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Virtual temperature
Virtual temperature
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In atmospheric thermodynamics, the virtual temperature () of a moist air parcel is the temperature at which a theoretical dry air parcel would have a total pressure and density equal to the moist parcel of air.[1] The virtual temperature of unsaturated moist air is always greater than the absolute air temperature, however, as the existence of suspended cloud droplets reduces the virtual temperature.

The virtual temperature effect is also known as the vapor buoyancy effect.[2] It has been described to increase Earth's thermal emission by warming the tropical atmosphere.[3][4]

Introduction

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Description

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In atmospheric thermodynamic processes, it is often useful to assume air parcels behave approximately adiabatically, and approximately ideally. The specific gas constant for the standardized mass of one kilogram of a particular gas is variable, and described mathematically as

where is the molar gas constant, and is the apparent molar mass of gas in kilograms per mole. The apparent molar mass of a theoretical moist parcel in Earth's atmosphere can be defined in components of water vapor and dry air as

with being partial pressure of water, dry air pressure, and and representing the molar masses of water vapor and dry air respectively. The total pressure is described by Dalton's law of partial pressures:

Purpose

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Rather than carry out these calculations, it is convenient to scale another quantity within the ideal gas law to equate the pressure and density of a dry parcel to a moist parcel. The only variable quantity of the ideal gas law independent of density and pressure is temperature. This scaled quantity is known as virtual temperature, and it allows for the use of the dry-air equation of state for moist air.[5] Temperature has an inverse proportionality to density. Thus, analytically, a higher vapor pressure would yield a lower density, which should yield a higher virtual temperature in turn.[citation needed]

Derivation

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Consider a moist air parcel containing masses and of dry air and water vapor in a given volume . The density is given by

where and are the densities the dry air and water vapor would respectively have when occupying the volume of the air parcel. Rearranging the standard ideal gas equation with these variables gives

and

Solving for the densities in each equation and combining with the law of partial pressures yields

Then, solving for and using is approximately 0.622 in Earth's atmosphere:

where the virtual temperature is

We now have a non-linear scalar for temperature dependent purely on the unitless value , allowing for varying amounts of water vapor in an air parcel. This virtual temperature in units of kelvin can be used seamlessly in any thermodynamic equation necessitating it.

Variations

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Often the more easily accessible atmospheric parameter is the mixing ratio . Through expansion upon the definition of vapor pressure in the law of partial pressures as presented above and the definition of mixing ratio:

which allows

Algebraic expansion of that equation, ignoring higher orders of due to its typical order in Earth's atmosphere of , and substituting with its constant value yields the linear approximation


With the mixing ratio expressed in g/g.[6]

An approximate conversion using in degrees Celsius and mixing ratio in g/kg is[7]

Knowing that specific humidity is given in terms of mixing ratio as , then we can write mixing ratio in terms of the specific humidity as . We can now write the virtual temperature in terms of specific humidity as

Simplifying the above will reduce to

and using the value of , then we can write

Virtual potential temperature

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Virtual potential temperature is similar to potential temperature in that it removes the temperature variation caused by changes in pressure. Virtual potential temperature is useful as a surrogate for density in buoyancy calculations and in turbulence transport which includes vertical air movement.

Density temperature

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A moist air parcel may also contain liquid droplets and ice crystals in addition to water vapor. A net mixing ratio can be defined as the sum of the mixing ratios of water vapor , liquid , and ice present in the parcel. Assuming that and are typically much smaller than , a density temperature of a parcel can be defined, representing the temperature at which a theoretical dry air parcel would have the a pressure and density equal to a moist parcel of air while accounting for condensates:[8]: 113 

Uses

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Virtual temperature is used in adjusting CAPE soundings for assessing available convective potential energy from skew-T log-P diagrams. The errors associated with ignoring virtual temperature correction for smaller CAPE values can be quite significant.[9] Thus, in the early stages of convective storm formation, a virtual temperature correction is significant in identifying the potential intensity in tropical cyclogenesis.[10]

