Noise, Sensitivity, and Receiver Design Noise Figure Fundamentals Informational

How do I convert between noise figure in dB and equivalent noise temperature in Kelvin?

To convert noise figure (NF in dB) to noise temperature: Te = 290 × (10^(NF/10) - 1). To convert noise temperature back to noise figure: NF = 10 × log10(1 + Te/290). These formulas are exact and reversible. Both metrics describe the same physical noise; the choice depends on whether your system reference temperature is near 290 K.
Category: Noise, Sensitivity, and Receiver Design
Updated: April 2026
Product Tie-In: LNAs, Noise Sources, Cables

Noise Figure and Noise Temperature Conversion

Noise figure and noise temperature are two representations of the same physical quantity: the noise added by a component or system. The conversion between them is exact, lossless, and always valid. The standard reference temperature T0 = 290 K (approximately 17°C or 62°F) serves as the bridge between the two scales.

ParameterSuperheterodyneDirect ConversionDigital IF
Image Rejection60-90 dB (filter)30-50 dB (mismatch)N/A (digital)
DC OffsetNo issueMajor issueNo issue
LO LeakageLowHighLow
IntegrationDifficultEasy (single chip)Moderate
Dynamic Range80-120 dB60-90 dB70-100 dB
Common Questions

Frequently Asked Questions

Is 290 K exactly room temperature?

No. 290 K (16.85°C) was chosen by the IEEE as the standard reference temperature for noise calculations. Actual room temperature is closer to 295-300 K, but 290 K is the universal standard used in all noise figure specifications and measurements.

Can noise temperature be negative?

No. A noise temperature of 0 K means the component adds no noise (perfect, noiseless device). Negative noise temperatures have no physical meaning in this context. The minimum noise figure is 0 dB, corresponding to Te = 0 K.

Which should I put on a datasheet?

Industry convention uses noise figure (NF in dB) for component specifications. Noise temperature is used in system-level specifications, particularly for satellite and radio astronomy receivers where G/T is the key figure of merit.

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