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Cascade Noise Figure

Two-stage Friis cascade — why the LNA wins.

InputF = F1 + (F2 − 1) / G1

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The engineering

Stage two's noise arrives divided by stage one's gain — so a 1 dB LNA with 20 dB of gain in front of a noisy 10 dB mixer yields a 1.35 dB system, not 11. Put the good part first and give it gain.

Corollary: any loss *before* the LNA (cable, filter, switch) adds dB-for-dB to system NF. The antenna-mounted preamp exists because of this equation.

Where this math comes from

The cascade formula is the second half of Friis's 1944 noise paper, and it reorganized receiver design permanently: sensitivity became a question of what touches the antenna first.

It's also why radio telescopes cool their first amplifier to 15 K while the racks behind run warm — everything after the first stage is nearly free.

  1. 1944Harald FriisCascade formula — first-stage dominance proven.
  2. 1963Maser/paramp eraCryogenic first stages exploit the formula for radio astronomy.

See the full timeline of the math behind every calculator →

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