Johnson–Nyquist noise (thermal noise, Johnson noise, or Nyquist noise) is the electronic noise generated by the thermal agitation of the charge carriers (usually the electrons) inside an electrical conductor at equilibrium, which happens regardless of any applied voltage.
Thermal noise is approximately white, meaning that the power spectral density is nearly equal throughout the frequency spectrum (however see the section below on extremely high frequencies). Additionally, the amplitude of the signal has very nearly a Gaussian probability density function.
Thermal noise is distinct from shot noise, which consists of additional current fluctuations that occur when a voltage is applied and a macroscopic current starts to flow. For the general case, the above definition applies to charge carriers in any type of conducting medium (e.g. ions in an electrolyte), not just resistors. It can be modeled by a voltage source representing the noise of the non-ideal resistor in series with an ideal noise free resistor.
For example, a 1 kΩ resistor at a temperature of 300 K has
For a given bandwidth, the root mean square (RMS) of the voltage, vn, is given by
where Δf is the bandwidth in hertz over which the noise is measured. For a 1 kΩ resistor at room temperature and a 10 kHz bandwidth, the RMS noise voltage is 400 nV. A useful rule of thumb to remember is that 50 Ω at 1 Hz bandwidth correspond to 1 nV noise at room temperature.
A resistor in a short circuit dissipates a noise power of
The noise generated at the resistor can transfer to the remaining circuit; the maximum noise power transfer happens with impedance matching when the Thévenin equivalent resistance of the remaining circuit is equal to the noise generating resistance. In this case each one of the two participating resistors dissipates noise in both itself and in the other resistor. Since only half of the source voltage drops across any one of these resistors, the resulting noise power is given by
where P is the thermal noise power in watts. Notice that this is independent of the noise generating resistance.
where the factor of 1000 is present because the power is given in milliwatts, rather than watts. This equation can be simplified by separating the constant parts from the bandwidth:
which is more commonly seen approximated as:
Noise power at different bandwidths is then simple to calculate:
|Bandwidth (Δf)||Thermal noise power||Notes|
|1 Hz||−174 dBm|
|10 Hz||−164 dBm|
|100 Hz||−154 dBm|
|1 kHz||−144 dBm|
|10 kHz||−134 dBm||FM channel of 2-way radio|
|100 kHz||−124 dBm|
|180 kHz||−121.45 dBm||One LTE resource block|
|200 kHz||−120.98 dBm||One GSM channel (ARFCN)|
|1 MHz||−114 dBm|
|2 MHz||−111 dBm||Commercial GPS channel|
|6 MHz||−106 dBm||Analog television channel|
|20 MHz||−101 dBm||WLAN 802.11 channel|
The actual amount of thermal noise received by a radio receiver having a 50 Ω input impedance, connected to an antenna with a 50 Ω radiation resistance would be scaled by the noise figure (NF), shown as follows:
Here Preceivernoise is the noise generated in the receiver itself. Presistornoise is the value from the table above for thermal noise from a resistor. NF is in dB. Ten raised to the power of NF/10 is called the noise factor and is simply the linear version of noise figure. We subtract one from the noise factor here because a noise factor of 1 is a perfect receiver (which contributes no noise to the signal). Noise factor is defined this way because in the laboratory, it is measured by connecting a resistor to the receiver's input and comparing the output noise to what one would expect if the noise of the resistor were simply amplified by the gain of the receiver. A ratio of 1 between the actual output noise in the numerator and the gain times the resistor thermal noise in the denominator means that the receiver added no noise of its own to the input.
Note that the radiation resistance of the antenna does not convert power to heat, and so is not a source of thermal noise. It dissipates power as electromagnetic radiation. Thus if the radiation incident on the antenna is blackbody radiation at the same temperature as the antenna then it will contribute noise in the same manner based on the radiation resistance, according to the zeroth law of thermodynamics as applied between the surrounding matter, the antenna, and the electromagnetic radiation. In an underground cave or mine, the antenna will be surrounded by earth which is opaque to the radiation, and thus, the radiation resistance will contribute to the thermal noise.
Likewise, the load impedance of the input of the receiver does not contribute directly to received noise. Therefore, it is indeed possible, and even common, for a receiver to have a noise factor of less than 2X (or equivalently, a noise figure of less than 3 dB).
