Published December 7, 1962
| Version public
Journal Article
Interplanetary Magnetic Fields
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1.
California Institute of Technology
Abstract
Preliminary analysis of Mariner II magnetometer data indicates a persistent interplanetary field varying between a least 2 and 10 gamma (1γ = 10^(-5) gauss). The interplanetary field appears to lie mainly in the ecliptic plane, although there is a substantial, fluctuating, transverse component. The Mariner II data agree reasonably well with the prior Pioneer V observations. Typically, variations as large as 5 to 10 gamma in the field component radial from the sun are measured. Correlations with the Mariner II plasma measurements have been observed.
Additional Information
© 1962 American Association for the Advancement of Science. Received 23 November 1962. We acknowledge the assistance of B. V. Connor, magnetometer project engineer, and K. Heftman, scientific data coordinator. Supported by contracts with the National Aeronautics and Space Administration.Additional details
Identifiers
- Eprint ID
- 62373
- Resolver ID
- CaltechAUTHORS:20151124-110517158
Related works
- Describes
- http://www.jstor.org/stable/1709490 (URL)
Funding
- NASA
Dates
- Created
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2015-11-24Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field