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FFT解析基礎用語集「サ行」

Sampling Theorem

If the sampling interval is Δt seconds (sampling once every Δt seconds), the sampling frequency will be 1/Δt (sampling 1/Δt points per second). The sampling theorem indicates the limit of information preserved regarding the relationship between a temporally continuous signal and the rate at which it is sampled, stating that "samples must be taken at a frequency of at least twice the highest frequency component contained in the signal." If the sampling frequency is lower than twice the frequency of the signal, aliasing occurs.

time axis calculus

differentiation

The computation of the first and second derivatives uses the 5th order Lagrange interpolation formula, obtaining one data point from the values of five points that include the points before and after.
ƒ 0、ƒ 1、ƒ 2、ƒ 3、ƒ 4 ・・・・are used as sample data.

first derivative

First Order Derivative_No.1

First Order Differential_No.2

First Order Differential No. 3

First Order Differential_No.4

First Order Differential_No.5

First-Order Derivative No. 6

First Order Differential No. 7

second derivative

Second Order Derivative_No.1

Second Derivative_No.2

Second Order Derivative_No.3

Second Order Derivative_No.4

Second Order Derivative_No.5

Second Order Derivative_No.6

Second Order Derivative_No.7

integration

The calculation of single and double integral values is performed using the trapezoidal rule.

Formula for the value of double integrals.

Formula for the value of double integral_No.1

Double Integral Value Operation Formula No. 2

Expression of Multiple Integral Value_No.3

Double Integral Value Operation Formula No. 4

Formula for double integral value

Double Integral Value Calculation Formula_No.1

Double Integral Value Calculation Formula_No.2

Double Integral Value Operation Formula No. 3

Double Integral Value Operation Formula No. 4

time axis waveform

Displays the instantaneous waveform of the signal input from the panel's input connector. One frame is displayed. At this time, the X-axis represents time (in seconds) starting from 0 at the beginning of the frame, and the Y-axis shows the instantaneous value. The full scale of the X-axis is set in accordance with the configured frequency range.

Statistical calculation of time waveforms

Mean (MEAN)

Mean (MEAN)


(2) Effective value (RMS)

(2) Effective value (RMS)


Standard Deviation (S.D.)

The second moment around the mean is called variance, and the square root of variance is referred to as standard deviation. The effective value of a signal, excluding the DC component, is the same as the standard deviation. These values are calculated using the following formula.

(3) Standard Deviation (S.D.) No. 1


The relationships of (1), (2), and (3) are as follows.

(3) Standard Deviation (S.D.)_No.2


(4) Skewness

It is the third moment around the mean normalized by σ 3, used as an indicator of the asymmetry around the mean. It is calculated by the following formula.

(4) Skewness


(5) Kurtosis

The fourth moment around the mean normalized by σ 4 is an indicator of the sharpness of the waveform. It is calculated using the following formula. Since the value of kurtosis for a normal distribution (Gaussian distribution) in time signals is 3, it is sometimes referred to as kurtosis by subtracting 3 from the value obtained from the following formula.

(5) Kurtosis


Crest Factor

Peak value (maximum value) / Effective value

effective value

It is the square root of the mean of the squares of the signal. In English, it is called root mean square (rms).

The formula is

effective value

For a sine wave, the effective value is 1/√2 of the peak value. The data for each line of the power spectrum corresponds to the square of the effective value of the signal in that band, which is the mean square value.

What is effective value?

For example, let's consider an electric heater. When a direct current voltage is applied to the electric heater, heat is generated. The nichrome wire of the electric heater (which may now be a ceramic heater) acts as a resistor, so the circuit can be represented as shown in Diagram 1 below.

  • Figure 1
    Figure 1

Considering the energy (heat) generated when the voltage is 100 V and the resistance is 100 Ω, the current flowing through the resistor is determined by Ohm's law.

What is Effective Value_No.1

Thus, I = E/R = 100 / 100 = 1 (A), and the power W is W = E × I = 100 × 1 = 100 (W). Since calculating current each time is cumbersome, it is generally stated that I = E/R.

