This report explores the environmental effects and societal and economic consequences that would follow in the weeks to decades after a nuclear war, beginning with a description of a plausible set of scenarios for the employment of nuclear weapons (Chapter 2). In this chapter, the discussion turns to the fire dynamics and resulting particulate and gaseous emissions resulting from the nuclear detonations and steps through a methodology by which a weapons scenario and the associated energy release, dependent on fuel characteristics and loading, can be converted into fire behavior and emissions. Subsequent chapters in this report explore the fate and transport of these emissions once aerosolized (Chapter 4), the subsequent effects on the climate and physical Earth system (Chapter 5), and the impacts on ecological and societal and economic systems (Chapters 6 and 7).
Combustible: Material that, in the form in which it is used and under the conditions anticipated, will ignite and burn (NFPA, 2021)
Combustion: Chemical process of oxidation that occurs at a rate fast enough to produce temperature rise and usually light either as a glow or flame.
Combustion Efficiency: Ratio of heat released by the fuel to the heat input by the fuel.
Conflagration: A large and uncontrolled fire.
Emission Factor: Mass of emitted pollutant per mass of fuel burned.
Fire Dynamics: How fires start, spread and develop.
Fire Load: The total heat energy of the complete combustion of combustible materials in a building, space, or area, expressed in MJ (or its equivalent energy unit). For buildings, it includes furnishing and contents and combustible building elements. There are distributed and localized fire loads. Distributed fire load refers to the overall fire load of the building, space, or area. Localized fire load is the fire load at a specific location; this may have a magnitude that is considerably larger or smaller than the distributed fire load.
Fire Load Density (FLD): The heat energy that could be released per unit area by the complete combustion of combustible materials in a building, space, or area, expressed in MJ/m2 (or an equivalent unit indicating heat energy per unit area).
Firestorm: Intense conflagration that creates its own convective wind patterns, radially drawing in air near the surface, with strong updrafts above the fire.
Fuel Load: Total wood equivalent mass of combustible materials in a building, space, or area, expressed in kilograms (or pounds) per unit area. Here the heat of combustion of dry wood of 18.6 MJ/kg (or 8,000 BTU/lb) is used as the basis for equivalent wood mass calculation.
Ignition: Initiation of combustion.
Non-methane Organic Gases (NMOG): Any number of volatile organic compounds in the gas-phase. These may include any organic compound other than methane.
Particulate Black Carbon (BC): Black carbon particles, or aerosol. This material absorbs light.
Particulate Organic Carbon (OC): All combustible, noncarbonate carbon that can be collected on a filter (Kharbush et al., 2020).
Particulate Organic Material (POM): Total organic matter that is part of measured particulate matter, including carbon, nitrogen, oxygen and hydrogen.
Rubblization: Process of a structure being reduced to rubble.
Smoke: Airborne solid and liquid particulates and gases evolved when a material undergoes pyrolysis or combustion, and often used as an informal term for a fire-emitted aerosol (NFPA, 2021).
Smoldering: Combustion of a solid without flame, often evidenced by visible smoke. (Note: Smoldering can be initiated by small sources of ignition, especially in dusts or fibrous or porous materials, and may persist for an extended time after which a flame may be produced.)
Smoldering Combustion: Ignition of combustible material where a transition to flaming combustion does not occur but a charred area indicating locations where embers landed can be observed and involves the exothermic oxidation of condensed-phase materials.
Soot1: Black particles of carbon produced in a flame (NFPA, 2021).
Wildland Urban Interface (WUI): Community that exists where humans and their development meet or intermix with wildland fuel.
Fire has long been recognized as a key outcome of the intense discharge of radiation, light, and heat produced by the detonation of a nuclear weapon. In the moments after the detonation, a thermal pulse would vaporize materials nearby and start fires at farther distances wherever it impinges on combustible materials with enough energy to ignite them. In addition, an expanding sphere of superheated air produced by the initial fireball would create a blast wave that breaks apart structures, creating rubble and igniting a second set of fires from damaged structures, vehicles, equipment, and other sources of fuel. Chapter 2 provides greater detail on the expected extent of the thermal and blast effects. With sufficiently high fuel loading, favorable atmospheric conditions, and widespread ignition, individual fires can merge into a large fire with a strong upwardly buoyant convective column, known as a firestorm. In areas with lower fuel loading, fires can occur in a line-like fire front, whose movement is often driven by ambient winds and interactions with local topography. Fires may produce environmental impacts on regional and
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1 There is a diversity of technical terminology used to identify combustion products across multiple disciplines. The definitions used in this report are sufficiently broad to be applicable across different chapters, however, the committee acknowledged that practitioners in specific research communities may use more precise definitions. For example, in the field of soot formation, soot is, “carbonaceous particles formed during the incomplete combustion or pyrolysis of hydrocarbons, including incipient soot particles, mature soot particles, and all of the intermediate particulate stages between inception, maturity, and complete oxidation to gas-phase species” (Michelsen et al., 2020).
global scales if the emissions have sufficient mass, energy, and atmospheric lifetime, as can occur if these emissions reach the stratosphere where removal mechanisms are inefficient.
There are three categories of material emissions that may result from a nuclear blast:
This chapter focuses on the emissions from fires after detonation (Category 3). Categories 1 and 2 were previously discussed in Chapter 2 and are less likely to be a concern in the detonation scenarios described in Chapter 2 due to employment of weapons 1 Mt in yield and below, which have less potential to directly inject material in the stratosphere when compared to weapons with yields greater than 1 Mt. The quantity of particulates in the nuclear cloud (Category 1) is likely small relative to that of the potential emissions from the subsequent fires (see Chapter 2, Box 2-3).
Emissions from fires, such as those started by a nuclear blast as explained above, can be estimated using a methodology previously developed to estimate pollutant emissions from biomass burning. The approach taken by Seiler and Crutzen (1980), which estimates biomass burning emissions as the product of several independent terms (Equation 3-1), may be useful for identifying the causes of diverging estimates from different studies and for drawing contrasts with the broader literature modeling aerosol and gas-phase emissions from wildfires. In this framework, the flux of a specific aerosol or gaseous constituent (E, with units of mass per unit time) is equal to the product of the area burned per unit time (A, with units of area per unit time), the fuel load (Fl, with units of mass per area), combustion completeness (CC; a unitless fuel consumption fraction), and an emission factor (Ef; with units of mass constituent per unit of mass dry fuel consumed) that describes the production of a specific constituent of interest under characteristic environmental conditions (e.g., moisture content and three-dimensional structure) of the fire under investigation.
| E = A ∙ Fl ∙ CC ∙ Ef, | Equation 3-1 |
This framework can also be used to predict the emissions of aerosol and gases in the context of a nuclear detonation, with A representing the area of fires ignited by the thermal pulse and air blast ; Fl representing the combined density of fuels in buildings, vehicles, structures, roads, and vegetation; CC being the fraction of these fuels in the environment that is consumed by the flash-ignited and subsequent fires (i.e., the combustion completeness fraction); and Ef being the production of pollutants, including particulate black carbon (BC), particulate organic carbon (OC), particulate matter less than 2.5 microns (PM2.5), and reactive gases, such as carbon monoxide (CO) and nitrogen oxides (NOx) per fuel that is consumed. The next sections of this chapter explore each of these terms separately, to understand the differences in and among several recent studies and to identify best practices for future work.
In this chapter, considerations for evaluating the fire dynamics and emissions from a nuclear blast (or multiple blasts within a scenario) and resulting fires are discussed. Section 3.2 explains the characteristic fuel loadings and fuel consumption. Section 3.3 describes ignition and fire spread, which define the area burned. Section 3.4 describes emission factors used to estimate specific pollutant emissions. Finally, Section 3.5 provides recommendations for improved understanding and best practices for how the current knowledge can be applied to the scenarios provided in Chapter 2.
