Magnetic Effects of Plasma Pressure Gradients in the Upper F Region

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Abstract

The Swarm satellites fly at altitudes that at polar latitudes are generally assumed to only contain currents that are aligned with the local magnetic field. Therefore, disturbances along the main field direction are mainly signatures of auroral electrojet currents, with a relatively smooth structure due to the distance from the currents. Here we show that superimposed on this smooth signal is an irregular pattern of small perturbations, which are anticorrelated with the plasma density measured by the Langmuir probe. We show that the perturbations can be remarkably well reproduced by assuming they represent a j × B force, which balances the plasma pressure gradient implied by the density variations. The associated diamagnetic current, previously reported to be most important near the equator, appears to be a ubiquitous phenomenon also at polar latitudes. A spectral analysis indicates that this effect dominates magnetic field intensity variations at small-scale sizes of a few tens of kilometers.

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Laundal, K. M., Hatch, S. M., & Moretto, T. (2019). Magnetic Effects of Plasma Pressure Gradients in the Upper F Region. Geophysical Research Letters, 46(5), 2355–2363. https://doi.org/10.1029/2019GL081980

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