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Everything about Radiative forcing

Concept for changes to the energy flows through a planetary atmosphere

Radiative forcing is a concept used to quantify a change to the balance of energy flowing through a planetary atmosphere. Various factors contribute to this change in energy balance, such as concentrations of greenhouse gases and aerosols, and changes in surface albedo and solar irradiance. In more technical terms, it is defined as "the change in the net, downward minus upward, radiative flux due to a change in an external driver of climate change." These external drivers are distinguished from feedbacks and variability that are internal to the climate system, and that further influence the direction and magnitude of imbalance. Radiative forcing on Earth is meaningfully evaluated at the tropopause and at the stratopause. It is quantified in units of watts per square meter, and often summarized as an average over the total surface area of the globe. Wikipedia →

🧭 Start here: a 6-step reading path

  1. Read the overview: Radiative forcingA 5-minute orientation
  2. Skim a recent paper: Opportunistic experiments to constrain aerosol effective radiative forcingInfluential work since 2022
  3. Pick up a classic book: Climate change, 1994The most-reprinted book on the subject
  4. Read the landmark paper: Radiative forcing by long‐lived greenhouse gases: Calculations with the AER radiative transfer modelsCited 4,237 times
  5. Go sideways: Causes of climate changeA closely related topic
  6. Go sideways: Earth's energy budgetA closely related topic

📖 Definitions

Noun The effect of greenhouse gases on the radiation of heat in the atmosphere.

🏆 Landmark papers (most cited)

🆕 Influential since 2022

📚 Books worth reading

Ranked by number of editions on Open Library, a rough measure of how lasting a book is.

🔗 Related topics