4.6 Article

Confronting the Challenge of Modeling Cloud and Precipitation Microphysics

Journal

Publisher

AMER GEOPHYSICAL UNION
DOI: 10.1029/2019MS001689

Keywords

microphysics; clouds; modeling

Funding

  1. US Department of Energy Atmospheric System Research (DOE ASR) [DE-SC0016579]
  2. DOE ASR [DE-SC0020171, DE-SC0016476, DE-SC0016237, DE-SC0018933]
  3. NASA Radiation Science Program
  4. National Science Foundation [AGS-1824243]
  5. European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme [714062]
  6. Polish National Science Center (NCN) [2016/23/B/ST10/00690, 2017/25/B/ST10/02383]
  7. MEXT KAKENHI [18h04448]
  8. National Center of Meteorology, Abu Dhabi, UAE, under the UAE Research Program for Rain Enhancement Science
  9. National Aeronautics and Space Administration
  10. U.S. Department of Energy (DOE) [DE-SC0018933, DE-SC0016579, DE-SC0016237, DE-SC0020171] Funding Source: U.S. Department of Energy (DOE)
  11. Grants-in-Aid for Scientific Research [18H04448] Funding Source: KAKEN

Ask authors/readers for more resources

In the atmosphere,microphysicsrefers to the microscale processes that affect cloud and precipitation particles and is a key linkage among the various components of Earth's atmospheric water and energy cycles. The representation of microphysical processes in models continues to pose a major challenge leading to uncertainty in numerical weather forecasts and climate simulations. In this paper, the problem of treating microphysics in models is divided into two parts: (i) how to represent the population of cloud and precipitation particles, given the impossibility of simulating all particles individually within a cloud, and (ii) uncertainties in the microphysical process rates owing to fundamental gaps in knowledge of cloud physics. The recently developed Lagrangian particle-based method is advocated as a way to address several conceptual and practical challenges of representing particle populations using traditional bulk and bin microphysics parameterization schemes. For addressing critical gaps in cloud physics knowledge, sustained investment for observational advances from laboratory experiments, new probe development, and next-generation instruments in space is needed. Greater emphasis on laboratory work, which has apparently declined over the past several decades relative to other areas of cloud physics research, is argued to be an essential ingredient for improving process-level understanding. More systematic use of natural cloud and precipitation observations to constrain microphysics schemes is also advocated. Because it is generally difficult to quantify individual microphysical process rates from these observations directly, this presents an inverse problem that can be viewed from the standpoint of Bayesian statistics. Following this idea, a probabilistic framework is proposed that combines elements from statistical and physical modeling. Besides providing rigorous constraint of schemes, there is an added benefit of quantifying uncertainty systematically. Finally, a broader hierarchical approach is proposed to accelerate improvements in microphysics schemes, leveraging the advances described in this paper related to process modeling (using Lagrangian particle-based schemes), laboratory experimentation, cloud and precipitation observations, and statistical methods.

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