Open Access

Overview of the development of the Aerosol Loading Interface for Cloud microphysics In Simulation (ALICIS)

  • Takamichi Iguchi1, 2Email author,
  • In-Jin Choi3,
  • Yousuke Sato4,
  • Kentaroh Suzuki5 and
  • Teruyuki Nakajima6
Progress in Earth and Planetary Science20152:45

DOI: 10.1186/s40645-015-0075-0

Received: 30 June 2015

Accepted: 7 December 2015

Published: 11 December 2015


This review summarizes the scientific background of and past/prospective update strategies for the development of the Aerosol Loading Interface for Cloud microphysics In Simulation (ALICIS). ALICIS provides a novel approach for coupling downscaled mesoscale cloud-resolving simulations to large-scale aerosol-transport simulations. Realistic aerosol loading, including spatio-temporal aerosol variations and particle-size spectra, is implemented in the cloud-resolving simulations. Prior studies employing ALICIS have demonstrated how the interface introduction significantly improves the reproducibility of the simulated microphysical cloud structure through better representation of aerosol effects on cloud.


Cloud microphysics Cloud and aerosol Regional modeling Dynamical downscaling



Aerosol effects on cloud in atmospheric models

The coexistence of the three phases of hydrogen monoxide is, within the solar system, unique to the Earth’s atmosphere. The liquid and solid phases in the atmosphere (i.e., cloud and precipitation) play critical roles in determining the Earth’s radiation balance and hydrological cycle by driving considerable changes in the atmospheric hydrometeor distribution and characteristics. The hydrometeor behavior is controlled by various factors, not limited to phase changes affected by temperature, dry-air and vapor pressure, advection by background winds, and gravitational falling.

Particulate matter that is dispersed colloidally with a variety of the particle sizes, shapes, and chemical components in the Earth’s atmosphere is referred to as aerosol. Aerosol particles are closely related to the liquid and solid particles making up clouds and precipitation; they are not only necessary for the nucleation process of hydrometeor particles but are also a source of impurities in these particles. To date, the aerosol influence on cloud has been investigated in a number of ways, from the perspectives of weather and climate research, as well as in the context of weather modification and geo-engineering, starting from a series of studies by Twomey and Squires who examined microphysical cloud structure under various airmass conditions using in situ aircraft measurements in the 1950s and 1960s (e.g., Squires 1956). A well-known example demonstrating the effects of aerosol is that of the systematic difference in microphysical properties between continental and oceanic clouds. Continental clouds generally have a smaller mean particle size and a higher particle number concentration than oceanic clouds. These differences are attributed to the disparity in aerosol concentration and characteristics between the regions.

Aerosol was not represented explicitly in most numerical models of the Earth’s atmosphere on global or regional scales until the 1990s, despite its significance for clouds and climate. This was due in part to the fact the models were generally aimed at analyses of the atmosphere’s dynamical structure and at land-surface rainfall predictions. Researchers thus considered aerosol unimportant in the basic framework of atmospheric models, because it had no direct influence on mass or energy conservation in the atmosphere and its fluid dynamics. In addition, computational resources were insufficient to explicitly include aerosol. Aerosol effects on cloud were thus tacitly included in the models in the form of parametrizations consisting of empirical equations. For example, saturation adjustment (Soong and Ogura 1973; Tao et al. 1989) is a reasonable assumption for calculations of the nucleation of cloud droplets and their condensation growth from water vapor. Even though the presence of aerosol is a requirement for the droplets’ nucleation process, the details are not important because of the wealth of aerosol particles that can be activated as cloud condensation nuclei (CCN) in the troposphere.

In the 1990s and 2000s, increasing interest in aerosol brought the issue under consideration even in the context of atmospheric modeling approaches. The most significant turning point was the recognition that aerosol might counter the anthropogenic gases that cause global warming through their greenhouse effect. Tropospheric aerosol particles have a direct impact on the Earth’s radiative balance through the scattering and absorption of short- and longwave radiation (i.e., aerosol direct radiative forcing). In addition, aerosol particles have an indirect influence on the Earth’s radiative balance through altering optical cloud properties by serving as CCN (i.e., aerosol indirect radiative forcing). An increase in the concentration of tropospheric aerosol particles may enhance cloud reflectance for solar irradiance as a result of the increased droplet number concentration and reduced droplet size for a fixed liquid water path (Twomey 1974, 1977; Twomey et al. 1984). On the other hand, a decrease in droplet size may inhibit droplet growth through collisional coagulation during warm-rain formation; this effect has an influence on the Earth’s cloud coverage through altering cloud lifetimes owing to the suppression of rain formation (Albrecht 1989).

Including the aerosol influence proved necessary in assessments of the Earth’s radiation balance and, consequently, the surface air temperature, not only in the future but also in the past. Simultaneously, researchers have become gradually more interested in changes in the precipitation amount through modification of cloud dynamical/microphysical structures by anthropogenic factors related to aerosol (Levin and Cotton 2008; Tao et al. 2012). Many numerical models have been developed competitively to represent aerosol–cloud interactions and their impacts on climate and weather phenomena on global and regional scales. In addition, remote and in situ measurements have been conducted worldwide to provide chances for modelers to justify their results. Satellite measurements have produced global projections of the distribution and characteristics of aerosol and clouds on the basis of measurements of their optical properties through spaceborne remote sensors (e.g., Nakajima et al. 2001; Rosenfeld et al. 2014). Continuous observations of aerosol by ground-based networks allow researchers to trace long-term transitions in their characteristics (e.g., Aerosol Robotic Network (AERONET) Holben et al. 1998; US Department of Energy (DOE), atmospheric radiation measurement (ARM) Stokes and Schwartz 1994). Many intensive field campaigns have also been conducted to produce comprehensive views of aerosol–cloud interaction by coupling observation results obtained from spaceborne satellites with ground-based, seaborne, and airborne instruments, as well as model simulations (e.g., INDian Ocean Experiment (INDOEX) Ramanathan et al. 2001; Asian Pacific Regional Aerosol Characterization Experiment (ACE–Asia) Huebert et al. 2003; Atmospheric Brown Clouds (ABC) Nakajima et al. 2007; Ramanathan et al. 2007; and Distributed Regional Aerosol Gridded Observation Networks (DRAGON) Eck et al. 2012).

Modeling approaches to aerosol and its activation in droplet nucleation

An essential physical process connecting aerosol with cloud is the nucleation of hydrometeor particles. All aerosol particles that can potentially be activated as nuclei of cloud droplets are referred to as condensation nuclei (CN). CCN are a subset of CN; they can be activated to initiate droplet formation at the low supersaturation observed in the troposphere. In contrast, ice-forming nuclei (IN) are defined as aerosol particles that act as the base of the deposition nucleation of cloud–ice particles or the heterogeneous freezing of supercooled droplets. At present, our knowledge of IN is less complete than that of CCN because of insufficient availability of measurements and experimental data to model the complicated ice-nucleation process (Pruppacher and Klett 1997).

A fundamental theory about CCN activation is summarized in a chart relating the relationship between the vapor saturation ratio and the equilibrium droplet size formed in CCN (Köhler 1936, Appendix 1). CN size distribution spectra, as well as ambient supersaturation and temperature, are essential factors in determining the droplet nucleation process. Several additional factors have a potential impact on the balance of the vapor saturation ratio and the equilibrium droplet size under more complex assumptions, other than the basic Köhler theory, such as changes in the amount of dissolving solutes in a droplet, temperature variations through latent heating/cooling by vapor condensation and evaporation, and the existence of insoluble and multiple soluble chemical components in impacted CN.

The question of how to numerically handle the two critical components (i.e., the size distribution spectra of aerosol particles and ambient supersaturation) is an important issue in the representation of the droplet nucleation process in cloud microphysics schemes. Existing approaches are generally categorized into the following four types, according to the temporal and spatial resolutions, and the aerosol representation in the models: (i) the use of supersaturation and aerosol size distribution spectra explicitly predicted for each spatial grid point; (ii) the use of parametrization involving predicted grid-scale supersaturation or updraft wind velocity, as well as the mass and/or number concentration of aerosol particles; (iii) the use of parametrization including the diagnosed maximum supersaturation or updraft wind velocity instead of predicted grid-scale values, as well as the mass and/or number concentration of aerosol particles; and (iv) the use of parametrization that implicitly assumes the presence of aerosol.

