Articles | Volume 43, issue 2
https://doi.org/10.5194/angeo-43-469-2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/angeo-43-469-2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Global evolution of flux transfer events along the magnetopause from the dayside to the far tail
Department of Physics, University of Helsinki, Helsinki, Finland
now at: CSC – IT Center for Science Ltd., Espoo, Finland
Konstantinos Papadakis
Department of Physics, University of Helsinki, Helsinki, Finland
Markku Alho
Department of Physics, University of Helsinki, Helsinki, Finland
Markus Battarbee
Department of Physics, University of Helsinki, Helsinki, Finland
Giulia Cozzani
Department of Physics, University of Helsinki, Helsinki, Finland
LPC2E, CNRS/CNES/University of Orléans, Orléans, France
Lauri Pänkäläinen
Department of Physics, University of Helsinki, Helsinki, Finland
Urs Ganse
Department of Physics, University of Helsinki, Helsinki, Finland
Fasil Kebede
Department of Physics, University of Helsinki, Helsinki, Finland
Department of Physics and Technology, University of Bergen, Bergen, Norway
Jonas Suni
Department of Physics, University of Helsinki, Helsinki, Finland
Konstantinos Horaites
Department of Physics, University of Helsinki, Helsinki, Finland
Cooperative Institute for Research in Environmental Sciences, University of Colorado, Boulder, CO, USA
National Oceanic and Atmospheric Administration National Centers for Environmental Information, Boulder, CO, USA
Maxime Grandin
Department of Physics, University of Helsinki, Helsinki, Finland
Finnish Meteorological Institute, Helsinki, Finland
Minna Palmroth
Department of Physics, University of Helsinki, Helsinki, Finland
Finnish Meteorological Institute, Helsinki, Finland
Data sets
Vlasiator 6D 'FHA' dataset Dataset Jonas Suni & Konstantinos Horaites http://urn.fi/urn:nbn:fi:att:3ce0f038-2c69-4c7c-8f67-7a71e9e57b56
Model code and software
Vlasiator Pfau-Kempf, Y., Ganse, U., Battarbee, M., Kotipalo, L., Koskela, T., von Alfthan, S., Honkonen, I., Alho, M., Sandroos, A., Papadakis, K., Zhou, H., Palmu, M., Grandin, M., Suni, J., Tarvus, V., Pokhotelov, D., Hokkanen, J., Rossi, T., Lankinen, J., Haaja, V., Mendez Pratt, A., Lalagüe, A., & Horaites, K. https://doi.org/10.5281/zenodo.3640593
Short summary
Flux ropes are peculiar structures of twisted magnetic field occurring in many regions of space, near Earth and other planets, at the Sun, and in astrophysical objects. We developed a new way of detecting flux ropes in large supercomputer simulations of near-Earth space, and we use it to follow the evolution of flux ropes for long distances past the Earth in the flow direction. This will be useful in future studies as these flux ropes are involved in the transport of matter and energy in space.
Flux ropes are peculiar structures of twisted magnetic field occurring in many regions of space,...