Abstract

Abstract. A dust storm of fearful proportions hit Phoenix in the early evening hours of 5 July 2011. This storm, an American haboob, was predicted hours in advance because numerical, land–atmosphere modeling, computing power and remote sensing of dust events have improved greatly over the past decade. High-resolution numerical models are required for accurate simulation of the small scales of the haboob process, with high velocity surface winds produced by strong convection and severe downbursts. Dust productive areas in this region consist mainly of agricultural fields, with soil surfaces disturbed by plowing and tracks of land in the high Sonoran Desert laid barren by ongoing draught. Model simulation of the 5 July 2011 dust storm uses the coupled atmospheric-dust model NMME–DREAM (Non-hydrostatic Mesoscale Model on E grid, Janjic et al., 2001; Dust REgional Atmospheric Model, Nickovic et al., 2001; Pérez et al., 2006) with 4 km horizontal resolution. A mask of the potentially dust productive regions is obtained from the land cover and the normalized difference vegetation index (NDVI) data from the Moderate Resolution Imaging Spectroradiometer (MODIS). The scope of this paper is validation of the dust model performance, and not use of the model as a tool to investigate mechanisms related to the storm. Results demonstrate the potential technical capacity and availability of the relevant data to build an operational system for dust storm forecasting as a part of a warning system. Model results are compared with radar and other satellite-based images and surface meteorological and PM10 observations. The atmospheric model successfully hindcasted the position of the front in space and time, with about 1 h late arrival in Phoenix. The dust model predicted the rapid uptake of dust and high values of dust concentration in the ensuing storm. South of Phoenix, over the closest source regions (~25 km), the model PM10 surface dust concentration reached ~2500 μg m−3, but underestimated the values measured by the PM10 stations within the city. Model results are also validated by the MODIS aerosol optical depth (AOD), employing deep blue (DB) algorithms for aerosol loadings. Model validation included Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO), equipped with the lidar instrument, to disclose the vertical structure of dust aerosols as well as aerosol subtypes. Promising results encourage further research and application of high-resolution modeling and satellite-based remote sensing to warn of approaching severe dust events and reduce risks for safety and health.

Highlights

  • Particular sandstorms, called haboobs (“habb” – to blow), are very frequent events in Sudan (Sutton, 1925)

  • About 40 years after the American haboob was recognized over the southwest US, computer power, modeling of atmospheric processes, and satellite observations advanced to the point where we are able to simulate such an extreme and local dust storm event

  • Despite the fact that DREAM model never has been applied in the simulation of such events, it managed to produce an accurate shape, duration and magnitude of the dust storm

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Summary

Introduction

Particular sandstorms, called haboobs (“habb” – to blow), are very frequent events in Sudan (Sutton, 1925). Available ground and radar measurements, National Weather Service Forecast Office and news media reports, amateur photos and videos of the storm, showed that this event was much like the one described by Idso et al (1972). All this information indicated that for successful numerical simulation of the event, the model must represent convective activity and active dust sources very well. This dust storm was created by the high surface winds generated from strong downbursts of cold air. In forecast operations, the dust sources are refreshed for model ingestion every 16 days

Phoenix dust storm on 5 July 2011
Model description and dust sources
Model results and discussion
Findings
Conclusions
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