The first approach has been employed in a limited number of cloud-resolving models (CRMs) that aim at accurate calculation of cloud microphysics (e.g., Kogan 1991; Chen and Lamb 1994; Feingold et al. 1999; Khain et al. 2000; Geresdi and Rasmussen 2005; Lynn et al. 2005a; Kuba and Fujiyoshi 2006; Suzuki et al. 2006, 2010; Li et al. 2008; Shima et al. 2009; Misumi et al. 2010; Xue et al. 2010; Fan et al. 2012). The so-called sectional representation (e.g., Abdul-Razzak and Ghan 2002) is employed to numerically handle aerosol size distribution spectra in most of these models. Köhler theory is used to directly calculate the CCN number concentration and, consequently, the increased cloud droplet number concentration (CDNC) from the predicted aerosol size distribution spectra and supersaturation. Consumption of aerosol particles through the nucleation process is explicitly represented in the size distribution spectrum predicted. Miscellaneous aerosol types are often simplified to monotype CN to reduce the complexity. These CRMs sometimes lack a grid structure of full three-dimensional Cartesian coordinates, i.e., they may have only a two- or one-dimensional grid structure. Large computational resources are required to ensure sufficient accuracy to explicitly resolve aerosol size distribution spectra. In addition, very fine grid spacings in both time and space are required to represent minute variations in supersaturation. Such CRMs are generally employed to simulate idealized and simplified clouds to investigate the basic mechanisms of cloud and precipitation formation, and to discuss the sensitivity to various factors, including aerosol concentration. Typical size distribution forms of aerosol particles are often prescribed using reference measurement data.

The second approach is employed in high-resolution regional models that can be used for aerosol–cloud interaction studies based on idealized experiments or case studies. Generalized aerosol size distribution functions are usually assumed instead of their explicitly resolved spectra. The total or species-distinguished aerosol concentration is explicitly predicted in bulk-moment forms in some models (e.g., Hashino and Tripori 2007; Muhlbauer and Lohmann 2009; Onishi and Takahashi 2012; Saleeby and van den Heever 2013; Thompson and Eidhammer 2014), whereas the aerosol concentration is not predicted but tacitly parametrized in some models (e.g., Rasmussen et al. 2002; Seifert and Beheng 2006; Morrison and Grabowski 2007; Seiki and Nakajima 2014; Seiki et al. 2015). In most of these models, the activated CCN number concentration is parametrized on the basis of the basic Köhler theory, using the predicted supersaturation or vertical wind velocity. An empirical parametrization was suggested by Twomey (1959a, 1959b) to calculate the activated CCN number concentration from the predicted supersaturation or vertical wind velocity and prescribed coefficients representing the ambient aerosol loading. A more generalized parametrization was proposed by Abdul-Razzak et al. (1998), which combines Twomey’s parametrization with a lognormal representation of the aerosol size distribution (Ghan et al. 1993); these authors also extended the parameterization to cases including multiple externally mixed aerosol types (Abdul-Razzak and Ghan 2000). On the other hand, Saleeby and Cotton (2004) proposed the use of pre-calculated lookup tables through Lagrangian parcel model calculations instead of empirical parametrizations; aerosol size distribution spectra are explicitly represented using a sectional approach in the parcel model. The lookup tables are used to calculate the proportion of aerosol particles activated for droplet nucleation by referring to the vertical wind velocity predicted in their main model framework.

The third approach is used in most global or coarse-resolution regional models for studies of aerosol–cloud interactions, even on a climatic scale (e.g., Storelvmo et al. 2006, 2008; Lohmann et al. 2007; Morrison and Gettelman 2008; Suzuki et al. 2008; Takemura et al. 2009; Wang et al. 2011; Wang et al. 2013; Park et al. 2014; Shi et al. 2014). Supersaturation and the vertical wind velocity cannot be resolved well on model grid points with coarse intervals. Saturation adjustment approaches are necessarily employed in the calculation of phase changes between vapor and cloud water/ice. The approach used to introduce aerosol-to-cloud effects is significantly different among models according to the type of bulk cloud microphysics employed. Models using double-moment bulk cloud microphysics generally employ empirical parametrizations (e.g., Abdul-Razzak et al. 1998; Abdul-Razzak and Ghan 2000) to obtain the relationship between the aerosol number concentration and CDNC. Since the grid-scale vertical velocity is not a suitable input into the parametrizations, diagnostic variables (e.g., turbulent kinetic energy) are often included in modified parametrizations to determine the activated CCN number concentration through diagnosis of the maxima of the vertical wind velocity and supersaturation (e.g., Morrison et al. 2005). In contrast, single-moment bulk cloud microphysics cannot directly incorporate the activated CCN number concentration into the microphysics calculations in the form of a CDNC change. Diagnosed CDNC can be included in the calculation of the autoconversion rate from cloud to rain to represent the ambient CN effect on clouds (e.g., Liu and Daum 2004).

The fourth approach is adopted in model simulations on any scale. Since aerosol particles are necessary for the nucleation of cloud particles, the presence of aerosol particles is always assumed in cloud microphysics in a steady form. Explicit representation of aerosol and its effect on cloud may cause excess computational costs and uncertainties in regular operational runs for short-time weather forecasting. Speedy and stable simulation is important in these runs. Even coarse parametrizations based on empirical formulas work reasonably well for such short-time simulations where aerosol loading has little direct influence and minor feedback on the prognostic variables.

Solutions to the problem related to aerosol-to-cloud modeling

The best approach to accurately simulating aerosol-to-cloud effects is obviously the first option discussed in “Modeling approaches to aerosol and its activation in droplet nucleation”, i.e., using the explicitly predicted supersaturation and aerosol size distribution. However, predictions of the two components under realistic conditions are contradictory problems in a single-model framework because of scale gaps between aerosol and cloud. A small computational domain is preferable to define the grid spacing as finely as possible to represent minor variations in supersaturation. In contrast, a large computational domain is preferred to strictly predict transitions in the aerosol concentration and size distribution from sources of aerosol-particle formation. The limited capability of present computational resources places results in insufficient domain size and grid spacing in a single-model framework.

Several methods can be employed to solve the scale dilemma in aerosol-to-cloud modeling in the present computing environment. Thompson and Eidhammer (2014) used monthly aerosol climatology data as input into their Weather Research and Forecasting (WRF) model simulations (Skamarock et al. 2005). The aerosol climatology data were derived from multiannual global aerosol model simulations using the NASA Goddard Earth Observing System model coupled with the Goddard Chemistry Aerosol Radiation and Transport model (GEOS–GOCART, Ginoux et al. 2001; Chin et al. 2002; Colarco et al. 2010). The climatological data were composed of mass-mixing ratios of the five aerosol species with 0.5° × 1.25° horizontal grid spacing. The mass-mixing ratios were converted into two bulk number concentrations. One is the number concentration of simplified hygroscopic aerosol particles based on combining all aerosol species except for dust and black carbon. The second is that of simplified ice-nucleating particles based on the accumulation of dust particles with diameters larger than 0.5 μm. Both number concentrations were explicitly predicted in the WRF model simulations as tracers affected by interactions with hydrometeors and emission from the land surface. The predicted aerosol number concentrations were used in calculating the activation process of aerosol particles in the bulk cloud microphysics scheme. Aerosol activation (i.e., cloud droplet nucleation) was calculated using a method employing pre-calculated lookup tables (e.g., Saleeby and Cotton 2004). Cloud-ice nucleation and heterogeneous freezing of supercooled droplets were calculated using the parametrizations of Bigg (1953), Koop et al. (2000), Phillips et al. (2008), and DeMott et al. (2010).

