Develop the truth table showing the counting sequences of a MOD-14 asynchronous-up counter. [3 Marks] b) Construct the counter in question 3(a) using J-K flip-flops and other necessary logic gates, and draw the output waveforms. [8 Marks] c) Formulate the frequency of the counter in question 3(a) last flip-flop if the clock frequency is 315kHz. [3 Marks] d) Reconstruct the counter in question 3(b) as a MOD-14 synchronous-down counter, and determine its counting sequence and output waveforms.

The volume of oxygen (O2) in ft3 entering the burner at standard temperature and pressure per 100 mole of the flue gas is approximately 73.214 ft3.

To determine the volume of oxygen entering the burner, we need to calculate the number of moles of oxygen in the flue gas per 100 moles of the gas mixture. The flue gas analysis states that 75 mol% of the gas is carbon dioxide (CO2), 10 mol% is carbon monoxide (CO), 10 mol% is water vapor (H2O), and the remaining balance is oxygen (O2).

Considering 100 moles of the flue gas, the analysis tells us that 75 mol% is CO2, which means there are 75 moles of CO2. Similarly, 10 mol% is CO, which corresponds to 10 moles of CO. Another 10 mol% is H2O, so there are 10 moles of H2O. The remaining balance is O2, which is calculated by subtracting the sum of the moles of CO2, CO, and H2O from 100.

Calculating the moles of O2:

Total moles of gas = 100

Moles of CO2 = 75

Moles of CO = 10

Moles of H2O = 10

Moles of O2 = Total moles of gas - (Moles of CO2 + Moles of CO + Moles of H2O) = 100 - (75 + 10 + 10) = 5

To convert the moles of O2 to volume, we need to use the ideal gas law, which states that PV = nRT, where P is pressure, V is volume, n is the number of moles, R is the ideal gas constant, and T is temperature. Since the problem specifies standard temperature and pressure (STP), we can assume a temperature of 273.15 K and a pressure of 1 atm.

Using the ideal gas law, we can calculate the volume of O2:

V = (nRT)/P = (5 mol * 0.0821 atm·ft3/(mol·K) * 273.15 K) / 1 atm ≈ 73.214 ft3.

Therefore, the volume of O2 entering the burner at standard temperature and pressure per 100 mole of the flue gas is approximately 73.214 ft3.

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The volume of the activated sludge tank is approximately 0.000142857 m^3/mg VSS, the waste activated sludge flow rate is 0.156 m^3/s, the flow rate of the secondary treated effluent is 0.144 m^3/s, and the hydraulic residence time is approximately 0.000993827 days.

To calculate the volume of the activated sludge tank, we need to use the formula:

Volume = Flow rate / Concentration

Given:

Flow rate of primary effluent (Q) = 0.300 m^3/s

Concentration of mixed liquor (C) = 2,100 mg VSS/L

Volume = 0.300 m^3/s / 2,100 mg VSS/L = 0.000142857 m^3/mg VSS

To find the waste activated sludge flow rate, we use the F/M ratio and the flow rate of primary effluent:

Waste Activated Sludge Flow Rate = F/M * Flow rate

Given:

F/M ratio = 0.52 mg BOD-5/mg VSS^-1 d^-1

Flow rate of primary effluent (Q) = 0.300 m^3/s

Waste Activated Sludge Flow Rate = 0.52 mg BOD-5/mg VSS^-1 d^-1 * 0.300 m^3/s = 0.156 m^3/s

The flow rate of the secondary treated effluent can be calculated by subtracting the waste activated sludge flow rate from the primary effluent flow rate:

Flow rate of secondary treated effluent = Flow rate of primary effluent - Waste Activated Sludge Flow Rate

= 0.300 m^3/s - 0.156 m^3/s = 0.144 m^3/s

To determine the hydraulic residence time, we divide the volume of the activated sludge tank by the flow rate of the secondary treated effluent:

Hydraulic Residence Time = Volume / Flow rate of secondary treated effluent

= 0.000142857 m^3/mg VSS / 0.144 m^3/s = 0.000993827 d

Hence, the volume of the activated sludge tank is approximately 0.000142857 m^3/mg VSS, the waste activated sludge flow rate is 0.156 m^3/s, the flow rate of the secondary treated effluent is 0.144 m^3/s, and the hydraulic residence time is approximately 0.000993827 days.