Fuel load describes the total amount of combustible materials present in an area that could potentially contribute to a fire. Combustible materials include any materials that can burn under normal conditions, such as wood, paper, plastic, nonmetal furniture, cooking oil, vegetation, and other items in buildings or outdoor environments such as urban areas, wildland, or at the wildland urban interface (WUI). The fuel load in a given area is a crucial factor in estimating fire risk and fire behavior, determining the potential intensity and spread of a fire, as well as assessing fire emissions and, ultimately, their ecological and social impacts.
Fire load refers to total heat energy of the complete combustion of the fuel load in a given space, expressed in megajoules (MJ, or its equivalent energy unit such as British Thermal Unit). The U.S. National Bureau of Standards developed the fire load concept in the 1920s for fire resistance specifications in regulatory documents, from which more recent definitions have derived (ASTM, 2024b; NFPA, 2023). A related term, fire load density (FLD), refers to the heat energy that could be released per unit area by the complete combustion of the fuel load, expressed in heat energy per unit area (such as MJ/m2). FLD may also be defined as the fire load per unit volume (MJ/m3). The FLD of an area containing different combustible materials can be calculated as:
| FLD = [Σi (mi × Hi)]/ A, | Equation 3-2 |
where mi denotes the mass of a combustible material i, Hi is the heat of combustion or specific energy released from combustion per mass unit of material i, and A is the area of the space of concern.
Fuel load can be measured in terms of the weight of combustible materials present and usually involves the calculation of the total equivalent wood mass (EWM) of the fuel load in a given space, expressed in mass per area (such as kg/m2). EWM quantifies the amount of fuel present, expressing it in terms of a hypothetical mass of wood to allow for a standardized comparison of the flammability and fire behavior of different types of fuels. Converting the fuel loading of a fuel (or fuel type) into EWM is typically done by comparing the energy content of the fuel to that of wood. The FLD to fuel load conversion can be done using the following equation:
| Fuel Load = FLD/Hwood, | Equation 3-3 |
where Hwood is the heat of combustion of wood and is typically 16.3 to 18.6 MJ/kg. The value of 18.6 MJ/kg) for dry wood (i.e., wood with all moisture removed, or “oven-dry”) has been used in many fire standards (ASTM, 2024a) as the “nominal” heat of combustion of dry wood. This value has been used for EWM calculations in the above equation.
Several methods have been developed to estimate fuel loading and FLD for urban landscapes. One approach bases the estimates of fuel load or FLD on urban land use (Frishcosy et al., 2021; Reisner et al., 2018; Small, 1989). Bush et al. (1991) developed fuel load estimates for U.S. cities for the three land-use types of residential, commercial/service, and industrial. Residential land use makes up a majority of the urban areas in the United States and the primary combustible material is wood. Residential U.S. fuel load estimates range from 7.7 kg/m2 in the South to 23.3 kg/m2 in the Northeast. Commercial and industrial areas have much higher fuel loads (see Table 3-1). Bush et al. (1991) inventoried most sources of combustible material in urban areas, and provided detailed analyses of building layouts, construction practices, combustible contents, building densities, regional variations, and demographic, social, and economic influences. They applied the obtained data to their matrix of buildings that comprise a city while accounting for different city morphologies and found that U.S. urban fuel loads range from 14 to 21 kg/m2.
Another approach to estimate fire load is to consider the end use of buildings and include the space or area outside the building (Frishcosy et al., 2021). For example, one can divide the urban area according to the designed land-use type classification and then investigate the differences in fire loads for different building types to assign the proper FLD to each area and calculate the available fuel energy. Based on the proportion of combustible materials for each land-use type, the model estimates the mass density of each type of combustible material in urban areas. Land-use types in urban areas can include agriculture, business, commercial, educational, entertainment, industrial, residential, or utility. The agriculture category can represent urban areas with large areas of vegetation. Table 3-2 shows the effective FLD and associated fuel load values for some of the land-use categories (Frishcosy et al., 2021).
TABLE 3-1 Building Structure and Content Fuel Loads in U.S. Urban Areas
| Land Use | Fuel Load of Building Structure and Contents within Land-Use Classification, kg/m2 | Percent of Ground Covered | Fuel Load Integrating Buildings and Open Space, kg/m2 |
|---|---|---|---|
| Residential | 134 | 9.7 | 13 |
| Commercial and services | 110 | 21.6 | 24 |
| Industrial | 225 | 19.6 | 44 |
SOURCE: Adapted from Bush et al., 1991.
TABLE 3-2 Effective Fire Load Density Values for Some Land-Use Categories in the United States
| Land-Use Type | Fire Load Density, MJ/m2 | Fuel Loada, kg/m2 | Corresponding Building Type |
|---|---|---|---|
| Residential | 848 | 46 | Residential building |
| Commercial | 1400 | 75 | Commercial building |
| Streets | - | - | - |
| Parks | 450 | 24 | Agriculture |
| Public facilities | 393 | 21 | Entertainment building |
| Institutional | 734 | 39 | Educational building |
| Transportation utilities | 157 | 8 | Utilities |
| Vacant | 450 | 24 | Agriculture |
| Federal | 500 | 27 | Business |
| Industrial | 1018 | 55 | Factory |
NOTE: a Fire load calculations are based on an energy content of 18.6 MJ/kg for dry wood.
SOURCE: Frishcosy et al., 2021.
Some researchers have also based estimates of urban fuel load or FLD on an assumption that, within urban zones, there is a direct relationship between the quantity of fuel and local population density; thus, allowing population density to serve as a surrogate for fuel loading or FLD (e.g., (Frishcosy et al., 2021; Toon et al., 2007; Toon et al., 2019)). A baseline per capita fuel load (Mf) of 11 million g/person was mentioned by Toon et al. (2007). Frishcosy et al. (2021) presented a study on FLD in urban areas using a refined method for calculating mass per capita. Their case study for Washington D.C. showed that fuel mass density per capita is variable across the entire city. Fuel mass density per capita values depend on the land-use type, ranging from of 3,200 to 37,900 kg of fuel per person for 10 different land-use areas of the city. Figure 3-1 illustrates the fuel load results from this study as compared to an earlier study. The figure demonstrates that fuel load is highly variable in urban areas because of the differences in land use. Among the influencing factors, building type shows the significant effect on the value of fuel loads.
The open literature contains additional fire load studies and data for countries or regions across the globe (Table 3-3). Unlike the studies mentioned above, the FLD studies and data in Table 3-3 were developed for fire protection engineering design or analysis purposes, and thus were derived assuming a uniform distribution of combustibles in the buildings only (without considering space or area outside buildings) and that all combustibles will burn and undergo complete combustion if a fire occurs.