Shi et al. (2014) used aerosol and chemical-transport model simulations as a tool to provide a realistically diagnosed aerosol field for their cloud microphysics calculation in the main model framework with the same domain configuration. They incorporated the following two individual models off-line: the GOCART solo-module version of the WRF coupled with chemistry (WRF–Chem; Grell et al. 2005), and the National Aeronautics and Space Administration (NASA) Unified WRF (NU–WRF; Peters-Lidard et al. 2015). The activated CCN number concentration in the NU–WRF simulation was diagnosed based on the air temperature and supersaturation on the NU–WRF side, and the mass concentration of multiple aerosol species on the WRF–Chem GOCART side. The diagnosed CCN number concentration was used to modulate the autoconversion rate from cloud to rain through CDNC diagnosis in the framework of the single-moment bulk cloud microphysics in the NU–WRF simulation.

Another compromise adopted to address this problem was suggested by Iguchi et al. (2008; hereafter IG08). Their approach was based on dynamical downscaling of realistic aerosol fields from large-scale aerosol (and chemical) transport model simulations to small-scale CRM simulations. The basic numerical framework of aerosol downscaling was similar to that of dynamical downscaling for standard prognostic variables such as wind velocity, temperature, and vapor-mixing ratio. Initial and time-variant aerosol boundary conditions were prepared using four-dimensional output from the large-scale simulation. However, aerosol size distribution spectra were incompletely resolved in the large-scale aerosol transport model. This deficiency might be problematic for accurate calculation of the activated CCN number concentration on the basis of Köhler theory on the CRM side. To deal with this problem in a reasonable manner, the authors proposed the use of an additional intermediate module. The intermediate aerosol loading module complemented the information of the aerosol size distribution spectra in the dynamical downscaling framework. The aerosol size distribution spectra and their total number/mass concentrations should be as realistic as possible, such as those observed at times and locations pertaining to the simulations.

The objective of this review is to summarize our development activities and prospective update strategies for the aerosol loading interface since the publication of IG08. The interface connects small-scale CRM simulations to large-scale aerosol transport simulations in a dynamical downscaling framework and complements information about aerosol size distribution spectra. This interface is currently undergoing development in order to couple it with regional models, including a detailed cloud microphysical scheme, referred to as spectral-bin microphysics (SBM; e.g., Khain et al. 2015). Since this paper aims at reviewing the aerosol loading interface in detail, detailed descriptions of SBM are not included. Such descriptions can be found in Khain et al. (2000, 2015), among others.

Description of ALICIS

Brief overview

Our aerosol loading module is referred to as the Aerosol Loading Interface for Cloud microphysics In Simulation (ALICIS). Figure 1 provides a schematic illustration of how ALICIS works as an intermediate module between large-scale aerosol transport models and regional-scale CRMs. So far, this interface has been employed in the framework connecting global-scale simulations using the spectral radiation transport model for aerosol species (SPRINTARS; e.g., Takemura et al. 2000) with regional-scale simulations using the Japan Meteorological Agency Non-Hydrostatic Model (JMA–NHM; Saito et al. 2006) coupled with SBM (IG08). The SBM scheme originates from the corresponding part of the Hebrew University Cloud Model (HUCM; e.g., Khain et al. 2000). ALICIS was first published by IG08 and subsequently updated by Sato et al. (2012; hereafter SA12) and Choi et al. (2014; hereafter CH14).
Fig. 1

Conceptual diagram of the coupling framework between a large-scale aerosol transport model and a regional-scale cloud resolving model using the ALICIS module. Gray components have not yet been implemented but will be included in future updates

CN modeling in the original HUCM

The representation of aerosol in the original HUCM is significantly simplified for idealized CRM simulations (e.g., Khain et al. 1999). The CN size distribution spectrum for a single chemical component is calculated as prognostic variables for each of the model’s spatial grid points. The chemical composition of CN is assumed to consist of pure ammonium sulfate. The CN particle shape is assumed to be completely spherical. The size distribution spectrum is approximated by 33 discrete size bins, covering a particle radius ranging from 1.23 × 10−3 to 2 μm. The representative particle radius of each CN size bin is defined as follows. The CN particle mass of the maximum size bin (i.e., the 33rd bin) is assumed to be identical to the particle mass of the smallest droplet size bin; the smallest droplet radius is assumed to be 2 μm. The CN particle mass of each size bin is determined by doubling the mass bins; that is, a series of CN bins are characterized in the form of a geometric progression of particle masses with a ratio of 2 between subsequent bins. The CN particle radius of each size bin is tied to the particle mass of the bin and the CN particle density.

The initial CN size distribution spectrum in the HUCM is determined using the Köhler equation (Eq. 11) and Twomey’s empirical parametrization described by N CCN = N 0 S k . Here, N CCN is the number concentration of CCN activated at supersaturation S, and N 0 and k are environment-dependent coefficients (e.g., Twomey 1959a, 1959b). The following equation for the CN number density function can be obtained by coupling both equations (Khain et al. 2000):
$$ \frac{\mathrm{d}{N}_{\mathrm{CN}}}{\mathrm{d}\left( ln{r}_{\mathrm{CN}}\right)}=1.5{N}_0k{\left(\frac{4{A}^3}{27B{r}_{\mathrm{CN}}}\right)}^{1.5k}, $$

where A and B are calculated from Eq. 8 for a temperature of 288.15 K, and the molecular weight, the van ’t Hoff factor, and the CN particle density are identical to those of a typical ammonium sulfate aerosol particle. The spectral shape of the initial CN size distribution is common to all spatial model grid points. The initial spatial distribution is vertically inhomogeneous, since the CN number density function decreases exponentially with a scale height of 2 km above an altitude of 2 km (Khain and Sednev 1996). CN particles with radii larger than 0.6 μm are eliminated from the size distribution spectrum in standard simulations to prevent artificially rapid formation of large droplets at the initial simulation stage.

The governing equation of the number density concentration in each CN bin (Eq. 3.4 of Khain and Sednev 1996) is calculated numerically for all model grid points and each time step. Gravitational sedimentation of CN particles is neglected. CN production in the atmosphere or on the terrain surface is ignored. No direct CN source term is assumed. The CN sink is limited to consumption through the droplet nucleation process. Scattering and absorption of short- and longwave radiative fluxes by CN particles are not included, because no radiation process is calculated in the HUCM. A flat horizontal gradient of the CN number density concentration is assumed at the model’s lateral boundaries; the CN size distribution spectra are thus horizontally constant near the lateral boundaries. Consequently, CN consumed within the simulation domain is replenished by advection from the lateral boundaries.

The microphysical process of CN is limited to activation of droplet nucleation. The process is calculated on the basis of the following approach. If the predicted supersaturation at a grid point is positive, the critical radius of CCN is calculated based on Eq. 11 using supersaturation and the air temperature. All CN larger than the critical radius are immediately activated and converted into cloud droplets, with their corresponding radii calculated using Eq. 10. Hygroscopic growth of CN is neglected.

An early version of ALICIS: Iguchi et al. (2008)

Recently, regional models using SBM have been widely applied, even to realistic simulations resolving clouds. However, most studies have employed a similarly coarse approach to the CN representation (Lynn et al. 2005a, 2005b; Khain et al. 2010; Fan et al. 2012; Iguchi et al. 2012a, 2012b, 2014). Such an approach may be insufficient in realistic simulations, because in reality, the spatial distribution of aerosol particles is inhomogeneous and variable. The environment-dependent parameters in Eq. 1, N 0 and k, are determined on the basis of limited reference observations (Pruppacher and Klett 1997). Substitution of arbitrary values for those parameters causes large uncertainties in determining the CN concentration and size distribution spectra that should be consistent with their real counterparts. In particular, the uncertainties may be increased under conditions where anthropogenic pollution has a large impact on the aerosol distribution. Aerosol–cloud interaction is of great interest as a research problem under such conditions. In addition, the simplified vertical CN distribution may be problematic. The vertical CN profile assumed in the HUCM is based on a typical observed profile of the vertical aerosol distribution. However, severe aerosol contamination is sometimes observed even in the middle troposphere (Marenco et al. 2014); such highly concentrated aerosol is transported from distant intensive sources through lifting by convection and it even has a significant impact on the local cloud properties as well as on the radiation balance.

