated from Pioneer/Voyager Observations. In: Proceedings of the 21st International Cosmic Ray Conference. Vol.6. Department of Physics and Mathematical Physics, The University of Adelaide , Northfield, South Australia, pp. 194-197. https://resolver.caltech.edu/CaltechAUTHORS:20140708-164245697
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Abstract
The radial and latitudinal gradients measured by the Pioneer 10 and Voyager 1 and 2 spacecraft, reported by Cummings and Stone (1990), provide a unique opportunity to calculate the cosmic ray perpendicular diffusion coefficient and drift velocity.
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| Additional Information: | © Organizing Committee of the 21st Int. Cosmic Ray Conference. Provided by the NASA Astrophysics Data System. I gratefully acknowledge stimulating discussions with A.C. Cummings and E.C. Stone, a.s well as the computational and technical assistance of KR. Lim. This work was supported in part by NASA under contract NAS-7-918 and grant NGR-05-002-160. | ||||||
| Group: | Space Radiation Laboratory | ||||||
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| Record Number: | CaltechAUTHORS:20140708-164245697 | ||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140708-164245697 | ||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 47090 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Deborah Miles | ||||||
| Deposited On: | 21 Jul 2014 21:20 | ||||||
| Last Modified: | 03 Oct 2019 06:49 |
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