| 6.3.4 Total Well-Mixed Greenhouse Gas Forcing Estimate The radiative forcing due to all well-mixed greenhouse gases since pre-industrial 
  times was estimated to be 2.45 Wm-2 in the SAR with an uncertainty 
  of 15%. This is now altered to a radiative forcing of 2.43 Wm-2 with 
  an uncertainty of 10%, based on the range of model results and the discussion 
  of factors leading to uncertainties in the radiative forcing due to these greenhouse 
  gases. The uncertainty in the radiative forcing due to CO2 is estimated 
  to be smaller than for the other well-mixed greenhouse gases; less than 10% 
  (Section 6.3.1). For the CH4 forcing the main 
  uncertainty is connected to the radiative transfer code itself and is estimated 
  to be about 15% (Section 6.3.2). The uncertainty in N2O 
  (Section 6.3.2) is similar to that for CO2, 
  whereas the main uncertainties for halocarbons arise from the spectroscopic 
  data. The estimated uncertainty for halocarbons is 10 to 15% for the most frequently 
  studied species, but higher for some of the less investigated molecules (Section 
  6.3.3). A small increase in the concentrations of the 
  well-mixed greenhouse gases since the SAR has compensated for the reduction 
  in radiative forcing resulting from improved radiative transfer calculations. 
  The rate of increase in the well-mixed greenhouse gas concentrations, and thereby 
  the radiative forcing, has been smaller over the first half of the 1990s compared 
  to previous decades (see also Hansen et al., 1998). This is mainly a result 
  of reduced growth in CO2 and CH4 concentrations and smaller 
  increase or even reduction in the concentration of some of the halocarbons.6.3.5 Simplified Expressions IPCC (1990) used simplified analytical expressions for the well-mixed greenhouse 
  gases based in part on Hansen et al. (1988). With updates of the radiative forcing, 
  the simplified expressions need to be reconsidered, especially for CO2 
  and N2O. Shi (1992) investigated simplified expressions for the well-mixed 
  greenhouse gases and Hansen et al. (1988, 1998) presented a simplified expression 
  for CO2. Myhre et al. (1998b) used the previous IPCC expressions 
  with new constants, finding good agreement (within 5%) with high spectral resolution 
  radiative transfer calculations. The already well established and simple functional 
  forms of the expressions used in IPCC (1990), and their excellent agreement 
  with explicit radiative transfer calculations, are strong bases for their continued 
  usage, albeit with revised values of the constants, as listed in Table 
  6.2. Shi (1992) has suggested more physically based and accurate expressions 
  which account for (i) additional absorption bands that could yield a separate 
  functional form besides the one in IPCC (1990), and (ii) a better treatment 
  of the overlap between gases. WMO (1999) used a simplified expression for CO2 
  based on Hansen et al. (1988) and this simplified expression is used in the 
  calculations of GWP in Section 6.12. For CO2 
  the simplified expressions from Shi (1992) and Hansen et al. (1988) are also 
  listed alongside the IPCC (1990)-like expression for CO2 in Table 
  6.2. Compared to IPCC (1990) and the SAR and for similar changes in the 
  concentrations of well-mixed greenhouse gases, the improved simplified expressions 
  result in a 15% decrease in the estimate of the radiative forcing by CO2 
  (first row in Table 6.2), a 15% decrease in the case of 
  N2O, an increase of 10 to 15% in the case of CFC-11 and CFC-12, and 
  no change in the case of CH4. 
   
    | Table 6.2: Simplified expressions for calculation 
      of radiative forcing due to CO2, CH4, N2O, 
      and halocarbons. The first row for CO2 lists an expression with 
      a form similar to IPCC (1990) but with newer values of the constants. The 
      second row for CO2 is a more complete and updated expression 
      similar in form to that of Shi (1992). The third row expression for CO2 
      is from WMO (1999), based in turn on Hansen et al. (1988). |   
    |  |   
    | Trace gas | Simplified expression Radiative forcing,  F 
        (Wm-2) | Constants |   
    |  |   
    | CO2 |  F =  ln(C/C0) |  = 5.35 |   
    |  |  F=  ln(C/C0) 
      + ß (  C -  C0) |  = 4.841, ß = 
      0.0906 |   
    |  |  F=  (g(C)–g(C0)) where g(C)= ln(1+1.2C+0.005C2 +1.4 x 10-6C3)
 |  = 3.35 |   
    |  |   
    | CH4 |  F=  (  M 
      –  M0) – 
      (f(M,N0) – f(M0,N0)) |  = 0.036 |   
    |  |   
    | N2O |  F=  (  N 
      –  N0) – (f(M0,N) 
      – f(M0,N0)) |  = 0.12 |   
    |  |   
    | CFC-11a |  F=  (X 
      – X0) |  = 0.25 |   
    |  |   
    | CFC-12 |  F=  (X 
      – X0) |  = 0.32 |   
    |  |   
    
   |