Spatio-Temporal Scales of Plasma Density in Topside Ionosphere
- 1Institute of Atmospheric Physics CAS, Department of Ionosphere and Aeronomy, Prague, Czechia (urbar@ufa.cas.cz)
- 2Istituto Nazionale di Geofisica e Vulcanologia, Italy
- 3University of Oslo, Norway
- 4University of Birmingham, United Kingdom
- 5University of L’Aquila, Italy
- 6SpacEarth Technology, Italy
Non-linear couplings of the Earth’s ionosphere with the geospace environment occur in a largely varying range of spatial and temporal scales. As some radio remote sensing techniques like GNSS measurements suffer from artificial radio frequency interference (RFI) at the smallest scales representing ionospheric scintillation, is it advantageous to have ionospheric scales observations based on in-situ measurements.
We investigated the variability of the in-situ plasma density and magnetic field measured by Swarm satellites creating the climatology of their scales by leveraging the Fast Iterative Filtering (FIF) technique.
FIF is able to provide a very fine time-frequency representation decomposing any non-stationary, nonlinear signals, into oscillating modes, called intrinsic mode components or functions (IMCs or IMFs), characterized by their specific frequency.
The results are obtained by time-integrating the instantaneous time-frequency representations, provided through the so-called “IMFogram”. These IMFograms have the potential to show the greater details of the scale sizes and their variations, illustrating the time development of the multi-scale processes during various disturbances of geospace.
How to cite: Urbar, J., Spogli, L., Cicone, A., Clausen, L., Jin, Y., Wood, A., Donegan-Lawley, E., Alfonsi, L., Cesaroni, C., Kotova, D., Høeg, P., and Miloch, W.: Spatio-Temporal Scales of Plasma Density in Topside Ionosphere, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-3387, https://doi.org/10.5194/egusphere-egu23-3387, 2023.