Simultaneous Optical and Radar Signatures of Poleward Moving Auroral Forms

A.THOROLFSSON ⁽¹⁾, J.-C. CERISIER ⁽¹⁾, M. LOCKWOOD⁽²⁾ , P. E. SANDHOLT ⁽³⁾, C. SENIOR ⁽¹⁾, M. LESTER ⁽⁴⁾

(1) CETP, France

(2) Rutherford Appleton Laboratory, UK

(3) University of Oslo, Norway

University of Leicester, UK

Dayside poleward moving auroral forms (PMAFs) were detected between 06:30 and 07:00 UT on December 16, 1998, by the meridian scanning photometer and the all-sky camera at Ny-Alesund, Svalbard. Simultaneous SuperDARN HF radar measurements permitted the study of the associated ionospheric convection velocity pattern. A good general agreement is observed between the location and movement of velocity enhancements (flow channels) and the PMAFs. Clear signatures of equatorward flow were detected in the vicinity of PMAFs. This flow is believed to be the signature of a return flow outside the reconnected flux tube, as predicted by the Southwood model [1]. The simulated signatures of this model reproduce globally the measured signatures. The differences with the experimental data can be explained by the simplifications of the model. Proposed schemes of the flow modification due to the presence of several flow channels and the modification of cusp and region~1 field-aligned currents at the time of sporadic reconnection events are shown to fit well with the observations.

[1] Southwood, D. J., J. Geophys. Res., 92, 3207, 1987.

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