Filling the gaps
Filling the gaps
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填补空白
DOI:
10.1093/astrogeo/atac080
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发表时间:
2022
影响因子:
0.8
通讯作者:
Beggan C
中科院分区:
文献类型:
--
作者:
Beggan C
UK. But the associated ground magnetic field variation also has potentially hazardous effects on power, rail, and pipeline systems (Kelly et al. 2017). As the auroral oval moves southwards over the UK, the magnetic field on the ground changes rapidly. But the equatorward boundary of that oval, rather than having a neat straight edge, has fluctuations, wiggles and bends on the order of a few hundred kilometres in wavelength. These can cause stronger-than-expected enhancements of the field along the leading edge, particularly at UK latitudes (Freeman et al. 2019). The UK has three long-established scientific geomagnetic observatories, in Lerwick (Shetland), Eskdalemuir (Dumfries and Galloway) and Hartland (Devon). These form an approximately north-south line but have little variation in longitude. Thus, we are unable to sense the magnetic field off this line and are missing vital information about local variations in the field from the wavy auroral oval edge. As part of the NERC-funded Space Weather Instrumentation, Measurement, Modelling and Risk (SWIMMR) Activities in Ground Effects (SAGE) project, the British Geological Survey geomagnetism team have installed three new variometer stations, in Northern Ireland, Leicestershire and Sussex, in order to expand the coverage in the east-west directions. These systems consist of a three-axis vector fluxgate magnetometer, a digitizer/logger computer and a 4G modem to transmit near-real-time data. The systems use batteries and a solar panel for independent power supply. The electronics and batteries are housed in a waterproof container within a repurposed garden shed. The magnetometer is buried in a barrel around 1 m below ground level, to reduce the effect of daily temperature changes, and around 6 m from the electronics and solar panels to reduce electromagnetic noise. The sensors were calibrated at the Eskdalemuir observatory to determine scaling and offset factors by comparison to simultaneous measurements from the science instruments. However, as the temperature is not kept constant and the calibration factors are not checked weekly (as they are at observatories), the magnetic field values from variometers are considered to be relative rather than absolute. They capture the short-term change of the magnetic field well on the order of hours–useful for space weather applications–but the measurements cannot be used for determining the angle of declination or long-term changes of the Earth’s core field. Two systems were installed in fields in rural areas, at Florence Court (FLO) National Trust, Fermanagh and near Market Harborough, Leicestershire (LEI). The third is located at the BGS Space Geodesy Facility in Herstmonceux (HTX) and is connected to mains power and communications. The three new variometers fill in the gaps between the BGS and other Intermagnet observatories, reducing the inter-site distance to less than 400 km thus improving the overall coverage. The six UK magnetic stations will allow very detailed real-time maps of the magnetic field to be created and, in combination with the ground resistivity, we can compute the induced geoelectric field every five minutes. Large geoelectric fields can flow through earthed conductors such as high-voltage transformers creating geomagnetically induced currents (Huebert et al. 2020). Such currents push transformers out of their optimal operating regime, causing temperature fluctuations and harmonic distortion on the 50 Hz operation frequency. If these become large enough the transformer safety systems engage to stop further damage (Boteler 2019). Real-time monitoring will help identify when conditions are hazardous. The …