What is Effective Value_No.2

is commonly used. We found that applying 100 V to a 100 Ω electric heater generates 100 W of heat. Household power supplies have an RMS voltage of 100 V, but rather than direct current, they provide 50 Hz alternating current (a sine wave) in the Kanto region. How many watts of heat will be generated when a 100 Ω electric heater is connected to this household power supply?
The answer is 100 W. In other words, “the RMS value is the DC voltage that does the same amount of work.” So, how many watts would the same heater generate if used with AC 200 V? <In reality, doing this would probably break the heater.>
AC 200 V has the same power as DC 200 V, so if we consider it as DC 200 V, 200 2 /100 = 400 W, not 200 W. This is because “when the voltage doubles, the current also doubles, and the power becomes four times as great, or 2 2.” So, what is the RMS value in the following Figure 2?

  • Figure 2
    Figure 2

Simply averaging the absolute values gives 1.5 V, but let's consider the actual power generated. Since calculating with a resistance of 100 Ω is cumbersome, we will use 1 Ω instead. The power generated at 1 V and 2 V can be calculated using the following formula, but omitting the resistance of 1 Ω does not change the results.

What is Effective Value_No.3

The square of the voltage corresponds to the power (electricity) generated in a 1 Ω resistor. When you see the square of the voltage or current, think of it as power. (In the case of 1 Ω, voltage and current are equal, so from equation 2, the square of the current also represents power.)

The average power is 2.5 W, as the interval of 1 W is 1/2 and the interval of 4 W is also 1/2. In other words, this waveform has the same power as a DC voltage that generates 2.5 W of power across a 1 Ω resistor.

What is Effective Value_No.4

It can be seen that the effective value is 1.58 V.

The effective value is the square root of the average power. In other words, the effective value is the average of the squares taken square root, which is referred to in English as 'root mean square', and when emphasizing that it is specifically the effective value, it is abbreviated as 'rms'.

The effective value of a sine wave is 1/√2 = 0.707 of the peak value, so the waveform of a household 100 V power supply has a peak value of 141 V, which is √2 times the effective value, as shown in Figure 3 below. (By the way, the average value is 2/π = 0.637.)

  • Figure 3
    Figure 3

Once again, let's connect a 100 Ω electric heater to this power source. Then, the maximum power is;

What is Effective Value_No.5

Therefore, it will be 200 W. It is clear that the minimum power is 0 W, so it is easy to imagine that the generated power fluctuates between 0 W and 200 W. This situation is illustrated in Figure 4 below. It is evident that the average value at this time is 100 W.

  • Figure 4
    Figure 4

frequency response function

The frequency response function (transfer function) represents the relationship between input and output in electrical systems and structural vibration transmission systems, expressed as the ratio of the Fourier spectrum of the input A(f) to the Fourier spectrum of the output B(f).

That is, the frequency response function H(ƒ) is

Frequency Response Function_No.1

In this device, we multiply the complex conjugate A*(ƒ) with the numerator and denominator of the right side of the above equation, and we perform the calculations as shown in the next expression.

Frequency Response Function_No.2

The denominator A(ƒ) × A*(ƒ) is the power spectrum of A(ƒ), and the numerator B(ƒ) × A*(ƒ) is the cross spectrum of A(ƒ) and B(ƒ). From this, the frequency response function H(ƒ) can be obtained by dividing the cross spectrum of the input and output by the power spectrum of the input.

The frequency response function can also be estimated using the following calculation method.

Frequency Response Function_No.3


The transfer function estimated by equation (2) is called H1, and the transfer function estimated by equation (3) is called H2.


Frequency Response Function_No.4

When there is a lot of external noise in the output signal b(t), it is possible to minimize random errors through averaging.

In the case of nonlinear systems, it is possible to linearize them using random signals through averaging (least squares approximation).


Frequency Response Function_No.5

When there is a lot of external noise in the input signal a(t), it is possible to minimize random errors through averaging.

If leakage errors are considered at resonance points, it is possible to reduce bias errors.

Now, if we denote the true transfer function as Ht(f), in cases where there is a lot of noise in both the input and output,

Frequency Response Function_No.6

This will be the relationship. (However, we assume that the system is a linear system.) Also, with respect to the phase, it will be equal to the phase of the cross-spectrum.

The relationship with coherence function is

Frequency Response Function_No.7

This means that γ 2 is the ratio of H2 to H1. If the ratio of the input-output power spectrum (transfer characteristics) is | Ha(ƒ) | 2 then

Frequency Response Function_No.8

Therefore,

Frequency Response Function_No.9

or taking the logarithm

Frequency Response Function_No.10

In other words, the average of the logarithmic values of the gains H1 and H2 is equal to the logarithmic value of the frequency response characteristic Ha.

