EGU23-3124
https://doi.org/10.5194/egusphere-egu23-3124
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Electrodynamic model of K-changes

Petr Kaspar1, Thomas Marshall2, Maribeth Stolzenburg2, Ivana Kolmasova1,3, and Ondrej Santolik1,3
Petr Kaspar et al.
  • 1Department of Space Physics, Institute of Atmospheric Physics CAS, Prague, Czechia (pk@ufa.cas.cz)
  • 2Department of Physics and Astronomy, University of Mississippi, University, Mississippi, USA,
  • 3Faculty of Mathematics and Physics, Charles University, Prague ,Czechia

K-changes are step-like electrostatic field changes, which occur during the final part of cloud flashes or between the return strokes in cloud-to-ground discharges. We numerically solve the full set of Maxwell’s equations coupled to the electrostatic Poisson’s equation for a given thundercloud charge structure to model the K-changes. We simulate the K-changes by a sequential increase of conductivity of the decayed vertical channel. This process creates a current pulse which attenuates as it propagates downward. We show how the modeled linear charge densities and electric potentials connected to K-changes evolve in time. We successfully compare our model with the electric field measured by a flat-plate E-change antenna with a sensor having a decay time constant of 1 s, a bandwidth of 0.16 Hz –2.6 MHz, and a sampling rate of 5 MS/s. The experimental data used for comparison with our model were obtained at KSC Florida in 2011.

How to cite: Kaspar, P., Marshall, T., Stolzenburg, M., Kolmasova, I., and Santolik, O.: Electrodynamic model of K-changes, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-3124, https://doi.org/10.5194/egusphere-egu23-3124, 2023.