TABLE 3-3 Fire Load Density Data in Countries and Regions Other than the United States
| Buildings and Location | Fire Load Densitya (Fuel Load) | Method Description |
|---|---|---|
| Residential buildings in Kanpur, India | Avg. FLD: 560 MJ/m2 (30 kg/m2); Range: 320–979 MJ/m2 (17–53 kg/m2); S.D. of FLD: Avg. 293 MJ/m2 (16 kg/m2); S.D. Range: 100-714 MJ/m2 (5–9 kg/m2); Max. FLD: 2,497 MJ/m2 (134 kg/m2) in a storeroom. Fuel load (FL) did not depend on the height of the building. Dead load (the permanent load from the physical structure) contributed to about 52.66% of total FL. FL decreases as the floor area increases. FLD can be calculated by considering the combined effects of category of housing, room use, and room floor area. |
FL survey using the inventory technique for 35 residential buildings covering a total of 4256.6 m2, from 09/1991 to 05/1992 Kumar and Rao, 1995 |
| Office Buildings in Kanpur, India | Avg. FLD: 348 MJ/m2 (19 kg/m2); S.D.: 262 MJ/m2 (14 kg/m2); 95th percentile: 1,030 MJ/m2 (55 kg/m2); Max. FLD of 1,860 MJ/m2 (100 kg/m2) in a storage room. Storage and file rooms have the most FLD. FLD was not dependent on the floor level. FLD decreases as the room floor area increases. The mean FL is practically independent of the room floor area. Wood and paper contribute to a substantial portion (98.7%) of total FLD. Movable combustible contents contribute to 88.3% of total FLD. |
FL survey using the inventory technique for 8 office buildings, 388 rooms, and a total area of 11720m2, from 07/1992 to 07/1993 Kumar and Rao, 1997 |
| High-rise buildings in Hong Kong, China | Avg. FLD range: 78 MJ/m2 (4 kg/m2) to 1,248 MJ/m2 (67 kg/m2); Median FLD range: 99 MJ/m2 (5 kg/m2) to 1,167 MJ/m2 (63 kg/m2) |
FL survey of 37 high-rise buildings Chow et al., 1999 |
| Offices in Hong Kong, China | Mean FLD: 911 MJ/m2 (49 kg/m2); FLD Range: 316 to 1,585 MJ/m2 (17–85 kg/m2) |
FL survey of 25 small and medium enterprises offices Chow et al., 2006 |
| Shopping malls in Hong Kong, China | 84% of the retail shops have FLD below the upper limit of 1,135 MJ/m2 (61 kg/m2) under the local code. A high value of 2,530 MJ/m2 (136 kg/m2) was found in a retail shop because of storing high amount of bedding products. |
FL survey of four shopping malls with 301 retail shops Fong and Chow, 2011 |
| Hotel buildings in six major cities across China | Mean FLD: 349.2 MJ/m2 (19 kg/m2); Range 117.8–886.4 MJ/m2 (6–48 kg/m2); S.D.=142.1 MJ/m2 (8 kg/m2); Median FLD: 340.4 MJ/m2 (18 kg/m2); A table comparing FLD in different studies showed the mean FLD ranges from 251 to 349 MJ/m2 (13–19 kg/m2). FL is affected by the regions. FL decreases with increasing floor area up to 25 m2; thereafter the FL increases with further increasing the floor area. |
FL survey via the combination method Gao et al., 2012 |
| Residential buildings in the Yangtze River Delta in Zhejiang Province, China | Avg. FLD: 473.8 MJ/m2 (25 kg/m2); living room: 335.75 MJ/m2 (18 kg/m2); bedroom: 612.28 MJ/m2 (33 kg/m2); kitchen 658.64 MJ/m2 (35 kg/m2); study room 542.66 MJ/m2 (29 kg/m2); bathroom 219.64 MJ/m2 (12 kg/m2); Other FLD in China according to this paper: Henan Province: 520.26 MJ/m2 (28 kg/m2); Beijing (city): 1,197.17 MJ/m2 (64 kg/m2); Hong Kong (city): 1,135 MJ/m2 (61 kg/m2); |
FL survey on 385 rooms covering 5,300 m2 Wang and Zhou, 2019 |
| Buildings and Location | Fire Load Densitya (Fuel Load) | Method Description |
|---|---|---|
| Residential buildings in Novi Sad, Serbia | Avg. FLD: 702 MJ/m2 (38 kg/m2); S.D.: 59 MJ/m2 (3 kg/m2); Range: 617-768 MJ/m2 (33–41 kg/m2); |
FL survey using the combination method, 120 three-room apartments, 8,700 m2 Džolev et al., 2021 |
| Office buildings in Islamabad, Pakistan | Avg. FLD: 603 MJ/m2 (32 kg/m2); S.D.: 322.38 MJ/m2 (17 kg/m2); government offices: 763.42 MJ/m2 (41 kg/m2); private offices: 431.49 MJ/m2 (23 kg/m2); FL changes for office room use: Max. FL in storerooms at 1,468.02 MJ/m2 (79 kg/m2); min. FL in general office at 247.05 MJ/m2 (13 kg/m2); Impact of wood is more than other materials. Paper has less impact on FL. Plastics contribute less than 30% of total FL. Fl increases as room area increases; which is contrary to other surveys. |
FL survey via the combination method, 175 hotel buildings, 92 rooms (44 private offices, 48 government offices) Noman et al., 2023 |
| High-rise buildings in Istanbul, Turkey | Small and large living rooms have FLD of 379 and 310 MJ/m2 (20 and 17 kg/m2), respectively. Small and large bedrooms have 650 and 518 MJ/m2 (35 and 28 kg/m2), respectively. The kitchen FL is estimated as 552 MJ/m2 (30 kg/m2); |
Inventory survey technique of 50 floor plans Dundar and Selamet, 2023 |
NOTE: a Fuel load (FL) in kg/m2 is obtained by dividing its FLD value by 18.6 MJ/kg and S.D. values are provided for 1 standard deviation,
Wildland fire fuels consist of the various vegetation, litter, fine and coarse woody debris, and duff components of the ecosystem that are potentially combustible, including ground, surface, and crown fuels. A comprehensive analysis by van Leeuwen et al. (2014) synthesized field measurements of fuel loadings, combustion completeness, and fuel consumption related to wildland fires. The compilation of global measurements resulted in average fuel loadings for savannas ranging from 0.76 to 1.1 kg/m2, and forests from 6.9 to 28.5 kg/m2, with significant variability. The mass fraction of carbon across biomass fuels does not vary significantly and is typically assumed to be 0.45 (e.g., Andreae, 2019). The chemical composition of woody biomass is well characterized, with less than 1% by mass of nitrogen, sulfur, chlorine, and other trace inorganic elements (NASEM, 2022).
TABLE 3-4 Summarized Fuel Loadings and Combustion Completeness in Wildland Fires
| Fuel Loading, kg/m2 | Combustion Completeness | |
|---|---|---|
| Savanna | 0.76 | 0.71 |
| Grassland savanna | 0.53 | 0.81 |
| Wooded savanna | 1.1 | 0.58 |
| Tropical forest | 28.5 | 0.49 |
| Temperate forest | 11.5 | 0.61 |
| Boreal forest | 6.9 | 0.51 |
| Pasture | 7.4 | 0.47 |
| Chapparral | 3.5 | 0.76 |
SOURCE: van Leeuwen et al., 2014.
The energy content of biomass has similarly been characterized, reaching up to 20 MJ/kg for vegetation producing higher heating values (NASEM, 2022). The FLD of biomass is, however, affected by the fuel water content, which is controlled in part by weather and climate, vegetation species, and whether the vegetation is alive or dead. Wet forests typically have higher fuel loading but are less likely to ignite. Other differences in vegetation can affect the combustion behavior and therefore emissions; for example, materials can smolder rather than undergo intense combustion, and materials can sustain or contribute to fire spread before undergoing complete combustion (NASEM, 2022).
Fuels burned in the fires resulting from a nuclear blast may combine different urban, commercial, and suburban land-use classes, as well as vegetation that is prevalent at the wildland–urban interface. The WUI is the area where built structures and other human development meet undeveloped wildland or vegetation fuels (NASEM, 2022). A combination of natural and human-made materials in the WUI leads to unique fire dynamics and atmospheric emissions and effluents not typically found in wildland or urban fires.
WUI fuels include biomass materials surrounding WUI structures, wood products in building construction and furniture, and synthetic combustible materials used in residential and urban environments. Large open WUI fires may also involve municipal service systems, commercial buildings, and industrial sites and facilities. There is a general lack of available information on the distribution of commercial and industrial structures, as well as their fuel loadings and composition. Furthermore, fuel loading, as well as the resulting fire behavior and emissions, from different vehicles (and propulsion systems) is lacking and deserves further investigation. Current understanding of fuel loading, fire behavior and fire emissions in the WUI is largely inferred based on information on wildland and urban fires. The National Academies report on the Chemistry of Fires at the Wildland-Urban Interface (NASEM, 2022) provides an excellent summary of the current understanding of materials, combustion, and emissions in the WUI.
