| Title | Assessment of GIC risk due to geomagnetic sudden commencements and identification of the current systems responsible
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| Author | Fiori, R A D; Boteler, D H; Gilliles, D M |
| Source | Space Weather vol. 12, 2014 p. 1-16, https://doi.org/10.1002/2013SW000967 (Open Access) |
| Year | 2014 |
| Alt Series | Earth Sciences Sector, Contribution Series 20130219 |
| Publisher | American Geophysical Union |
| Document | serial |
| Lang. | English |
| Media | paper; on-line; digital |
| File format | pdf; html |
| Subjects | extraterrestrial geology; geophysics; Health and Safety; geomagnetism; geomagnetic fields; geomagnetic variations; magnetic disturbances; magnetic field; magnetic storms; solar variations |
| Illustrations | plots; histograms |
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| Program | Northern Canada Geohazards Project, Public Safety Geoscience |
| Released | 2014 01 29 |
| Abstract | During periods of enhanced geomagnetic activity, geomagnetically induced currents (GIC) flow in power systems potentially causing damage to system components or failure of the system. The largest GIC
are produced when there are large rates of change of the geomagnetic field (dB/dt). It is well established that the main phase of a geomagnetic storm, particularly the magnetic substorms occurring during that period, is a cause of large GIC and hence
a risk factor for power systems. However, some power system disturbances have been associated with the occurrence of a storm sudden commencement (SSC) prior to the main phase. We investigate the magnetic signature observed on the ground and the
associated solar wind and interplanetary magnetic field (IMF) conditions for both SSC and sudden impulse (SI) events, which are grouped together as sudden commencements (SC). SCs are primarily attributed to a sudden enhancement of the magnetopause
current. For some events, we show that there is a high-latitude enhancement (HLE) of the SC amplitude and corresponding dB/dt. The limited spatial extent suggests an ionospheric current source. Examination of the polarity of the change in the
X-component magnetic field shows that the HLE is due to a sudden increase of the ionospheric convection electrojets. The occurrence of the HLE is more prevalent for SSC-type SCs, SCs caused by coronal mass ejections as opposed to corotating
interaction regions, and SCs associated with a large solar wind speed (vsw) prior to the SC or a large Dvsw at the time of the SC. |
| Summary | (Plain Language Summary, not published)
Space weather refers to the dynamic conditions on the Sun and in the space environment, in particular, in the near-Earth environment, that can affect
critical infrastructure. NRCan operates the Canadian Space Weather Forecast Centre and conducts research into space weather effects on power systems, pipelines, radio communications and GNSS positioning to help Canadian industry understand and
mitigate the effects of space weather. During periods of enhanced geomagnetic activity, geomagnetically induced currents (GIC) flow in power systems potentially causing damage to system components or failure of the system. This paper examines
factors leading to an increased risk of GIC in high-latitude power systems in association with geomagnetic sudden commencements. |
| GEOSCAN ID | 293041 |
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