Abstract

Abstract. An extensive magnetometer network in Alaska and Canada (consisting of 6 auroral and sub-auroral stations) and at Macquarie Is. (Australia) was used to study magnetoconjugate phenomena in 2003, using the H-component magnetograms. Altogether 193 magnetically disturbed days (with ΣKp≥10) were used in the analysis. The maximum negative swing in the H-component (ΔH) was assigned for each day from the auroral conjugate station's data. Two types of magnetoconjugate data were found: Type-1 when the daily (00:00–24:00 h UT) substorm activity was faithfully reproduced in the H-component variations in the northern and southern auroral zones, and Type-2 when a major peak in disturbance was largely missing in one conjugate location. A distinct maximum in the occurrence of the Type-1 events was in the southern summer (northern winter), reaching almost 70 per cent of cases. A minimum in this type of events was in the southern autumn and winter (around 40%). The correlation between ΣKp and ΔH for auroral stations faithfully reproduced the percentage occurrence of the Type-1 events for various seasons, with the maximum correlation coefficient r≈0.8 in summer. The time conjugacy of the events (i.e. the events occurring with a small time displacement in the southern and northern auroral zones) was highest for the auroral stations located close to the theoretical conjugate point location at L-value ≈ 5 (i.e. College and Macquarie Is.). The substorm onsets started earlier at the stations positioned east of the conjugate point of Macquarie Is. in spring and winter, indicating a westward drift of auroral disturbance with velocities of 1.4–1.6 km/s. The magnitude of average ΔH increased rapidly past the invariant latitude of Macquarie Is. towards the latitude of its nearest northern conjugate station College , particularly in spring. The average level of disturbance was consistently lower by about 30% at Macquarie Is. than at College. Since Macquarie Is. is the only available auroral station in the southern auroral zone the maximum southern auroral activity level (maximum iso-aurorae) should be inferred from magnetic data obtained at a northern conjugate station positioned at a slightly higher L-value, such as College (L-value = 5.73). It is concluded from the above considerations that the maximum iso-aurorae is located at a shell with L-value ≥ 5.73 in both hemispheres.

Highlights

  • Simultaneous recordings of similar auroral features, at the northern and southern auroral ovals, are associated with charged particles bouncing between mirroring points along a field line

  • The yearly analysis of the H-component magnetic data from seven auroral stations, positioned in the southern and northern magnetoconjugate areas yielded the following results: (a) There is a high degree of conjugacy, on the diurnal basis (00:00–24:00 UT), in the onset of geomagnetic substorms, at the stations close to the theoretical conjugate point locations

  • Gakona and Macquarie Is., were classified as Type-1 as opposed to Type-2 which showed imperfect conjugacy, with at least one peak in the negative swing of the H-component magnetograms missing in one conjugate location (i.e. C or M)

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Summary

Introduction

Simultaneous recordings of similar auroral features, at the northern and southern auroral ovals, are associated with charged particles bouncing between mirroring points along a field line. (Buckles Bay) – Kotzebue, positioned at almost identical invariant latitudes and magnetic longitudes (Macquarie Is.: 64.05◦ S, 243.64◦ E; Kotzebue: 63.98◦ N, 242.52◦) He reported that increases and decreases in the brightness of corresponding auroral forms occurring simultaneously at both stations, to be within 1 min and were assessed to be of the same intensity. Hajkowicz (1970) used yearly cosmic noise absorption data from vertical incidence riometers situated in Alaska (Kotzebue and College) and at Macquarie Is. He reported that increases and decreases in the brightness of corresponding auroral forms occurring simultaneously at both stations, to be within 1 min and were assessed to be of the same intensity. Hajkowicz (1984) analysed 10 years (1971– 1981) of magnetic K-index data for College-Macquarie Is. The longitudinal shift between College and Macquarie Is. conjugate, combined with the absorption occurrence time lag, indicated an auroral disturbances drift of about 2 km/s both towards east and west. Recent establishment of the Alaskan (HAARP) magnetometer chain made it possible to extrapolate the southern latitudinal properties of the conjugate substorm onsets

Method and results
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Conclusions and discussion
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