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Noise figure

Noise figure (NF) and noise factor (F) are figures of merit that indicate degradation of the signal-to-noise ratio (SNR) that is caused by components in a signal chain. These figures of merit are used to evaluate the performance of an amplifier or a radio receiver, with lower values indicating better performance.

The noise factor is defined as the ratio of the output noise power of a device to the portion thereof attributable to thermal noise in the input termination at standard noise temperature T0 (usually 290 K). The noise factor is thus the ratio of actual output noise to that which would remain if the device itself did not introduce noise, or the ratio of input SNR to output SNR.

The noise factor and noise figure are related, with the former being a unitless ratio and the latter being the same ratio but expressed in units of decibels (dB).[1]

General

The noise figure is the difference in decibels (dB) between the noise output of the actual receiver to the noise output of an “ideal” receiver with the same overall gain and bandwidth when the receivers are connected to matched sources at the standard noise temperature T0 (usually 290 K). The noise power from a simple load is equal to kTB, where k is the Boltzmann constant, T is the absolute temperature of the load (for example a resistor), and B is the measurement bandwidth.

This makes the noise figure a useful figure of merit for terrestrial systems, where the antenna effective temperature is usually near the standard 290 K. In this case, one receiver with a noise figure, say 2 dB better than another, will have an output signal to noise ratio that is about 2 dB better than the other. However, in the case of satellite communications systems, where the receiver antenna is pointed out into cold space, the antenna effective temperature is often colder than 290 K.[2] In these cases a 2 dB improvement in receiver noise figure will result in more than a 2 dB improvement in the output signal to noise ratio. For this reason, the related figure of effective noise temperature is therefore often used instead of the noise figure for characterizing satellite-communication receivers and low-noise amplifiers.

In heterodyne systems, output noise power includes spurious contributions from image-frequency transformation, but the portion attributable to thermal noise in the input termination at standard noise temperature includes only that which appears in the output via the principal frequency transformation of the system and excludes that which appears via the image frequency transformation.

Definition

The noise factor F of a system is defined as[3]

 

where SNRi and SNRo are the input and output signal-to-noise ratios respectively. The SNR quantities are unitless power ratios. The noise figure NF is defined as the noise factor in units of decibels (dB):

 

where SNRi, dB and SNRo, dB are in units of (dB). These formulae are only valid when the input termination is at standard noise temperature T0 = 290 K, although in practice small differences in temperature do not significantly affect the values.

The noise factor of a device is related to its noise temperature Te:[4]

 

Attenuators have a noise factor F equal to their attenuation ratio L when their physical temperature equals T0. More generally, for an attenuator at a physical temperature T, the noise temperature is Te = (L − 1)T, giving a noise factor

 

Noise factor of cascaded devices

If several devices are cascaded, the total noise factor can be found with Friis' formula:[5]

 

where Fn is the noise factor for the n-th device, and Gn is the power gain (linear, not in dB) of the n-th device. The first amplifier in a chain usually has the most significant effect on the total noise figure because the noise figures of the following stages are reduced by stage gains. Consequently, the first amplifier usually has a low noise figure, and the noise figure requirements of subsequent stages is usually more relaxed.

Noise factor as a function of additional noise

 
The source outputs a signal of power   and noise of power  . Both signal and noise get amplified. However, in addition to the amplified noise from the source, the amplifier adds additional noise to its output denoted  . Therefore, the SNR at the amplifier's output is lower than at its input.

The noise factor may be expressed as a function of the additional output referred noise power   and the power gain   of an amplifier.

 

Derivation

From the definition of noise factor[3]

 

and assuming a system which has a noisy single stage amplifier. The signal to noise ratio of this amplifier would include its own output referred noise  , the amplified signal   and the amplified input noise  ,

 

Substituting the output SNR to the noise factor definition,[6]

 

In cascaded systems   does not refer to the output noise of the previous component. An input termination at the standard noise temperature is still assumed for the individual component. This means that the additional noise power added by each component is independent of the other components.

Optical noise figure

The above describes noise in electrical systems. Electric sources generate noise with a power spectral density equal to kT, where k is the Boltzmann constant and T is the absolute temperature. However, there is also noise in optical systems. In these, the sources have no fundamental noise. Instead the energy quantization causes notable shot noise in the detector, corresponding to a noise power spectral density of hf where h is the Planck constant and f is the optical frequency.

