## 1. Introduction

Longwave spectra observed from space have been used for retrieving atmospheric temperature vertical profiles (e.g., Wark and Fleming 1966; Chahine 1968, 1977), water vapor amounts and vertical profiles (e.g., Susskind et al. 2003), and cloud-top heights (e.g., Kahn et al. 2007; Menzel et al. 2008; Minnis et al. 2007). The atmospheric changes expected to occur in response to a forcing, therefore, can in principle be inferred from longwave spectrum changes. Retrieving atmospheric properties such as temperature and water vapor profiles, however, usually requires clear-sky scenes (e.g., Chahine et al. 2006; Susskind et al. 2006), although some recently developed retrieval algorithms allow clouds in a field of view (Zhou et al. 2007; Liu et al. 2007, 2009). As a consequence, the retrieval yield varies temporally and spatially depending on clear-sky occurrence. Temperature and water vapor profiles in atmospheric conditions that are preferentially avoided are absent in the retrieved data. Furthermore, results of cloud screening algorithms (e.g., Ackerman et al. 1998; Frey et al. 2008) and cloud property retrievals (e.g., Nakajima and King 1990; Minnis et al. 1998; Platnick et al. 2001) using visible wavelengths often contain a viewing zenith angle dependent error (e.g., Loeb and Coakley 1998; Zuidema and Evans 1998) that must also be accounted for when inferring mean cloud property changes. In order for instantaneously retrieved properties to be used to infer atmospheric changes over time, the effects of the instantaneous retrieval error on the mean value need to be investigated. While earlier studies investigated the temperature and humidity retrieval accuracy and yield (e.g., Tobin et al. 2006; Fetzer et al. 2003; Fetzer et al. 2004), as well as the effects of cloud optical thickness and particle size retrieval errors on a domain average (e.g., Kato et al. 2006; Kato and Marshak 2009), further studies are required to understand the effects on climate data.

An alternative to the retrieve-and-average approach to inferring atmospheric changes is an average-and-retrieve approach. Earlier studies have used temporally and spatially averaged spectral radiance differences from two time periods to infer atmospheric and cloud property changes. For example, Leroy et al. (2008) used clear-sky-averaged spectral radiance to estimate the temperature and humidity changes between two time periods. Huang et al. (2010) extended the optimal detection technique of Leroy et al. (2008) to all-sky conditions. The study by Huang et al. (2010) is based on climate model simulations so that cloud properties may be different from actual clouds (e.g., Norris and Weaver 2001; Bony et al. 2004). Due to computational restrictions, earlier studies have not accounted for temporal scale variabilities of less than a month and spatial scale variabilities of less than several hundred kilometers. As shown in section 2, the temporally and spatially averaged spectral radiance observed by a satellite instrument is affected by variability occurring at instantaneous temporal and spatial sampling scales. In this study, we further extend earlier studies to consider the variability present at an instantaneous sampling scale and to investigate how the variability affects inferring the atmospheric change from highly averaged spectral radiance differences.

Toward understanding the variability present at an instantaneous sampling scale by satellite instruments, three objectives of this study are

to understand how the variability present at a satellite instrument’s temporal and sampling spatial scales (small-scale variability) affects the retrieval of atmospheric and cloud property changes from highly averaged spectral radiances,

to quantify how small-scale variability influences the atmospheric and cloud property change detection method, and

to understand how clouds affect the variability and spectral signals.

In this study, we simulate instantaneous nadir-view spectral radiances using cloud properties derived from satellite observations on a 20-km footprint to achieve the objectives above. We then perturb the atmospheric properties and compute the spectral radiances, maintaining the instantaneous temporal and spatial resolutions to test the effects of variability on the spectral signal. Our simulation, therefore, differs from the earlier studies that used climate-model-derived monthly mean atmospheric properties (Huang et al. 2010). We use a linear regression to retrieve the temperature, humidity, and cloud property changes from the nadir-view spectral radiance change, similar to earlier studies (Leroy et al. 2008; Huang et al. 2010).

The retrieval is performed by seeking consistent atmospheric and cloud property changes with the observed spectral radiance change. Our retrieval goal is to infer changes that occur on a shorter time scale (up to a decade) instead of a longer time scale (~100 yr), as was sometimes used in earlier studies. As the observation continues, the trend of the atmospheric and cloud property changes can be inferred from these retrieved properties, or changes can be detected by directly applying the average-and-retrieve technique to the spectral radiance difference derived from a longer time period. Our purpose in inferring atmospheric changes contrasts with studies that find the best combination of responses to a particular external forcing modeled by climate models, and how the response changes the top-of-the-atmosphere (TOA) spectral radiance. As a result, we do not distinguish between changes caused by anthropogenic forcing and those from natural variability in this study.

Section 2 briefly explains the motivation for investigating the effects of small-scale variability and section 3 describes the modeling of spectral radiance. Section 4 describes the results of the spectral radiance change at nadir caused by atmospheric and cloud property perturbations, and tests the necessary conditions for retrieving atmospheric changes by a linear regression. Finally, the retrieval process is demonstrated in section 5 while a discussion of the findings and our conclusions are presented in sections 6 and 7, respectively.