Further reading

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Virtual temperature is a fictitious temperature in atmospheric thermodynamics that represents the temperature a sample of dry air would need to achieve the same as a given sample of moist air at the same total and moisture content. It accounts for the lower molecular weight of water vapor compared to dry air, making moist air less dense than dry air at the same actual and , and thus virtual temperature is always slightly higher than the actual for humid conditions. The concept derives from the applied to moist air, where total pressure p=pd+ep = p_d + e (dry air partial pressure plus partial pressure) and total density ρ=ρd+ρv+ρl\rho = \rho_d + \rho_v + \rho_l (dry air, vapor, and liquid water densities), leading to the defining relation p=ρRdTvp = \rho R_d T_v, with RdR_d as the for dry air. A common approximation for the virtual temperature TvT_v is TvT(1+0.608q)T_v \approx T (1 + 0.608 q), where TT is the actual temperature in and qq is the water vapor mixing ratio (mass of vapor per mass of dry air); this factor 0.608 arises from the ratio of gas constants for and dry air (ϵ0.622\epsilon \approx 0.622). For more precision including liquid water, the formula extends to Tv=T1+q/ϵ1+q+lT_v = T \frac{1 + q/\epsilon}{1 + q + l}, where ll is the liquid water mixing ratio. In , virtual temperature is essential for evaluating air parcel and static stability, as it allows the use of dry-air equations for moist conditions in calculations like convective available potential energy (), which is critical for forecasting development. It also facilitates of atmospheric profiles, such as via radio acoustic sounding systems (RASS), and is used in modeling turbulent fluxes and hydrostatic balance in prediction models. By simplifying the treatment of moisture's effects, virtual temperature enhances accuracy in , numerical , and climate simulations without altering the fundamental dry-air framework.

Overview

Definition

Virtual temperature, denoted TvT_v, is defined as the temperature that a theoretical parcel of dry air would need to possess in order to have the same total and as an actual parcel of moist air at the same location. This construct arises in to account for the effects of on air while allowing moist air behavior to be approximated using dry air equations. The definition presupposes the ideal gas law for dry air, expressed as p=ρRdT,p = \rho R_d T, where pp is the total pressure, ρ\rho is the density, RdR_d is the specific gas constant for dry air (approximately 287 J kg⁻¹ K⁻¹), and TT is the temperature. In this framework, TvT_v adjusts the temperature term to reflect the lower density of moist air due to the lighter molecular weight of water vapor compared to dry air constituents. In unsaturated moist air, TvT_v exceeds the actual temperature TT because the presence of water vapor reduces the parcel's density relative to dry air at the same TT and pp. Conversely, in saturated air with suspended liquid water droplets (known as liquid water loading), the added mass of these denser droplets increases the overall density, resulting in TvT_v being lower than TT. Virtual temperature is measured in kelvin and functions as a scalar multiplier that can substitute for actual temperature in thermodynamic relations originally formulated for dry air.

Significance

The serves a critical purpose in by permitting the dry-air to be applied to moist air through a simple scaling, which streamlines hydrostatic balance computations and thermodynamic analyses in and climate models. This adjustment accounts for the lower of compared to dry air, avoiding the need for separate moist-air formulations and reducing in regions with significant . The concept of virtual temperature was first introduced by Cato Guldberg and Henrik Mohn in 1876. It has since been used to overcome shortcomings in representations of moist air dynamics, as exemplified in D. K. Lilly's 1968 analysis of cloud-topped mixed layers, where virtual temperature facilitated more accurate modeling of and stability under strong inversions. Without incorporating virtual temperature, miscalculations in humid environments can lead to errors in pressure-to-height conversions of up to 10-20 meters across tropospheric layers, particularly in the where moisture content is high. A key impact of virtual temperature lies in its representation of the vapor effect, which introduces an approximate 1 K warming in the tropical relative to actual ; this enhancement promotes greater in moist air parcels, thereby intensifying convective processes and contributing to increased clear-sky by about 1 W m⁻² globally. Such effects help stabilize the tropical through negative feedbacks that mitigate excessive warming in dry subsiding regions.