In the baseline scenario for Turco et al. (1983), the total smoke emission from all sources was ~225 Tg, of which ~70 Tg was BC, the rest OC. The total quantity of urban fuels consumed amounted to 4950 Tg (items 1, 2, and 4), and the corresponding total urban fire smoke emission was 145 Tg, including about 46 Tg of BC (of which ~3.5 Tg BC reached the stratosphere). These emissions included:
To determine a per capita fuel loading, Toon et al. (2007) used a baseline estimation of the total amount of fuels in the developed world and compared to approaches based on structures predicted by Small (1989) and Bush et al. (1991). As referenced above in Section 3.2.1.1, the resulting fuel load was calculated as 1.1 × 107 g/person, and scaling for population density, 0.0011 g/cm2 per person/km2, noting the need to adjust for comparative fuel loading in different regions of the world.
Comparisons with earlier literature should consider the change in understanding of fuel loads (a sample of which are in Table 3-5) from when previous assessments were performed.
Historical examples such as past urban fires and fires from World War II may not be appropriate as analogs for those that would result today, due to intervening changes in land-use patterns, building materials and structures, furniture materials, changing standards for fire-resistive construction, and other factors. Further, the world population and urbanization have grown significantly since World War II, producing more materials and structures available for destruction and burning. Although some data are available to estimate the characteristics and quantity of urban and vegetative fuels that would be burned in fires caused by the detonation of a nuclear bomb, many uncertainties remain. Specifically, constraints on the fuel loading and FLD of various land uses and land cover (LULC), such as industrial, commercial, residential, and wildland areas, across rural and urban landscapes are highly variable and not well constrained. There is a lack of systematic consideration of how roads, sidewalks, and other areas with low-density fuels contribute to fuel loading at a regional scale. Further, there are significant variations in the fuel loadings that may occur in these various LULC classes within and across different cities in different parts of the world. The composition of the fuels, including the construction material composition and the carbon and metals content of the fuels, are highly variable and not well defined. These characteristics may also vary significantly across land uses, not only in the United States, but across the globe. The variables—fuel loadings and fuel composition—are critical for the determination of emissions from fires, as well as the intensity of the fire and the height to which the smoke plume rises since the fuel density and composition drive both emissions and fire behavior.
| Fuel Loading | Source |
|---|---|
|
30 kg/m2 Suburban; |
Turco et al. 1983 |
|
234.4, 410.1, 625 kg/m2 City Center; |
Larson and Small, 1982; DCPA, 1973 |
| 9.2 kg/m2 Live northern U.S. Forests avg | USFS NRS, 2021 |
|
40 kg/m2 Urban; |
NRC, 1985 |
| 100 kg/m2 | Reitter et al., 1982 |
|
15.0 kg/m2 Generic; |
Veregin, 1993 |
|
48.8–97.6 kg/m2 Residential; |
Rodden et al., 1965 |
|
7.7–23.3 kg/m2 Residential; |
Bush et al., 1991 |
SOURCE: Brown et al., 2023.
Several fires occurring during World War II that were ignited by incendiary bombing or nuclear detonations were characterized as “firestorms,” rather than conflagrations. Firestorms are associated with a strong convective column of rising air and smoke, in which air enters the fire radially, near the surface. The fire front is stationary, as the inward winds near the surface inhibit fire spread. Nearly all combustible fuels are consumed in a firestorm. By contrast, a conflagration is a fire with a wind-driven, moving fire front. Historically, it has been assumed that conflagrations have lower plume heights. Therefore, they have been of less interest in climate studies of nuclear effects, as it has been assumed that the smoke would be removed in the troposphere, and thus would be short-lived. However, more recent Earth system modeling have shown that smoke injected into the middle and upper troposphere can be stabilized by solar heating, and may even loft into the stratosphere. Hence, attention has also focused on smoke injection from less intense fires. Moreover, instances of wildfire conflagrations and pyrocumulus plumes injecting smoke directly into the stratosphere have been documented. It is possible that a nuclear detonation could result in either a firestorm or a conflagration.
Researchers have previously attempted to determine the necessary criteria for the formation of a firestorm using the limited data from these events. Rodden et al. (1965) lists the following criteria: (1) fuel loading must have at least 39 kg/m2 of combustibles, (2) at least 50% of structures must simultaneously be on fire, (3) surface winds must be less than 3.6 m/s, and (4) the fire area must be greater than 1.3 km2. Furthermore, an unstable atmosphere will likely increase the likelihood of a firestorm, while a stable atmosphere will decrease the likelihood. Although these criteria have been developed, the committee was not aware of their application in climate studies of the effects of firestorms. Instead, it is most frequently assumed that each detonation will result in a firestorm.
Historical fires from World War II that are generally agreed to have been firestorms followed the bombings of Hamburg, Dresden, and Hiroshima (Rodden et al., 1965). The fuel loading in Hamburg was reported as 156.2 kg/m2 by a German fire chief (Schubert, 1969) and in the range of 146.4 to 195.3 kg/m2 by Rodden et al. (1965). Rodden estimated the fuel loading in Hiroshima at 39 kg/m2, which became the minimum value for fuel loading in the firestorm criteria. The firestorm areas at Hamburg and Hiroshima were 10.35 and 11.65 km2 respectively and the Dresden firestorm was reported as 20.72 km2. The smallest firestorm of WWII was in Darmstadt, reported to be 3.88 km2. In Hamburg, where building density was described as 30–40%, it was reported that fires became widespread within the first 30 minutes, the peak intensity of the fire occurred 2 to 3 hours after the bombing, and the fire burned for 5 to 6 hours. Hiroshima followed a similar timeline but reports of the total duration range from 4 to 12 hours.
As described in Chapter 2 of this report, the major effects of nuclear detonations include (a) kinetic energy via blast and shock, (b) thermal energy via thermal radiation, (c) initial nuclear radiation, and (d) residual nuclear radiation. For fire ignition and fire spread, the effects from thermal energy and kinetic energy are of major concern. Thermal radiation can start fires at considerable distances and scale. Kinetic energy can damage buildings and structures and make more combustible materials more readily available for combustion.
Following a nuclear blast, there are two surface-temperature pulses and two pulses of thermal emission of thermal radiation from the fireball (Glasstone and Dolan, 1977). The first is of very short duration (one-tenth of a second for a 1-megaton explosion) with high temperature and much of the radiation in the UV range, less for skin burns but capable of permanent or temporary effects on the eyes. The second radiation pulse may last for several seconds (~10 seconds for a 1-megaton explosion), carries about 99% of total thermal radiation energy, most of the rays reaching Earth are visible and infrared light. This radiation is the main cause of skin burns up to 12 miles or more away, and of eye effects at even greater distance. The radiation from the second pulse can also cause fires to start under suitable
conditions. Under normal atmospheric conditions, combustible materials require a certain level of surface temperature or heat flux level to ignite.
Table 3-6 lists some typical temperatures and the expected response from different materials or fire conditions in a building. Table 3-7 lists the representative heat flux levels and examples of physical phenomena. Some cellulosic materials will undergo autoignition when their surface temperature reaches 200 °C. The minimum flux for ignition of plastics or wood-based materials can be as low as 10 kW/m2. After a nuclear blast, ignition may occur wherever a combustible material’s surface has one of these ignition conditions. In fire modeling, average fuel temperature values have been used as the target ignition temperatures, such as 1000 K for thin fuels and 600 K for thick fuels (Reisner et al., 2018).
| Temperature, °C | Response |
|---|---|
| 200 | Autoignition of some cellulosic materials |
| 250 | Temperature when charring of natural cotton begins |
| >300 | Surface temperature for piloted ignition of woods and similar materials Modern synthetic protective clothing fabrics begin to char |
| ≥400 | Temperature of gases at the beginning of room flashover |
| ≈600 | Flashover condition of hot-layer temperature in enclosure fires |
| ≈1,000 | Temperature inside a room undergoing flashover |
SOURCE: NIST, 2010.