## 2. Effects of observed high temporal and spatial variabilities on atmospheric change detection

*I*measured over the time period 1 is

**is an atmospheric property such as temperature, humidity, or cloud property. The overbar indicates the annual mean,**

*x**δ*

*x*is its small-scale variability (i.e., deviation from the mean) present at satellite sampling scale, and

*n*is the number of satellite observations used to determine the annual mean value. Many atmospheric properties influence the TOA spectral radiance. The different variables are expressed by the subscript

*j*. The subscript

*i*indicates an individual sampling during time period 1. The spectral radiance sensitivity to the variable

*x*at an instantaneous observation

_{j}*δ*

*x*and

_{ji}*x*is the atmospheric or cloud property deviation from the mean value of the time period 1 and

*x*when the mean atmospheric and cloud properties are from time period 1. The second term in the bracket accounts for the deviation of the sensitivity at an instantaneous scale from the sensitivity of the mean atmospheric and cloud properties of time period 1.

_{j}*x*in Eq. (2) into two components—the mean change of time period 2 from the mean value of time period 1 and the small-scale variability,

_{ji}## 3. Spectral radiance computations

To include the small-scale variability present at the satellite sampling scale, we use satellite-observed cloud fields in our simulations because, as shown in section 4b, spectral radiance variability is largely caused by clouds. Therefore, it is important to use realistic cloud fields to test the effects of variability on atmospheric and cloud change detection.

### a. Cloud fields

The cloud fields used in this study were derived from Moderate Resolution Imaging Spectroradiometer (MODIS) spectral radiance observations. MODIS-retrieved cloud properties are included in the Clouds and the Earth’s Radiant Energy System (CERES) Single Scanner Footprint (SSF) product. Cloud properties derived from MODIS are output from the second edition (Ed2) of the CERES cloud algorithm (Minnis et al. 2007) based on the assumption of a single-layer overcast cloud in a 1-km pixel. As a result, there are no overlapping clouds within a CERES footprint and up to two single-layer cloud properties were kept within a CERES footprint.

### b. Computation of TOA spectra viewed from nadir

Two years’ worth of MODIS-derived cloud fields from January 2003 through December 2004 are used as a control run. Temperature and water vapor profiles from the Goddard Earth Observing System Data Assimilation System (GEOS-4; Bloom et al. 2005) are used for the simulation. Ozone profiles are retrieved daily from the Solar Backscatter Ultraviolet instrument (SBUV/2; Bhartia et al. 1996). For the polar region during polar night, the ozone profiles are retrieved from the Television and Infrared Observation Satellite (TIROS) Operational Vertical Sounder (TOVS) by the algorithm of Neuendorffer (1996). Retrieved ozone profiles are sorted into daily maps of 2.5° × 2.5° grids with 24 pressure levels (Yang et al. 2011).

TOA longwave nadir-view spectra from 50 to 2760 cm^{−1} are computed with a 1.0 cm^{−1} resolution by the Principal Component-based Radiative Transfer Model (PCRTM; Liu et al. 2006) using the independent column approximation (Stephens et al. 1991; Cahalan et al. 1994). The spectroscopic High-Resolution Transmission Molecular Absorption Database (HITRAN 2000) is used for atmospheric molecular transmittance calculations. Spectral radiances are computed at *Terra* overpass times and are averaged to obtain zonal and global means.

We adapt a method that performs cloud radiative transfer calculations using precomputed cloud transmittances and reflectances (Yang et al. 2001; Wei et al. 2007; Huang et al. 2004; Niu et al. 2007). The complex refractive indexes of ice and water are taken from Warren (1984) and Segelstein (1981). The individual ice cloud particle size distributions are derived from various field campaigns as described by Baum et al. (2007). The single-scattering properties, such as phase function and single-scattering albedo, are derived from the finite-difference time domain method, the improved geometric optics method, or Lorenz–Mie theory, depending on the size and shape of the cloud particles. A gamma size distribution is assumed for water clouds. The surface emissivity depends on surface type but does not vary with time.

In addition to the control run, we perturb the atmospheric properties and compute the TOA spectral radiance (perturbed runs). Only the first 15 days in each month are selected for perturbation calculations due to computational constraints. Fifteen cloud and atmospheric properties listed in Table 1 are perturbed independently. In perturbing cloud properties, clouds are separated into three types depending on their top height, according to the International Satellite Cloud Climatology Project (ISCCP) cloud classifications (Rossow and Schiffer 1991). Clouds with cloud-top heights of 6.5 km or higher are classified as high-level clouds, clouds with cloud top heights of 3.5 km or lower are classified as low-level clouds, and clouds in between are midlevel clouds. For perturbation 5 in Table 1, thin cirrus clouds were defined as having an optical thickness of less than 1. The values listed in Table 1 are used to perturb the atmospheric and cloud properties uniformly at all latitudes.

