Summary
The observational features of the arc are fairly well established. At present, the thermal conduction model appears to explain the red arc features most consistently, but it must be noted that a soft electron flux would give very similar results. Ion temperature measurements in the vicinity of an arc, which should be forthcoming in the very near future, can establish conclusively whether transverse electric fields play any important role in the formation of the arcs. Accepting the assumption that the arcs are the result of energy flowing down from the plasmasphere, the major remaining question is: where does the energy come from and how does it get into the plasmasphere? The various proposed mechanisms discussed in the previous chapter appear feasible, but much work needs to be done before this problem is completely resolved.
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On leave from the Department of Electrical Engineering, The University of Michigan, Ann Arbor.
The National Center for Atmospheric Research is sponsored by the National Science Foundation.
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Nagy, A.F., Roble, R.G. & Hays, P.B. Stable mid-latitude red arcs: Observations and theory. Space Sci Rev 11, 709–727 (1970). https://doi.org/10.1007/BF00177029
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DOI: https://doi.org/10.1007/BF00177029