EGU25-14248, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-14248
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Identifying Kinetic Phase Space Signatures of Turbulent Dissipation
Trevor Bowen1, Tamar Ervin1, Alexandros Chasapis2, Oreste Pezzi3, Andrea Larosa3, Kris Klein4, Alfred Mallet1, and Stuart Bale1
Trevor Bowen et al.
  • 1University of California, Berkeley, Space Sciences Laboratory, United States of America (tbowen@berkeley.edu)
  • 2LASP, University of Colorado, USA
  • 3ISTP, CNR, Italy
  • 4Department of Planetary Sciences \& Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721

How to cite: Bowen, T., Ervin, T., Chasapis, A., Pezzi, O., Larosa, A., Klein, K., Mallet, A., and Bale, S.: Identifying Kinetic Phase Space Signatures of Turbulent Dissipation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14248, https://doi.org/10.5194/egusphere-egu25-14248, 2025.

This abstract has been withdrawn on 14 Apr 2025.