In the 1990s, an optical noise figure has been defined.[7] This has been called Fpnf for photon number fluctuations.[8] The powers needed for SNR and noise factor calculation are the electrical powers caused by the current in a photodiode. SNR is the square of mean photocurrent divided by variance of photocurrent. Monochromatic or sufficiently attenuated light has a Poisson distribution of detected photons. If, during a detection interval the expectation value of detected photons is n then the variance is also n and one obtains SNRpnf,in = n2/n = n. Behind an optical amplifier with power gain G there will be a mean of Gn photons. In the limit of large n the variance of photons is Gn(2nsp(G-1)+1) where nsp is the spontaneous emission factor. One obtains SNRpnf,out = G2n2/(Gn(2nsp(G-1)+1)) = n/(2nsp(1-1/G)+1/G). Resulting optical noise factor is Fpnf = SNRpnf,in / SNRpnf,out = 2nsp(1-1/G)+1/G.

Fpnf is in conceptual conflict compared to the electrical noise factor, which is now called Fe:

Photocurrent is proportional to optical power. Optical power is proportional to squares of a field amplitude (electric or magnetic). So, the receiver is nonlinear in amplitude. The power needed for SNRpnf calculation is proportional to the 4th power of the signal amplitude. But for Fe in the electrical domain the power is proportional to the square of the signal amplitude.

At a certain electrical frequency, noise occurs in phase (I) and in quadrature (Q) with the signal. Both these quadratures are available behind the electrical amplifier. The same holds in an optical amplifier. But the direct detection photoreceiver needed for measurement of SNRpnf takes mainly the in-phase noise into account whereas quadrature noise can be neglected for highn. Also, the receiver outputs only one quadrature. So, one quadrature is lost.

For an optical amplifier with large G it holds Fpnf ≥ 2 whereas for an electrical amplifier it holds Fe ≥ 1.

Moreover, today's long-haul optical fiber communication is dominated by coherent optical I&Q receivers but Fpnf does not describe the SNR degradation observed in these.

The above conflicts are resolved by the optical in-phase and quadrature noise figure Fo,IQ.[9] It can be measured using a coherent optical I&Q receiver. In these, power of the output signal is proportional to the square of an optical field amplitude because they are linear in amplitude. They pass both quadratures. For an optical amplifier it holds Fo,IQ = nsp(1-1/G)+1/G ≥ 1. Quantity nsp(1-1/G) is the input-referred number of added noise photons per mode.

Fo,IQ and Fpnf can easily be converted into each other. For large G it holds Fo,IQ = Fpnf/2 or, when expressed in dB, Fo,IQ is 3 dB less than Fpnf.

Unified noise figure

Total noise power spectral density per mode is kT + hf. In the electrical domain hf can be neglected. In the optical domain kT can be neglected. In between, say, in the low THz or thermal domain, both will need to be considered. It is possible to blend between electrical and optical domains such that a universal noise figure is obtained.

This has been attempted by a noise figure Ffas[10] where the subscript stands for fluctuations of amplitude squares. At optical frequencies Ffas equals Fpnf and involves detection of only 1 quadrature. But the conceptual difference to Fe cannot be overcome: It seems impossible that for increasing frequency (from electrical to thermal to optical) 2 quadratures (in the electrical domain) gradually become 1 quadrature (in optical receivers which determine Ffas or Fpnf). The ideal noise factor would need to go from 1 (electrical) to 2 (optical), which is not intuitive. For unification of Fpnf with Fe, squares of signal amplitudes (powers in the electrical domain) must also gradually become 4th powers of amplitudes (powers in optical direct detection receivers), which seems impossible.

A consistent unification of optical and electrical noise figures is obtained for Fe and Fo,IQ. There are no contradictions because both these are in conceptual match (powers proportional to squares of amplitudes, linear, 2 quadratures, ideal noise factor equal to 1). Thermal noise kT and fundamental quantum noise hf are taken into account. The unified noise figure is FIQ = (kTFe + hfFo,IQ) / (kT + hf) = (kT(T + Te)) + hf(nsp(1-1/G)+1/G)) / (kT + hf).[9]

