EGU2020-2641, updated on 09 Jan 2024
https://doi.org/10.5194/egusphere-egu2020-2641
EGU General Assembly 2020
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Determining the position of the of thunder infrasound source using a large aperture micro barometer array

Jan Rusz, Jaroslav Chum, and Jiří Baše
Jan Rusz et al.
  • Institute of Atmospheric Physics Czech Academy of Sciences, Prague, Czech Republic (rusz@ufa.cas.cz)

Large aperture array of absolute micro‑barometers located in Western Czechia was used to register distinct infrasound pulses generated by thunderstorm activity. Only cases with a sufficient signal-to-noise ratio on all four micro‑barometers were selected for further processing. Using data from the European lightning detection network and electric field monitor, a corresponding flash was assigned to each set of signals. The position of the infrasound source was calculated from the time delay of signal arrival, assuming propagation of spherical waves from the source. The calculation includes changes in sound speed as a function of temperature variation with altitude. Wind speed value and its variance is also taken into account to estimate the uncertainties. The calculated vertical positions of the infrasound sources are located at the altitudes between 3‑6 km. The horizontal position for most of the selected cases corresponds to the horizontal position of the flash specified by lightning detection network. The recorded infrasound signals followed only intracloud (IC) or mixed (multiple IC+CG) lightning strokes. Thus, the sources of the analyzed infrasound events are most likely IC discharges.

How to cite: Rusz, J., Chum, J., and Baše, J.: Determining the position of the of thunder infrasound source using a large aperture micro barometer array, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-2641, https://doi.org/10.5194/egusphere-egu2020-2641, 2020.

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