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- W2034156771 endingPage "2397" @default.
- W2034156771 startingPage "2387" @default.
- W2034156771 abstract "Fluxes of energetic electrons of terrestrial origin are frequently found beyond the bow shock on the sunward side of the earth. The duration of individual events is from less than a minute up to several minutes, but they tend to occur in clusters lasting as long as several hours. Their flux is usually a few hundred cm−2 sec−1, but occasionally it reaches 3 × 104 cm−2 sec−1 for electrons > 40 kev. The upstream electron spikes are associated with rapid motion of the bow shock. The best interpretation of upstream spikes is that they are simply electrons moving up interplanetary field lines from the magnetosheath just behind the shock where they originated as bow shock spikes." @default.
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- W2034156771 date "1968-04-01" @default.
- W2034156771 modified "2023-10-02" @default.
- W2034156771 title "Energetic electrons of terrestrial origin upstream in the solar wind" @default.
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- W2034156771 doi "https://doi.org/10.1029/ja073i007p02387" @default.
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