EventsThe 1st International Online Conference on Earth Science
Published
This submission belongs to the session S3. Climate Dynamics, Variability and Change of the event The 1st International Online Conference on Earth Science
Published date
31 Aug, 2026
Academic Editor
author-avatarCharles Jones
Citation
Pranaba K Nayak, R Biswasharma, N Umakanth, A S Patil, P K Mohanty, S K Gupta, Y Hayashi, S Kawakami, S R Dugad, S D Pawar, A Jain, P Jagadeesan, B Hariharan, M Rameez, K Ramesh, A Oshima, Evolution of Thunderstorm Electrification and Cloud Microphysics during an Intense Convective Storm: A Multi-Instrument and Modeling Study, in Proceedings of The 1st International Online Conference on Earth Science, 2 September–4 September 2026, MDPI: Basel, Switzerland
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Evolution of Thunderstorm Electrification and Cloud Microphysics during an Intense Convective Storm: A Multi-Instrument and Modeling Study

R Biswasharma 2
N Umakanth 3
A S Patil 2
P K Mohanty 1
S K Gupta 1
Y Hayashi 4
S Kawakami 4
S R Dugad 1
S D Pawar 2
A Jain 1
P Jagadeesan 1
B Hariharan 1
M Rameez 1
K Ramesh 1
A Oshima 5
1. Tata Institute of Fundamental Research, Mumbai 400005, India
2. Thunderstorm Dynamics, IITM, Ministry of Earth Sciences, Pune 411008, India
3. Indian National Center for Ocean Information, Hyderabad 500090, India
4. Graduate School of Science, Osaka Metropolitan University, Osaka, 558 8585, Japan
5. College of Engineering, Chubu University, Kasugai, Aichi, 487 8501, India
Abstract

Thunderstorm electrification arises from complex interactions among cloud microphysics, dynamics, and charge separation processes. Lightning and surface electric-field measurements alone cannot fully resolve the three-dimensional electrical structure of convective storms. Cosmic-ray muons, owing to their high penetrating power, provide a complementary probe of electrified cloud regions. Here, we investigate an intense convective thunderstorm over southern India on 27 April 2020 using a multi-instrumental framework that combines directional muon observations from the GRAPES-3 telescope [1], surface electric-field measurements, lightning location network data, satellite observations, ERA5 reanalysis, and high-resolution WRF simulations. After correcting the muon data for atmospheric pressure and solar-induced anisotropy, we identify a transient ~0.5% decrease in muon flux from the Southeast direction during the storm's mature phase [2-3]. This directional deficit occurs concurrently with enhanced electric-field variability, peak lightning activity, and the development of a vigorous mixed-phase region conducive to non-inductive charge separation, as indicated by satellite observations and WRF simulations. The consistency in timing and direction among these independent datasets provides compelling evidence for a close linkage between thunderstorm electrification and secondary cosmic-ray particles. These results demonstrate the value of directional muon observations as an independent diagnostic of electrified thunderstorms and highlight the potential of multi-instrumental analyses for investigating storm-scale electrical processes.

References

  1. PK Nayak et al., Observation of thunderstorm-induced muon events in GRAPES-3 experiment, J. Atmos. Sol.–Terr. Phys. 258 (2024) 106231.
  2. P.K. Nayak et al., Thunderstorm-induced muon event on 20 March 2020: Insights from the Ooty muon telescope, INSAT-3DR, and lightning observations, Physical Review D 112 (2025) 083046
  3. P.K. Nayak et al., The Ooty muon telescope reveals what climate did in 2022 summer, Ind. J. Phys. 98 (2024) 4239.
Keywords
Thunderstorm electrification
Cloud microphysics
Cosmic-ray muons
Lightning activity
WRF modeling
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