What we count
Solar-radiation energy intercepted by the Earth system using a long-term average incoming power of roughly 173,000 TW.
How much solar energy reaches the sunlit Earth during a day.
Solar-radiation energy intercepted by the Earth system using a long-term average incoming power of roughly 173,000 TW.
Solar-radiation energy intercepted by the Earth system using a long-term average incoming power of roughly 173,000 TW.
The source combines national energy balances, reported production, reserves and other official energy statistics.
This is a physical flux at the top of the atmosphere, not energy available to solar panels; much is reflected or absorbed.
The calculation uses the latest published daily value from NASA Earth energy budget for long-term physical average; no single reference year.
How the value is used: The running number shows the share corresponding to time since midnight.
We distribute the published daily value evenly across time elapsed since midnight.
V(t) = Vday × elapsed share of the dayDaily reference value4,152,000,000,000long-term physical average; no single reference year · MWh
Average per hour173,000,000,000even time-based calculation
Calculation interval0.1 sContinuously calculated
NASA Earth energy budget reports the latest published figure used on this page for long-term physical average; no single reference year.
We distribute the published daily value evenly across time elapsed since midnight.
The result is recalculated on screen every 0.1 seconds.
The source value comes from NASA Earth energy budget and refers to long-term physical average; no single reference year. It is the latest figure published by this source. The source combines national energy balances, reported production, reserves and other official energy statistics.