— Ch. 1 · Defining Radiative Forcing —
Radiative forcing.
~3 min read · Ch. 1 of 6
The year 2019 marked a specific moment when human activity generated a radiative forcing of 2.72 watts per square meter relative to the baseline year 1750. This value represents the net change in downward minus upward radiative flux due to external climate drivers. Scientists measure this energy imbalance at the tropopause and top of the stratosphere to understand how Earth's temperature responds to changes. The concept distinguishes these external forces from internal feedbacks like water vapor or cloud formation that react to initial warming. A planet in equilibrium with its star exhibits zero net radiative forcing, maintaining a stable average global temperature. When this balance shifts, the resulting gain or loss of energy drives long-term climate trends rather than short-term weather fluctuations.
Historical Development Of Theory
Physicists developed comprehensive descriptions of radiative transfer during the first half of the 20th century before applying them to stellar atmospheres. Studies of radiative-convective equilibrium matured through the 1960s and 1970s as models began accounting for complex material flows within the energy balance. The term gained widespread traction in scientific literature by the 1980s after researchers distilled perturbation frameworks into usable metrics. Early work focused on homogeneous disturbances imposed onto the top-of-atmosphere energy balance to estimate state changes. Modern calculations now distinguish between instantaneous radiative forcing without stratospheric adjustments and effective radiative forcing which includes both tropospheric and stratospheric responses. These evolving definitions allow scientists to compare different drivers of climate change on a consistent scale.