IG08 developed the aerosol loading module ALICIS to overcome the deficiencies in CN modeling associated with the original HUCM. The module provides inhomogeneous initial CN and time-variant lateral boundary conditions with a specified particle-size distribution through a dynamical downscaling approach using output from global aerosol transport simulations of SPRINTARS (e.g., Takemura et al. 2000). The SPRINTARS model includes the five types of tropospheric aerosol, i.e., organic carbonaceous, black carbonaceous, soil dust, sulfate, and sea salt. Aerosol mass-mixing ratios are predicted in the framework of the atmospheric general circulation model (AGCM). Aerosol particle size spectra are incompletely resolved in SPRINTARS.

Aerosol transport simulations using the SPRINTARS model have been validated in various ways. For example, the simulated aerosol optical thickness and Ångström exponents have been compared with those retrieved from the space-borne Advanced Very High Resolution Radiometer (AVHRR) measurements on a global scale (Takemura et al. 2000); these authors also evaluated the surface aerosol concentration at multiple global locations by comparison with those estimated from optical measurements of the AERONET network. The single-scattering albedo of simulated aerosol was also validated using AERONET data (Takemura et al. 2002). An aerosol data assimilation system has been developed on the basis of a four-dimensional variational data assimilation method (Yumimoto and Takemura 2013). The vertical aerosol distribution was validated through a comparison of the aerosol extinction with lidar measurements at several locations in Japan (Goto et al. 2015). In addition, the SPRINTARS model is included in the Aerosol Comparisons between Observations and Models (AEROCOM) project (e.g., Kinne et al. 2006). Model performance has been evaluated by comparing the global modeling outcomes of numerous aerosol modules.

IG08 determined the CN size distribution spectrum of the initial and time-variant lateral boundary conditions in their nested model simulations through the following process. Among the five types of tropospheric aerosol, organic carbonaceous, sulfate, and sea salt aerosol particles are assumed to be CN activatable as CCN. Bulk number concentrations of the three types of aerosol in SPRINTARS are calculated based on the predicted mass-mixing ratios for the grid points of the global simulation under the assumption that all aerosol particles are dry. The calculated bulk number concentrations are then temporally and spatially interpolated at the grid points of the simulation domain of the nested model. The interpolated bulk number concentrations are converted into aerosol size distribution spectra at each grid point. The conversion employs different built-in size distribution functions, according to aerosol type. Finally, accumulating the three-type aerosol size spectra yields the CN size distribution spectrum at a given grid point for the initial and boundary conditions.

The particle size distribution of organic carbonaceous aerosol is assumed to be a lognormal function with a single mode. The corresponding fraction of organic carbonaceous aerosol in the CN size distribution spectrum is given in units of the number density concentration,
$$ \frac{\mathrm{d}{N}_{\mathrm{CN}\left(\mathrm{O}\mathrm{C}\right)}}{\mathrm{d}\left( ln{r}_{\mathrm{CN}}\right)}=\frac{N_{\mathrm{b}\left(\mathrm{O}\mathrm{C}\right)}}{\sqrt{2\pi }{\sigma}_{\mathrm{OC}}} exp\left[-\frac{1}{2}{\left\{\frac{ln\left({B}_{\mathrm{CN}}^{1/3}/{B}_{\mathrm{OC}}^{1/3}\cdot {r}_{\mathrm{CN}}/{r}_{\mathrm{m}\left(\mathrm{O}\mathrm{C}\right)}\right)}{\sigma_{\mathrm{OC}}}\right\}}^2\right], $$

where N b is the bulk aerosol number concentration of the SPRINTARS simulation, and r m and σ are the mode radius and the standard deviation of the lognormal aerosol size distribution, respectively. The subscripts, CN and OC, distinguish the variables pertaining to CN and organic carbonaceous aerosol, respectively; r m(OC) = 0.1 μm and σ OC = 1.8 is assumed. Note that Eq. 2 applies the adjustment of the difference in the B coefficients (Eq. 8) between organic carbonaceous aerosol and CN with a certain soluble component.

Sulfate aerosol is also assumed to have a single-mode lognormal particle size distribution. The corresponding portion of the sulfate aerosol in the CN size distribution spectrum is also given by Eq. 2 in units of the number density concentration, but for parameters typical of sulfate aerosol; r m  = 0.0695 μm and σ = 2.03 is assumed.

The particle size distribution function of sea salt aerosol is assumed to be a power law. The corresponding fraction of sea salt aerosol in the CN number density concentration is given by
$$ \frac{\mathrm{d}{N}_{\mathrm{CN}\left(\mathrm{S}\mathrm{A}\right)}}{\mathrm{d}\left( ln{r}_{\mathrm{CN}}\right)}=1.5{N}_{\mathrm{b}\left(\mathrm{S}\mathrm{A}\right)}k{\left(\frac{B_{\mathrm{SA}}}{B_{\mathrm{CN}}}\frac{r_{\mathrm{m}\left(\mathrm{S}\mathrm{A}\right)}}{r_{\mathrm{CN}}^3}\right)}^k, $$

where r m(SA) = 0.1 μm and k = 0.6 is assumed. The subscript SA denotes sea salt aerosol. This equation also includes adjustment of the difference in the B coefficient between CN and sea salt aerosol.

In the version of ALICIS presented here, the CN size spectrum is discretely approximated by 13 size bins with a radius ranging from 10−3 to 1 μm. The use of a small number of CN bins compared with the 33 bins in the original HUCM yields improved computational efficiency. The CN concentration in each bin is numerically computed every time step, using almost the same governing equations as the standard scalar tracers.

The chemical component of CN in the nested model can be arbitrarily determined by substituting a proper, corresponding value into the B coefficient of CN in the conversion equations (Eqs. 2 and 3). No microphysical processes causing a change in the CN size spectra are assumed, except for activation to droplet nucleation. Droplet nucleation is calculated using the same approach as that employed in the original HUCM; the value of the B coefficient of CN in Eqs. 2 and 3 is substituted into Eqs. 10 and 11 to determine the critical CCN radius and the corresponding radius of the generated cloud droplet. Although atmospheric radiation is calculated in the nested model, absorption and scattering of the radiative fluxes by CN are not included at present. The reason for this is that the optical properties of each aerosol species are eliminated once the multiple aerosol types have been bundled into standardized CN. In addition, the other two types of aerosol (i.e., black carbonaceous and dust aerosol) are not included in the nested model, so that this version of ALICIS has a limited capability to simulate direct aerosol effects on atmospheric radiation.

IG08 demonstrated the validity and effectiveness of the aerosol loading module in model simulations of two precipitation events observed during the 3rd Experiment of the Asian Atmospheric Particulate Environment Change Studies (APEX–E3). First, vertical profiles of the CCN number concentration in the nested model simulations were evaluated in direct comparison with those acquired by aircraft in situ measurements. The measurement methods of the CCN number concentration using a CCN counter were summarized by Ishizaka (2004) and Adhikari et al. (2005); some additional detailed information about the measurements on the event days can also be found in IG08. Figure 2 compares the results for the two individual cases. The simulations reproduced the observed CCN concentration profiles reasonably well. In the April 2 case (Fig. 2a), the observed CCN concentration ranged from approximately several tens to close to 1000/cm3. The observed concentration decreased a little with increasing altitude. The three-type simulated CCN concentrations ranged from approximately 100 to 1000 cm−3 at heights of up to 5500 m; the small decrease with increasing altitude was generally reproduced. In the April 8 case (Fig. 2b), the observed CCN concentration was approximately 1000 cm−3 at heights below 1000 m, which decreased with increasing altitude to roughly 100 cm−3 at 3000 m. The vertical profiles of the simulated CCN concentrations showed a log-linear decrease with increasing altitude, similar to the observed profile.
Fig. 2

Vertical distribution of the observed and simulated CCN number concentrations over the East China Sea on a April 2, 2003 and b April 8, 2003. The observed CCN number concentration in the flight measurements was obtained for liquid-phase supersaturation ranges of 0.07–0.22 % on April 2 and 0.09–0.32 % on April 8. The simulated CCN number concentration in the regional model was calculated for a liquid-phase supersaturation of 0.1 % in the April 2 case and 0.2 % in the April 8 case. Lines of simulated concentration show vertical profiles of horizontal averages in three domains of radius ±0.5° centered at 129.5° E and 30.5° N, 31.5° N, or 32.5° N. The two types of simulated concentration are plotted separately from the control and cloud-free runs (where all cloud microphysical processes were switched off to prevent CN consumption through droplet nucleation). Adapted from Iguchi et al. (2008)