Perturbed values in the simulation.

* RMS computed with all ice clouds.

We make a subtle but important modification to the GEOS-4 temperature profile to make the temperature profile consistent with the MODIS-derived cloud-top heights. When the low-level cloud height is increased by 250 m in the cloud-top perturbation run, the temperature inversion present at the top of boundary layer clouds is also moved with the cloud to prevent the resulting cloud-top height from becoming higher than the temperature inversion height. To adjust the temperature profile, we first compute the lapse rate in the boundary layer with the original GEOS-4 temperature profile. Second, when the low-level cloud is moved upward by 250 m, we extend the boundary layer so that the lapse rate from the surface to the new cloud top is the same as the original lapse rate below the cloud.

Note that the boundary layer cloud-top height and the height of the temperature inversion do not necessarily agree in the control run. In the case when the cloud-top and temperature inversion heights do not agree in the control run, the temperature inversion height is adjusted in the same way described above. Hence, the temperature inversion height also agrees with the boundary layer cloud-top height in the control run.

Table 1 lists the magnitudes of the perturbations used for perturbed runs. Each perturbation magnitude is determined in one of two ways. One way is to match approximately the root-mean-square (RMS) difference of 10° zonal monthly means computed from the 2003 and 2004 atmospheres (approximately equal to the standard deviation of deseasonalized anomalies). The other way is to use the expected global mean changes between the first two decades (2000–09 and 2010–19) of a simulation of the Intergovernmental Panel on Climate Change (IPCC) Special Report on Emission Scenario (SRES) A1B forced by the National Center for Atmospheric Research (NCAR) Community Climate System Model (CCSM), version 3.0 (Collins et al. 2006). A reasonable magnitude of expected atmospheric and cloud property changes are used to test the linear relationship between these properties and TOA spectral irradiance changes in the presence of small-scale variability.

## 4. Results

As noted in the previous section, atmosphere and cloud properties are perturbed at a 20-km spatial resolution and an instantaneous temporal resolution to include the effects of small-scale variability. Because our purpose is to compute a spectral radiance change for the atmospheric and cloud property change retrieval, all perturbations listed in Table 1 are applied to all regions uniformly. Instantaneous spectral radiances are averaged monthly at 10° latitude intervals. Monthly zonal mean spectral radiance changes due to perturbations are computed by differencing the control run and perturbed run spectral radiances. The global mean spectral radiance or brightness temperature change is computed by averaging the zonal mean spectral radiances weighted by their area, and subtracting the global mean radiance (or brightness temperature) of the control run from the global mean value of a perturbed run.

### a. Spectral radiance change

Figure 1 shows the global annual mean brightness temperature difference caused by perturbations listed in Table 1. The shape of the spectral radiance changes from some perturbations is expected to be similar for the following reasons.

The contribution function of the atmospheric emission to the TOA radiance for a given wavenumber peaks at the height where the absorption optical thickness is approximately equal to one (Goody and Yung 1989). The absorption optical thickness of the clear-sky atmosphere is often less than one in the window spectral regions from 800 to 1200 cm^{−1} and beyond 2000 cm^{−1}. Therefore, the emission in these spectral regions mostly comes from the surface. In spectral regions where gaseous absorption is strong, the atmosphere is opaque. Therefore, changes in the surface temperature have little effect on the TOA radiance in spectral regions of the water vapor rotation band below 500 cm^{−1}, the *ν*_{2} vibration-rotation band centered at 1595 cm^{−1}, and the CO_{2} vibration-rotation band centered at 667 cm^{−1}. Because most low-level clouds are opaque at infrared wavelengths, increasing the low-level cloud height, which reduces the cloud-top temperature, yields a spectral radiance change similar to the surface temperature increase with an opposite sign in the window regions. However, the emissivity of low-level clouds in the window region is not spectrally constant. As a consequence, the cloud-top height perturbation gives a nonuniform effective cloud-top temperature change as opposed to a spectrally constant radiance change in response to the surface temperature perturbation. This difference leads to spectral shape differences in the window region.

The spectral shapes of the brightness temperature change due to cirrus cloud optical thickness perturbation and due to upper-tropospheric relative humidity perturbation are quite different (Fig. 1). When the cirrus cloud optical thickness is increased, the emission height changes from a lower altitude to a higher altitude in the spectral region in which clouds are translucent. In contrast, the spectral change due to upper-tropospheric humidity perturbation occurs in stronger water vapor lines where the emission from water vapor originates in the upper troposphere.

The effects of the cloud particle size change are one order of magnitude smaller than the spectral radiance change by the optical thickness, cloud height, and fraction perturbations (Fig. 1). The longwave radiance is sensitive to cloud particle size change when the clouds are translucent and the particle sizes are not so large [e.g., ~100-*μ*m diameter for ice particles; Cooper et al. (2006)]. The distinct feature of the spectral shape can potentially help to separate cloud microphysical changes from macrophysical changes, if particle size changes occur in optically thin clouds.

