Abstract

This paper reports simultaneous observations of ionospheric scintillation during an auroral substorm that were made using an all-sky full-color digital single-lens reflex (DSLR) camera (ASC) and a Global Positioning System (GPS) ionospheric scintillation and total electron content monitor (GISTM) in Tromsø (69.60 N, 19.20 E), Norway. On the night of November 19, 2009, a small substorm occurred in northern Scandinavia. The ASC captured its temporal evolution from the beginning of the growth phase to the end of the recovery phase. The amplitude scintillation, as monitored by the S4 index from the GISTM, did not increase in any substorm phase. By contrast, phase scintillation, as measured by the σ φ index, occurred when discrete auroral arcs appeared on the GPS signal path. In particular, the phase scintillation was significantly enhanced for a few minutes immediately after the onset of the expansion phase. During this period, bright and discrete auroral forms covered the entire sky, which implies that structured precipitation on the scale of a few kilometers to a few tens of kilometers dominated the electron density distribution in the E region. Such inhomogeneous ionization structures probably produced significant changes in the refractive index and eventually resulted in the enhancement of the phase scintillation.

Highlights

  • It is well known that small-scale electron density irregularities are frequently formed in the terrestrial ionosphere

  • In this study, we investigated the effects of auroral substorms on ionospheric scintillations in the Global Positioning System (GPS) L1 band

  • Phase scintillation occurred when discrete auroral arcs appeared in the signal path

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Summary

Introduction

It is well known that small-scale electron density irregularities are frequently formed in the terrestrial ionosphere. Statistical maps of amplitude and phase scintillations at high latitudes were derived by Spogli et al (2009) by using data from a regional network of a GPS scintillation monitoring system in northern Europe They showed that, in the high-latitude ionosphere, phase scintillation is much more pronounced than amplitude scintillation and its occurrence frequency is clearly higher in the nighttime auroral region during the disturbance. This tendency has been confirmed by more recent statistical analyses of GPS ionospheric scintillation measurements (Li et al 2010; Alfonsi et al 2011; Tiwari et al 2012). To date, investigations of the relationship between scintillation and substorm-related auroral disturbances have been primarily statistical; the temporal evolution of the scintillation during a substorm has not yet been clarified

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