An explicit lumped model makes the cancellation understandable. Treat the receiver as having uniform temperature , heat capacity , heater power deposited in the receiver, net parasitic input , and outward heat transfer to a reference at temperature . With incident radiant flux and radiometric absorptance , conservation of energy gives
The dark state has no admitted beam. Compare settled dark and light states, denoted and ; each has . Subtracting their balances gives
where and . At identical and , with unchanged surroundings and parasitic heating, both correction differences vanish. Thus , and . Notice the signs: extra stray thermal radiation admitted with the beam also reduces heater power, so it must be subtracted from that reduction before attributing the result to the intended beam.
Measure the heater's own terminal voltage and electric current : for steady electrical heating, , where is its electrical resistance. A supply voltage that includes wire voltage drops counts Joule heating in the leads too; only the portion deposited in the receiver belongs in this balance. Changes in that deposited lead heat belong in . Optical-electrical heating non-equivalence adds a further instrument-specific correction when the uniform-temperature model is insufficient.[ref]
A radiometer thermal link is the intentional path for thermal conduction from receiver to reference block. Near a chosen operating point, write with local conductance in . A weaker link increases the steady temperature rise per added power, , but also increases the uncontrolled relaxation time when the link dominates other heat transfer. These are local linear approximations: actual thermal conductivity depends on temperature, and active feedback control introduces its own response. NIST explicitly describes the tradeoff between weaker links and smaller receiver heat capacity.[ref]
Stipulate a model receiver held at with a reference at . Choose , so outward thermal conduction is . Ignore other heat transfer, take in both states, and stipulate perfect optical/electrical thermal equivalence. These values specify an original example; they are not measurements or claimed performance of a NIST instrument.
With the beam blocked, supply . With light admitted, the required heater power is . For stipulated radiometric absorptance at the chosen single wavelength,
The illuminated receiver still gets of heating. The remaining of incident radiant flux escapes without heating it. Calling the measured heater reduction “incident power” would underestimate the stipulated incident radiant flux by .
Figure 1.
The same receiver temperature with different electrical and optical heating
. Original stipulated steady-state example, not experimental data. Both columns total of deposited heating and balance the same outward thermal conduction. Incident radiant flux is , of which is absorbed; the that escapes is outside the heating column. No response time or measured uncertainty is implied. Details.
Two variations expose different pitfalls. First, if admitting the beam also adds of stray heating while the same is absorbed from the intended beam, the heater falls to . The apparent reduction is now ; subtracting recovers the beam's absorbed power. Second, keep the original heater readings but stipulate a light-state receiver offset at fixed reference temperature. The link carries an extra ; the inferred absorbed power becomes , and incident radiant flux becomes . This second variation deliberately violates exact fixed-temperature substitution.
The heater can supply only nonnegative power in this model. Consequently an absorbed beam above the available dark heater power cannot be compensated at the chosen setpoint merely by reducing the heater. The operating point, link, or admitted radiant flux must change; zero heater demand is a range boundary, not evidence of greater radiant flux sensitivity.

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