Second, the horizontal distribution of the liquid cloud properties in the nested model simulations was compared with that estimated from data of the Modulate Resolution Imaging Spectroradiometer on the Terra satellite (Terra/MODIS) based on the satellite’s retrieval algorithm (Nakajima and Nakajima 1995; Nakajima et al. 2005); plots of the horizontal distribution are shown in Fig. 6 of IG08. Figure 3 shows the relationship between the liquid cloud-top temperature and the droplets’ effective radius near the cloud tops in the satellite measurements and the simulation for the April 2 case. These parameters were averaged separately in the northern and southern halves of the simulation domain to highlight spatial differences in the droplet radius distribution. The north–south difference is likely to have resulted from a horizontal bias in the CN concentration. The model simulation performed satisfactorily in reproducing the overall tendency of the north–south gradients of the observed droplet radius in warm-cloud regimes with temperatures in excess of 273 K, despite some overestimation (Fig. 3a). The observed radius monotonously increased with decreasing cloud-top temperature. The observed radii averaged in the northern half had larger values than those in the southern half; the maximum north–south difference was roughly 5 μm. The simulated radius generally increased with decreasing cloud-top temperature down to 275 K and roughly decreased or remained constant below 275 K. The simulated radii in the northern half attained larger values than those in the southern half for temperatures greater than 275 K; the north–south difference was roughly 5 μm on average. In addition, two sensitivity simulations were conducted to highlight the effects of the aerosol loading module on the simulation results (Fig. 3b, c). The simulation assuming horizontally homogeneous initial and boundary CN conditions failed to reproduce the structure of the north–south gradients (Fig. 3b). The simulated profiles of the average droplet effective radius are almost identical for the northern and southern halves. The simulated north–south gradients in the control run were thus caused by a horizontally inhomogeneous CN distribution introduced by aerosol downscaling. This result proved that the implementation of realistic, inhomogeneous CN fields is essential for more accurate simulations of cloud microphysical properties. On the other hand, the simulation assuming a doubled CN number concentration compared with the control run had smaller effective radii (Fig. 3c). The simulated effective radius profiles were in better agreement with the observed profiles than those in the control run. This result indicates that the control run underestimated the CCN number concentration.
Fig. 3

Dependence of droplet effective radii near cloud tops on cloud-top temperature calculated based on simulations with three different settings and from the retrieval results derived from Terra/MODIS measurements over the East China Sea on April 2, 2003. Simulation profiles are calculated in a the control run, b the run characterized by a homogenous CN field, and c the run with doubled CN. Plotted radii are averaged individually in the northern and southern halves of the analysis domain. Adapted from Iguchi et al. (2008)

Update by Choi et al. (2014): Aerosol particle size distribution revision and type multiplication

The IG08 version of ALICIS still contained many limitations. Among them was the absence of two aerosol species, i.e., black carbonaceous aerosol and dust particles. In reality, they often work as CCN if soluble components are combined with the particles, either externally or internally (e.g., Sullivan et al. 2009). In addition, the modeling of the other three types of aerosol still offered room for significant improvements. For example, the application of a power-law function to the size distribution spectra of sea salt aerosol might cause an overestimation of the activated CCN number concentration because of the continuous increase in the CCN number concentration with increasing supersaturation.

The aerosol loading module was comprehensively updated by CH14. The conversion from the various types of aerosol to standardized CN, as implemented by IG08, has been removed. The same five aerosol species used in the SPRINTARS model are employed in nested models. The discretization of the size distribution spectra of each aerosol type has been extended to 17 size bins with radii ranging from 10−3 to 10 μm. The use of more size bins and a wider range of particle sizes compared with those in the old version allows the representation of aerosol particles with radii larger than 1 μm. Such large aerosol particles are possibly included in the sea salt and dust aerosol categories (Fig. 4).
Fig. 4

Size distribution spectra of the five aerosol species, i.e., a sulfate, b dust, c sea salt, d organic carbon, and e black carbon, assumed in the updated and outdated ALICIS modules, and obtained from in situ measurements during ACE–Asia 2001 and ABC–EAREX 2005. Cited from Choi et al. (2014)

The size distribution function of each aerosol type was assumed to be of a multi-modal lognormal form by CH14. The size distribution spectra described in this manner are consistent with those observed in reality (e.g., Brechtel et al. 1998). The number density concentration of the size distribution of each aerosol type is given by
$$ \frac{\mathrm{d}N}{\mathrm{d}\left( ln{r}_a\right)}={\displaystyle \sum_{i=1}^{n_{\mathrm{m}}}\frac{N_{\mathrm{SPR}}{f}_i}{\sqrt{2\pi }{\sigma}_i}} exp\left(-\frac{ln{r}_a- ln{r}_{mi}}{2{\sigma_i}^2}\right), $$

where r a is the aerosol particle radius, i the index of a given mode, n m the total number of modes in the size distribution, N SPR the bulk number concentration of each aerosol type obtained from the SPRINTARS simulation, and f the weight factor required to normalize the multi-modal distribution. The variables n m, f, r m, and σ are the functions of aerosol type as listed in Table 1 of CH14; the values have been determined on the basis of observational results (d’Almeida et al. 1991; Chuang et al. 1997; Penner et al. 1998; Herzog et al. 2004).

Figure 4 compares the aerosol size distribution spectra. Two size distribution spectra were calculated for each aerosol type using the assumptions employed by CH14 and IG08. No size distribution was assumed for dust or black carbonaceous aerosol in the study by IG08. A set of observed spectra was obtained from in situ measurements during the ACE–Asia field campaign in 2001 (Huebert et al. 2003). The set of spectra was calculated from the size-segmented aerosol mass concentration measured using the Micro-Orifice Uniform Deposit Impactor (MOUDI) onboard a research vessel; the marine aerosol sampling performed during ACE–Asia 2001 is summarized by Mochida et al. (2007). Another set of observed spectra was obtained from ground-based measurements using MOUDI at the Gosan site on Jeju Island (Republic of Korea) during the Atmospheric Brown Cloud–East Asian Regional Experiment (ABC–EAREX) in 2005 (Nakajima et al. 2007).

In Fig. 4, the size distribution spectra employed by CH14 are in better agreement with those from the measurements, although the observed size spectra lack multi-modal distributions. The observed aerosol number densities monotonously decrease with increasing aerosol particle size. The observed size distributions of sulfate and organic/black carbonaceous aerosol extend to the radii of 2 μm, whereas those of dust and sea salt aerosol extend to over 5 μm. The spectra of CH14 reproduce the distinct structure of the observed spectra according to aerosol type reasonably well, especially those of sulfate and organic/black carbonaceous aerosol. In contrast, the spectra of IG08 exhibit several severe insufficiencies. The number density concentration of sulfate aerosol is overestimated across the full particle size range shown and the sea salt aerosol concentration is significantly underestimated. The organic carbonaceous aerosol concentration is underestimated for particle radii smaller than 0.1 μm and overestimated for radii larger than 0.4 μm.

The activation process of aerosol particles to form cloud droplets was calculated for each aerosol type on the basis of basic Köhler theory by CH14, unlike in IG08. Because the five types of aerosol have different soluble capabilities, different B coefficients are employed in determining the critical radius of CCN in Eq. 11. The B coefficients are assumed to be 0.51 for sulfate, 1.16 for sea salt, 0.14 for dust, 0.14 for organic carbonaceous, and 0.05 × 10−5 for black carbonaceous aerosol (Ghan et al. 2001).

CH14 employed the same build-up process of initial and time-variant boundary conditions of binned aerosol concentrations in their nested model simulations as IG08. The time evolution of each binned concentration was numerically computed for each time step. Microphysical processes producing or losing aerosol particles were excluded, except for consumption through the nucleation of cloud droplets. Any direct aerosol effects on atmospheric radiation were excluded, even by CH14, although the five types of aerosol were fully managed.

