Abstract

We analyse geomagnetic recordings at four subauroral and midlatitude Russian observatories in 1850–1862. The data consist of spot readings made once in hour of the north and east components of the magnetic field. We use the hourly change of the horizontal field vector as the measure of activity. We compare these values to data from modern observatories at corresponding magnetic latitudes (Nurmijarvi, Finland, magnetic latitude ~57 N; Tartu, Estonia, ~54.5 N; Dourbes, Belgium, ~46 N) by reducing their data to the 1-h format. The largest variations at the Russian observatories occurred during the Carrington storm in September 1859 and they reached about 1000 nT/h, which was the instrumental off-scale limit. When the time stamp for the spot readings happens to be optimal, the top variation in the Nurmijarvi data is about 3700 nT/h (July 1982), and at Tartu the maximum is about 1600 nT/h (November 2004). At a midlatitude site Nertchinsk in Russia (magnetic latitude ~45 N), the variation during the Carrington storm was at the off-scale limit, and exceeded the value observed at Dourbes during the Halloween storm in October 2003. At Nertchinsk, the Carrington event was at least four times larger than any other storm in 1850–1862. Despite the limitations of the old recordings and in using only hourly spot readings, the Carrington storm was definitely a very large event at midlatitudes. At higher latitudes, it remains somewhat unclear whether it exceeds the largest modern storms, especially the one in July 1982.

Highlights

  • The Carrington storm in the end of August and beginning of September 1859 belongs to the largest space weather events in the known record (e.g., Tsurutani et al 2003; Cliver & Svalgaard 2004; Clauer & Siscoe 2006; Cliver & Dietrich 2013)

  • The largest variations at the Russian observatories occurred during the Carrington storm in September 1859 and they reached about 1000 nT/h, which was the instrumental off-scale limit

  • At a midlatitude site Nertchinsk in Russia, the variation during the Carrington storm was at the off-scale limit, and exceeded the value observed at Dourbes during the Halloween storm in October 2003

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Summary

Introduction

The Carrington storm in the end of August and beginning of September 1859 belongs to the largest space weather events in the known record (e.g., Tsurutani et al 2003; Cliver & Svalgaard 2004; Clauer & Siscoe 2006; Cliver & Dietrich 2013). If a similar storm happened it could cause wide damage to the modern technology in space and on the ground. It is important to try to quantify the magnitude of the Carrington event based on fairly sparse historic data. At those times, there were only a few observatories around the world that were capable to measure geomagnetic variations. Its determination from observations at a single site is somewhat controversial (e.g., Akasofu & Kamide 2005)

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