Tanja Petersen
GNS Science
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Featured researches published by Tanja Petersen.
Space Weather-the International Journal of Research and Applications | 2017
Daniel H. Mac Manus; Craig J. Rodger; M. Dalzell; Alan Thomson; Mark A. Clilverd; Tanja Petersen; Moritz M. Wolf; Neil R. Thomson; Tim Divett
Transpower New Zealand Limited has measured DC currents in transformer neutrals in the New Zealand electrical network at multiple South Island locations. Near-continuous archived DC current data exist since 2001, starting with 12 different substations and expanding from 2009 to include 17 substations. From 2001 to 2015 up to 58 individual transformers were simultaneously monitored. Primarily, the measurements were intended to monitor the impact of the high-voltage DC system linking the North and South Islands when it is operating in “Earth return” mode. However, after correcting for Earth return operation, as described here, the New Zealand measurements provide an unusually long and spatially detailed set of geomagnetically induced current (GIC) measurements. We examine the peak GIC magnitudes observed from these observations during two large geomagnetic storms on 6 November 2001 and 2 October 2013. Currents of ~30–50 A are observed, depending on the measurement location. There are large spatial variations in the GIC observations over comparatively small distances, which likely depend upon network layout and ground conductivity. We then go on to examine the GIC in transformers throughout the South Island during more than 151 h of geomagnetic storm conditions. We compare the GIC to the various magnitude and rate of change components of the magnetic field. Our results show that there is a strong correlation between the magnitude of the GIC and the rate of change of the horizontal magnetic field (H′). This correlation is particularly clear for transformers that show large GIC current during magnetic storms.
Space Weather-the International Journal of Research and Applications | 2017
Craig J. Rodger; Daniel H. Mac Manus; M. Dalzell; Alan Thomson; Ellen Clarke; Tanja Petersen; Mark A. Clilverd; Tim Divett
Geomagnetically induced current (GIC) observations made in New Zealand over 14xa0years show induction effects associated with a rapidly varying horizontal magnetic field (dBH/dt) during geomagnetic storms. This study analyzes the GIC observations in order to estimate the impact of extreme storms as a hazard to the power system in New Zealand. Analysis is undertaken of GIC in transformer number six in Islington, Christchurch (ISL M6), which had the highest observed currents during the 6 November 2001 storm. Using previously published values of 3,000xa0nT/min as a representation of an extreme storm with 100xa0year return period, induced currents of ~455xa0A were estimated for Islington (with the 95% confidence interval range being ~155–605xa0A). For 200xa0year return periods using 5,000xa0nT/min, current estimates reach ~755xa0A (confidence interval range 155–910xa0A). GIC measurements from the much shorter data set collected at transformer number 4 in Halfway Bush, Dunedin, (HWB T4), found induced currents to be consistently a factor of 3 higher than at Islington, suggesting equivalent extreme storm effects of ~460–1,815xa0A (100xa0year return) and ~460–2,720xa0A (200xa0year return). An estimate was undertaken of likely failure levels for single-phase transformers, such as HWB T4 when it failed during the 6 November 2001 geomagnetic storm, identifying that induced currents of ~100xa0A can put such transformer types at risk of damage. Detailed modeling of the New Zealand power system is therefore required to put this regional analysis into a global context.
Journal of Geophysical Research | 2015
Yuki Obana; C. L. Waters; M. D. Sciffer; F. W. Menk; Robert L. Lysak; K. Shiokawa; Anthony W. Hurst; Tanja Petersen
Quarter-wave modes are standing shear Alfven waves supported along geomagnetic field lines in space. They are predicted to be generated when the ionosphere has very different conductance between the north compared with the south ionosphere. Our previous observation reported that the resonant frequency is sometimes very low around the dawn terminator and suggested these were due to quarter-wave modes. In this paper, we examine the resonance structure that provides further evidence of the presence of quarter-wave modes. Data from three magnetometers in New Zealand were analyzed. Four events are discussed which show extraordinarily low eigenfrequencies, wide resonance widths, and strong damping when the ionosphere above New Zealand was in darkness while the conjugate northern hemisphere ionosphere was sunlit. Later in the morning, the eigenfrequencies and resonance widths changed to normal daytime values. The wide resonance width and the strong damping of the quarter-wave modes arise from strong energy dissipation in the dark side ionosphere. One event exhibited field line resonance structure continuously through a transition from very low frequency to the normal daytime values. The frequency change began when the dawn terminator passed over New Zealand and finished 1u2009h later when the ratio of the interhemispheric ionospheric conductances decreased and reached ~5. These observations are strong evidence of the presence of quarter-wave modes and mode conversion from quarter- to half-wave resonances. These experimental results were compared with the ULF wave fields obtained from a 2.5-dimensional simulation model.