TABLE 3-7 Examples of Heat Flux Rates of Heat Energy Transferred per Surface Unit Area
| Heat Flux, kW/m2 | Example |
|---|---|
| 1.0 | Sunny day |
| 2.5 | Typical firefighter exposure |
| 3.0–5.0 | Pain to skin within seconds |
| 10.0–15.0 | Minimum flux for ignition of plastics or wood-based materials |
| 20.0 | Threshold flux to floor at flashover |
| 84.0 | NFPA 1971: Thermal Protective Performance Test (NFPA, 2018) |
| 60.0–200.0 | Flames over surface |
SOURCE: NIST, 2010.
Table 3-8 shows the typically expected damage to buildings and structures at specific overpressure values. Most buildings will be completely destroyed with 34 to 83 kPa (5 to 10 psi) of overpressure from the air blast. Rubblization from the nuclear denotation may reduce initial fire activities up to 30–40% in some cases (Glasstone and Dolan, 1977). However, it is not clear how rubblization will affect the secondary ignitions and fire propagation at later stages.
TABLE 3-8 Damage Approximations at Specific Overpressure Values
| Damage | Incident Overpressure, psi | Incident Overpressure, kPa |
|---|---|---|
| Typical window glass breakage | 0.15–0.22 | 1–1.5 |
| Minor damage to some buildings | 0.5–1.1 | 3.4–7.6 |
| Panels of sheet metal buckled | 1.1–1.8 | 7.6–12 |
| Failure of concrete block walls | 1.8–2.9 | 12–20 |
| Collapse of wood-framed buildings | Over 5.0 | 34 |
| Serious damage to steel-framed buildings | 4–7 | 28–48 |
| Severe damage to reinforced concrete structures | 6–9 | 41–62 |
| Probable total destruction of most buildings | 10–12 | 69–83 |
SOURCE: Adapted from FEMA, 2003.
The initial burn areas after nuclear blasts can be estimated using the radiant energy equation, Equation 2-5 in Chapter 2, and ignition criterion (e.g., ignition temperature). An example of this calculation is provided in Table 2-6 for different yields and a given radiant exposure level. Different fuels will ignite at different radiant exposure levels, leading to a smaller or larger possible fire start area. Typical ignition criteria include a minimum ignition energy (e.g., heat flux received by the fuel) or a minimum ignition temperature (e.g., surface temperature of the fuel). For simplicity of implementation, most fire models define fire ignition as the time when the surface temperature reaching a predefined ignition temperature of the fuel. Some fire models, such as the study using HIGRAD-FIRETEC simulations (Reisner et al., 2018), can consider the influence of rubblization on fire ignition and burn area.
Three elements are required to start a fire: fuel, oxygen, and a heating source (the so-called fire triangle). Under normal atmospheric conditions, available combustible materials are fuels, and air supplies oxygen. The thermal radiation from a nuclear denotation will be the heating source. After a detonation, fires can be caused by both direct ignition of combustible materials from the thermal radiation, and from secondary ignition sources due to infrastructure damaged from the blast wave (e.g., broken gas lines and damaged equipment generating heat). After ignition, the fire will keep burning, grow, and propagate if the heat energy generated from the fire is greater than the energy needed to ignite the combustible materials nearby. The fire will continue to grow for as long as this self-sustained chain reaction continues. The fire will lessen and eventually become extinguished when the oxidation reaction cannot generate sufficient heat energy to sustain the chain reaction. The thermal radiation effects from a nuclear detonation are described in Chapter 2, Section 2.3.3 Thermal Radiation Effects.
Extreme fires such as firestorms and conflagrations can occur after nuclear detonations. Depending on the ground fuel loading and other factors, a firestorm would develop following a nuclear detonation in some urban areas (as happened in Hiroshima), or a large-scale conflagration would evolve in other urban areas (as happened with the conventional bombing of Tokyo and other cities during WWII). Consistent with Rodden et al. (1965), Glasstone and Dolan (1977) pointed out that firestorms can occur when the following conditions are met: (a) a fuel loading of at least 40 kg/m2, (b) simultaneous burning of half the structures in an area, (c) ambient wind of less than 3.6 m/s, and (d) a minimum burning area of about 1.3 km2. Firestorms will almost completely consume all combustibles in the area, although combustibles covered by rubble would not completely burn. Whereas firestorm formation requires relatively specific conditions, conflagrations can develop more easily. The most important factors for conflagrations are available fuels and wind conditions. When separate smaller fires burn simultaneously over a large area under high winds, their moving fire fronts can merge and form a massive conflagration. Conflagrations will continue to propagate as long as there is sufficient fuel, as seen in large forest fires, wildland-urban interface fires, and urban fires. Conflagrations in urban and industrial areas would likely be more intense due to their high fuel loading. Nuclear firestorms and conflagrations may ultimately have similar impacts on fuel consumption and smoke injection heights (Toon et al., 2019).
Depending on ground conditions (e.g., fuel characteristics and terrain) and weather conditions, and assuming no human intervention or suppression, fires can continue to burn after initial ignition and propagate outside the initial burn area (beyond “ground zero”). Fire growth will follow general pathways for fire spread in large open fires through radiation, convection (including direct flame contact), and spotting via ember exposure (Caton et al., 2017). Secondary ignitions in the Hiroshima firestorm (NRC, 1985) and incendiary bombs in Dresden and Hamburg (Hewitt, 1983) led to unique fire conditions that resulted in significantly enhanced fire behavior. The exposure conditions, nearby combustibles and their burning, as well as smoke and volatile production need to be considered specifically for the impacted areas. Less is known, however, about the ignition and smoke hazards of dust clouds and special elements (e.g., metals) during and after nuclear blasts. When studying fires and smoke production after the initial ignition, other factors such as self-heating and smoldering and transition between smoldering and flaming are important to consider.
Fire modeling entails the use of a combination of tools to simulate and predict fire behavior and effects, including empirical data, experimental studies, mathematical equations, and numerical simulations to represent the complex phenomena associated with fire behavior and effects. Fire models can be either probabilistic or deterministic. Probabilistic, or stochastic, fire modeling incorporates
uncertainty and probability into fire modeling to assess likelihood and variability of fire behavior and its associated impacts. Deterministic fire modeling provides specific single-valued predictions of fire behavior and its effects without explicitly considering uncertainty or variability in input parameters. Deterministic fire models include empirical models using simple mathematical equations derived from field observations and experimental data (Quintiere and Wade, 2016), zone or grid models where the space is divided into zones or grid of cells with each zone or cell representing a specific state such as hot or cool and burned or unburned (Walton et al., 2016), and physics-based models using sophisticated computational simulations considering the physical process involved such as heat transfer, fluid dynamics, and combustion chemistry (McGrattan and Miles, 2016). Modern computational fire models can consider many factors including fuel characteristics, weather conditions, topography, presence of structures or other obstacles, and even interaction with the surrounding environment.
Different deterministic fire models have been developed for different purposes. Compartment fire models focus on prediction of the behavior and effects of fires within enclosed spaces such as buildings, considering factors such as compartment size and geometry, fuel characteristics, ventilation conditions, heat transfer mechanisms, and fire products (e.g., smoke and toxic gases). Compartment fire modeling has been widely used in fire protection engineering, building design, and firefighting to understand fire behavior and develop effective strategies for fire protection and suppression. Open-space fire modeling predicts or simulates the behavior and effects of fire in outdoor or unconfined environments such as wildlands, forests, grasslands, and WUI areas (Morvan et al., 2022). Open-space fire models can consider factors such as fuel characteristics, terrain conditions, wind conditions (e.g., speed and direction) and other atmospheric conditions. Open-space fire models are used for a variety of purposes, such as fire management, fire risk assessment, fire prevention and planning, fire emergency response, etc.