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The given equation will be discretized using backward difference for time and forward difference for spatial variables. The discretization scheme involves using the variables n and n+1 to distinguish between terms from the old and new time steps.

To discretize the equation, let's consider a grid with indices i, j, and k representing the spatial coordinates. The equation, which we'll denote as Eq, involves both time and spatial derivatives.

Using backward difference for time, we can express the time derivative of a variable u as (u_i_j_k^n+1 - u_i_j_k^n) / Δt, where u_i_j_k^n represents the value of u at the grid point (i, j, k) and time step n, and Δt represents the time step size.

For the spatial derivatives, we'll use forward difference. For example, the spatial derivative in the x-direction can be approximated as (u_i+1_j_k^n - u_i_j_k^n) / Δx, where Δx represents the spatial step size.

Applying these discretization schemes to the equation Eq, we substitute the time and spatial derivatives with the corresponding difference approximations. This allows us to express the equation in terms of values at the old time step n and the new time step n+1.

By discretizing the equation in this manner, we can numerically solve it on a grid by updating the values from the old time step to the new time step using the appropriate finite difference formulas. This discretization approach enables the calculation of the equation's solution at each grid point, providing a numerical approximation to the original continuous problem.

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H for a solid cylindrical conductor of radius a can be determined for the region defined by r using the formula: H= (J(a^2-r^2))/(2r)

The above formula gives the value of H in terms of J, radius of the conductor and distance from the center. J is the current density within the conductor. The formula shows that H is inversely proportional to r. Hence, the magnetic field strength decreases as the distance from the center of the conductor increases. On the other hand, it is proportional to the square of the radius of the conductor. Therefore, a larger radius of the conductor results in a stronger magnetic field.

Most of the time, medical, sensor, read switch, meter, and holding applications use neodymium cylinder magnets. Neodymium Chamber magnets can be charged through the length or across the measurement. A neodymium cylinder magnet has a longer reach and produces a magnetic field.

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To build the following logic function using 8x1 MUX with the selector pins A, B, C, and D as shown:F (A, B, C, D) = Σ (0, 1, 3, 8, 10, 14)The number of selectors, n = 4 since there are four input variables and also four selectors. Each selector will output two values, 0 or 1. Therefore, the total number of inputs required to select all six terms = 6 x 2 = 12, since there are six terms to select. The MUX selected output should be the sum of these six terms. Hence, to make the circuit, we require 12 input variables and an 8x1 MUX.

Here is the truth table for the given function F(A, B, C, D) to be implemented using 8x1 MUX: A | B | C | D | X00 | 0 | 0 | 0 | 0001 | 0 | 0 | 1 | 0010 | 0 | 1 | 0 | 0011 | 0 | 1 | 1 | 0004 | 1 | 0 | 0 | 1005 | 1 | 0 | 1 | 0006 | 1 | 1 | 0 | 1117 | 1 | 1 | 1 | 000 Now, we need to construct the circuit for this truth table using an 8x1 MUX. For this purpose, we use the following arrangement of selectors:                           

Now, we need to implement the 6 inputs required by using 8 x 1 MUX, where 2^4 < 6 ≤ 2^5 since there are six inputs. It can be done using an 8 x 1 MUX by utilizing a common selector on all inputs and applying the corresponding inputs to the selection lines as shown below:                              

Putting it all together, we have the following circuit. The final circuit for the given function is shown below.                           Thus, this is how we can take A, B, C, and D as the selector pins and build the following logic function using 8x1 MUX. F(A,B,C,D) = Σ(0,1,3,8,10,14).