See also

References

  1. ^ "Noise temperature, Noise Figure and Noise Factor".
  2. ^ Agilent 2010, p. 7
  3. ^ a b Agilent 2010, p. 5.
  4. ^ Agilent 2010, p. 7 with some rearrangement from Te = T0(F − 1).
  5. ^ Agilent 2010, p. 8.
  6. ^ Aspen Core. Derivation of noise figure equations (DOCX), pp. 3–4
  7. ^ E. Desurvire, „Erbium doped fiber amplifiers: Principles and Applications“, Wiley, New York, 1994
  8. ^ H. A. Haus, "The noise figure of optical amplifiers," in IEEE Photonics Technology Letters, vol. 10, no. 11, pp. 1602-1604, Nov. 1998, doi: 10.1109/68.726763
  9. ^ a b R. Noe, "Consistent Optical and Electrical Noise Figure," in Journal of Lightwave Technology, 2022, doi: 10.1109/JLT.2022.3212936, https://ieeexplore.ieee.org/document/9915356
  10. ^ H. A. Haus, "Noise Figure Definition Valid From RF to Optical Frequencies," in IEEE JOURNAL OF SELECTED TOPICS IN QUANTUM ELECTRONICS, VOL. 6, NO. 2, MARCH/APRIL 2000, pp. 240-247
  • Keysight, Fundamentals of RF and Microwave Noise Figure Measurements (PDF), Application Note, 57-1, Published September 01, 2019., archived (PDF) from the original on 2022-10-09

External links

  • Noise Figure Calculator 2- to 30-Stage Cascade
  • Mobile phone noise figure

  This article incorporates public domain material from Federal Standard 1037C. General Services Administration. (in support of MIL-STD-188).