Fire modeling methods have been used for the study of fire behavior and fire impacts due to nuclear wars, such as the fire model HIGRAD-FIRETEC used in Reisner et. al. (2018). The Weather Research and Forecasting model coupled with a fire model (WRF-Fire) has been used to model fire spread and plume rise (Redfern et al., 2021). When implemented properly, fire modeling can be useful in predicting ignition, fire spread, burned area, and fire products after the initial nuclear blast.
The combustion completeness (CC) is the fraction of fuel that is burned in a fire. For all fires, combustion completeness is controlled by the fire characteristics, which are dependent on fuel loading, composition, and density, as well as meteorological parameters. Of note, combustibility is often delimited to specific fire-exposure conditions. For example, building materials are considered combustible if they are capable of undergoing combustion in air at a pressure and temperature that might occur during a fire in a building. Similarly, some materials that are not combustible under such conditions may be combustible when exposed to a higher temperature or pressure or to an oxygen-enriched environment. Materials that are not combustible in bulk form may be combustible in finely divided form.
Characterization of fuel density and fuel thickness is important for understanding combustion completeness. In wildfires, thin fuels, such as leaves and tree limbs, usually burn first, while thick fuels, such as tree trunks, may not burn. Urban fires may burn a higher percentage of thick fuels than wildfires, as buildings can retain the heat of combustion within the structure (Brown et al., 2023), and in a firestorm, nearly all combustible material may burn. Fuel moisture content also determines the extent of combustion. In wildland fires, moisture content of the vegetation can control the combustion completeness. This may be different from urban areas, where wood-based building materials may have less than 5% moisture content (Hedayati et al., 2018) and significant amounts of synthetic material may be present.
Combustion completeness for wildland biomass burning is included in Table 3-4, where values range from 0.47 to 0.81 (van Leeuwen et al., 2014), with values dependent on the ecosystem, among other things, such as fuel condition and weather. Values for combustion completeness within the nuclear winter literature are presented by Brown et al. (2023) and are included here in Table 3-9. Note that these values
are estimates and highly uncertain, as there is a lack of data on combustion completeness in urban fires. Many studies report the fuel consumed or fire parameters, such as the heat flux, without quantifying an assumption for combustion completeness. These past studies have accounted for the possibility of incomplete combustion. In urban areas, it is also possible that noncombustible materials that are rubblized in the blast may cover combustible materials and prevent them from burning, a factor that could reduce the combustion completeness significantly in areas that primarily contain concrete structures.
TABLE 3-9 Combustion Completeness Assumptions for Studies Focusing on Urban Scenarios
| Fraction Burned | Study |
|---|---|
| 0.19 urban | Turco et al., 1983 |
| 0.75 urban 0.20–0.25 forest |
NRC, 1985 |
| 0.50 | Reitter et al., 1982 |
| 0.50 | Veregin, 1993 |
SOURCE: Brown et al. 2023.
There are numerous uncertainties related to fire ignition, spread, burned area, and fuel consumption. Fuel characteristics (e.g., moisture content, albedo) are not well characterized or constrained, leading to uncertainty in the conditions required for ignition and fire spread. Additionally, there is a lack of understanding regarding the importance of ignition from thermal output of the weapon relative to ignition from blast-damaged buildings and infrastructure (see Chapter 2 for additional discussion) (Glasstone and Dolan, 1977). In the Hiroshima firestorm, secondary ignitions were reported to have played a large role in the initial fire starts, reminiscent of the fires following the San Francisco earthquake in 1906 (Scawthorn, 1986; Wilton et al., 1981).
Fire-spread models often do not predict the observed behavior well, due to the lack of available fuel data, parameterization of physical processes, and limited validation, particularly those in the WUI and in urban areas. Few models include chemistry and there are remaining questions about chemistry near the interior of the fire area, including oxygen-limited zones that may impact fuel combustion and fire spread. The amount of flaming versus smoldering combustion is important for the determination of fuel consumption and resulting emissions, and calculating plume height; however, current models do not constrain these well.
It might be expected that the urban fuels are rubblized in the initial stages of the blasts. However, it is not well understood how rubblized fuels, versus standing fuels, would burn in a fire or whether in certain scenarios subsequent detonations closely spaced in time could serve to quench fires from earlier detonations. It is possible that ruptured fuel lines and smoldering debris from a previous detonation could restart fires and increase fuel consumption. Fire spread will also be impacted by the ambient atmospheric conditions—including weather and seasonality—and by fire weather and winds, and the turbulence associated with a fire, which are not well constrained. These interactions may result in negative feedbacks to fire spread. Many studies of the climate effects from nuclear detonations assume that every detonation will become a mass fire; however, this outcome is unlikely. Improved fuel characterization and fire modeling tools will enable improved predictions of fire behavior, and previously developed criteria for firestorm formation can be applied to determine the likelihood of a mass fire for given fuel and atmospheric conditions.
The efficacy of firefighting as a means to constrain fire spread and burn area after a detonation is unknown. In Hiroshima and Nagasaki, most of the firefighting equipment was destroyed, and firefighting personnel were killed or unable to approach the fire (U.S. Strategic Bombing Survey, 1946). Damage was
sustained to the water distribution system resulting in a drop in water pressure, which also limited firefighting abilities (Maurer et al., 2009). The degree to which modern fire-resistive construction and firefighting will limit fire spread after a nuclear detonation is not well understood.
Overall, the type and amount of fuel that is burned, which is important in the determination of the emissions, is very important, and not well constrained, particularly when it is a combination of urban and vegetative fuels and overestimating the fire effects can lead to predicting more emissions to the atmosphere and more climatic and environmental impacts.
The emissions of aerosols and gases from fires can be parameterized by emission factors, expressed as the mass of emitted pollutant per quantity of fuel burned. The type of fuel that is burned can control what is emitted and the quantity. Emission factors from wildland fires have been characterized through laboratory studies (e.g., (Hatch et al., 2019; Stockwell et al., 2014) and in the field (e.g., Karl et al., 2007; Kaufman et al., 1998; Permar et al., 2021; Warneke et al., 2023). There have been several efforts to compile the results of these many studies to produce consistent and summarized data for use in modeling applications (e.g., (Akagi et al., 2011; Andreae, 2019; Holder et al., 2023; May et al., 2014).
Many hundreds of gas-phase species have been measured from wildland fire burning, as well as bulk particulate species and chemical components of particulate matter. Andreae (2019) compiled wildland fire emission factors from recent studies (some of which are included in Table 3-10). This compilation includes factors representing a complete wildland fire (rather than emissions calculated from different fuel components, such as the duff, crown, or trunk), although it is recognized that emissions are also dependent on the fire stage and the fuel conditions.
| Species | Savanna and grassland | Tropical forest | Temperate forest | Boreal forest | Forest average | Garbage burning |
|---|---|---|---|---|---|---|
| OC | 3.04 | 4.45 | 10.87 | 5.89 | 7.07 | 5.49 |
| BC or EC | 0.53 | 0.51 | 0.55 | 0.43 | 0.50 | 1.38 |
| BC/OC | 0.18 | 0.11 | 0.05 | 0.07 | 0.08 | 0.25 |
| Total NMOG, including unidentified | 29.90 | 51.90 | 39.00 | 58.70 | 49.9 | 22.60 |
| NOx (as NO) | 2.49 | 2.81 | 3.02 | 1.18 | 2.34 | 1.45 |
| PAHs | 0.012 | 0.15 | 0.017 | 0.72 | 0.2944 | 0.0280 |
NOTE: BC = black carbon; EC = elemental carbon; OC = particulate organic carbon; NMOG = non-methane organic gases; PAHs = polycyclic aromatic hydrocarbons.
