Observing Earth’s magnetic environment with the GRACE-FO mission

Earth, Planets and Space

Th. Usbeck¹  C. Xiong²  Y. Yamazaki²  M. Rother²  J. Rauberg²  I. Michaelis²  K. Styp-Rekowski³  C. Stolle⁴ 

[1] Airbus Defence and Space GmbH, Claude-Dornier-Straße, 88090, Immenstaad am Bodensee, Germany;Helmholtz Centre Potsdam, GFZ German Research Centre for Geosciences, Telegrafenberg, 14473, Potsdam, Germany;Helmholtz Centre Potsdam, GFZ German Research Centre for Geosciences, Telegrafenberg, 14473, Potsdam, Germany;Electrical Engineering and Computer Science, Technical University of Berlin, Ernst-Reuter-Platz 7, 10587, Berlin, Germany;Helmholtz Centre Potsdam, GFZ German Research Centre for Geosciences, Telegrafenberg, 14473, Potsdam, Germany;Faculty of Science, University of Potsdam, Karl-Liebknecht-Str. 24-25, 14476, Potsdam, Germany;

关键词: Earth’s magnetic field;    Geomagnetism;    Ionospheric currents;    Magnetospheric ring current;    Satellite-based magnetometers;    Platform magnetometers;    GRACE-FO;   

DOI  :  10.1186/s40623-021-01364-w

来源: Springer

【 摘 要 】

The Gravity Recovery and Climate Experiment Follow-On (GRACE-FO) mission carries magnetometers that are dedicated to enhance the satellite’s navigation. After appropriate calibration and characterisation of artificial magnetic disturbances, these observations are valuable assets to characterise the natural variability of Earth’s magnetic field. We describe the data pre-processing, the calibration, and characterisation strategy against a high-precision magnetic field model applied to the GRACE-FO magnetic data. During times of geomagnetic quiet conditions, the mean residual to the magnetic model is around 1 nT with standard deviations below 10 nT. The mean difference to data of ESA’s Swarm mission, which is dedicated to monitor the Earth’s magnetic field, is mainly within ± 10 nT during conjunctions. The performance of GRACE-FO magnetic data is further discussed on selected scientific examples. During a magnetic storm event in August 2018, GRACE-FO reveals the local time dependence of the magnetospheric ring current signature, which is in good agreement with results from a network of ground magnetic observations. Also, derived field-aligned currents (FACs) are applied to monitor auroral FACs that compare well in amplitude and statistical behaviour for local time, hemisphere, and solar wind conditions to approved earlier findings from other missions including Swarm. On a case event, it is demonstrated that the dual-satellite constellation of GRACE-FO is most suitable to derive the persistence of auroral FACs with scale lengths of 180 km or longer. Due to a relatively larger noise level compared to dedicated magnetic missions, GRACE-FO is especially suitable for high-amplitude event studies. However, GRACE-FO is also sensitive to ionospheric signatures even below the noise level within statistical approaches. The combination with data of dedicated magnetic field missions and other missions carrying non-dedicated magnetometers greatly enhances related scientific perspectives.

【 授权许可】

CC BY