ScholarGate
المساعد

قارن الطرق

راجع الطرق التي اخترتها جنبًا إلى جنب؛ الصفوف المختلفة مميَّزة.

الفيزياء المجهرية الطيفية×نظرية كولر×
المجالعلم الأرصاد الجويةعلم الأرصاد الجوية
العائلةProcess / pipelineProcess / pipeline
سنة النشأة19991936
صاحب الطريقةKhain, OvtchinnikovHilding Kohler
النوعExplicit particle size distribution modelThermodynamic equilibrium framework
المصدر التأسيسيKhain, 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 ↗Köhler, H. (1936). The nucleus in and the growth of hygroscopic droplets. Transactions of the Faraday Society, 32, 1152-1161. DOI ↗
الأسماء البديلةBin microphysics, Spectral microphysics, Explicit microphysicsKohler theory, Kohler equilibrium, Cloud droplet nucleation
ذات صلة33
الملخصSpectral 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.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.
ScholarGateمجموعة البيانات
  1. v1
  2. 2 المصادر
  3. PUBLISHED
  1. v1
  2. 2 المصادر
  3. PUBLISHED

انتقل إلى البحث تنزيل الشرائح

ScholarGateقارن الطرق: Spectral Bin Microphysics · Kohler Theory. استُرجع بتاريخ 2026-06-18 من https://scholargate.app/ar/compare