the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Peering into the heart of thunderstorm clouds: Insights from cloud radar and spectral polarimetry
Abstract. Lightning is a natural phenomenon that can be dangerous to humans. It is however challenging to study thunderstorm clouds using direct observations since it can be dangerous to fly into thunderstorm clouds. In this study, cloud radar at 35 GHz is used to study the properties and dynamics of thunderstorm clouds. It is based on a case of thunderstorm on 18 June 2021 from 16:10 to 17:45 UTC near Cabauw, the Netherlands. The technique of spectral polarimetric analysis at millimeter wavelength, which has not been used in previous studies about thunderstorm clouds so far, is used to help understand the behaviours of different types of particles within a radar resolution volume. Spectral polarimetric radar variables are used to investigate possible hydrometeors in the clouds and look for vertical alignment of ice crystals that is expected due to electric torque. Due to challenges posed by Mie scattering, scattering simulations are carried out to aid the interpretation of spectral polarimetric variables. It is shown that the start of the Mie regime in the Doppler spectrum can be identified by the use of the spectral differential phase. From the results, there is a high chance that supercooled liquid water and conical graupel are present in thunderstorm clouds. There is also a possibility of ice crystals arranged in chains at the cloud top. Ice crystals become vertically aligned a few seconds before lightning and return to their usual horizontal alignment afterwards. However, this phenomenon has been witnessed in only a few cases, specifically when the lightning strike is in close proximity to the radar's line of sight or when the lightning is exceptionally strong. Doppler analyses show that updrafts are found near the core of the thunderstorm cloud, while downdrafts are observed at the edges. Strong turbulence is also observed as reflected by the large Doppler spectrum width.
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Status: closed
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RC1: 'Comment on egusphere-2024-1232', Anonymous Referee #1, 19 Jun 2024
- AC1: 'Reply on RC1', Ho Yi Lydia Mak, 14 Oct 2024
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RC2: 'Comment on egusphere-2024-1232', Anonymous Referee #2, 20 Jun 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1232/egusphere-2024-1232-RC2-supplement.pdf
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AC2: 'Reply on RC2', Ho Yi Lydia Mak, 14 Oct 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1232/egusphere-2024-1232-AC2-supplement.pdf
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AC2: 'Reply on RC2', Ho Yi Lydia Mak, 14 Oct 2024
- AC1: 'Reply on RC1', Ho Yi Lydia Mak, 14 Oct 2024
Status: closed
-
RC1: 'Comment on egusphere-2024-1232', Anonymous Referee #1, 19 Jun 2024
- AC1: 'Reply on RC1', Ho Yi Lydia Mak, 14 Oct 2024
-
RC2: 'Comment on egusphere-2024-1232', Anonymous Referee #2, 20 Jun 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1232/egusphere-2024-1232-RC2-supplement.pdf
-
AC2: 'Reply on RC2', Ho Yi Lydia Mak, 14 Oct 2024
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2024/egusphere-2024-1232/egusphere-2024-1232-AC2-supplement.pdf
-
AC2: 'Reply on RC2', Ho Yi Lydia Mak, 14 Oct 2024
- AC1: 'Reply on RC1', Ho Yi Lydia Mak, 14 Oct 2024
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