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Cited by 188

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Correlation of changes in the outer‐zone relativistic‐electron population with upstream solar wind and magnetic field measurements

Blake, J. B., Baker, D. N., Turner, N., Ogilvie, K. W., Lepping, R. P.·1997·Geophysical Research Letters
DOI 10.1029/97gl00859
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Abstract

A study has been made of the correlation of the population of relativistic electrons in the outer‐zone magnetosphere with the properties of the solar wind (speed, density, magnetic field) during a solar minimum period. The study is based upon observations made in the Spring of 1995 with sensors aboard 1994‐026 and WIND. It is found that a large relativistic electron enhancement depends upon a substantial solar‐wind speed increase associated with precursor solar‐wind density enhancement, and, in particular, upon a southward turning of the interplanetary magnetic field.

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Metadata

Authors
Blake, J. B., Baker, D. N., Turner, N., Ogilvie, K. W., & Lepping, R. P.
Venue
Geophysical Research Letters
Publisher
American Geophysical Union (AGU)
Published
1997-04-15
Volume
24
Issue
8
Pages
927-929
ISSN
  • 0094-8276 (ISSN-L)
  • 1944-8007
DOI
10.1029/97gl00859
OpenAlex
W2094137558
Cited by
188
References
0
FWCI
11.52
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Correlation of changes in the outer‐zone relativistic‐electron population with upstream solar wind and magnetic field measurements. https://app.cochat.ai/papers/10.1029/97gl00859
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Blake, J. B., Baker, D. N., Turner, N., Ogilvie, K. W., & Lepping, R. P. (1997). Correlation of changes in the outer‐zone relativistic‐electron population with upstream solar wind and magnetic field measurements. Geophysical Research Letters. https://doi.org/10.1029/97gl00859

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.