Statistical Distribution of Decameter Scale (50 m) Ionospheric Irregularities at High Latitudes

We present a study of decameter scale ionospheric irregularities using in-situ electron density data from the NorSat-1 satellite. During the current period of low solar activity, NorSat-1 frequently observes significant plasma irregularities from several 10 s km down to several decameter. These are often observed near the dayside cusp and dawnside auroral zone. The decameter-scale irregularities are positively correlated with intermediate-scale (10 km) density gradients, for both negative and positive gradients encountered by the satellite. The statistical distribution of electron density over two winter months in the northern hemisphere along NorSat-1 orbits, shows significant density increases in the cusp ionosphere (75 degrees-80 degrees Magnetic LATitude) and in regions near the dawnside auroral oval. Intermediate scale density gradients and small-scale irregularities are clearly associated with these density enhancements. We postulate that these density enhancements and irregularities are due to auroral particle precipitation/plasma dynamics.

Automated summary

In this study, decameter-scale ionospheric irregularities were investigated using in-situ electron density data from the NorSat-1 satellite. These irregularities are frequently observed near the dayside cusp and dawnside auroral zone at low solar activity.