### b. Necessary conditions for a linear regression

To accurately retrieve atmospheric and cloud property changes by a linear regression, several conditions must be satisfied. First, the sum of the spectral changes caused by individual perturbations must be approximately equal to the spectral change caused by all individual properties perturbed simultaneously. Second, although all wavenumbers used in the retrieval do not need to respond linearly, the radiance for a given wavenumber needs to change approximately linearly in response to an atmospheric or cloud property perturbation. Third, the spectral shape caused by each atmospheric or cloud property change must be unique, meaning that a linear regression can identify individual spectral shapes from the sum of all spectral signals.

To test the effects of small-scale variability on the first condition, we combined perturbations (1 and 5–12 listed in Table 1) and computed the global annual mean spectra to evaluate whether the sum of the spectral changes computed independently is equal to the spectral change from the combined run in which all are perturbed together. Because small-scale variability is included in both the individual and combined runs, term 2 in Eq. (4) is the same in both the individual and combined runs. In addition, because the independent runs and combined run use the same time period, the small-scale variabilities in those runs are the same. Hence, terms 4 and 5 in Eq. (4) cancel out when one result is subtracted from the other. Therefore, the spectral radiance difference is due to the nonlinear term [term 3 in Eq. (4)] that is included in the combined run but excluded in the sum of the independent runs.

Figure 2 shows that the difference is less than 10% (relative difference less than 0.1) of the signal, except around 1200 and 2000 cm^{−1} (Fig. 2, bottom left). Note that large differences around 650 cm^{−1} are due to dividing by a small value, as indicated by the top-left plot in Fig. 2. A nonlinear effect can occur, for example, when a larger surface area with a higher temperature is exposed to space as a result of a mean cloud fraction decrease and a mean surface temperature increase. If the cloud fraction change is not included (i.e., the combined run includes 1, 5–8, and 12 in Table 1), the nonlinear term is 1% (Fig. 2, bottom left). Therefore, the cloud fraction change significantly contributes to the nonlinear term. Water vapor amount perturbations also cause a nonlinear effect when both the surface temperature and humidity are perturbed. The transmittance of the signal from the surface temperature change is altered as a result of a smaller atmospheric water vapor amount. The atmospheric transmission change by the humidity perturbation is, however, smaller than the cloud fraction perturbation.

(top left) Absolute value of the annual global mean spectral radiance change computed by perturbing 1 and 5–12 listed in Table 1 simultaneously (top curve) and the spectral radiance difference between the spectral radiance change of all perturbed simultaneously and the sum of the spectral radiance changes computed by perturbing 1 and 5–12 independently and then summing the spectral radiance changes (bottom curve). (top right) As in the top-left panel, but here cloud fraction perturbations are excluded (i.e., perturbation 1, 5–8, and 12 in Table 1). The bottom two plots show the ratio of the bottom curve to the top curve shown in the top two plots.

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

(top left) Absolute value of the annual global mean spectral radiance change computed by perturbing 1 and 5–12 listed in Table 1 simultaneously (top curve) and the spectral radiance difference between the spectral radiance change of all perturbed simultaneously and the sum of the spectral radiance changes computed by perturbing 1 and 5–12 independently and then summing the spectral radiance changes (bottom curve). (top right) As in the top-left panel, but here cloud fraction perturbations are excluded (i.e., perturbation 1, 5–8, and 12 in Table 1). The bottom two plots show the ratio of the bottom curve to the top curve shown in the top two plots.

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

(top left) Absolute value of the annual global mean spectral radiance change computed by perturbing 1 and 5–12 listed in Table 1 simultaneously (top curve) and the spectral radiance difference between the spectral radiance change of all perturbed simultaneously and the sum of the spectral radiance changes computed by perturbing 1 and 5–12 independently and then summing the spectral radiance changes (bottom curve). (top right) As in the top-left panel, but here cloud fraction perturbations are excluded (i.e., perturbation 1, 5–8, and 12 in Table 1). The bottom two plots show the ratio of the bottom curve to the top curve shown in the top two plots.

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

In addition, Fig. 3 shows, for each 10° latitude zone, the annual mean RMS relative difference between the spectral radiance change computed by perturbing the atmospheric and cloud properties of 1 and 5–12 listed in Table 1 (solid line) simultaneously (Δ*I _{s}*) and the sum of the spectral radiance change computed by perturbing these properties individually (Δ

*I*). The 10° mean relative RMS difference is computed from Δ

_{i}*I*− Δ

_{s}*I*over wavenumber and divided by the RMS of Δ

_{i}*I*computed also over wavenumber using monthly mean spectral radiances. The annual mean RMS difference is computed by averaging the monthly relative differences. The percent error in the estimated spectral radiance difference obtained by assuming linear combinations of individual perturbations expressed as an RMS difference is 10%–15%, except over Antarctica (Fig. 3). The maximum and minimum relative differences of the monthly 10° zonal means are 16% and 3%, respectively, when the two southernmost 10° latitudinal zones are excluded. Figure 3 also shows that when cloud fraction changes are excluded, the RMS difference is less than 2% for most 10° zones. The magnitude of the nonlinear term with clouds is consistent with a study by Huang et al. (2010), who perturbed the monthly mean atmospheres to test this condition. However, our results show that the magnitude of the nonlinear term changes significantly with and without cloud fraction perturbation, while the results of Huang et al. (2010) show that the magnitude and shape of the nonlinear term are similar with and without cloud property changes.

