EGU22-4497
https://doi.org/10.5194/egusphere-egu22-4497
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Estimating radial diffusion using a hybrid-Vlasov simulation

Harriet George1, Adnane Osmane1, Emilia Kilpua1, Solene Lesjone2, Milla Kalliokoski1, Sanni Hoilijoki1, and the Vlasiator team*
Harriet George et al.
  • 1Department of Physics, University of Helsinki, Helsinki, Finland
  • 2Space Sciences Laboratory, University of California, Berkeley, CA, USA
  • *A full list of authors appears at the end of the abstract
Radial diffusion coefficients quantify non-adiabatic transport of energetic particles by electromagnetic field fluctuations in planetary radiation belts. Theoretically, radial diffusion occurs for an ensemble of particles that experience irreversible violation of their third adiabatic invariant, which is equivalent to a change in their Roederer L* parameter. Thus, the Roederer L* coordinate is the fundamental quantity from which radial diffusion coefficients can be computed. We present a methodology to calculate the Lagrangian derivative of L* from global magnetospheric simulations, and test it with an application to Vlasiator, a hybrid-Vlasov model of near-Earth space. We use a Hamiltonian formalism for particles confined to closed drift shells with conserved first and second adiabatic invariants to compute changes in the guiding center drift paths from background electric and magnetic field fluctuations. Performing this calculation for different energies allows the rate of change of L* to be evaluated for different populations travelling along the same guiding center drift path without the need to inject and trace test particles. We investigate the feasibility of this methodology by computing the time evolution of L* for an equatorial ultrarelativistic electron population travelling along four guiding center drift paths in the outer radiation belt of a five minute portion of a Vlasiator simulation. Due to the short time scale and geometry of the test run, low amplitude Pc3 fluctuations are the primary driver of radial diffusion, which results in preliminary estimates for the radial diffusion coefficients that are two to six orders of magnitude below those corresponding to more active magnetospheric conditions with Pc5 fluctuations as the primary driver. However, our results show that an alternative methodology to compute detailed radial diffusion transport is now available and could form the basis for comparison studies between numerical and observational measurements of radial transport in the Earth’s radiation belts.
Vlasiator team:

Lucile Turc (1), Maxime Grandin (1), Urs Ganse (1), Markku Alho (1), Markus Battarbee (1), Maarja Bussov (1), Maxime Dubart (1), Andreas Johlander (3,1), Talgat Manglayev (1), Kostantinos Papadakis (1), Yann Pfau-Kempf (1), Jonas Suni (1), Vertti Tarvus (1), Hongyang Zhou (1), and Minna Palmroth (1,4)

How to cite: George, H., Osmane, A., Kilpua, E., Lesjone, S., Kalliokoski, M., and Hoilijoki, S. and the Vlasiator team: Estimating radial diffusion using a hybrid-Vlasov simulation, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-4497, https://doi.org/10.5194/egusphere-egu22-4497, 2022.

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