Abstract

Abstract. We investigate an omega-band event that took place above northern Scandinavia around 02:00–02:30 UT on 9 March 1999. In our analysis we use ground based magnetometer, optical and riometer measurements together with satellite based optical images. The optical and riometer data are used to estimate the ionospheric Hall and Pedersen conductances, while ionospheric equivalent currents are obtained from the magnetometer measurements. These data sets are used as input in a local KRM calculation, which gives the ionospheric potential electric field as output, thus giving us a complete picture of the ionospheric electrodynamic state during the omega-band event. The overall structure of the electric field and field-aligned current (FAC) provided by the local KRM method are in good agreement with previous studies. Also the E×B drift velocity calculated from the local KRM solution is in good qualitative agreement with the plasma velocity measured by the Finnish CUTLASS radar, giving further support for the new local KRM method. The high-resolution conductance estimates allow us to discern the detailed structure of the omega-band current system. The highest Hall and Pedersen conductances, ~50 and ~25 S, respectively, are found at the edges of the bright auroral tongue. Inside the tongue, conductances are somewhat smaller, but still significantly higher than typical background values. The electric field shows a converging pattern around the tongues, and the field strength drops from ~40 mV/m found at optically dark regions to ~10 mV/m inside the areas of enhanced conductivity. Downward FAC flow in the dark regions, while upward currents flow inside the auroral tongue. Additionally, sharp conductance gradients at the edge of an auroral tongue are associated with narrow strips of intense FACs, so that a strip of downward current flows at the eastern (leading) edge and a similar strip of upward current is present at the western (trailing) edge. The Joule heating follows the electric field pattern, so that it is diminished inside the bright auroral tongue.

Highlights

  • Omega-bands are meso-scale undulations in the poleward boundary of diffuse auroras

  • The ionospheric electrodynamics of omega-bands has been studied in several papers, which all support the overall picture of a sequence of upward and downward field-aligned currents (FACs) located in the bright and dark regions of the structure, respectively

  • We have studied the electrodynamics of an omega-band event with the local KRM method (Vanhamaki and Amm, 2007) that uses magnetometer, riometer and optical data as input and generates the electric field as output

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Summary

Introduction

Omega-bands are meso-scale (usually 400–1000 km) undulations in the poleward boundary of diffuse auroras. In the present study we will revisit the omega-band electrodynamics once again with a method that uses magnetic, optical and riometer data as input for the calculation of electric fields and currents. The purpose of this paper is two-fold: Firstly, we want to present the first case study where the local KRM technique developed by Vanhamaki and Amm (2007) is applied to real data This demonstrates the capabilities and limitations of the new analysis method, e.g. in respect to input data requirements. Vanhamaki and Amm (2007) verified the new method using synthetic examples of typical ionospheric current systems, but in this study we compare the calculated electric field with direct measurements done by a coherent scatter radar.

Ionospheric equivalent currents
UVI conductance estimates
Electric field measurements
Local KRM method
Data processing
Large scale structure with UVI conductance estimate
Small scale structure with emap conductance estimate
Components of FAC
Joule heating
Comparison with CUTLASS measurements
Findings
Discussion and conclusions
Full Text
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