_{s}Annual and 10° zonal mean RMS relative difference between the spectral radiance change computed by perturbing atmospheric properties of 1 and 5–12 listed in Table 1 (solid line) simultaneously (Δ**I*** _{s}*) and the sum of the spectral radiance change computed by perturbing these properties individually (Δ

**I**

*). The annual mean relative difference is computed by the RMS of Δ*

_{i}**I**

*Δ*

_{s}−**I**

*computed over the wavenumber and divided by the RMS of Δ*

_{i}**I**

*computed also over the wavenumber using monthly mean values and averaging the monthly relative differences. The wavenumber region used for the RMS computation is from 200 to 2000 cm*

_{s}^{−1}. The vertical line indicates the maximum and minimum value among monthly means. The lower dashed line indicates the annual and zonal mean RMS relative difference computed without cloud fraction perturbations (i.e., 1, 5–8, and 12 in Table 1).

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

Annual and 10° zonal mean RMS relative difference between the spectral radiance change computed by perturbing atmospheric properties of 1 and 5–12 listed in Table 1 (solid line) simultaneously (Δ**I*** _{s}*) and the sum of the spectral radiance change computed by perturbing these properties individually (Δ

**I**

*). The annual mean relative difference is computed by the RMS of Δ*

_{i}**I**

*Δ*

_{s}−**I**

*computed over the wavenumber and divided by the RMS of Δ*

_{i}**I**

*computed also over the wavenumber using monthly mean values and averaging the monthly relative differences. The wavenumber region used for the RMS computation is from 200 to 2000 cm*

_{s}^{−1}. The vertical line indicates the maximum and minimum value among monthly means. The lower dashed line indicates the annual and zonal mean RMS relative difference computed without cloud fraction perturbations (i.e., 1, 5–8, and 12 in Table 1).

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

Annual and 10° zonal mean RMS relative difference between the spectral radiance change computed by perturbing atmospheric properties of 1 and 5–12 listed in Table 1 (solid line) simultaneously (Δ**I*** _{s}*) and the sum of the spectral radiance change computed by perturbing these properties individually (Δ

**I**

*). The annual mean relative difference is computed by the RMS of Δ*

_{i}**I**

*Δ*

_{s}−**I**

*computed over the wavenumber and divided by the RMS of Δ*

_{i}**I**

*computed also over the wavenumber using monthly mean values and averaging the monthly relative differences. The wavenumber region used for the RMS computation is from 200 to 2000 cm*

_{s}^{−1}. The vertical line indicates the maximum and minimum value among monthly means. The lower dashed line indicates the annual and zonal mean RMS relative difference computed without cloud fraction perturbations (i.e., 1, 5–8, and 12 in Table 1).

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

To further test the effects of small-scale variability on signal linearity (second condition listed above), we doubled the perturbation amount and evaluated whether or not the spectral radiance change is also doubled. Figure 4 shows the difference in the monthly and annual 10° zonal mean spectral changes due to Δ*x _{i}* and 2Δ

*x*–Δ

_{i}*x*. The spectral radiance changes linearly for temperature changes so that

_{i}*x*and 2Δ

_{i}*x*–Δ

_{i}*x*computed from the monthly mean and annual mean are similar, indicating that for given mean atmospheric and cloud property changes, the linear relationship is nearly insensitive to the length of the temporal averaging period. A better linear response is achieved by using a longer temporal averaging period because the mean atmospheric and cloud property changes are smaller when a longer temporal period is used.

_{i}Ratio of the mean difference of the 10° zonal monthly spectral radiance changes computed by doubling the perturbation amount Δ**I**(2Δ**x**) minus Δ**I**(Δ**x**) to Δ**I**(Δ**x**) (blue line), where Δ**x** is the amount of atmospheric and cloud property perturbation given by Table 1. The ratio is computed with monthly 10° mean spectral radiance changes, and 12 monthly mean ratios from 70°S to 90°N (16 zones) are averaged. The red line is the same as the blue line except that the annual 10° zonal mean radiance changes are used to compute the ratio and 16 zonal ratios are averaged. When the response is linear to the perturbation, the ratio is 1 at all wavenumbers. A 10-wavenumber moving window is used to eliminate spikes caused by dividing by a small number.

