Predicting ice shape evolution in a bulk microphysics model.Source: Journal of the Atmospheric Sciences:;2017:;Volume( 074 ):;issue: 006::page 2081DOI: 10.1175/JAS-D-16-0350.1Publisher: American Meteorological Society
Abstract: novel bulk microphysics scheme that predicts the evolution of ice properties including aspect ratio (shape), mass, number, size, and density is described, tested, and demonstrated. The scheme is named the Ice-Spheroids Habit Model with Aspect-ratio EvoLution (ISHMAEL). Ice is modeled as spheroids and is nucleated as one of two species depending on nucleation temperature. Microphysical process rates determine how shape and other ice properties evolve. A third aggregate species is also employed, diversifying ice properties in the model. Tests of ice shape evolution during vapor growth and riming are verified against wind-tunnel data revealing that the model captures habit-dependent riming and its effect on fall speed. Lagrangian parcel studies demonstrate that the bulk model captures ice property evolution during riming and melting compared to a bin model. Finally, the capabilities of ISHMAEL are shown in a 2D kinematic framework with a simple updraft. A direct result of predicting ice shape evolution is that various states of ice from unrimed to lightly rimed to densely rimed can be modeled without converting ice mass between pre-defined ice categories (e.g. snow and graupel). This leads to a different spatial precipitation distribution compared to the traditional method of separating snow and graupel and converting between the two categories because ice in ISHMAEL sorts in physical space based on the amount of rime which controls the thickness and therefore fall speed. Predicting these various state of rimed ice leads to a reduction in vapor growth rate and an increase in riming rate in a simple updraft compared to the traditional approach.
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contributor author | Jensen, Anders A. | |
contributor author | Harrington, Jerry Y. | |
contributor author | Morrison, Hugh | |
contributor author | Milbrandt, Jason A. | |
date accessioned | 2017-06-09T17:00:01Z | |
date available | 2017-06-09T17:00:01Z | |
date issued | 2017 | |
identifier issn | 0022-4928 | |
identifier other | ams-77663.pdf | |
identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4220246 | |
description abstract | novel bulk microphysics scheme that predicts the evolution of ice properties including aspect ratio (shape), mass, number, size, and density is described, tested, and demonstrated. The scheme is named the Ice-Spheroids Habit Model with Aspect-ratio EvoLution (ISHMAEL). Ice is modeled as spheroids and is nucleated as one of two species depending on nucleation temperature. Microphysical process rates determine how shape and other ice properties evolve. A third aggregate species is also employed, diversifying ice properties in the model. Tests of ice shape evolution during vapor growth and riming are verified against wind-tunnel data revealing that the model captures habit-dependent riming and its effect on fall speed. Lagrangian parcel studies demonstrate that the bulk model captures ice property evolution during riming and melting compared to a bin model. Finally, the capabilities of ISHMAEL are shown in a 2D kinematic framework with a simple updraft. A direct result of predicting ice shape evolution is that various states of ice from unrimed to lightly rimed to densely rimed can be modeled without converting ice mass between pre-defined ice categories (e.g. snow and graupel). This leads to a different spatial precipitation distribution compared to the traditional method of separating snow and graupel and converting between the two categories because ice in ISHMAEL sorts in physical space based on the amount of rime which controls the thickness and therefore fall speed. Predicting these various state of rimed ice leads to a reduction in vapor growth rate and an increase in riming rate in a simple updraft compared to the traditional approach. | |
publisher | American Meteorological Society | |
title | Predicting ice shape evolution in a bulk microphysics model. | |
type | Journal Paper | |
journal volume | 074 | |
journal issue | 006 | |
journal title | Journal of the Atmospheric Sciences | |
identifier doi | 10.1175/JAS-D-16-0350.1 | |
journal fristpage | 2081 | |
journal lastpage | 2104 | |
tree | Journal of the Atmospheric Sciences:;2017:;Volume( 074 ):;issue: 006 | |
contenttype | Fulltext |