the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
The impacts of secondary ice production on microphysics and dynamics in tropical convection
Abstract. Secondary ice production (SIP) is an important physical phenomenon that results in an increase of ice particle concentration and can therefore have a significant impact on the evolution of clouds. In this study, idealized simulations of a mesoscale convective systems (MCS) was conducted using a high-resolution (250-m horizontal grid spacing) mesoscale model and a detailed bulk microphysics scheme in order to examine the impacts of SIP on the microphysics and dynamics of a simulated tropical MCS. The simulations were compared to airborne in situ and remote sensing observations collected during the High Altitude Ice Crystals – High Ice Water Content (HAIC-HIWC) field campaign in 2015. It was found that simulated ice particle size distributions are highly sensitive to the parameterization of SIP. Inclusion of SIP processes in the microphysics scheme is crucial for the production and maintenance of high ice water content in the simulated tropical convection. It was shown that SIP can enhance the strength of the existing convective updrafts and result in the initiation of new updrafts above the melting layer. Agreement between the simulations and observations highlights the impacts of SIP on the maintenance of tropical MCSs in nature and the importance of including SIP parameterizations in models.
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Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
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Preprint
(3217 KB)
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The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(3217 KB) - Metadata XML
- BibTeX
- EndNote
- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
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RC1: 'Comment on egusphere-2022-235', Anonymous Referee #1, 16 Jun 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-235/egusphere-2022-235-RC1-supplement.pdf
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AC1: 'Reply on RC1', Zhipeng Qu, 02 Aug 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-235/egusphere-2022-235-AC1-supplement.pdf
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AC1: 'Reply on RC1', Zhipeng Qu, 02 Aug 2022
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RC2: 'Comment on egusphere-2022-235', Alain Protat, 20 Jun 2022
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AC2: 'Reply on RC2', Zhipeng Qu, 02 Aug 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-235/egusphere-2022-235-AC2-supplement.pdf
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AC2: 'Reply on RC2', Zhipeng Qu, 02 Aug 2022
Interactive discussion
Status: closed
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RC1: 'Comment on egusphere-2022-235', Anonymous Referee #1, 16 Jun 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-235/egusphere-2022-235-RC1-supplement.pdf
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AC1: 'Reply on RC1', Zhipeng Qu, 02 Aug 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-235/egusphere-2022-235-AC1-supplement.pdf
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AC1: 'Reply on RC1', Zhipeng Qu, 02 Aug 2022
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RC2: 'Comment on egusphere-2022-235', Alain Protat, 20 Jun 2022
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AC2: 'Reply on RC2', Zhipeng Qu, 02 Aug 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-235/egusphere-2022-235-AC2-supplement.pdf
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AC2: 'Reply on RC2', Zhipeng Qu, 02 Aug 2022
Peer review completion
Journal article(s) based on this preprint
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Alexei Korolev
Jason A. Milbrandt
Ivan Heckman
Yongjie Huang
Greg M. McFarquhar
Hugh Morrison
Mengistu Wolde
Cuong Nguyen
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(3217 KB) - Metadata XML