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Bi‐directional streaming of solar wind electrons >80 eV: ISEE evidence for a closed‐field structure within the driver gas of an interplanetary shock
Publication with shared reference
10.1029/gl008i002p00173
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Publications
Bi‐directional streaming of solar wind electrons >80 eV: ISEE evidence for a closed‐field structure within the driver gas of an interplanetary shock
Publication with shared reference
10.1029/gl008i002p00173
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Bi‐directional streaming of solar wind electrons >80 eV: ISEE evidence for a closed‐field structure within the driver gas of an interplanetary shock
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