Abstract. The hydroxyl radical (OH), which is the dominant sink of methane (CH4),
plays a key role in closing the global methane budget. Current top-down
estimates of the global and regional CH4 budget using 3D models usually
apply prescribed OH fields and attribute model–observation mismatches almost
exclusively to CH4 emissions, leaving the uncertainties due to
prescribed OH fields less quantified. Here, using a variational Bayesian
inversion framework and the 3D chemical transport model LMDz, combined with
10 different OH fields derived from chemistry–climate models (Chemistry–Climate Model Initiative, or CCMI, experiment), we evaluate the influence of OH burden, spatial distribution,
and temporal variations on the global and regional CH4 budget. The
global tropospheric mean CH4-reaction-weighted [OH] ([OH]GM-CH4)
ranges 10.3–16.3×105 molec cm−3 across 10 OH fields
during the early 2000s, resulting in inversion-based global CH4
emissions between 518 and 757 Tg yr−1. The uncertainties in CH4
inversions induced by the different OH fields are similar to the CH4
emission range estimated by previous bottom-up syntheses and larger than the
range reported by the top-down studies. The uncertainties in emissions
induced by OH are largest over South America, corresponding to large
inter-model differences of [OH] in this region. From the early to the late
2000s, the optimized CH4 emissions increased by 22±6 Tg yr−1
(17–30 Tg yr−1), of which ∼25 % (on average) offsets
the 0.7 % (on average) increase in OH burden. If the CCMI models represent
the OH trend properly over the 2000s, our results show that a higher
increasing trend of CH4 emissions is needed to match the CH4
observations compared to the CH4 emission trend derived using constant
OH. This study strengthens the importance of reaching a better representation
of OH burden and of OH spatial and temporal distributions to reduce the
uncertainties in the global and regional CH4 budgets.