An unusual SAR arc observed during ring current development, 4 August 1972

Abstract

Measurements made from the ISIS-II spacecraft at 1400 km and ground-based measurements from New Zealand provide a detailed description of an unusual SAR arc observed at dusk on 4 August 1972, during the growth phase of the ring current. Proton precipitation was observed over a latitude range of a few degrees, with electron temperature enhancements throughout the region but espeically at its boundaries, and an F-region trough was present at the equatorward boundary. SAR arcs usually occur at equatorward proton boundaries but this one appeared at the poleward boundary, which seems to have given rise to a number of unusual features. Characteristics unique to this event are a high flux of low energy electrons at the SAR arc location, associated with an upward field-aligned current there, and a "slot" in the ambient electron density, which falls to 5% of the background density over a region of 1.5 km half-width. Immediately poleward of the low energy electron flux, intense whistler mode noise (0.1-0.4 MHz) is evident. The 6300 A emission, which has a total intensity of 10.6 kR, appears divided into two components, one at 285 km excited by the low energy electrons, and the other at 400 km, excited thermally by the electron gas. Comparisons are made with S3-A spacecraft observations made in the equatorial region at the same time, with ISIS-II observations of a more normal SAR arc, and with other observations reported in the literature. The kinetic Alfven wave process described by Hasegawa and Mima (1978) seems a candidate for the acceleration of these low energy electrons, but it is not possible to entirely exclude the alternative of an auroral-type acceleration process.