The frequency response function is represented by gain characteristics and phase characteristics. The gain characteristic represents how the amplitude changes as the signal passes through the system, with the X-axis showing frequency and the Y-axis displaying 20log 10 H(ƒ) in decibels (the amplitude ratio of output to input). Additionally, the phase characteristic represents the lead and lag of the phase between the input signal and the output signal, with the X-axis showing frequency and the Y-axis displayed in degrees or radians.

Frequency Axis Calculus

Differentiation operations in the frequency domain are performed by multiplying (ω)n in the power spectrum and (jω)n in the frequency response function.
(j is the imaginary unit, ω=2πf)

Frequency Axis Calculus_No.1

(Note 1) In the power spectrum, the first derivative is proportional to ω squared and the second derivative is proportional to ω to the fourth power, because they are power values.

(Note 2) The frequency response function involves complex number calculations, so the imaginary unit j is also multiplied.

The integration operation in the frequency domain is performed by dividing by (ω)n in the power spectrum and by (jω)n in the frequency response function.
(j is the imaginary unit, ω=2πf)

Frequency Axis Calculus No. 2

(Note 1) In the power spectrum, the single integral is proportional to the square of omega (ω^2) and the double integral is proportional to the fourth power of omega (ω^4) because they represent power values.

(Note 2) The frequency response function involves complex number operations, so the imaginary unit j is also involved in division.

frequency resolution

The frequency resolution is the value obtained by dividing the frequency range at that time by the number of analysis lines (analysis data length ÷ 2.56). For example, when the frequency range is 10 kHz and the number of sample points (analysis data length) is 4096, the number of analysis lines becomes 1600 lines, so the frequency resolution Δf is 6.25 Hz (=10000/1600).

The frequency resolution during zoom analysis is calculated as (frequency span) ÷ (number of analysis lines).

amplitude probability distribution function

It represents the probability that the instantaneous value of a fluctuating time-axis signal is below a certain amplitude level. The amplitude probability distribution function can be obtained by integrating the amplitude probability density function.

Amplitude Probability Density Function

The amplitude probability density function is used to determine the probability that a fluctuating signal exists at a specific amplitude level, with the horizontal axis representing amplitude (V) and the vertical axis normalized from 0 to 1. This software decomposes the amplitude into 1/512 of the voltage range. The amplitude probability density function allows for the analysis of how much fluctuation the input signal has around certain amplitudes, which can be utilized for pass/fail judgments based on its shape.

Zoom function

In a standard FFT analysis, the range from 0 to the frequency range is analyzed over a number of lines (for example, 800 lines). However, the zoom function allows for analysis at any center frequency over a certain frequency span. By using this function, it becomes possible to analyze even in high frequency bands with high frequency resolution (where Δf is small). At this time, the number of data acquisition points required is proportional to the zoom factor, which can take time.

correlation function

There are autocorrelation functions and cross-correlation functions.

autocorrelation function

The autocorrelation function is defined as a function of the shift amount τ, using the waveform x(t) and the waveform x(t + τ) shifted by τ, as shown in the following equation.

autocorrelation function

The autocorrelation function is effective for examining the periodicity of waveforms. The autocorrelation function reaches its maximum value when τ=0, which is when it takes its own product, and if the waveform is periodic, the autocorrelation function will also show peaks at the same period. Additionally, in irregular signals, if the fluctuations are slow, it will have high values at larger τ, and when the fluctuations are fine, it will show high values at smaller τ, indicating that τ serves as a temporal reference for the variations.

We are calculating the autocorrelation function using the inverse Fourier transform of the power spectrum.

cross-correlation function

The cross-correlation function is defined as a function of the shift amount τ when one of the waveforms of the two signals is delayed by τ, as expressed in the following equation.

cross-correlation function

The cross-correlation function is used to measure the similarity and time delay between two signals. If the two signals are completely different, the cross-correlation function approaches zero regardless of the time lag (τ). It is used to estimate time delays in systems corresponding to input and output signals, detect the presence of signals buried in external noise, and determine signal propagation paths.

It is obtained by the inverse Fourier transform of the cross spectrum.