noise, figure, noise, factor, figures, merit, that, indicate, degradation, signal, noise, ratio, that, caused, components, signal, chain, these, figures, merit, used, evaluate, performance, amplifier, radio, receiver, with, lower, values, indicating, better, p. Noise figure NF and noise factor F are figures of merit that indicate degradation of the signal to noise ratio SNR that is caused by components in a signal chain These figures of merit are used to evaluate the performance of an amplifier or a radio receiver with lower values indicating better performance The noise factor is defined as the ratio of the output noise power of a device to the portion thereof attributable to thermal noise in the input termination at standard noise temperature T0 usually 290 K The noise factor is thus the ratio of actual output noise to that which would remain if the device itself did not introduce noise or the ratio of input SNR to output SNR The noise factor and noise figure are related with the former being a unitless ratio and the latter being the same ratio but expressed in units of decibels dB 1 Contents 1 General 2 Definition 3 Noise factor of cascaded devices 4 Noise factor as a function of additional noise 4 1 Derivation 5 Optical noise figure 6 Unified noise figure 7 See also 8 References 9 External linksGeneral EditThe noise figure is the difference in decibels dB between the noise output of the actual receiver to the noise output of an ideal receiver with the same overall gain and bandwidth when the receivers are connected to matched sources at the standard noise temperature T0 usually 290 K The noise power from a simple load is equal to kTB where k is the Boltzmann constant T is the absolute temperature of the load for example a resistor and B is the measurement bandwidth This makes the noise figure a useful figure of merit for terrestrial systems where the antenna effective temperature is usually near the standard 290 K In this case one receiver with a noise figure say 2 dB better than another will have an output signal to noise ratio that is about 2 dB better than the other However in the case of satellite communications systems where the receiver antenna is pointed out into cold space the antenna effective temperature is often colder than 290 K 2 In these cases a 2 dB improvement in receiver noise figure will result in more than a 2 dB improvement in the output signal to noise ratio For this reason the related figure of effective noise temperature is therefore often used instead of the noise figure for characterizing satellite communication receivers and low noise amplifiers In heterodyne systems output noise power includes spurious contributions from image frequency transformation but the portion attributable to thermal noise in the input termination at standard noise temperature includes only that which appears in the output via the principal frequency transformation of the system and excludes that which appears via the image frequency transformation Definition EditThe noise factor F of a system is defined as 3 F S N R i S N R o displaystyle F frac mathrm SNR text i mathrm SNR text o where SNRi and SNRo are the input and output signal to noise ratios respectively The SNR quantities are unitless power ratios The noise figure NF is defined as the noise factor in units of decibels dB N F 10 log 10 F 10 log 10 S N R i S N R o S N R i dB S N R o dB displaystyle mathrm NF 10 log 10 F 10 log 10 left frac mathrm SNR text i mathrm SNR text o right mathrm SNR text i dB mathrm SNR text o dB where SNRi dB and SNRo dB are in units of dB These formulae are only valid when the input termination is at standard noise temperature T0 290 K although in practice small differences in temperature do not significantly affect the values The noise factor of a device is related to its noise temperature Te 4 F 1 T e T 0 displaystyle F 1 frac T text e T 0 Attenuators have a noise factor F equal to their attenuation ratio L when their physical temperature equals T0 More generally for an attenuator at a physical temperature T the noise temperature is Te L 1 T giving a noise factor F 1 L 1 T T 0 displaystyle F 1 frac L 1 T T 0 Noise factor of cascaded devices EditMain article Friis formulas for noise If several devices are cascaded the total noise factor can be found with Friis formula 5 F F 1 F 2 1 G 1 F 3 1 G 1 G 2 F 4 1 G 1 G 2 G 3 F n 1 G 1 G 2 G 3 G n 1 displaystyle F F 1 frac F 2 1 G 1 frac F 3 1 G 1 G 2 frac F 4 1 G 1 G 2 G 3 cdots frac F n 1 G 1 G 2 G 3 cdots G n 1 where Fn is the noise factor for the n th device and Gn is the power gain linear not in dB of the n th device The first amplifier in a chain usually has the most significant effect on the total noise figure because the noise figures of the following stages are reduced by stage gains Consequently the first amplifier usually has a low noise figure and the noise figure requirements of subsequent stages is usually more relaxed Noise factor as a function of additional noise Edit The source outputs a signal of power S i displaystyle S i and noise of power N i displaystyle N i Both signal and noise get amplified However in addition to the amplified noise from the source the amplifier adds additional noise to its output denoted N a displaystyle N a Therefore the SNR at the amplifier s output is lower than at its input The noise factor may be expressed as a function of the additional output referred noise power N a displaystyle N a and the power gain G displaystyle G of an amplifier F 1 N a N i G displaystyle F 1 frac N a N i G Derivation Edit From the definition of noise factor 3 F S N R i S N R o S i N i S o N o displaystyle F frac mathrm SNR text i mathrm SNR text o frac frac S i N i frac S o N o and assuming a system which has a noisy single stage amplifier The signal to noise ratio of this amplifier would include its own output referred noise N a displaystyle N a the amplified signal S i G displaystyle S i G and the amplified input noise N i G displaystyle N i G S o N o S i G N a N i G displaystyle frac S o N o frac S i G N a N i G Substituting the output SNR to the noise factor definition 6 F S i N i S i G N a N i G N a N i G N i G 1 N a N i G displaystyle F frac frac S i N i frac S i G N a N i G frac N a N i G N i G 1 frac N a N i G In cascaded systems N i displaystyle N i does not refer to the output noise of the previous component An input termination at the standard noise temperature is still assumed for the individual component This means