For example a 6 MHz wide channel such as a television channel received signal would compete with the tiny amount of power generated by room temperature in the input stages of the receiver, which, for a TV receiver with a noise figure of 3 dB would be −106 dBm, or one fortieth of a picowatt. For a TV with a noise figure of 1 dB, the noise power would be −112 dBm. The actual source of this noise is a combination of thermal noise in physical resistances of wires and semiconductors, thermal noise in other lossy devices such as transformers, as well as shot noise.
The 6 MHz bandwidth could be the 6 MHz between 54 and 60 MHz (corresponding to TV channel 2) or the 6 MHz between 470 MHz and 476 MHz (corresponding to TV channel UHF 14) or any other 6 MHz in the spectrum for that matter. The bandwidth of any channel should never be confused with the transmitting frequency of a channel. For example, a channel transmit frequency may be as high as 2450 MHz for a WIFI signal, but the actual width of the channel may be only 20 MHz, and that 20 MHz would be the correct value to use in computing the Johnson–Nyquist noise.
Note that it is quite possible to detect a signal whose amplitude is less than the noise contained within its bandwidth. The Global Positioning System (GPS) and Glonass system both have signal amplitudes that are less than the received noise in a typical receiver at ground level. In the case of GPS, the received signal has a power of −133 dBm. The newer batch of satellites have a more powerful transmitter. To achieve this feat, GPS uses spread spectrum techniques, while some other communication systems use error control coding. There is still a fundamental limit to the ability to discern the meaning of a signal in the midst of noise, given by the Shannon–Hartley theorem.
The noise source can also be modeled by a current source in parallel with the resistor by taking the Norton equivalent that corresponds simply to divide by R. This gives the root mean square value of the current source as:
Thermal noise is intrinsic to all resistors and is not a sign of poor design or manufacture, although resistors may also have excess noise.
Thermal noise on capacitors is referred to as kTC noise. Thermal noise in an RC circuit has an unusually simple expression, as the value of the resistance (R) drops out of the equation. This is because higher R contributes to more filtering as well as to more noise. The bandwidth of the RC circuit is 1/(4RC), which can substituted into the above formula to eliminate R. The mean-square and RMS noise voltage generated in such a filter are:
Thermal noise accounts for 100% of kTC noise, whether it is attributed to the resistance or to the capacitance.
In the extreme case of the reset noise left on a capacitor by opening an ideal switch, the resistance is infinite, yet the formula still applies; however, now the RMS must be interpreted not as a time average, but as an average over many such reset events, since the voltage is constant when the bandwidth is zero. In this sense, the Johnson noise of an RC circuit can be seen to be inherent, an effect of the thermodynamic distribution of the number of electrons on the capacitor, even without the involvement of a resistor.
The noise is not caused by the capacitor itself, but by the thermodynamic equilibrium of the amount of charge on the capacitor. Once the capacitor is disconnected from a conducting circuit, the thermodynamic fluctuation is frozen at a random value with standard deviation as given above.
The reset noise of capacitive sensors is often a limiting noise source, for example in image sensors. As an alternative to the voltage noise, the reset noise on the capacitor can also be quantified as the electrical charge standard deviation, as
Since the charge variance is kBTC, this noise is often called kTC noise.
Any system in thermal equilibrium has state variables with a mean energy of kT/2 per degree of freedom. Using the formula for energy on a capacitor (E = ½CV2), mean noise energy on a capacitor can be seen to also be ½C(kT/C), or also kT/2. Thermal noise on a capacitor can be derived from this relationship, without consideration of resistance.
The kTC noise is the dominant noise source at small capacitors.
|1 fF||2 mV||12.5 e–|
|10 fF||640 µV||40 e–|
|100 fF||200 µV||125 e–|
|1 pF||64 µV||400 e–|
|10 pF||20 µV||1250 e–|
|100 pF||6.4 µV||4000 e–|
|1 nF||2 µV||12500 e–|
The above equations are good approximations at any practical radio frequency in use (i.e. frequencies below about 80 gigahertz). In the most general case, which includes up to optical frequencies, the power spectral density of the voltage across the resistor R, in V2/Hz is given by:
(this assumption is valid until few terahertz at room temperature) then the exponential can be expressed in terms of its Taylor series. The relationship then becomes:
In general, both R and T depend on frequency. In order to know the total noise it is enough to integrate over all the bandwidth. Since the signal is real, it is possible to integrate over only the positive frequencies, then multiply by 2. Assuming that R and T are constants over all the bandwidth Δf, then the root mean square (RMS) value of the voltage across a resistor due to thermal noise is given by
that is, the same formula as above.