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- W2004563025 abstract "A challenging problem of cusp/cleft auroral research is to identify the boundary between open and closed magnetic field lines. In order to unambiguously distinguish between viscous and reconnection modes of solar wind-magnetosphere coupling, it is mandatory to know whether or not the auroral features observed in the ionosphere are associated with open or closed magnetic flux. In this paper we approach this issue by using particle data from NOAA-12 crossings through a certain category of transient dayside auroral features. This category of events has usually been attributed to time-varying magnetopause reconnection. The transient auroral forms were coincident with an intense flux of magnetosheath-like plasma. As expected these events were located poleward of the trapping boundary. A secondary population of energetic ions, however, refines the particle test of open or closed magnetic field topology." @default.
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- W2004563025 date "1998-01-01" @default.
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- W2004563025 title "NOAA-12 satellite and ground correlative study of cusp/cleft aurora above Svalbard" @default.
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- W2004563025 doi "https://doi.org/10.1016/s0273-1177(98)00179-3" @default.
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