that the additional noise power added by each component is independent of the other components Optical noise figure EditThe above describes noise in electrical systems Electric sources generate noise with a power spectral density equal to kT where k is the Boltzmann constant and T is the absolute temperature However there is also noise in optical systems In these the sources have no fundamental noise Instead the energy quantization causes notable shot noise in the detector corresponding to a noise power spectral density of hf where h is the Planck constant and f is the optical frequency In the 1990s an optical noise figure has been defined 7 This has been called Fpnf for photon number fluctuations 8 The powers needed for SNR and noise factor calculation are the electrical powers caused by the current in a photodiode SNR is the square of mean photocurrent divided by variance of photocurrent Monochromatic or sufficiently attenuated light has a Poisson distribution of detected photons If during a detection interval the expectation value of detected photons is n then the variance is also n and one obtains SNRpnf in n2 n n Behind an optical amplifier with power gain G there will be a mean of Gn photons In the limit of large n the variance of photons is Gn 2nsp G 1 1 where nsp is the spontaneous emission factor One obtains SNRpnf out G2n2 Gn 2nsp G 1 1 n 2nsp 1 1 G 1 G Resulting optical noise factor is Fpnf SNRpnf in SNRpnf out 2nsp 1 1 G 1 G Fpnf is in conceptual conflict compared to the electrical noise factor which is now called Fe Photocurrent is proportional to optical power Optical power is proportional to squares of a field amplitude electric or magnetic So the receiver is nonlinear in amplitude The power needed for SNRpnf calculation is proportional to the 4th power of the signal amplitude But for Fe in the electrical domain the power is proportional to the square of the signal amplitude At a certain electrical frequency noise occurs in phase I and in quadrature Q with the signal Both these quadratures are available behind the electrical amplifier The same holds in an optical amplifier But the direct detection photoreceiver needed for measurement of SNRpnf takes mainly the in phase noise into account whereas quadrature noise can be neglected for highn Also the receiver outputs only one quadrature So one quadrature is lost For an optical amplifier with large G it holds Fpnf 2 whereas for an electrical amplifier it holds Fe 1 Moreover today s long haul optical fiber communication is dominated by coherent optical I amp Q receivers but Fpnf does not describe the SNR degradation observed in these The above conflicts are resolved by the optical in phase and quadrature noise figure Fo IQ 9 It can be measured using a coherent optical I amp Q receiver In these power of the output signal is proportional to the square of an optical field amplitude because they are linear in amplitude They pass both quadratures For an optical amplifier it holds Fo IQ nsp 1 1 G 1 G 1 Quantity nsp 1 1 G is the input referred number of added noise photons per mode Fo IQ and Fpnf can easily be converted into each other For large G it holds Fo IQ Fpnf 2 or when expressed in dB Fo IQ is 3 dB less than Fpnf Unified noise figure EditTotal noise power spectral density per mode is kT hf In the electrical domain hf can be neglected In the optical domain kT can be neglected In between say in the low THz or thermal domain both will need to be considered It is possible to blend between electrical and optical domains such that a universal noise figure is obtained This has been attempted by a noise figure Ffas 10 where the subscript stands for fluctuations of amplitude squares At optical frequencies Ffas equals Fpnf and involves detection of only 1 quadrature But the conceptual difference to Fe cannot be overcome It seems impossible that for increasing frequency from electrical to thermal to optical 2 quadratures in the electrical domain gradually become 1 quadrature in optical receivers which determine Ffas or Fpnf The ideal noise factor would need to go from 1 electrical to 2 optical which is not intuitive For unification of Fpnf with Fe squares of signal amplitudes powers in the electrical domain must also gradually become 4th powers of amplitudes powers in optical direct detection receivers which seems impossible A consistent unification of optical and electrical noise figures is obtained for Fe and Fo IQ There are no contradictions because both these are in conceptual match powers proportional to squares of amplitudes linear 2 quadratures ideal noise factor equal to 1 Thermal noise kT and fundamental quantum noise hf are taken into account The unified noise figure is FIQ kTFe hfFo IQ kT hf kT T Te hf nsp 1 1 G 1 G kT hf 9 See also EditNoise Noise electronic Noise figure meter Noise level Thermal noise Signal to noise ratio Y factorReferences Edit Noise temperature Noise Figure and Noise Factor Agilent 2010 p 7harvnb error no target CITEREFAgilent2010 help a b Agilent 2010 p 5harvnb error no target CITEREFAgilent2010 help Agilent 2010 p 7harvnb error no target CITEREFAgilent2010 help with some rearrangement from Te T0 F 1 Agilent 2010 p 8harvnb error no target CITEREFAgilent2010 help Aspen Core Derivation of noise figure equations DOCX pp 3 4 E Desurvire Erbium doped fiber amplifiers Principles and Applications Wiley New York 1994 H A Haus The noise figure of optical amplifiers in IEEE Photonics Technology Letters vol 10 no 11 pp 1602 1604 Nov 1998 doi 10 1109 68 726763 a b R Noe Consistent Optical and Electrical Noise Figure in Journal of Lightwave Technology 2022 doi 10 1109 JLT 2022 3212936 https ieeexplore ieee org document 9915356 H A Haus Noise Figure Definition Valid From RF to Optical Frequencies in IEEE JOURNAL OF SELECTED TOPICS IN QUANTUM ELECTRONICS VOL 6 NO 2 MARCH APRIL 2000 pp 240 247 Keysight Fundamentals of RF and Microwave Noise Figure Measurements PDF Application Note 57 1 Published September 01 2019 archived PDF from the original on 2022 10 09External links EditNoise Figure Calculator 2 to 30 Stage Cascade Noise Figure and Y Factor Method Basics and Tutorial Mobile phone noise figure This article incorporates public domain material from Federal Standard 1037C General Services Administration in support of MIL STD 188 Retrieved from https en wikipedia org w index php title Noise figure amp oldid 1122097793, wikipedia, wiki, book, books, library,

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