Physical Principles

Air Density and Water Vapor Effects

The density of moist air arises from its composition as a mixture of dry air and water vapor, treated as ideal gases following Dalton's law of partial pressures. According to this law, the total atmospheric pressure pp equals the sum of the partial pressure of dry air pdp_d and the vapor pressure ee: p=pd+ep = p_d + e. This partial pressure framework allows the densities of each component to be calculated separately using the ideal gas law. The molecular weight of dry air is approximately 29 g/mol, primarily from (28 g/mol) and oxygen (32 g/mol), whereas has a lower molecular weight of 18 g/mol. The total of moist air ρ\rho is thus the sum of the dry air ρd\rho_d and the ρv\rho_v: ρ=ρd+ρv\rho = \rho_d + \rho_v. Since molecules are lighter than the average dry air molecules they displace, the presence of reduces the overall mass per unit volume, making moist air less dense than dry air at the same and . This density reduction stems from variations in the ideal gas law for moist air. The specific gas constant for dry air is Rd287R_d \approx 287 J kg⁻¹ K⁻¹, while for water vapor it is Rv461R_v \approx 461 J kg⁻¹ K⁻¹, reflecting the inverse relationship with molecular weight. The effective gas constant RR for moist air can be expressed as R=Rd[1ep(1ϵ)]1R = R_d \left[1 - \frac{e}{p} (1 - \epsilon)\right]^{-1}, where ϵ=0.622\epsilon = 0.622 is the ratio of the molecular weight of water vapor to dry air (ϵ=Mv/Md\epsilon = M_v / M_d). At constant temperature TT and total pressure pp, the higher effective RR causes moist air to occupy a greater volume than dry air, further lowering its density by replacing heavier dry air molecules with lighter water vapor ones. In humid regions like the , where mixing ratios can exceed 20 g kg⁻¹, this effect becomes notable; for instance, at 30°C and a mixing ratio of 20 g kg⁻¹, the of moist air is reduced by approximately 1.2% compared to dry air at the same conditions. Overall, reductions reach up to 2-3% in highly saturated tropical air, enhancing and influencing atmospheric processes. This physical mechanism underpins the virtual temperature concept, which equates the of moist air to that of dry air at an adjusted .

Vapor Buoyancy Mechanism

In the atmosphere, the buoyancy acceleration of a rising air parcel is determined by b=gΔρρb = g \frac{\Delta \rho}{\rho}, where gg is the acceleration due to gravity, Δρ\Delta \rho is the density difference between the parcel and its environment, and ρ\rho is the environmental . This acceleration drives vertical motion, with positive occurring when the parcel density is lower than the surrounding air. Water contributes to this by reducing the overall of the moist parcel relative to dry air at the same and , as its molecular weight (18 g/mol) is lower than that of dry air (29 g/mol), thereby enhancing the ascent rate compared to an equivalent dry parcel. The vapor effect, quantified through , provides an equivalent perturbation that amplifies in moist air. For a mixing ratio of 10 g/kg, this effect corresponds to roughly 1-2 of warming in typical tropospheric conditions (around 280-300 ), promoting stronger updrafts in moist convective processes by making vapor-laden parcels effectively warmer and lighter. This dynamic enhancement is particularly pronounced in regions with high , where even modest increases in mixing ratio can significantly boost convective vigor. A key aspect of this mechanism is its dependence on the phase of water in the parcel. During unsaturated ascent, the virtual temperature directly increases owing to the low of alone. However, once saturation occurs and forms clouds, the added mass of liquid water droplets (liquid loading) increases the parcel's , often counteracting or reversing the vapor-induced gain and potentially slowing or inhibiting further ascent. This mechanism also influences Earth's global energy budget, particularly in the . By elevating the virtual temperature in moist regions and inducing compensatory warming in adjacent drier columns to maintain hydrostatic balance, the vapor buoyancy effect enhances clear-sky by approximately 1-3 W/m², providing a stabilizing feedback that increases as surface temperatures rise.