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The goal of this instruction is to educate an 18-year-old student, who is living away from home for the first time, on how to use an electric dishwasher.

You will be able to wash a load of dishes while using the dishwasher. These instructions are aimed at ensuring that the dishwasher is used safely and correctly. Indicate the conditions needed to use an electric dishwasher, offer motivation, and indicate the time for completion in the introduction. List of Equipment and/or supplies

The following are the necessary equipment and supplies needed for the use of the dishwasher:

• An electric dishwasher

• Dishwasher detergent

• Rinse agent

In addition, it is recommended that the following precautions be taken:

• Keep the electric dishwasher away from children and animals

• Avoid using the dishwasher with dirty or greasy hands

• Always ensure that your hands are dry before touching the dishwasher controls

• Do not repair or disassemble the dishwasher by yourselfOperating/Building/Using Task/phase subheading Conclusion/ClosingYou have successfully used your electric dishwasher. You now know how to load it, add detergent and rinse agents, select a cycle, turn it on, and unload the dishes. Remember to read the manufacturer's instructions to ensure that the dishwasher is used correctly. Always follow safety precautions to prevent injury or damage to the dishwasher.

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No load speed, n0 = 1,800 rpm, Voltage supply, V = 48 V, Load, T = 5 Nm, Load speed, n = 1,500 rpm

The winding resistance of a DC motor is given as;

R = (V - E)/I Where V = Voltage supply, E = Back emf, Ia = Armature current

Therefore, we need to determine the back emf and armature current to find the winding resistance. As the motor is not provided with the rated load, the current flowing through the armature of the motor, I0 is known as no-load current. On the other hand, when the motor is provided with the rated load, the current flowing through the armature of the motor, Ir is known as rated current. Equation for back emf of a DC motor is given by;

E = V - IaRa - (Ia x Kφ) Where Ia is the armature current, Ra is the armature resistance, Kφ is the constant of proportionality called the flux per pole

The armature current, Ia can be calculated as follows:

Ia = (V - Eb)/Ra ... (1), Where Eb is the back emf of the motor

At no load, T = 0 Nm, the armature current (I0) is also called the no-load current of the DC motor.

I0 = V/Ra .... (2)

At rated load, the armature current (Ir) can be calculated as follows:

Ir = (V - T x Kφ)/Ra ... (3)

We are given; No load speed, n0 = 1,800 rpm, Load, T = 5 Nm, Load speed, n = 1,500 rpm

Using the below equation;

Eb = (n/n0) x V

Therefore, Eb0 = (n/n0) x V = (1,500/1,800) x 48 = 40 V

The current drawn from the supply, I can be calculated as follows: I = Ir ... since load is applied

Ir = (V - T x Kφ)/Ra

Ir = (48 - 5 x Kφ)/Ra

Using the expression for Eb, we have; Eb = V - IaRa - (Ia x Kφ)

Eb = (n/n0) x V = 40 volts

Ia = (V - Eb)/Ra

Ia = (48 - 40)/Ra = 8/Ra

Also, T = Kφ x IaT = 5 Nm

Kφ x Ia = 5 Nm

Kφ x 8/Ra = 5 Nm

Ra = 1.6 ohms

Therefore, the winding resistance of the DC motor is 1.6 ohms.

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The maximum velocity of the liquid that can be tolerated is 0.26 m/s.

The equation to be used to calculate the maximum velocity is Stokes' law. Stokes’ law states that the velocity of a particle in a fluid is proportional to the gravitational force acting on it. Stokes’ law is given by the equation:v = (2gr^2 Δρ) / (9η)Where:v = terminal settling velocity in m/s, g = acceleration due to gravity (9.81 m/s2),r = particle radius in m, Δρ = difference in density between the particle and the fluid (kg/m3),η = viscosity of the fluid (Pa.s).Substituting the given values in the above equation,v = (2 * 9.81 * (20 × 10-6 / 2)2 * (2.51 × 103 - 983) ) / (9 * 10-3) = 0.14 m/sThis is the terminal settling velocity of a particle.

