Mutual Iinformation exchange in solar wind density fluctuations
- 1ISTP - CNR, Bari, Italy (lucasorriso@gmail.com)
- 2IIA - CNR, Rende, Italy (francesco.carbone42@gmail.com)
- 3OATO - INAF, Torino, Italy (daniele.telloni@inaf.it)
The fluctuations of proton density in the slow solar wind are analyzed by means of joint Empirical Mode Decomposition (EMD) and Mutual Information (MI) analysis. The analysis reveal that, within the turbulent inertial range, the EMD modes associated with nearby scales have their phases correlated, as shown by the large information exchange. This is a qunatitative measure of the information flow occurring in the turbulent cascade. On the other hand, at scales smaller than the ion gyroscale, the information flow is lost, and the mutual information is low, suggesting that in the kinetic range the nonlinear interacions are no longer sustaining a turbulent energy cascade.
How to cite: Sorriso-Valvo, L., Carbone, F., and Telloni, D.: Mutual Iinformation exchange in solar wind density fluctuations, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-11410, https://doi.org/10.5194/egusphere-egu2020-11410, 2020
This abstract will not be presented.