EGU25-5950, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-5950
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 29 Apr, 16:15–18:00 (CEST), Display time Tuesday, 29 Apr, 14:00–18:00
 
Hall X5, X5.211
An Estimation of the Efficacy of Methane Radiative Forcing Using Radiative Kernels
Sumit Kumar1, Ashwin K. Seshadri1,2, and Govindasamy Bala1
Sumit Kumar et al.
  • 1Centre for Atmospheric and Oceanic Sciences (CAOS), Indian Institute of Science Bangalore, India.
  • 2Divecha Centre for Climate Change (DCCC), Indian Institute of Science Bangalore, India.

Methane (CH4) and carbon dioxide (CO2) are two major greenhouse gases with distinct radiative properties and climate responses. Using the National Centre for Atmospheric Research (NCAR) Community Atmosphere Model (CAM5) in two configurations (prescribed sea surface temperature and slab ocean) to estimate radiative forcing and climate response and radiative kernel analyses, we compare their slow feedback mechanisms and implications for climate sensitivity. We perform simulations with a 10X increase in CH4 and 1.35X CO2 concentration to simulate global mean warming of about 1.5 K in both cases. We find that CH4 requires a larger effective radiative forcing, indicating a lower efficacy relative to CO2.

We attribute CH4's lower efficacy to differences in slow feedback processes. CH4 exhibits more negative lapse rate feedback (difference of -0.10 Wm-2K-1) and more positive water vapor feedback (difference of 0.06 Wm-2K-1) due to equatorially concentrated radiative forcing and stronger upper-tropospheric warming. Feedback differences also include weaker positive shortwave cloud (difference of -0.05 Wm-2K-1) and smaller albedo (difference of -0.04 Wm-2K-1) feedback responses for CH4, resulting in a net feedback difference of -0.12 Wm-2K-1. These findings underscore the role of spatial forcing patterns, including CH4’s near-infrared shortwave absorption bands and low-latitude warming, in shaping feedback processes.

We find that CO2 forcing results in relatively stronger polar warming, enhancing albedo feedback, and induces larger mid-latitude cloud reductions, amplifying shortwave cloud feedback. Both gases have comparable positive longwave cloud feedback, broadly consistent with fixed anvil temperatures. All individual feedback differences are statistically significant. Our results highlight that distinct feedback responses arise from basic physical mechanisms, such as differing meridional warming patterns and small but distinct relative humidity changes.

Our study advances the understanding of radiative forcing structure and feedbacks in determining greenhouse gas impacts on climate sensitivity. It also highlights the need for multi-model assessments and Earth system modeling to evaluate feedback uncertainties and refine projections of long-term climate responses as relative contributions to radiative forcing evolve.

How to cite: Kumar, S., Seshadri, A. K., and Bala, G.: An Estimation of the Efficacy of Methane Radiative Forcing Using Radiative Kernels, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5950, https://doi.org/10.5194/egusphere-egu25-5950, 2025.