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

Ratio of the mean difference of the 10° zonal monthly spectral radiance changes computed by doubling the perturbation amount Δ**I**(2Δ**x**) minus Δ**I**(Δ**x**) to Δ**I**(Δ**x**) (blue line), where Δ**x** is the amount of atmospheric and cloud property perturbation given by Table 1. The ratio is computed with monthly 10° mean spectral radiance changes, and 12 monthly mean ratios from 70°S to 90°N (16 zones) are averaged. The red line is the same as the blue line except that the annual 10° zonal mean radiance changes are used to compute the ratio and 16 zonal ratios are averaged. When the response is linear to the perturbation, the ratio is 1 at all wavenumbers. A 10-wavenumber moving window is used to eliminate spikes caused by dividing by a small number.

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

Ratio of the mean difference of the 10° zonal monthly spectral radiance changes computed by doubling the perturbation amount Δ**I**(2Δ**x**) minus Δ**I**(Δ**x**) to Δ**I**(Δ**x**) (blue line), where Δ**x** is the amount of atmospheric and cloud property perturbation given by Table 1. The ratio is computed with monthly 10° mean spectral radiance changes, and 12 monthly mean ratios from 70°S to 90°N (16 zones) are averaged. The red line is the same as the blue line except that the annual 10° zonal mean radiance changes are used to compute the ratio and 16 zonal ratios are averaged. When the response is linear to the perturbation, the ratio is 1 at all wavenumbers. A 10-wavenumber moving window is used to eliminate spikes caused by dividing by a small number.

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

**I**is expressed by a linear combination of the spectral signature matrix

**a**:

**I**

*and*

_{b}*are, respectively, the modeling bias and random errors. The spectral radiance difference Δ*

**ϵ****I**is a column vector of dimension

*m*. The spectral signature matrix

*m*row ×

*n*column matrix that contains distinguishing spectral radiance changes where

*m*is the number of wavenumbers and

*n*is the number of perturbed atmospheric properties used to compute the spectral changes. Columns of

**S**are the average of

**S**are the same as Δ

**I**, elements of

**a**are nondimensional. Elements of

**a**are, therefore, scaling factors to the perturbed amount Δ

**x**used to compute the elements of

**I**in this study, the modeling errors have no impact on the retrieval. Note that the effects of small-scale variability (terms 4 and 5) are estimated in section 5.

**I**. We use the spectral radiance change Δ

**I**computed by perturbing the variables listed in Table 1 (i.e., variables 1, 4–10, and 14) simultaneously to test whether or not the shape of the spectral radiance change given by an individual perturbation is correctly separated by a linear regression. When there is no error term, a simple linear regression for retrieving the atmospheric and cloud property changes is

For a perfect retrieval, the elements of **a** are all unity in this simulation. When we obtained **a** by neglecting a nonlinear term, the error was less than 10% except for the midlevel cloud fraction (Table 2). When the nonlinear term (term 3) is included in **a**. This result suggests that all spectral shapes of radiance changes used in this study are different and can be separated by a linear regression.

Effects of nonlinear terms. Computed from monthly mean 10° retrievals. Numbers in parenthesis are RMS errors computed from 10° monthly means (192 values, 12 months × 16 zones).

In summary, our results suggest that the TOA spectral radiance change can be expressed approximately by a linear combination of the TOA spectral radiance changes computed by perturbing the atmospheric properties independently. The spectral difference between the linear combination of the spectra perturbed independently and the spectrum computed by simultaneously perturbing all atmospheric variables is approximately 10%–15% expressed by the relative RMS difference over the wavenumber between 200 and 2000 cm^{−1} (Fig. 3). The relative difference around spectral regions 1200 and 2000 cm^{−1} can be as large as 100% when the cloud fraction change is included (Fig. 2). The TOA longwave spectrum changes linearly in the perturbation of the atmospheric temperature and water vapor when it is perturbed within the variability of 10° zonal deseasonalized monthly anomalies or within the magnitude of a decadal change predicted by a climate model (Fig. 4). TOA longwave spectral radiance also changes linearly in the perturbation of a cloud property except for low- and middle-level cloud-height perturbations. When the low- and midlevel cloud-height perturbations are doubled, the annual 10° zonal mean spectral radiance change at water vapor absorption bands, wavenumbers less than 500 cm^{−1}, and between 1300 and 2000 cm^{−1} significantly deviates from a linear relationship. The broad spectral feature that deviates from a linear relationship is an error source when Eq. (8) is applied to Δ**I** when the change in the atmospheric properties or cloud properties is large. The shape of the spectral radiance changes is different such that the individual spectral radiance changes can be separated from the spectral radiance change computed by perturbing all variables simultaneously using a linear regression. When the nonlinear term is neglected in a spectral signature matrix, the retrieval error is less than 10% for most cases (Table 2). The spectral difference by midlevel cloud fraction perturbation is, however, approximately 20%. Presumably, the spectral shape of the nonlinear term is somewhat similar to the spectral shape of the midlevel cloud fraction perturbation.

## 5. Retrieval simulation

Two error terms (terms 4 and 5) do not affect the retrieval result of a simple simulation, as demonstrated in the previous section. In this section, we assess the effects of terms 4 and 5 in the retrieval. For the simulation, we use the annual 10° zonal mean spectral radiance in this study. In the simulation, we treat the spectral difference of the 2003 and 2004 control runs as the observed spectral difference and test whether or not temperature, humidity, and cloud property differences between the 2003 and 2004 data used for control runs can accurately be retrieved.