Formulation

Derivation

The derivation of the virtual temperature begins with the equation of state for moist air, treated as an mixture of dry air and under the assumptions of and of s. The of dry air is pd=pep_d = p - e, where pp is the total and ee is the . The density of dry air is given by ρd=pdRdT=peRdT,\rho_d = \frac{p_d}{R_d T} = \frac{p - e}{R_d T}, where RdR_d is the specific for dry air and TT is the actual temperature in . Similarly, the density of is ρv=eRvT,\rho_v = \frac{e}{R_v T}, with RvR_v as the specific for . The total density ρ\rho of unsaturated moist air (neglecting liquid water) is then ρ=ρd+ρv=peRdT+eRvT.[](http://www.atmo.arizona.edu/students/courselinks/spring10/atmo551b/VirtualTemperature.pdf)\rho = \rho_d + \rho_v = \frac{p - e}{R_d T} + \frac{e}{R_v T}.[](http://www.atmo.arizona.edu/students/courselinks/spring10/atmo551b/VirtualTemperature.pdf) The virtual temperature TvT_v is defined such that the moist air equals that of dry air at the same total pressure pp and TvT_v, using the dry air : ρ=pRdTv.[](http://www.atmo.arizona.edu/students/courselinks/spring10/atmo551b/VirtualTemperature.pdf)\rho = \frac{p}{R_d T_v}.[](http://www.atmo.arizona.edu/students/courselinks/spring10/atmo551b/VirtualTemperature.pdf) Equating the two expressions for ρ\rho, pRdTv=peRdT+eRvT.\frac{p}{R_d T_v} = \frac{p - e}{R_d T} + \frac{e}{R_v T}. Multiplying through by RdTR_d T yields pTTv=(pe)+eRdRv.\frac{p T}{T_v} = (p - e) + e \frac{R_d}{R_v}. The of gas constants is ε=RdRv0.622\varepsilon = \frac{R_d}{R_v} \approx 0.622, derived from the molar masses of dry air (Md28.97M_d \approx 28.97 g/mol) and (Mv=18M_v = 18 g/mol) via ε=MvMd\varepsilon = \frac{M_v}{M_d}, since Rd=RMdR_d = \frac{R^*}{M_d} and Rv=RMvR_v = \frac{R^*}{M_v} with RR^* the universal . Substituting gives pTv=pe(1ε)T,\frac{p}{T_v} = \frac{p - e(1 - \varepsilon)}{T}, and solving for TvT_v produces the exact formula Tv=T1ep(1ε).[](http://www.atmo.arizona.edu/students/courselinks/spring10/atmo551b/VirtualTemperature.pdf)T_v = \frac{T}{1 - \frac{e}{p} (1 - \varepsilon)}.[](http://www.atmo.arizona.edu/students/courselinks/spring10/atmo551b/VirtualTemperature.pdf) This derivation assumes ideal gas behavior for both components, negligible liquid water content (valid for unsaturated air), and that all constituents share the same TT. It is applicable below the homopause (approximately 90 km altitude) where dry air is well-mixed.

