Simulations of the magnetosphere - ionosphere coupling to estimate the Physical Properties of Magnetospheric Generators from Observations of Quiet Discrete Auroral Arcs

We designed a method to estimate the properties of the auroral generator from low-altitude observations of aurora.

The method is based on a magnetosphere – ionosphere quasi-stationary coupling model, a parametric description of a magnetospheric interface generator and a minimization procedure that finds the generator model whose auroral effects best fit in-situ observations.

The database includes the results of the magnetosphere-ionosphere coupling model used to test the methodology. The method can be generalized to other types of generators and observables.

Data and Resources

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Cite this as (APA format)

Echim, M., Lamy, H., De Keyser, J., & Maggiolo, R. (2019). Simulations of the magnetosphere - ionosphere coupling to estimate the Physical Properties of Magnetospheric Generators from Observations of Quiet Discrete Auroral Arcs (Version 1) [Data set]. Royal Belgian Institute for Space Aeronomy. https://doi.org/10.18758/71021051
Retrieved: 04:17 08 Dec 2024 (UTC)
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Author(s)
Principal

Echim, Mariusorcid, Royal Belgian Institute for Space Aeronomy
Other(s)

Lamy, Hervé, Royal Belgian Institute for Space Aeronomy; De Keyser, Johanorcid, Royal Belgian Institute for Space Aeronomy; Maggiolo, Romain, Royal Belgian Institute for Space Aeronomy;
Contact data-contact of Royal Belgian Institute for Space Aeronomy

Technical info
Is referenced by

https://doi.org/10.1029/2019JA026969

Temporal features

Additional info
Funding details

  • Belgian BRAIN-BE project

  • MOMA 444 BR/175/A2/MOMA

  • Belgian Solar Terrestrial Center of Excellence (STCE)
Repository homepage

https://data.aeronomie.be/dataset/
Last Updated

September 10, 2024
Created

April 25, 2019

Spatial features

No spatial information