SOURCE: Adapted from Andreae, 2019.
In forest biomes, wildfires oxidize most of the carbon in fuels to carbon dioxide and carbon monoxide (>99%), with the production of methane, non-methane organic gases (NMOGs), and OC accounting for most of the remainder (Andreae, 2019). BC typically is only 5% to 11% of primary OC production. Emission factors for BC are remarkably similar across tropical, temperate, and boreal forest ecosystems, with the mean values from the Andreae (2019) synthesis varying between 0.44 and 0.55 g/kg.
These estimates are relatively well constrained by observations from 26 separate field campaigns and standard deviations across different biomes varying between 0.21 and 0.36 g/kg (Table 3-10).
The physical and optical properties of aerosols emitted from biomass burning have also been characterized in numerous studies. Kaufman et al. (1998) and Remer and Kaufman (1998) found that the single-scattering albedo, or ratio of scattering efficiency to total extinction efficiency of a particle, of biomass burning aerosol in Brazil ranged from 0.82 to 0.94). The mean diameter of particles released by biomass burning are correlated with the combustion efficiency of the fire (Adler et al., 2011; Eck et al., 2001). The Fire Laboratory at Missoula Experiments study measured the geometric mean diameter of fresh biomass burning emissions of 0.20 – 0.57 µm and aerosol effective refractive indexes with values ranging from 1.41 to 1.61 (Levin et al., 2010).
Analogs, although imperfect, for emissions from urban fires ignited from a nuclear exchange may come from emission factors derived from the burning of other human-based materials, such as garbage and the burning of buildings and vehicles in the WUI. Garbage-burning measurements are sparse in the Andreae (2019) synthesis, with only three available studies. The BC emission factor for this class of burning (1.4 g/kg with a standard deviation of 5.1 g/kg), which presumably contains a broader range of combustible materials, including plastics, is nearly a factor of 3 higher than the mean of emission factors measured for forests. Gullett et al. (2017) estimated the emissions of BC, OC, polycyclic aromatic hydrocarbons (PAHs) and other pollutants of the Deepwater Horizon surface oil burns and derived a BC emission factor of 53 g/kg and OC of 4.1 g/kg. Middlebrook et al. (2012) estimated a BC emission factor of 39 g/kg from their in-situ measurements around the same event.
Brown et al. (2023) suggests a 2.5% smoke yield for a mix of fuels representative of urban areas and notes the importance of categorizing thick and thin fuels, which is not typically done in urban inventories, so that fire spread models can later use this information when calculating the rate and completeness with which the fuels will burn. Emissions from the combustion of urban fuels are described at length in the National Academies report on Chemistry of Fires at the Wildland-Urban Interface (NASEM, 2022). Current understanding of urban fire emissions is derived primarily from experimental fires, typically enclosure fires, with limited full-scale fire simulations. The results were highly variable as experiments were performed with differing fuel types, fuel loading, and combustion conditions (e.g., temperature and ventilation) (NASEM, 2022). Further, Holder et al. (2023) synthesize emission factors from the burning of urban fuels. For structures, they recommend an BC emission factor of 7.68 g/kg and an EC/OC ratio of 4.4 (much higher than the average waste burning emission factor from Andreae 2019). They report the emission factors of other trace gases, toxic compounds and metals that are emitted when urban fuels are burned. Table 3-11 shows a sample of the compiled emission factors from Holder et al. (2023).
TABLE 3-11 Key Emission Factors (g/kg) from Urban Fuels
| Species Name | Structure | Vehicle |
|---|---|---|
| PM | 39.3 | 57.2 |
| Elemental carbon (EC) | 7.68 | |
| Organic carbon (OC) | 1.76 | |
| EC/OC | 4.4 | |
| NOx | 0.331 | 4 |
| NO | 0.5 | 2 |
| SO2 | 0.0625 | 1.9 |
| PAHs | 0.0677 | 1.1 |
SOURCE: Adapted from Holder et al., 2023.
In contrast to the varied field observations from studies of wildfires and urban environments, the representation of emissions in nuclear studies has primarily been limited to BC. In addition, the representation of the BC emission factors in nuclear war studies is considerably higher than those used for wildland and urban fires. Small (1989) describes the fuel burned and smoke emissions from 4300 target areas in the United States (between the 30- and 60-degree latitude bands) based on the fuel loading at various land-use categories (residential; commercial; industrial; transportation, utility, communication; hydrocarbon stores; urban open; nonurban). In their scenarios, all biomass within an urban target area is assumed to burn, and smoke emissions ranges from 1 to 10 Tg from the various land-use categories, totaling 37 Tg for all sites.
The various nuclear studies differed in many ways, from the amount of BC injected into the atmosphere, the height and locations of the injections, the model resolution and top height, the implementation of coupled Earth system components, the inclusion of additional emitted species, the physical and optical properties of the emitted particles, and the length of the simulations. For example, Reisner et al. (2018; 2019) do not use an emission factor for BC and rather assumed that all the carbon in the fuel participated in the reaction and was turned into BC in their modeling. This is equivalent to using a 1,000 g/kg BC emission factor. Their estimates represent upper bounds for the given fuel loadings (worst case) and are higher than they would be if a detailed chemical-combustion soot production model was used. For fuel conditions, the worst case “no-rubble” scenario was compared with the more realistic “rubble” scenario. The no-rubble simulation produced a significantly more intense fire, with more fire spread and a significantly stronger plume resulting in larger amounts of BC reaching into the upper atmosphere. Assuming a linear relationship between BC loading and climate response, the use of a range of emission factors measured in urban and biomass fuels studies in this study would have yielded a negligible global impact, which most likely would have been indistinguishable from internal climate variability in the ensemble of control simulations. Toon et al. (2019) assumed that all the available fuel in the initial target-area fire zone is consumed when a firestorm forms. For conflagrations, they allowed 50% of the fuel within the initial ignition zone to be burned. They adopted average BC emission factor of 20 g BC/kg fuel burned, with the consideration of the range of fuel types and combustion conditions expected under nuclear attack scenarios. This value is more than 2.6 times higher than the mean of structure burns (Holder et al., 2023) and about 40 times higher than the mean reported for wildfires in forests (Andreae, 2019). Differences in emission factors are influenced by the composition and condition of the fuels, as well as the combustion conditions (e.g., ventilation, temperatures).
There are global biomass burning inventories that can be used as a comparison to these nuclear war studies. For example, at a global scale, the Global Fire Emissions Database version 4 with small fires (GFEDv4.1s) estimates that, on average, between 1997 and 2016, total BC emissions summed from fires in all biomes was 1.86 Tg BC/yr (van der Werf et al., 2017). This global estimate includes fire emissions from savannas, shrublands, peatlands, and agriculture, in addition to forest fires. Estimates of aerosol emissions from bottom-up fire emissions inventories often underestimate observed trends and variability in aerosol optical depth (AOD) measurements when they are used as a surface boundary condition in atmospheric models. Starting with the GFEDv4.1s emissions, Xu et al. (2021) used Aeronet AOD stations (Holben et al., 1998) in high-fire regions to optimize the magnitude of fire aerosol emissions. This optimization considerably improves model comparisons with Moderate Resolution Imaging Spectroradiometer (MODIS) satellite AOD observations that were held in reserve for validation and leads to an annual global flux of 3.9 Tg of BC and 46 Tg of primary particulate organic matter (POM) emissions. These estimates for BC and POM flux from global fires help provide context for recent studies exploring the climate impacts of nuclear war. For example, the Reisner et al. (2018) no-rubble scenario generated a total of 3.69 Tg of BC from the detonation of nuclear weapons in 100 cities across Pakistan and India. Similarly, the lowest nuclear exchange scenario explored for climate impacts by Toon et al. (2019) assumed emissions of 5 Tg BC. Both of these estimates are comparable to the annual BC production from all global contemporary wildfires.
