Garrard, T. L. and Gibner, P. S. and Israel, M. H. and Klarmann, J. and Waddington, C. J. and Binns, W. R.
(1987)
Anisotropy of Galactic Iron of Energy 30 to 500 GeV/amu Studied by HEAO-3.
In:
Proceedings of the 21st International Cosmic Ray Conference.
Vol.1.
, Nakau, Russia, p. 348.
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Abstract
The anisotropy of cosmic ray iron observed by the Heavy Nuclei Experiment
[1] on the HEA0-3 spacecraft has been studied. A high rigidity data set was
chosen by requiring the Stoermer cutoff be greater than 7 GV, and the energy of
individual events was determined by relativistic rise in the ion chamber signal [2].
Events which have estimated rigidity well above their Stoermer cutoff rigidity
were chosen in order to reduce the effect of the geomagnetic field on the cosmic
ray trajectories. Selecting events with estimated rigidity greater than ~58 GV
from eight months of data yields 2459 events. This data set allows an anisotropy
measurement with a statistical uncertainty of 3%. We will continue to try
increasing the size. of the selected data set while limiting systematic errors due to
the geomagnetic and interplanetary fields.
Item Type: | Book Section |
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Additional Information: | © INR. Provided by the NASA Astrophysics Data System.
This research was supported in part by NASA under grants NAG 8-498, 500,
and 502 and NGR 05-002-160, 24-005,050, and 26-008-001. |
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Group: | Space Radiation Laboratory |
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Funders: | Funding Agency | Grant Number |
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NASA | NGR 05-002-160 | NASA | NGR 26-008-001 | NASA | NGR 24-005-050 | NASA | NAG 8-498 | NASA | NAG 8-500 | NASA | NAG 8-502 |
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Other Numbering System: | Other Numbering System Name | Other Numbering System ID |
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Space Radiation Laboratory | 1987-04 |
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Record Number: | CaltechAUTHORS:20140512-132135742 |
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Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140512-132135742 |
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Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
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ID Code: | 45691 |
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Collection: | CaltechAUTHORS |
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Deposited By: |
Joy Painter
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Deposited On: | 12 May 2014 20:31 |
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Last Modified: | 09 Mar 2020 13:18 |
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