Space Weather-the International Journal of Research and Applications | 2017
M. Ingham; Craig J. Rodger; Tim Divett; M. Dalzell; Tanja Petersen
Transfer functions are calculated for periods between 2 and 1000 minutes between geomagnetically induced currents (GIC) measured at three transformers in the South Island of New Zealand and variations in the horizontal components of the geomagnetic field measured at the Eyrewell Observatory near Christchurch. Using an inverse Fourier Transform, the transfer functions allow the GIC expected in these transformers to be estimated for any variation of the inducing magnetic field. Comparison of the predicted GIC with measured GIC for individual geomagnetic storms shows remarkable agreement, although the lack of high frequency measurements of GIC and the need for interpolation of the measurements leads to a degree of underestimation of the peak GIC magnitude. An approximate correction for this is suggested. Calculation of the GIC for a magnetic storm in November 2001 which led to the failure of a transformer in Dunedin suggests that peak GIC were as large as about 80 A. Use of spectral scaling to estimate the likely GIC associated with a geomagnetic storm of the magnitude of the 1859 Carrington Event indicate that GIC of at least 10 times this magnitude may occur at some locations. Although the impact of changes to the transmission network on calculated transfer functions remains to be explored, it is suggested that the use of this technique may provide a useful check on estimates of GIC produced by other methods such as thin-sheet modelling. Plain Language Summary Rapid changes in Earth’s magnetic field, such as occur during a magnetic storm, induce electric currents in the ground. These currents, known as geomagnetically induced currents (GIC), are able to enter a power transmission network through the ground connection of a substation transformer. Not only can such currents cause damage to transformers, but in extreme situations they may cause failure of the entire power transmission network. We relate measurements of GIC in the New Zealand power transmission network to variations in the magnetic field at a local magnetic observatory. This allows us to construct mathematical relationships between GIC and magnetic field variations which enable us to predict the magnitude of GIC that might occur in the event of a magnetic storm such as the so-called Carrington Event of 1859 – the largest such storm ever recorded. It is found that GIC of almost 1000 A might occur.
Seismological Research Letters | 2011
Tanja Petersen; Ken Gledhill; Mark Chadwick; Nora H. Gale; John Ristau
Archive | 2009
Tanja Petersen; John Ristau; John Beavan; Paul Denys; M. Denham; Bryan Field; Caroline François-Holden; Neville Palmer; Martin Reyners
Space Weather-the International Journal of Research and Applications | 2018
Mark A. Clilverd; Craig J. Rodger; James B. Brundell; M. Dalzell; Ian Martin; Daniel H. Mac Manus; Neil R. Thomson; Tanja Petersen; Yuki Obana
Space Weather-the International Journal of Research and Applications | 2017
M. Ingham; Craig J. Rodger; Tim Divett; M. Dalzell; Tanja Petersen
Space Weather-the International Journal of Research and Applications | 2017
Daniel H. Mac Manus; Craig J. Rodger; M. Dalzell; Alan Thomson; Mark A. Clilverd; Tanja Petersen; Moritz M. Wolf; Neil R. Thomson; Tim Divett
Space Weather-the International Journal of Research and Applications | 2017
Craig J. Rodger; Daniel H. Mac Manus; M. Dalzell; Alan Thomson; Ellen Clarke; Tanja Petersen; Mark A. Clilverd; Tim Divett