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Cloud Condensation Nuclei Analysis×ケーラー理論×スペクトルビン微物理×WRFモデル×
分野気象学気象学気象学気象学
系統Process / pipelineProcess / pipelineProcess / pipelineProcess / pipeline
提唱年1959193619992000
提唱者Twomey, WoodardHilding KohlerKhain, OvtchinnikovSkamarock and Klemp
種類Cloud microphysical measurementThermodynamic equilibrium frameworkExplicit particle size distribution modelAtmospheric simulation system
原典Dusek, U., Frank, G. P., Hildebrandt, L., et al. (2006). Size matters more than chemistry for cloud-nucleating ability of aerosol particles. Science, 312(5778), 1375-1378. DOI ↗Köhler, H. (1936). The nucleus in and the growth of hygroscopic droplets. Transactions of the Faraday Society, 32, 1152-1161. DOI ↗Khain, A. P., Ovtchinnikov, M., Pinsky, M., Pokrovsky, A., & Krugliak, H. (2000). Notes on the state-of-the-art numerical modeling of cloud microphysics. Atmospheric Research, 55(3–4), 159-224. DOI ↗Skamarock, W. C., Klemp, J. B., Dudhia, J., et al. (2008). A Description of the Advanced Research WRF Version 3. NCAR Technical Note NCAR/TN-475+STR. link ↗
別名CCN analysis, Cloud condensation nuclei, CCN measurementKohler theory, Kohler equilibrium, Cloud droplet nucleationBin microphysics, Spectral microphysics, Explicit microphysicsWeather Research and Forecasting, WRF, ARW, NMM
関連3334
概要Cloud condensation nuclei (CCN) analysis examines the number and properties of aerosol particles capable of nucleating cloud droplets at various supersaturation levels. This field involves measuring CCN concentrations, characterizing their chemical composition and size, and relating aerosol properties to cloud microphysical processes.Köhler theory is a foundational framework in cloud microphysics that predicts the equilibrium supersaturation required for an aerosol particle of given size and composition to grow into a cloud droplet. Published in 1936 by Hilding Köhler, it combines the Kelvin effect (vapor pressure enhancement over curved surfaces) with the Raoult effect (vapor pressure depression from dissolved solute) to explain cloud droplet formation.Spectral bin microphysics is a detailed cloud microphysical modeling approach that explicitly represents the particle size distribution (PSD) by dividing particles into discrete size bins. Rather than assuming a fixed shape for the PSD, bin models track the number and mass of particles in each size category, allowing detailed simulation of cloud and precipitation processes.The Weather Research and Forecasting (WRF) model is a mesoscale atmospheric simulation system used for weather forecasting, research, and climate applications. Developed cooperatively by NCAR, NOAA, and academic institutions, WRF became operational in 2004 and has become one of the most widely used atmospheric models worldwide.
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ScholarGate手法を比較: Cloud Condensation Nuclei Analysis · Kohler Theory · Spectral Bin Microphysics · WRF Model. 2026-06-19に以下より取得 https://scholargate.app/ja/compare