摘要：This study uses supervised and unsupervised machine learning (ML) methods to correct unwanted offsets observed in the NOAA GOES-16 magnetometer data. All GOES satellites have an inboard and outboard magnetometer sensor mounted along a long boom. Post-launch testing of the GOES-16 magnetometers found that the inboard sensor suffers significant thermally induced magnetic contamination and currently only the outboard sensor is used in NOAA operations. The contamination varies both diurnally and seasonally making it very difficult to correct using basic statistical methods. For simplicity in explaining the offsets we are trying to correct, and methods used, we focus on correcting only one of the inboard vector components, the E-component (Earthward). We start by applying the unsupervised k-Shape method to the magnetic field vector E-component outboard minus inboard sensor time series, ΔE, resulting in four clusters that are closely related to the time of year and the solar β angle, which is a measure of the amount of time that a satellite is in direct sunlight. We then utilized LSTM networks as regressors to correct the offsets observed in GOES-16 inboard sensor E-component data. We trained our LSTMs using GOES-17 magnetometer data, which we show to exhibit much less variability compared with the GOES-16 data. The correction results reduced the offsets in the clusters from between 3–5 nT and 0–2 nT standard deviations. The combining of unsupervised and supervised ML methods is a powerful technique that can be applied to space-based instruments that produce time series data.
