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dc.contributor.authorDeepak Waman
dc.contributor.authorSachin Patade
dc.contributor.authorArti Jadav
dc.contributor.authorAkash Deshmukh
dc.contributor.authorAshok Kumar Gupta
dc.contributor.authorVaughan T. J. Phillips
dc.contributor.authorAaron Bansemer
dc.contributor.authorPaul J. DeMott
dc.date.accessioned2023-04-12T18:41:18Z
dc.date.available2023-04-12T18:41:18Z
dc.date.copyright2022/12/05
dc.date.issued2022
dc.identifier.otherJAS-D-21-0278.1.pdf
dc.identifier.urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4290073
dc.description.abstractVarious mechanisms of secondary ice production (SIP) cause multiplication of numbers of ice particle, after the onset of primary ice. A measure of SIP is the ice enhancement ratio (“IE ratio”) defined here as the ratio between number concentrations of total ice (excluding homogeneously nucleated ice) and active ice-nucleating particles (INPs). A convective line observed on 11 May 2011 over the Southern Great Plains in the Mesoscale Continental Convective Cloud Experiment (MC3E) campaign was simulated with the “Aerosol–Cloud” (AC) model. AC is validated against coincident MC3E observations by aircraft, ground-based instruments, and satellite. Four SIP mechanisms are represented in AC: the Hallett–Mossop (HM) process of rime splintering, and fragmentation during ice–ice collisions, raindrop freezing, and sublimation. The vertical profile of the IE ratio, averaged over the entire simulation, is almost uniform (10
dc.publisherAmerican Meteorological Society
dc.titleDependencies of Four Mechanisms of Secondary Ice Production on Cloud-Top Temperature in a Continental Convective Storm
dc.typeJournal Paper
dc.journal.volume79
dc.journal.issue12
dc.journal.titleJournal of the Atmospheric Sciences
dc.identifier.doi10.1175/JAS-D-21-0278.1
dc.journal.fristpage3375
dc.journal.lastpage3404
dc.page3375–3404
dc.treeJournal of the Atmospheric Sciences:;2022:;volume( 079 ):;issue: 012
dc.contenttypeFulltext


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