Approximate Expressions

In , linear approximations for virtual temperature simplify computations by relating it directly to the actual air temperature and a measure of , bypassing the need for precise calculations. A standard form uses specific humidity qq (in kg/kg):
TvT(1+0.608q),T_v \approx T (1 + 0.608 q),
valid for q<0.02q < 0.02 kg/kg, which encompasses most tropospheric scenarios where moisture content is moderate. This expression assumes small perturbations from dry air conditions and leverages the for moist air.
The coefficient 0.608 arises from the physical properties of air components, specifically (1ϵ)/ϵ0.608(1 - \epsilon)/\epsilon \approx 0.608, where ϵ=0.622\epsilon = 0.622 is the ratio of the molecular weight of water vapor to dry air (or equivalently, the ratio of their specific gas constants). This approximation holds under the condition of small e/pe/p, the ratio of vapor pressure to total pressure. For cases where mixing ratio ww (in g/kg) is the available humidity metric, equivalent approximations are:
TvT+w6T_v \approx T + \frac{w}{6}
(with TT and TvT_v in °C), or in Kelvin,
TvT(1+0.608w1000).T_v \approx T \left(1 + 0.608 \frac{w}{1000}\right).
These derive from the specific humidity form by noting w1000qw \approx 1000 q for low moisture levels, facilitating practical use in field measurements or models.
These linear forms yield errors below 0.5 in typical tropospheric conditions (e.g., w<20w < 20 g/kg), as higher-order terms in the expansion are negligible; however, inaccuracies grow in extreme exceeding these limits. They prove valuable for rapid assessments in analyses or forecasting tools lacking full thermodynamic data.

Virtual Potential Temperature

Virtual potential temperature, denoted θv\theta_v, is defined as the potential temperature derived from the virtual temperature TvT_v rather than the actual temperature TT. Specifically, θv=θ×(Tv/T)\theta_v = \theta \times (T_v / T), where θ\theta is the dry potential temperature given by θ=T(p0/p)Rd/Cp\theta = T (p_0 / p)^{R_d / C_p}, p0p_0 is the reference pressure (typically 1000 hPa), pp is the pressure, RdR_d is the specific gas constant for dry air, and CpC_p is the specific heat capacity of dry air at constant pressure. An approximate form is θvθ(1+0.608q)\theta_v \approx \theta (1 + 0.608 q), where qq is the water vapor mixing ratio (kg/kg); this approximation holds for typical atmospheric conditions in unsaturated moist air. In unsaturated moist air, θv\theta_v is conserved during adiabatic processes, such as vertical ascent or descent of an air parcel up to the lifting condensation level. Unlike virtual temperature TvT_v, which depends on and is not conserved in vertical motion, θv\theta_v remains constant under adiabatic conditions, providing a height-independent measure of potential. This property makes θv\theta_v valuable in stability and convective parcel , where it helps assess the potential for atmospheric without effects. The conservation of θv\theta_v applies only to unsaturated conditions, as condensation releases latent heat and deviates from dry adiabatic behavior. Parcel theory applications of θv\theta_v also assume no entrainment of environmental air, which can dilute buoyancy in real updrafts.

Density Temperature

Density temperature, denoted as TρT_\rho, is defined as the temperature that dry air would need to have in order to match the density of a moist air parcel containing both water vapor and condensed phases such as liquid droplets or ice crystals, at the same pressure. This concept extends the virtual temperature TvT_v by incorporating the mass loading effect of non-gaseous water substances. The formulation is given by Tρ=T1+w/ϵ1+wT,T_\rho = T \frac{1 + w / \epsilon}{1 + w_T}, where TT is the actual temperature of the moist air, ww is the water vapor mixing ratio (kg/kg), ϵ=0.622\epsilon = 0.622 is the ratio of the gas constants for dry air and water vapor, and wT=w+wL+wIw_T = w + w_L + w_I is the total water mixing ratio, with wLw_L and wIw_I representing the liquid water and ice mixing ratios, respectively. In unsaturated air, where wL=wI=0w_L = w_I = 0, TρT_\rho approximates TvT_v. The primary purpose of density temperature is to correct for the increased density caused by condensed water phases, which are denser than an equivalent mass of and thus reduce the buoyancy of cloudy air parcels compared to what virtual temperature alone would predict. Cloud droplets and ice particles add mass without contributing to the gas-phase , leading to a heavier parcel that sinks more readily; this loading effect is particularly significant in precipitating clouds, where Tρ<TvT_\rho < T_v by amounts on the order of 1 or more, depending on the condensed water content. For ice phases, the formula incorporates adjustments via wIw_I, accounting for the lower of relative to liquid , though the overall effect remains a density increase over vapor-only scenarios. Unlike virtual temperature, which addresses only the buoyancy enhancement from water vapor's lower molecular weight, density temperature explicitly includes the non-gaseous water to provide a more complete density equivalent for cloudy conditions. This distinction is crucial in assessing parcel , as the added weight from condensed phases can suppress . Density temperature is essential in cumulus parameterization schemes within numerical and models, where it helps evaluate the stability and vertical motion of updrafts by integrating both vapor and condensate effects.

