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The GPM Validation Network and Evaluation of Satellite-Based Retrievals of the Rain Drop Size Distribution
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Quantifying Particle Size Distribution Errors Derived from SAGE III/ISS Observations
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Stratospheric Aerosol Size Distributions and Optical Depth: Long-term GEOS-Chem-UCX/APM Simulations and Comparisons with Measurements
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Investigating Size Distributions of Chaos “Blocks” on Europa, Mars, and Pluto
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Impact of Size Distribution Assumption on PM2.5 Simulation
Aerosol particles, especially those with diameter that is smaller than 2.5um, i.e. PM2.5, have detrimental impact on public health. As a regulated criteria air pollutant, PM2.5 is monitored by ground networks using various instruments. At the same time aerosol assimilation modeling system is developed to simulate the aerosol distribution with continuous global coverage. In this study we compared the PM2.5 simulated by NASA’s MERRA-2 modeling system with the measurements made at US Embassy sites around the globe on diurnal cycle, monthly average, and interannual variabilities. We focused the comparison in the places that are significantly impacted by the desert dust. Simulations based on both aerodynamic and geometric diameters are compared with available measurements. Aerodynamic diameter assumption shows better model-observation agreements over several dust belt stations.
Exploring the Climatic Impact of Bi-Modal Dust Particle Size Distributions During the MY34/2018 Global Dust Storm with the NASA Ames Mars Global Climate Model.
We have implemented a bi-modal dust lifting scheme in the NASA Ames Mars Global Climate Model (GCM) and investigated the climatic impact on the MY34/2018 Global Dust Storm (GDS). We found that the climate is measurably responsive to the inclusion of a second, smaller dust mode. Dust tends to be lifted through a deeper column in the atmosphere, which is reflected in the climate as changes to atmospheric temperature, tide amplitudes, and surface temperatures. Adding a modest fraction of a smaller dust mode improves simulations during the GDS compared to Curiosity semi-diurnal tide observations as well as Mars Climate Sounder (MCS) T15 brightness temperatures
Variations in Simulated GMI Brightness Temperatures Due to Varying Particle Size Distribution Models and Hydrometeor Characteristics in a Severe Hailstorm
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Particle Size Distribution Parameters from SAGE III/ISS Extinction Spectra, with Application to the 2022 Hunga Tonga Eruption
The Stratospheric Aerosol and Gas Experiment (SAGE) on the International Space Station (ISS)
Size distributions of coastal ocean suspended particulate inorganic matter: Amorphous silica and clay minerals and their dynamics
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Retrieving Rain Drop Size Distribution Moments from GPM Dual-Frequency Precipitation Radar
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Eolianite Grain Size Distributions as a Proxy for Large Changes in Planetary Atmospheric Density
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The Importance of the Shape of Cloud Droplet Size Distributions in Shallow Cumulus Clouds. Part I: Bin Microphysics Simulations
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High fidelity, discrete element method simulation of magnetorheological fluids using accurate particle size distributions in LIGGGHTS extended with mutual dipole method
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The Retrieval of Drop Size Distribution Parameters Using a Dual-Polarimetric Radar
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The GPM Validation Network and Evaluation of Satellite-Based Retrievals of the Rain Drop Size Distribution
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Temperatures of lunar impact flashes: mass and size distribution of small impactors hitting the Moon
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