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Solar Constant

1838
  • Claude Pouillet
  • John Herschel
19th-century laboratory with scientists studying solar radiation measurements.

(generated image for illustration only)

The solar constant is the mean solar electromagnetic radiation per unit area measured at the top of Earth’s atmosphere, perpendicular to the rays. Its value is approximately 1361 watts per square meter (\(W/m^2\)). This figure varies slightly with solar activity and Earth’s orbital distance, but serves as a fundamental baseline for climate science, satellite design, and renewable energy calculations.

The solar constant represents the total solar irradiance (TSI) at a distance of one astronomical unit (AU) from the Sun. While termed a ‘constant’, its value is not perfectly fixed. It fluctuates by about 0.1% over the 11-year sunspot cycle and has longer-term variations. These small changes are significant for Earth’s climate system. Early measurements, like those by Claude Pouillet in 1838 using his pyrheliometer, were crucial first steps but were inaccurate due to not fully accounting for atmospheric absorption. It was only with the advent of satellite-based radiometers in the late 20th century that a precise and continuous measurement of the solar constant became possible. The accepted value of approximately 1361 W/m² is a cornerstone for calculating Earth’s energy balance, determining the equilibrium temperature of the planet, and designing systems that operate in space. For instance, engineers must know this value precisely to design thermal control systems for satellites to prevent overheating or freezing, and to calculate the power output of their solar arrays. It is the fundamental input for global climate models that simulate Earth’s past and future climate.

Note: while it does represent the total energy received by earth from the sun as a whole, in all electromagnetic ways, it is not directly the value that can be used for solar panels located on the ground.

UNESCO Nomenclature: 2506
– Geophysics

Type

Physical Property

Disruption

Foundational

Usage

Widespread Use

Precursors

  • Isaac Newton’s work on optics and the spectrum of light
  • development of thermodynamics and the concept of energy transfer
  • invention of the thermometer for measuring temperature changes
  • early astronomical observations of the sun
  • William Herschel’s discovery of infrared radiation

Applications

  • climate modeling
  • satellite thermal design
  • solar power generation forecasting
  • spacecraft power systems engineering
  • earth’s energy budget calculations
  • atmospheric science research

Patents:

NA

Potential Innovations Ideas

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Related to: solar constant, solar irradiance, earth’s atmosphere, watts per square meter, climate science, solar activity, satellite design, energy budget, pyrheliometer, claude pouillet.

Historical Context

Solar Constant

1800
1838
1872
1910
1940
1940
1946
1650
1800
1852
1900
1912
1940
1940
1950

(if date is unknown or not relevant, e.g. "fluid mechanics", a rounded estimation of its notable emergence is provided)

Related Invention, Innovation & Technical Principles

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