CH14 evaluated the performance of the updated version of the aerosol loading module in their simulation analysis. They conducted numerical simulations of two cloudy cases observed during the ABC–EAREX 2005 field campaign over an East China Sea region. Corresponding simulations using the old version of the aerosol loading module of IG08 were performed simultaneously for comparison.

First, the simulated CN and CCN number concentrations were evaluated in comparison with those obtained from ground-based measurements. The CN comparison yielded a new perspective on the validation of ALICIS, in addition to the CCN comparison also discussed by IG08. Figure 5 compares the concentrations (CCN at 0.6 % supersaturation) derived from the different assumptions made by both IG08 and CH14 with those obtained from in situ measurements at the Gosan site. The observed CN and CCN concentrations were measured using a TSI (Shoreview, MN, USA) condensation particle counter model 3010, which detected particles with diameters larger than 10 nm, and using a stream-wise thermal-gradient CCN counter (Roberts and Nenes 2005); details of the measurements can be found in Yum et al. (2007). The large underestimation of the number concentrations in the outdated IG08 version has been alleviated in the updated CH14 version. The improvement is attributed to the application of more realistic distribution functions to the aerosol size spectra rather than the new inclusion of dust and black carbonaceous aerosol into the categories. However, underestimation of CN and CCN concentrations still remained in the simulations using the updated CH14 version, especially for the second case. This insufficiency is probably caused by an underestimation of the aerosol concentration in the SPRINTARS simulation over highly polluted regions affected by anthropogenic aerosol emissions.
Fig. 5

Surface-level a CN and b CCN (at 0.6 % liquid-phase supersaturation) number concentrations simulated near the ABC–EAREX 2005 Gosan site and measured at the site on March 13, 2005 (case 1) and March 25, 2005 (case 2). Green bars show number concentrations in a regional model simulation using the ALICIS module based on Iguchi et al. (2008); the concentrations are calculated at grid points near the site (averaged within an area of 126.0° E–126.4° E and 33.1° N–33.5° N at the model bottom level) for the initial time step of the simulation. Error bars show standard deviations from the averages. Red bars show the same concentrations but using assumptions proposed by Choi et al. (2014). Observed CN and CCN were measured simultaneously using a TSI condensation particle counter and a stream-wise thermal gradient CCN counter deployed at the Gosan site, respectively

Second, CH14 evaluated droplet effective radii near cloud tops, liquid water paths, and cloud optical thicknesses calculated in their simulations in comparison with those obtained from the Terra/MODIS satellite measurements through retrieval (see Table 2 in CH14); details of the retrieval algorithm are described by Nakajima et al. (2005). Simulations using the updated and outdated aerosol loading modules led to different values of the variables, although the cloud distribution patterns were similar. The droplet effective radii were smaller, and the liquid water paths and cloud optical thicknesses were larger in the updated simulation compared with the outdated simulation. These differences resulted from larger CDNC attributed to the larger CN and CCN number concentrations. Overall, the values in the updated simulation were in better agreement with those estimated from the satellite measurements, reflecting the better reproduction of the CN and CCN concentrations in the updated version.

Update by Sato et al. (2012): Aerosol emission from evaporated cloud droplets

SA12 introduced an aerosol particle generation process from completely evaporated droplets into the framework of the HUCM SBM, coupled with the ALICIS module. Absence of an aerosol regeneration process might cause underestimation of the CN and CCN number concentrations and, consequently, an underestimation of CDNC, particularly in long-term simulations. The process was not included in the original HUCM SBM, and was not considered by IG08 or CH14, mostly because of the following technical issue. Once the activation to droplet nucleation has been calculated in the models, the size and composition information about the aerosol particles used was eliminated. Some state-of-the-art models fully predict solute components in hydrometeor particles at the expense of increased computational cost (e.g., Chen and Lamb 1994). Such models have the advantage of enabling explicit calculations of aerosol particle emission from completely evaporated or sublimated hydrometeor particles.

The parametrization of the aerosol emission process by SA12 was based on the third approach described by Feingold et al. (1996). SA12 assumed that one aerosol particle was regenerated when one droplet had completely evaporated (Mitra et al. 1992). Solute components in the droplet were not fully predicted, so that the sizes of regenerated aerosol particles could not be calculated explicitly; alternatively, the size distribution spectrum of the regenerated aerosol was determined based on the change of the domain-averaged aerosol number concentration from the initial condition to the present time step. The additional aerosol number concentration to the k-th aerosol size bin resulting from this regeneration process (R k) is as follows (see Eqs. 3 and 4 in Feingold et al. 1996):
$$ {R}_{\mathrm{k}}={N}_{\mathrm{R}}\frac{\phi_k}{{\displaystyle \sum_{k=1}^{n_{\mathrm{bin}}}{\phi}_k}}; $$
$$ {\phi}_k=\frac{{\overline{N}}_{0,\mathrm{k}}-{\overline{N}}_{\mathrm{k}}}{{\overline{N}}_{0,\mathrm{k}}}, $$

where N R is the total number concentration of the regenerated aerosol particles, which is equivalent to the number concentration of completely evaporated droplets; n bin is the total number of aerosol size bins; and \( {\overline{N}}_{0,\mathrm{k}} \) and \( {\overline{N}}_{\mathrm{k}} \) are the domain-averaged aerosol number concentrations of the k-th size bin in the initial and present conditions, respectively. SA12 assumed that all CN were composed of ammonium sulfate; therefore, the chemical component of aerosol particles generated through this emission process was assumed to be ammonium sulfate.

SA12 evaluated the performance of the aerosol regeneration parametrization in their simulations by resolving stratocumulus over a region off the coast of California. Two types of simulation (i.e., with and without the regeneration parametrization) were conducted simultaneously to investigate the influence of this process. The simulation results were validated using retrieval results from the space-borne AVHRR/2 data over the region of interest (Nakajima and Nakajima 1995).

Figure 6 shows the horizontal distribution of the cloud optical thickness retrieved from the AVHRR/2 space-borne measurements (Nakajima and Nakajima 1995) and calculated in the regional model simulations excluding or including the aerosol regeneration process. Cloud optical thickness ranged from 10 to 60 over the domain of interest in the observation region. The southern half of the domain exhibited relatively thick stratocumulus. In contrast, the simulated cloud fields show a more dispersed structure. Cloud optical thicknesses simulated with the aerosol regeneration parametrization were at least in better agreement with the satellite measurements than those not based on this parameterization. Large optical thicknesses of more than 30 are patchily and widely distributed in the simulation including the regeneration process, whereas the corresponding values were less than 20 in the simulation without the regeneration process, except for areas that were close to a lateral boundary of the simulation. Implementation of the aerosol regeneration process caused an increase of approximately 20 % in the aerosol number concentration averaged over the domain. A large fraction of aerosol particles emitted from evaporated droplets was used again as CCN. The regeneration of aerosol particles caused increased CDNC and cloud optical thickness.
Fig. 6

Horizontal distribution of cloud optical thickness observed at 1500 UTC on July 10, 1987: a retrieved from the space-borne AVHRR/2 measurement results, b simulated by the regional model without aerosol regeneration parametrization (CTL-run) at 1400 UTC on the same day, and c with regeneration parameterization (RGN-run). The red rectangle in the top panel shows the model simulation domain

Sato (2012) tested another approach used by Feingold et al. (1996) for the aerosol regeneration process, because the parametrization based on Eq. 5 was not very appropriate for downscaled realistic simulations. The new approach assumed that the particle size distribution of regenerated aerosol was the same as the horizontal average at the corresponding vertical level for the initial conditions. Sato’s (2012) tests using this approach showed that the reproducibility of cloud optical thickness was improved as well.

SA12 also conducted a quantitative comparison on the basis of correlation analysis between the droplet effective radii and cloud optical thicknesses (e.g., Fig. 8 of SA12). Only simulations including the aerosol regeneration parametrization reproduced a characteristic pattern in the correlation plots based on the satellite measurements. Their results demonstrate that implementation of the aerosol regeneration process is necessary to adequately simulate the cloud microphysical structure of stratocumulus over the region of interest.