^{−12}, while the radiance change is of the order of 10

^{−4}W m

^{−2}sr

^{−1}cm. When the matrix is inverted to obtain

**a**, small errors in the elements of

**a**(Twomey 1977). To avoid a large error in

**a**, we introduce a smoothing constraint:

*λ*is a Lagrange multiplier. For the simulation, we use an identity matrix

**a**

*(Twomey 1977), which simply increases all eigenvalues by a constant amount. To determine the value of*

_{c}*λ*, we compute the RMS difference between the retrieved

**a**

*and the true values for the annual 10° zonal means as a function of*

_{c}*λ*. Based on the result of the RMS difference as a function of

*λ*, we use

*λ*= 1.0 × 10

^{−7}for our simulation.

We derive **a*** _{c}* over a 10° latitudinal zone separately using Eq. (9). We then compare

**a**

*multiplied by the perturbed value used in perturbed runs Δ*

_{c}**x**

^{T}

**a**

*with the atmospheric and cloud property changes computed from atmospheric and cloud properties used to compute spectral radiances in the control run (true values). Figure 5 shows the retrieved values versus the true values. While atmospheric temperatures, especially stratospheric temperatures, are retrieved well, our results indicate that the retrieved cloud properties obtained with this average-and-retrieve approach have sizable errors and large estimated uncertainties.*

_{c}Comparison of retrieved atmospheric and cloud property changes by Eq. (9) (open blue circles) vs true values (filled red circles) used in spectral radiance computations. One data point represents a retrieval result from the annual 10° zonal spectral radiance difference. The atmospheric property differences from 2004 to 2003 are used for the plots. The error bars are the square root of the diagonal terms of * ϵ* is the sum of terms 4 and 5 in Eq. (4), multiplied by the perturbed amount. The error bars for retrieved cloud properties are omitted because they span the entire range of the

*y*axis used for the plots.

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

Comparison of retrieved atmospheric and cloud property changes by Eq. (9) (open blue circles) vs true values (filled red circles) used in spectral radiance computations. One data point represents a retrieval result from the annual 10° zonal spectral radiance difference. The atmospheric property differences from 2004 to 2003 are used for the plots. The error bars are the square root of the diagonal terms of * ϵ* is the sum of terms 4 and 5 in Eq. (4), multiplied by the perturbed amount. The error bars for retrieved cloud properties are omitted because they span the entire range of the

*y*axis used for the plots.

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

Comparison of retrieved atmospheric and cloud property changes by Eq. (9) (open blue circles) vs true values (filled red circles) used in spectral radiance computations. One data point represents a retrieval result from the annual 10° zonal spectral radiance difference. The atmospheric property differences from 2004 to 2003 are used for the plots. The error bars are the square root of the diagonal terms of * ϵ* is the sum of terms 4 and 5 in Eq. (4), multiplied by the perturbed amount. The error bars for retrieved cloud properties are omitted because they span the entire range of the

*y*axis used for the plots.

Citation: Journal of Climate 24, 24; 10.1175/JCLI-D-10-05005.1

**x**(04–03), by the perturbed amount Δ

**x**,

*m × l*error matrix

*′, where*

**ϵ***m*is the number of wavenumbers and

*l*is the number of 10° zones (=16 because the two southernmost zones are dropped) and the prime indicates that the mean over 10° zones is subtracted so that the mean is zero for each wavenumbers (i.e.,

*l × l*matrix of which elements are all 1). We compute an

*n × n*covariance matrix by

*′*

**ϵ***′*

**ϵ**^{T})

*n*is the number of retrieved variables. We set

*λ*= 0, which gives the upper limit of the uncertainty estimate due to terms 4 and 5 to crudely account for using

*′ (the mean = 0) instead of*

**ϵ***. For this limit, the expression is equivalent to*

**ϵ***y*range of the plot, the error bars were omitted from the retrieved cloud property plots. The uncertainties averaged over eighteen 10° zones are ±2.0 km, ±0.2, and ±0.4 for low cloud height, low cloud fraction, and high cloud fraction, respectively.

Note that brightness temperature differences can be used in the spectral signature matrix and Δ**I** for the retrieval, but we find that the retrieval errors are significantly smaller, especially for cloud properties, when radiance differences are used. The exact reason is unknown but when brightness temperature differences are used, the difference in the far- and near-infrared spectral regions is emphasized compared to the difference computed from radiances.

## 6. Discussion

*δx*is largely due to the variability of cloud properties.

