Preprints
https://doi.org/10.5194/acp-2016-368
https://doi.org/10.5194/acp-2016-368
18 May 2016
 | 18 May 2016
Status: this preprint was under review for the journal ACP but the revision was not accepted.

Investigating the Impacts of Saharan Dust on Tropical Deep Convection Using Spectral Bin Microphysics, Part 1: Ice Formation and Cloud Properties

Matthew Gibbons, Qilong Min, and Jiwen Fan

Abstract. To better understand the impacts of dust aerosols on deep convective cloud (DCC) systems revealed by previous observational studies, a case study in the tropical eastern Atlantic was investigated using the Weather Research and Forecasting (WRF) model coupled with a Spectral Bin Microphysics (SBM) model as a two-part study. A detailed set of ice nucleation parameterizations linking ice formation with aerosol particles have been implemented in the SBM for this study. It is found that, dust, transported from the Sahara desert and acting as ice nuclei (IN), increases heterogeneous formation of ice particles at temperatures above −38 °C by approximately a factor of four per IN magnitude increase from 0.12 cm−3. Homogeneous ice formation is reduced below −38 °C by up to 79 %, due to greater conversion of liquid drops to ice at warmer temperatures. The ice particle size distribution (PSD) is shifted towards smaller sizes at heterogeneous temperatures and median sizes at colder temperatures due to increased vapor competition and crystal aggregation. Graupel sizes are reduced due to increased riming of more numerous, but smaller, ice particles. Liquid mass is reduced by up to 85 % at midlevels due to increased riming, drop freezing and Bergeron process evaporation. Despite the enhanced vertical motion in the dust cases (up to 30 %), average cloud top height was found to be lowered by up to 3.29 km in comparison with the background aerosol (Clean) case, which is consistent with observations. This is due to increased sedimentation rates resulting from earlier formation of precipitation sized particles.

Matthew Gibbons, Qilong Min, and Jiwen Fan
 
Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
Printer-friendly Version - Printer-friendly version Supplement - Supplement
 
Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
Printer-friendly Version - Printer-friendly version Supplement - Supplement
Matthew Gibbons, Qilong Min, and Jiwen Fan
Matthew Gibbons, Qilong Min, and Jiwen Fan

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Short summary
Observations suggest cloud systems evolve differently under dusty conditions compared to other aerosols. We have used numerical modeling to study one such case. Dust increases the formation of small sized ice in the mid-troposphere. This enhanced convective intensity, shifted precipitation top height to higher altitudes, and glaciated clouds at lower altitudes. Consistent with observations, average cloud height was lowered due to a greater number of heavy particles forming near the cloud tops.
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