Recreating the Horizontal Magnetic Field at Colaba during the Carrington Event with Geospace Simulations
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Date
2021-03-14
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Citation of Original Publication
Blake, Sá. P., Pulkkinen, A., Schuck, P. W., Glocer, A., Oliveira, D. M., Welling, D., et al. (2021). Recreating the Horizontal Magnetic Field at Colaba during the Carrington Event with Geospace Simulations. Space Weather, 19, e2020SW002585. https://doi.org/10.1029/2020SW002585
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This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law
Public Domain Mark 1.0
This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law
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Abstract
An intriguing aspect of the famous 2 September 1859 geomagnetic disturbance (or ‘Carrington’ event) is the horizontal magnetic (B H ) dataset measured in Colaba, India (magnetic latitude approximately 20 degrees N). The field exhibits a sharp decrease of over 1600 nT and a quick recovery of about 1300 nT, all within a few hours during the daytime. The mechanism behind this has previously been attributed to magnetospheric processes, ionospheric processes or a combination of both. In this paper, we outline our efforts to replicate this low‐latitude magnetic field using the Space Weather Modelling Framework (SWMF). By simulating an extremely high pressure solar wind scenario, we can emulate the low‐latitude surface magnetic signal at Colaba. In our simulation, magnetospheric currents adjacent to the near‐Earth magnetopause and strong Region 1 field‐aligned currents (FACs) are the main contributors to the large Colaba B H . The rapid recovery of B H in our simulated scenario is due to the retreat of these magnetospheric currents as the magnetosphere expands, as opposed to ring current dynamics. In addition, we find that the scenario that best emulated the surface magnetic field observations during the Carrington event had a minimum calculated Dst value between ‐431 and ‐1191 nT, indicating that Dst may not be a suitable estimate of storm intensity for this kind of event.