The SAR reported that several studies found a higher forcing due to CH₄ than IPCC (1990), up to 20%; however the recommendation was to use the same value as in IPCC (1990). The higher radiative forcing estimates were obtained using band models. Recent calculations using LBL and band models confirm these results (Lelieveld et al., 1998; Minschwaner et al., 1998; Jain et al., 2000). Using two band models, Myhre et al. (1998b) found the computed radiative forcing to differ by almost 10%. This was attributed to difficulties in the treatment of CH₄ in band models since, given its present abundance, the CH₄ absorption lies between the weak line and the strong line limits (Ramanathan et al., 1987). After updating for a small increase in concentration since the SAR, the radiative forcing due to CH₄ is 0.48 Wm^-2 since pre-industrial times. This estimate for forcing due to CH₄ is only for the direct effect of CH₄; for radiative forcing of the indirect effect of CH₄, see Sections 6.5 and 6.6.

The problem mentioned above with the band models for CH₄ does not occur to the same degree in the case of N₂O, given the latter’s present concentrations. Three recent studies, Myhre et al. (1998b) (two models), Minschwaner et al. (1998) (one model), and Jain et al. (2000) (one model), calculated lower radiative forcing for N₂O than reported in previous IPCC assessments, viz., 0.13, 0.12, 0.11, and 0.12 Wm^-2, respectively, compared to 0.14 Wm^-2 in the SAR. For N₂O, effects of change in spectroscopic data, stratospheric adjustment, and decay of the mixing ratio in the stratosphere are all found to be small effects. However, effects of clouds and different radiation schemes are potential sources for the difference between the newer estimates and the SAR. A value of 0.15 Wm^-2 is now suggested for the radiative forcing due to N₂O, taking into account an increase in the concentration since the SAR, together with a smaller pre-industrial concentration than assumed in IPCC (1996a; Table 2.2) (see Chapter 4).

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