Prospective ALICIS update strategy

IN modeling

The behavior of aerosol particles as IN is implicitly included in the framework of the HUCM SBM tied to the present ALICIS module. The IN effect is tacitly contained in parametrizations to calculate ice-nucleation and freezing processes without consumption of predicted aerosol particles in the model. This coarse approach is due to the present poor knowledge about complicated microphysics in ice/mixed-phase clouds. Nevertheless, introducing an explicit representation of IN activation and the resultant depletion is important for developing a more comprehensive scheme of cloud microphysics for aerosol–cloud interaction studies. Improvement of the SBM and ALICIS to manage the IN effect is a worthwhile challenge.

Solid hydrometeor particles in the atmosphere primarily form through either homogenous freezing of supercooled droplets without IN action or heterogeneous nucleation/freezing with catalysis by IN. In addition, the latter heterogeneous processes can be divided into four different categories (Vali 1985): deposition nucleation, condensation-freezing nucleation, contact freezing, and immersion freezing.

Deposition nucleation is completed when water vapor directly deposits onto the surface of an aerosol particle, provided that supersaturation with respect to ice is positive. The aerosol particle does not have to be hydroscopic. On the other hand, condensation-freezing nucleation originates from the nucleation process of a droplet under the condition that supersaturation with respect to water is positive. The aerosol particle is activated as CCN but does not have to completely dissolve in the droplet. The droplet that is formed then immediately freezes from the non-dissolved impurity. Distinguishing these two types of nucleation process is difficult in measurements where supersaturation with respect to water is positive. Supersaturation (i.e., humidity) rather than temperature is an important factor controlling the progress of these processes. Contact freezing possibly occurs when supercooled droplets collide with aerosol particles. The collision is usually caused by Brownian diffusion, thermophoresis, diffusiophoresis, electrophoresis, and/or inertial impaction. The concentration of aerosol particles that can act as contact-freezing IN at the relevant temperature is the most important factor in determining the freezing probability. Immersion freezing originates from impurities already present inside a supercooled droplet. Unlike condensation-freezing nucleation, immersion freezing does not have to start immediately upon the formation of a supercooled droplet. The freezing can occur when the temperature of the supercooled droplet decreases.

Among the four types of heterogeneous cloud glaciation processes, deposition nucleation is the simplest because the process does not proceed through a state of supercooled droplets. An increase in the number of aerosol particles that can work as deposition IN directly causes the number of ice cloud particles to increase, just like the relationship between CCN and cloud droplets. In contrast, cloud glaciation through the other three processes is more complicated. If the number concentrations of all types of aerosol increase, promotion of heterogeneous freezing through increasing IN may be in competition with depression of the freezing efficiency caused by a decrease in the particle sizes of supercooled droplets through increasing CDNC. In contrast, increased cloud height and decreased cloud temperature caused by the particle size change of supercooled droplets (e.g., Pincus and Baker 1994) may accelerate cloud glaciation through heterogeneous or homogenous freezing.

Unlike droplet nucleation summarized in Köhler theory, no comprehensive theory has been developed to formulate each ice-nucleation or freezing process. Parametrizations of these processes are constructed empirically on the basis of in situ measurement data or experimental laboratory data acquired under certain conditions. The four types of mechanisms of heterogeneous nucleation/freezing can rarely be distinguished through measurements or experiments, so that empirical parametrization may cover multiple components for each of the four types of the mechanisms. In addition, identifying the chemical components of IN is difficult for most measurements.

Appendix 2 summarizes our testbed for how to improve IN parametrization in the HUCM SBM coupled with the ALICIS module. Fan et al. (2014) improved the ice-nucleation parts of the HUCM SBM by introducing up-to-date IN parametrizations that include prognostic dust aerosol concentrations. The parametrizations were based on results by Tobo et al. (2013) and DeMott et al. (2015) for deposition/condensation-freezing nucleation and immersion freezing, and by Muhlbauer and Lohmann (2009) for contact freezing. We may modify the parametrizations into suitable forms to use the aerosol size distribution spectra predicted by models coupled with the ALICIS module. In addition, more comprehensive and generalized parametrizations of heterogeneous ice-nucleation/freezing should be implemented in future updates. Phillips et al. (2008, 2013) proposed a flexible framework where various empirical parametrizations can be bundled into a versatile form since parameters in the formulation can be easily constrained by various observational data. Note that the application of any proposed parametrizations to actual model simulations is still affected by large uncertainties. The uncertainties come from the limited applicability of findings from in situ measurement and laboratory experiment results for IN, and the coarse translation from results to developer-friendly parametrizations in a numerical scheme.

Introduction of regional variability into the aerosol size distribution and hygroscopicity parameters

The present ALICIS module includes fixed aerosol size distribution functions with constant parameters, as described in “An early version of ALICIS: Iguchi et al. (2008)”. The size distribution spectra were validated for application to simulations of regions in Northeast Asia through comparisons with those obtained from on-site measurements. The spectra might thus be inappropriate if applied to simulations pertaining to other regions. For example, mineral dust aerosol particles in East Asia and North Africa (Sahara) have different physical and chemical properties (Formenti et al. 2011). The dust properties depend not only on the source region but also on the distance from the emission site.

We will introduce regional variability into the aerosol size distribution functions and the hygroscopicity parameters assumed in the ALICIS module. First, these functions and parameters should have different forms and values in accordance with the type of simulation region, e.g., continental, coastal, or maritime. For example, the parameters determining the particle size distribution of sulfate aerosol used by CH14 originate from those for maritime scenes from Chuang et al. (1997). The latter authors assumed a bimodal function with different parameter values for continental regions instead of the trimodal function employed for maritime scenes. An average of the two size spectrum forms can also be used for intermediate (i.e., coastal) scenes.

Second, introducing intercontinental variability into the ALICIS module is a valuable challenge for further improvement. Although many measurements of the aerosol size distribution have been conducted worldwide, most obtained a bulk aerosol size distribution containing all chemical components. Internal mixing of aerosol particles is highly problematic in constraining the aerosol size distribution of an individual chemical component in relation to the measurement data. Few recent studies have conducted global simulations using an aerosol transport model predicting the aerosol size distribution (e.g., Spracklen et al. 2005; Zhang et al. 2010; Jacobson 2012). These simulation results are useful for complementary provision of aerosol size distribution information, particularly over pelagic regions and in the upper troposphere where few in situ measurements are available. The results may be employed to construct climatology data of the aerosol size distribution or they may be used as direct input to simulations through dynamical downscaling approaches.

Introduction of aerosol representation to internal mixing, source/sink, and direct radiative effects

Compared with typical aerosol transport models, the present SBM coupled with the ALICIS module still lacks modeling of many aspects of aerosol behavior and its effects. Some may have a critical influence on cloud micro- and macrophysics. Their implementation is necessary to conduct more comprehensive simulations of aerosol–cloud interactions (e.g., Saleeby and van den Heever 2013). Various approaches have been proposed to introduce these aspects into models. We will include them in future updates while considering the limitations of the available computational resources.

In reality, aerosol particles are often characterized by internally mixed states with multiple chemical compositions. These aerosol particles are mostly dominant in regions at great distances from their major emission sources. The chemical and physical properties of aerosol particles may change through gas absorption/deposition or they may coagulate with other particles during migration. The question of how to numerically model an internal mixture is a delicate problem in calculating the nucleation process of cloud hydrometeor particles from aerosol particles, as well as their scattering and absorption of atmospheric radiation. Various modifications of the Köhler theory have been proposed to represent the hygroscopic growth of internally mixed particles. For example, reformulation of the Köhler equation was suggested to consider the effects of soluble gases and slightly soluble solid substances in the droplet nucleation process (Laaksonen et al. 1998). A modified Köhler theory with a single solute hygroscopicity parameter (κ-Köhler theory) has also been proposed (Petters and Kreidenweis 2007); the new parameter represents the CCN capability of dry particles with arbitrary mixtures and can be constrained easily with observational data.