As noted above, nuclear war studies up to this point have primarily included only the emissions of BC. However, many other species are emitted in fires that can have an important influence on the resulting atmospheric and environmental impacts. Specifically, OC or POM can be emitted in significant amounts and can also control the lofting, chemistry, and physical composition of the plume. Although the original TTAPS simulations included a substantial fraction of OC in their smoke emissions (70%, Section 3.2.1.5), only a few recent studies (Pausata et al., 2016; Wagman et al., 2020) included the emissions of both BC and POM in their simulations. Further, emissions of NMOG can impact gas-phase chemistry and form secondary organic aerosol in the atmosphere, thus, playing a role in the atmospheric aerosol composition and physical characteristics.
Other pollutants, such as sulfur dioxide, ammonia, nitrogen oxides, halogen-containing compounds, and metals can all have important downwind impacts to be considered when evaluating the environmental impacts of nuclear war. For example, in the troposphere, emissions of NOx and NMOCs in fire plumes may impact tropospheric ozone formation (e.g., (Jaffe et al., 2020). NOx and water vapor may also have chemical impacts in the stratosphere. Bardeen et al. (2021) included the combined emissions of NO and BC from different nuclear war scenarios. Here, they assumed 1x1032 molecules of NO injected per Mt of yield (NRC, 1985) for the fireball and 2 g NO per kg fuel burned (Bardeen et al., 2021). This value is within the values reported for wildland and urban combustion (Andreae, 2019; Holder et al., 2023). NOx in the stratosphere may lead to the decrease in stratospheric ozone (see Chapter 4 and 5).
There are many uncertainties and key data gaps associated with the parameterization and inclusion of emissions from fires that result from a nuclear blast. Prior nuclear war studies primarily included emissions of BC; only a few studies included the emissions of other pollutants, namely POM and NO. Emissions of pollutants other than BC are likely, even though they have not been typically included in past studies. Further, the emission factors of BC applied in many of the past studies are much larger than those from published literature from wildland and urban fires. For example, some nuclear war studies assumed a BC emission factor of 20 g BC/kg, whereas BC emission factors from wildland and structure fires range from 0.5 g BC/kg to ~ 8 g BC/kg. Emission factors of BC from urban fires are highly uncertain, as are the emission factors of other key pollutants such as OC. The inclusion of OC, as well as the ratio of emitted BC to emitted OC is important to quantify the lofting, deposition, and ultimately, the atmospheric lifetime of particles in the atmosphere. The optical properties of the emitted aerosols are not well constrained and could influence the atmospheric and climatic impacts of the emitted aerosols.
The inclusion of NO emissions in these studies can be important when considering the tropospheric and stratospheric impacts. One study (Bardeen et al., 2021; Mills et al., 2014) included a reasonable emission factor for NO. Yet, these emissions are also not well constrained. There are many other pollutants that may be emitted in wildland and urban fires. These include NMOGs, some of which can react to affect tropospheric ozone or form secondary organic aerosols and thereby influence the aerosol loading of the plume; NO and water vapor that may impact the ozone chemistry in the troposphere and stratosphere; metals, dioxins, PAHs, and other contaminants that can produce negative downwind air quality and ecological impacts. The emission factors of these pollutants are highly uncertain and vary significantly between different urban, rural and wildland fuels.
As discussed in Chapter 2, there are scenarios in which surface debris can be injected directly into the stratosphere when a blast occurs. These emissions are not included in the fire emission factor estimates; the amount and characteristics are not constrained.
The estimated emissions from various nuclear blast scenarios are dependent on the components discussed in these earlier sections. The area of the blast and resulting fires, and features including topography and weather, the fuels to be burned, the amount of fuel consumed in the initial blast and
resulting fires all determine the fire behavior and emissions. To predict the emissions of a given scenario of a nuclear detonation(s), the fuel loading on the surface—including the structure density and composition as well as the vegetation—needs to be well constrained. The type of blast will determine the extent to which the resulting fires and blast will impact those fuels. And based on the type of fuel and the extent to which the fuels are burned, the emissions can be estimated. These factors also relate to the heat flux and energy of the fires and lofting of emissions, the longevity of emissions in the atmosphere, and associated impacts as will be discussed in the following chapters. These are further complicated depending on the spatiotemporal relationship of subsequent blasts and the scenario, with questions as to whether these would have additive or somehow otherwise interacting characteristics.
FINDING 3-1: Fuel composition and loading—which are important in the estimation of fire spread and fuel consumption, the assignment of emission factors, and the prediction of the resulting plume height—of urban, suburban, and industrial areas are not well-characterized and vary significantly across the world. These also differ significantly from those of rural and wildland regions, for which more is known. Accurately characterizing fuel loading for a given nuclear exchange scenario is important in determining downstream environmental effects.
RECOMMENDATION 3-1: The National Nuclear Security Administration should coordinate with other federal agencies (e.g., the U.S. Departments of Agriculture, Defense, and Justice, the Federal Emergency Management Agency, the National Institute of Standards and Technology, and the National Science Foundation) to fund research by national laboratories and independent researchers with requisite capabilities to develop an ecosystem of modeling of urban fuels and buildings that would reduce uncertainties in the estimate of fire spread and emissions. These efforts should include:
FINDING 3-2: Physical and environmental conditions, including rubblization, humidity, and topography, will have significant impact on the ignition and spread of fires following the detonation of a nuclear weapon.
FINDING 3-3: Existing ignition and spread models lack the detail needed to evaluate fire behavior in urban and wildland–urban interface areas that may result from a nuclear detonation, both in understanding the physics of fire dynamics and spread, and at the level needed to understand the resultant chemistry.
RECOMMENDATION 3-2: The National Nuclear Security Administration should coordinate with other federal agencies (e.g., U.S. Departments of Agriculture, Defense, and Justice, the Federal Emergency Management Agency, the National Institute of Standards and Technology, and the National Science Foundation) to fund research by national laboratories and independent researchers with requisite capabilities to support model development and experimental studies to improve understanding of fire ignition, spread,
and fuel consumption, and validate the models and assumptions particularly for urban and wildland–urban interface areas. These studies should consider the conditions that will produce likely upper and lower bounds with respect to fire ignition, spread, and fuel consumption, including dampening effects such as shielding, rubblization, and atmospheric humidity.
FINDING 3-4: The quantities of emitted black carbon and organic carbon, as well as optical and physical properties of emitted particulate matter, are important for determining plume behavior and potential downstream environmental effects from fires resulting from a nuclear detonation, but highly uncertain.
RECOMMENDATION 3-3: When estimating the emissions from a nuclear explosion and resulting fires, appropriate ranges of all emissions—including black carbon and organic carbon, trace gases, and other pollutants—should be determined and sensitivity analyses performed.
RECOMMENDATION 3-4: EENW researchers should improve on estimates of the quantity and physical and optical properties of black carbon and organic carbon including size upon emission to evaluate the environmental impacts of a nuclear explosion and resulting fires.
FINDING 3-5: Emissions of other trace gases and toxins during a nuclear blast have not been studied but can have important impacts on potential EENW. These emissions, particularly from burning of urban and wildland–urban interface fuels, are highly uncertain.
RECOMMENDATION 3-5: Researchers and firefighting agencies (e.g., the Federal Emergency Management Agency) should work together to measure aerosol and trace gas composition of fires in urban and suburban environments. This recommendation is directly related to the research agenda in the NASEM (2022) WUI report, and the information from these campaigns would also advance many goals related to better understanding fire effects on human health.
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