_{ji}There are several possible ways to reduce the retrieval error. If, for example, terms 4 and 5 are related to the standard deviation of the spectral radiance, it might be possible to estimate these terms from the mean and standard deviation of the spectral radiance. Subsequently, they are subtracted from ΔI before the inversion. Another possible way to reduce the error in the retrieval is by separating clear-sky scenes from cloudy-sky scenes because clouds are responsible for much of the small-scale variability. Using only clear-sky spectral change reduces the error in retrieving temperature and humidity profile changes. Subsequently, constraining the temperature and humidity changes in the retrieval under the all-sky conditions might reduce the error in the retrieved cloud property changes. Investigating the method to reduce the retrieval error is left for future studies.

Optimizing a linear regression using empirical orthogonal functions (EOFs) of a covariance matrix (* ϵ*′

*′*

**ϵ**^{T}) and omitting smaller eigenvalues instead of using Eq. (9), is an alternative approach. We, however, used Eq. (9) in this study because the retrieval result is sensitive to the covariance matrix, as the results of Huang et al. (2010) imply. Perhaps the proper way to form the covariance matrix is to use temporal correlation instead of spatial correlation. We did not have enough simulated spectral radiances to form the temporal correlation in this study. Therefore, to exclude the effects of the covariance matrix, we used Eq. (9). We found, however, that applying the covariance matrix based on spatial correlation worsens the retrieval result. Unlike the instrument noise, which has a different spectral shape than the signals, terms 4 and 5 are caused by the small-scale variability of clouds and atmospheric properties. As a consequence, they could have similar spectral shapes as signals. Whether EOFs and a properly formed covariance matrix help to improve the retrieval still needs to be tested in the future.

## 7. Conclusions

To understand the effects of small-scale variability on atmospheric temperature, humidity, and cloud property change detection, we computed the spectral radiance using high temporal (instantaneous) and spatial (~20 km) resolutions and simulated the variability of observed radiances in the nadir direction. We tested the necessary conditions to retrieve atmospheric and cloud property changes from spatially and temporally averaged spectral radiances by a linear regression. Our results show that the annual 10° zonal mean spectral radiance changes linearly with respect to the temperature and humidity perturbations when they are perturbed either by the amount of changes expected to happen in a decade or by the RMS difference of 10° zonal monthly means between 2003 and 2004. The spectral radiance due to cloud-height perturbations changes nonlinearly outside the window region, especially for low-level clouds. The sum of the spectral changes computed by perturbing atmospheric properties independently is equal to within 10%–15% of the spectral change computed by perturbing all properties simultaneously for most spectral regions. Cloud fraction changes are largely responsible for the difference. When cloud fraction changes are excluded, the difference decreases to less than 2%. Spectral shapes of the radiance change caused by different atmospheric and cloud property changes are separated by a linear regression. Variability present at an instantaneous resolution does not affect the establishment of these conditions necessary for atmospheric and cloud property change detections by a linear regression as much as it affects the retrieval. Our simulation indicates that retrieved atmospheric and cloud property changes from the annual 10° zonal mean spectral radiance changes contain errors, especially in retrieved cloud properties, because small-scale variability affecting the mean spectral radiance from two periods does not necessarily cancel. As a consequence, the residual becomes a bias error in the spectral radiance difference computed from two time periods. Two possible ways to improve the retrieval are 1) to perform the retrieval using clear sky only and constrain the temperature and humidity changes in the all-sky retrieval and 2) to seek the relationship between the standard deviation of the spectral radiance and small-scale variability terms. Using the relationship, bias errors caused by small-scale variability can be subtracted from the spectral radiance difference. Investigating ways to improve the retrieval is left for future studies.

## Acknowledgments

We thank Drs. Stephen Leroy, John Dykema, Yi Huang, Xianglei Huang, Robert Knuteson, Norman Loeb, and Oleg Dubovik for helpful discussions and suggestions and two anonymous reviewers for constructive and very helpful comments. We also thank Ms. Amber Richards for proofreading the manuscript. The work was supported by the NASA Science Directorate through the CLARREO project.

## APPENDIX A

### Cloud Effects on the TOA Spectral Radiance

*B*is the Planck function,

_{ν}*T*

_{sfc}is the surface temperature, and

*τ*

_{ν0}is the optical thickness of the atmosphere. The subscript

*ν*indicates that the optical thickness is wavelength dependent. The nadir-view radiance for overcast cloudy sky is

*τ*

*is the spectral-dependent cloud optical thickness and the source function*

_{νc}*J*is

_{ν}*ω*

_{0}is the single-scattering albedo,

*P*(

*μ*,

*ϕ*) is the phase function,

*μ*is the cosine of the zenith angle, and

*ϕ*is the azimuth angle. For the partly cloudy sky, the nadir-view radiance is assumed to be the sum of the clear-sky and overcast radiances weighted by the cloud fraction

*f*.

*T*

_{sfc}and Δ

*T*, respectively. When we expand the Planck function by a Taylor expansion and keep the first term, the nadir-view radiance difference is

*I*

_{cld}has a different spectral dependence from Δ

*I*

_{clr}because the spectrally dependent deference is between

*τ*

_{ν0}and

*τ*

_{νc}.

## APPENDIX B

### Contribution of Terms 4 and 5 to the Covariance of Retrieved Properties

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