Wet scavenging (i.e., impaction of aerosol particles by hydrometeor particles) does not only cause a significant decrease in aerosol concentration but also triggers several cloud microphysical processes, such as contact or immersion freezing. The scavenging process is divided into two types: dissolution or impaction as a result of the nucleation process through condensation or deposition of water vapor on aerosol particles, and impaction through collision between aerosol particles and already extant hydrometeor particles. As highlighted in the section about contact freezing, Brownian diffusion, thermophoresis, diffusiophoresis, electrophoresis, and/or inertial impaction are major causes of collisions between aerosol and hydrometeor particles. There are significant uncertainties associated with modeling these effects, especially as regards the electromagnetic attraction between aerosol and hydrometeor particles, because of insufficient theoretical knowledge and measurement data. In addition, tracing solutions and impurity components in hydrometeor particles is technically difficult if only limited computational resources are available. At present, a few models explicitly predict solution and impurity components in hydrometeor particles in their SBM frameworks (e.g., Chen and Lamb 1994). As an alternative approach, solution and impurity components are assumed to be statistically (Poissonian) distributed according to the volume of a hydrometeor particle when the total mass of the components scavenged by hydrometeor particles is predicted (Phillips et al. 2008). Although these authors applied this approach to their parametrization for immersion freezing, the same approach is applicable to the calculation of aerosol particle emission from evaporated hydrometeor particles.

Scattering and absorption of atmospheric radiation by aerosol particles can change the radiation budget in the different atmospheric layers and on the Earth’s surface; this is a well-known direct effect of aerosol on the Earth’s radiation balance. Direct aerosol effects on atmospheric radiation have a little impact on cloud physics. However, strong absorption of the solar irradiance by aerosol particles potentially has a drastic influence on cloud structure. Heating through absorption may affect the surroundings of the particles on a minor scale. When such absorptive aerosol particles or impurities in hydrometeor particles exist in great volumes at layers near the cloud top, an increase in temperature through heating may promote evaporation of hydrometeor particles. This effect may cause a change in the Earth’s radiation balance through cloud structure change. This kind of aerosol influence is referred to as the aerosol semi-direct radiative effect (Ackerman et al. 2000).

Aerosol optical properties are a key determinant of their influence on the Earth’s radiation budget. We plan to follow standard methods employed in existing aerosol transport models (e.g., GOCART, SPRINTARS, ECHAM: Pozzoli et al. 2011; the Hadley Centre Global Environment Model HadGEM: Bellouin et al. 2011) to determine the aerosol optical properties. The single-scattering properties of spherical aerosol particles can be approximated using Mie scattering theory in radiative flux calculations. The wavelength of light, the radius of a particle, and the refractive index of its medium at the relevant wavelength are required to determine the extinction coefficient, single-scattering albedo, and asymmetry factor. The effect of water uptake on hygroscopic aerosol particles is approximated by calculating the particle radius and refractive index for a series of relative humidity values; the refractive indices are calculated on the basis of the volume-weighted mixing assumption between water and dry components (e.g., Haywood et al. 1997; Takemura et al. 2002; Eq. 3). The internal mixture effect is also approximated using the volume-weighted mixing assumption for multiple different components. Non-spherical dust particles are approximated as their corresponding spherical particles in calculating their optical properties, because relative errors introduced by this assumption are very small (Fu et al. 2009). We will generate lookup tables of extinction coefficients, single-scattering albedos, and asymmetry factors computed using a Mie theory program for the discretized series of aerosol particle radii, relative humidity values, and band wavelengths as applicable to each aerosol type. An internal mixture will be assumed only for organic and black carbonaceous aerosol particles at this stage to avoid heavy computational loads by including all mixture combinations; lookup tables for the mixed particles will also be prepared.


This review paper describes the scientific background and update strategies in the development of the aerosol loading module referred to as ALICIS. The module is used for coupling a downscaled CRM simulation with a large-scale aerosol transport simulation. The most important function of the module is to provide realistic temporally and spatially inhomogeneous distributions of aerosol combined with accurate aerosol size distribution information for downscaled simulations. Introduction of the module yields better simulations of cloud microphysical structure by avoiding the adoption of inadequate aerosol loading as artificially defined by users.

ALICIS has been subject to two major updates since its initiation by IG08. The assumption of the aerosol size distribution spectra was significantly improved as the spectrum shapes better matched their observed counterparts in the first update (CH14). The aerosol emission process from evaporated cloud droplets was added in the second update (SA12). However, many points remain to be improved in future updates, including but not limited to the management of heterogeneous ice nucleation/freezing, aerosol direct/semi-direct effects on atmospheric radiation, addressing internal mixtures of different chemical components in aerosol particles, the introduction of regional variability into the aerosol size distribution, and the representation of wet scavenging.

So far, ALICIS has been employed only in the framework connecting SPRINTARS aerosol transport simulations to JMA–NHM coupled with the HUCM SBM. We are now working on implementing the aerosol loading module into the bridge between the Modern Era Retrospective analysis for Research and Applications Aerosol Reanalysis (MERRAero) or GEOS–GOCART model simulations and WRF coupled with HUCM SBM (WRF–SBM) (e.g., Iguchi et al. 2012a). This extension will readily increase the applicability of ALICIS to more diverse simulation scenes and styles. In addition, we plan to develop the coupling of ALICIS to bulk cloud microphysics instead of SBM to enhance the simulation capability.

In future updates, models coupled with the ALICIS module will include a more comprehensive representation of aerosol and related chemical species, like the WRF–Chem model. Such state-of-the-art models also enable better simulation of cloud microphysics, although they require much larger computational resources and loads. Improvement in model functionality is in competition with improvement in various resolutions such as spatial grid spacing, time-step sampling, and/or particle size bins. Keeping a balance between model performance and computational efficiency in the context of limited resources is a delicate problem in model development. Adequate sorting of the priorities between the introduction of various model functions and improvement in various resolutions is an important task assigned to researchers.



Atmospheric Brown Clouds


Atmospheric Brown Cloud–East Asian Regional Experiment


Asian Pacific Regional Aerosol Characterization Experiment


Aerosol Comparisons between Observations and Models


AErosol RObotic NETwork


atmospheric general circulation model


Aerosol Loading Interface for Cloud microphysics In Simulation


3rd Experiment of the Asian Atmospheric Particulate Environment Change Studies


Atmospheric Radiation Measurement


(space-borne) Advanced Very High Resolution Radiometer


cloud condensation nuclei


cloud droplet number concentration


condensation nuclei


cloud resolving model


Department of Energy


Distributed Regional Aerosol Gridded Observation Networks


NASA Goddard Earth Observing System model


Goddard Chemistry Aerosol Radiation and Transport model


Hadley Centre Global Environment Model


Hebrew University Cloud Model


ice-forming nuclei


INDian Ocean EXperiment


Japan Meteorological Agency Non-Hydrostatic Model


Modern Era Retrospective analysis for Research and Applications Aerosol Reanalysis


Modulate Resolution Imaging Spectroradiometer


Micro-Orifice Uniform Deposit Impactor


National Aeronautics and Space Administration


NASA Unified WRF


spectral bin microphysics


Spectral Radiation Transport model for Aerosol Species


Weather Research and Forecasting model


Weather Research and Forecasting model coupled with chemistry


WRF coupled with HUCM SBM



This research was supported by the Global Environment Research Fund B-4 of the Ministry of Environment, Japan, by project RR2002 and the Data Integration for Earth Observation project of the Japanese Ministry of Education, Sports, Science, Culture, and Technology (MEXT). YS was supported by a Grant-in-Aid for JSPS Fellows (22-7893). IC was supported by the research and development project on the development of global numerical prediction systems of the Korea Institute of Atmospheric Prediction Systems (KIAPS), funded by the Korea Meteorological Administration (KMA). The authors thank the two anonymous reviewers and the journal editor for their helpful comments in improving this paper.

Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (, which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.

Authors’ Affiliations

Earth System Science Interdisciplinary Center, University of Maryland
Code 612 NASA Goddard Space Flight Center
Korea Institute of Atmospheric Prediction Systems
RIKEN Advanced Institute for Computational Science
Atmosphere and Ocean Research Institute, The University of Tokyo
Earth Observing Research Center, Japan Aerospace Exploration Agency


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