Auroral Joule heating and its consequences - From global to regional scales

Auroral Joule

Understanding the dynamics of the space environment is a perquisite for providing space weather forecasts to protect vulnerable technological systems. Satellites at low Earth orbit (LEO) experience increased orbital decay during large auroral storms. We'll study auroral heating of the upper atmosphere using state-of-the-art research facilities, inclusing EISCAT_3D located in northern Fennscandia.

Project information

Project duration

-

Funded by

Research Council of Finland

Project coordinator

University of Oulu

Contact information

Project leader

Project description

Understanding the dynamics of the space environment is a key task in the solar-terrestrial research. It's also a perquisite for providing space weather forecasts to protect vulnerable technological systems. For example, satellites at low Earth orbit (LEO) experience increased orbital decay during large auroral storms.


In this project we'll study auroral heating of the upper atmosphere, which is due to the Ohmic heating of electrical currents and the impact of energetic particles that create auroral emissions. In addition to global observation networks, we'll utilize two new research infrastructures being build in Lapland: the EISCAT_3D radar system measures the ionized plasma in the upper atmosphere, while a network of Scanning Doppler Imagers (SDI-3D) detects the motion of the neutral gas. These two new facilities, together with existing ground-based instruments and frequent overpasses by research satellites makes northern Fennoscandia the best place in the world to study aurora.

For a related project concentrating on space weather effects to LEO satellites, see the JOIN project funded by the European Space Agency.

Project results

[1]: Kärhä O., E. Tanskanen, H. Vanhamäki: Large regional variability in geomagnetic storm effects in the auroral zone. Scientific Reports, https://doi.org/10.1038/s41598-023-46352-0, 2023.

[2]: Juusola L., A. Viljanen, N. Partamies, H. Vanhamäki, M. Kellinsalmi, and S. Walker: Three principal components describe the spatiotemporal development of meso-scale ionospheric equivalent currents around substorm onsets. Ann. Geophys., https://doi.org/10.5194/angeo-41-483-2023, 2023.

[3]: Pitkänen T., G.S. Chong, M. Hamrin, A. Kullen, H. Vanhamäki, J.-S. Park, M. Nowada, A. Schillings, E. Krämer: Fast earthward convection in the magnetotail and nonzero IMF By: MMS statistics. J. Geophys. Res., https://doi.org/10.1029/2023JA031593, 2023.

[4]: Wang X., L. Cai, A. Aikio, H. Vanhamäki, I. Virtanen, Y. Zhang, B. Luo, and S. Liu: Ionospheric conductances due to electron and ion precipitations: A comparison between EISCAT and DMSP estimates. J. Geophys. Res., https://doi.org/10.1029/2023JA032354, 2024.

[5]: Oyama S., H. Vanhamäki, L. Cai, A. Shinbori, K. Hosokawa, T. Sakanoi, K. Shiokawa, A. Aikio, I. Virtanen, N. Nishitani, Y. Ogawa, Y. Miyoshi, S. Kurita: Thermospheric wind response to March 2023 storm: Largest wind ever observed with a Fabry-Perot interferometer in Tromsø, Norway since 2009. Space Weather, http://doi.org/10.1029/2023SW003728, 2024.

[6]: Laitinen J., L. Holappa and H. Vanhamäki: A Combined effect of the Earth's magnetic dipole tilt and IMF By in controlling auroral electron precipitation. J. Geophys. Res., https://doi.org/10.1029/2023JA032040, 2024.

[7]: Madelaire M., K. Laundal, S. Hatch, H. Vanhamäki, J. Reistad, A. Ohma, V. Merkin, D. Lin: Estimating the Ionospheric Induction Electric Field using Ground Magnetometers. Geophys. Res. Lett., https://doi.org/10.1029/2023GL105443, 2024.

[8]: Hatch S.M., H. Vanhamäki, K.M. Laundal, J.P. Reistad, J. Burchill, L. Lomidze, D. Knudsen, M. Madelaire, and H. Tesfaw: Does high-latitude ionospheric electrodynamics exhibit hemispheric mirror symmetry? Ann. Geophys., https://doi.org/10.5194/angeo-42-229-2024, 2024.

[9]: Cai L., A. Aikio, S. Oyama, N. Ivchenko, H. Vanhamäki, I. Virtanen, S. Buchert, M. L. Mekuriaw, and Y. Zhang: Effect of polar cap patches on the high-latitude upper thermospheric winds. J. Geophys. Res., http://dx.doi.org/10.1029/2024JA032819, 2024.

[10]: Reistad J.P., S.M. Hatch, K.M. Laundal, K. Oksavik, M. Zettergren, H. Vanhamäki, and I. Virtanen: Volumetric reconstruction of ionospheric electric currents from tri-static incoherent scatter radar measurements. J. Geophys. Res., https://doi.org/10.1029/2024JA032744, 2024.

[11]: Laitinen J., L. Holappa and H. Vanhamäki: The polarity of IMF By strongly modulates particle precipitation during high-speed streams. Geophys. Res. Lett., http://dx.doi.org/10.1029/2024GL110877, 2024.

[12]: Ellahouny N.M., A. Aikio, H. Vanhamäki, I. Virtanen, L. Cai, A. Marchaudon, P.-L. Blelly, A. Coster, J. Norberg, A. Maute, S.-I. Oyama: EISCAT observations of depleted high-latitude F-region during an HSS/SIR-driven magnetic storm. J. Geophys. Res., https://doi.org/10.1029/2024JA032910, 2024.

Research groups