Applications

Atmospheric Stability and Convection

Virtual temperature plays a crucial role in evaluating atmospheric stability and convective processes by accurately accounting for the buoyancy effects of in air parcels. In the calculation of (CAPE), which measures the potential for atmospheric , is integrated along the ascent path of a lifted parcel using virtual potential temperature (θ_v). The standard formulation involves CAPE=LFCELgθv,parcelθv,envθv,envdz\text{CAPE} = \int_{\text{LFC}}^{\text{EL}} g \frac{\theta_{v,\text{parcel}} - \theta_{v,\text{env}}}{\theta_{v,\text{env}}} \, dz where gg is gravitational acceleration, LFC is the level of free convection, and EL is the equilibrium level; this integration is typically performed on skew-T log-P diagrams to visualize parcel trajectories and environmental profiles. In atmospheric soundings, plotting virtual temperature (T_v) profiles enables adjustments to moist adiabats, uncovering hidden instabilities in humid layers where actual temperature alone might suggest stability. This correction highlights the enhanced of moist air relative to dry air, preventing underestimation of convective potential in vapor-rich environments. In tropical regions, neglecting the virtual correction can lead to substantial underestimation of in highly moist conditions, with relative errors increasing as decreases. Studies from the , such as those by Yang and Seidel, illustrate how virtual temperature effects contribute to stabilizing feedbacks in the through enhanced in moist columns.

Numerical Modeling and Forecasting

In (NWP) models, virtual temperature is incorporated into the hydrostatic equation, dpdz=ρg\frac{dp}{dz} = -\rho g, to compute air ρ\rho accurately and derive heights, ensuring precise vertical structure representations in moist atmospheres. This approach has been standard in major models since the 1990s, including the Weather Research and Forecasting (WRF) model, where dedicated functions calculate virtual temperature from and mixing ratio outputs for post-processing and diagnostic analyses. Similarly, the European Centre for Medium-Range Weather Forecasts (ECMWF) Integrated Forecasting System (IFS) employs virtual temperature in its spectral transformations for horizontal wind, , and , supporting hydrostatic balance computations across grid points. In climate modeling, virtual temperature parameterizes effects within general circulation models (GCMs) such as the Community Earth System Model (CESM), particularly in moist schemes that account for vapor's influence on atmospheric stability and vertical motion. For instance, CESM's Community Atmosphere Model uses virtual temperature to adjust thermodynamic profiles in microphysics and , enhancing simulations of convective processes. This incorporation extends to large-scale tropical dynamics, where virtual temperature profiles help model moisture-modified circulations and patterns in GCMs, improving fidelity in regions dominated by humid air masses. Post-2023 developments in AI-hybrid NWP systems, such as ECMWF's blending of the physics-based IFS with the Forecasting System (AIFS), utilize virtual temperature profiles to nudge large-scale components toward AI predictions, enabling faster assessments of atmospheric stability. These hybrids address limitations in older models by integrating virtual temperature into forecasts. Computationally, approximations of virtual temperature—such as those using mixing ratio directly with temperatures—reduce runtime in lower-resolution runs, while exact formulations are retained in high-resolution simulations to maintain accuracy in buoyancy-driven dynamics.

References

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