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Record W6991316269

GIC produced by Solar Wind transients

2018· dissertation· en· W6991316269 on OpenAlexaboutno aff

Bibliographic record

VenueOtago University Research Archive (University of Otago) · 2018
Typedissertation
Languageen
FieldPhysics and Astronomy
TopicIonosphere and magnetosphere dynamics
Canadian institutionsnot available
Fundersnot available
KeywordsEarth's magnetic fieldGeomagnetically induced currentSolar windGeomagnetic stormSpace weatherIonospheric dynamo regionInterplanetary magnetic fieldInterplanetary spaceflightStorm
DOInot available

Abstract

fetched live from OpenAlex

Geomagnetic storms are potentially hazardous to the activities and technological infrastructure of modern civilisation. The storms cause large and comparatively rapid changes in the geomagnetic field at the Earth’s surface, leading to Geomagnetically Induced Currents (GICs) in electrical power transmission networks. GICs can disrupt and potentially damage equipment in power transmission networks; examples of such damage have occurred in Canada, South Africa, Sweden, USA, and also New Zealand. Large geomagnetic storms are triggered by reconfiguration of the geomagnetic field due to forcing from space, and in particular the plasma which flows from the Sun termed the solar wind. \n \nIn this thesis we examine the link between processes in space, geomagnetic field variations, and GIC observations. We utilise the large dataset of GIC measurements which we have created from the long-lived and spatially extensive set of Direct Current (DC) observations undertaken by Transpower New Zealand. The goal of our research is to better understand the link between processes in space and GIC in New Zealand. This is a step towards providing warning of events likely to cause large and potentially damaging GICs at mid-latitude locations. \n \nThis research particularly focuses on solar wind magnetosphere-ionosphere coupling. In this topic it is critical to understand how the solar wind and the frozen-in Interplanetary Magnetic Field (IMF) couple to activity at the Earth’s surface. We compare the timing of spikes in ground-based magnetic field observations with OMNIweb predicted arrival time at Earth of solar wind shock events, but find these times rarely agree. Instead, we use a case-by-case test to link the SOHO reported shock events to Earth arrival times. This produces an empirical relationship between solar wind pressure measurements and the associated horizontal magnetic field rate of change (H') measurements, which is found to strongly depend on IMF orientation and magnetic latitude. \n \nThe arrival of the solar wind shocks drive H' spikes in New Zealand, as reported by the magnetic field observatory at Eyrewell. The shock-produced H' spikes lead to GIC enhancements detected at transformers throughout the South Island of New Zealand. The magnitude of these GIC events is found to strongly depend on local time; larger GIC magnitudes are found during local midday compared to local midnight events, for the same level of H'. Sunward facing locations typically experience 50% larger currents than nightside locations. Various possible causes of this are investigated, with mixed results. It is determined that public/non-public holidays, IMF orientation, and the directional change in the declination angle strongly affect the local time dependence.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.003
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.024
Threshold uncertainty score0.048

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.003
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0020.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.011
GPT teacher head0.236
Teacher spread0.225 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations0
Published2018
Admission routes1
Has abstractyes

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