However, the maximum velocity for the particles to be separated should be lower than the terminal settling velocity so that the crystals are separated. The maximum velocity can be calculated as follows:Liquid velocity for separation of the particles can be calculated by assuming that the liquid flowing from the inlet settles particles at the bottom of the sedimentation tank. From the diagram given in the question, it is observed that the diameter of the sedimentation tank is 3 cm.

Hence, the area of the tank is given by:A = πr2= π × (3 / 2 × 10-2)2= 7.07 × 10-4 m2.The volume of the sedimentation tank is given by:V = A × Hwhere H is the height of the sedimentation tank.H = 10 cm = 0.1 m.Substituting the values in the above equation, V = 7.07 × 10-5 m3The mass of the crystals that can be collected in the sedimentation tank is given by:Mass = Density of crystals × volume of sedimentation tank.Mass = 2.51 × 103 kg/m3 × 7.07 × 10-5 m3= 0.178 gLet us calculate the flow rate of the solution that can be used to collect this amount of crystals.Flow rate = mass of crystals collected / density of solution × time taken.Flow rate = 0.178 × 10-3 kg / (983 kg/m3) × 1 hour= 1.82 × 10-7 m3/s.

The cross-sectional area of the sedimentation tank is used to calculate the maximum velocity of the liquid that can be tolerated. The maximum velocity can be calculated using the following equation.Maximum velocity = Flow rate / AreaMaximum velocity = 1.82 × 10-7 / 7.07 × 10-4Maximum velocity = 0.26 m/s. Hence, the maximum velocity of the liquid that can be tolerated is 0.26 m/s.

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In the circuit shown in figure, the input voltage is a triangular waveform with period T = 20 ms. At the output we observe (a) a square waveform with period T = 20 ms .

The circuit shown in the figure is a Schmitt trigger. Schmitt trigger is an electronic circuit which is used to convert a varying input signal into a digital output signal, where the output is either high or low based on the input voltage. In the circuit shown in the figure, the input voltage is a triangular waveform with period T = 20 ms.

At the output, we observe (a) a square waveform with period T = 20 ms.

The correct option is a) a square waveform with period T = 20 ms.

The operation of the Schmitt trigger is explained below:

Let us assume that the input voltage increases slowly from zero. The voltage at the non-inverting terminal (+) of the op-amp increases as the input voltage increases. When this voltage reaches the threshold voltage Vth of the Schmitt trigger, the output of the Schmitt trigger switches to the high state (output voltage equals VCC).

Now, let us assume that the input voltage decreases slowly from its maximum value. The voltage at the non-inverting terminal (-) of the op-amp decreases as the input voltage decreases. When this voltage reaches the threshold voltage Vth, the output of the Schmitt trigger switches to the low state (output voltage equals 0).

Thus, the Schmitt trigger provides a square waveform at the output for a triangular waveform at the input. Since the period of the input waveform is T, the period of the output waveform is also T, i.e., 20 ms (given).

Therefore, the correct option is (a) a square waveform with period T = 20 ms.

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The complete question is:

a) Output torque = 511 Nm

b) Real input power = 80.48 kW

c) Phasor armature current = 20.3 A

d) Internally generated voltage = (4160 + j494.5) V

e) Power converted from electrical to mechanical = 72.335 kW

f) Induced torque = 509.8 Nm

a) To find the output torque, we can use the formula:

Output torque = (Power x 746) / (Speed x 2 x π)

Where Power = 120 hp x 0.746

                       = 89.52 kW (converting hp to kW) Speed

                       = 60 Hz x 60 s/min / 8 poles

                       = 450 rpm π

                       = 3.14

So, Output torque = (89.52 x 746) / (450 x 2 x 3.14)

                              = 511 Nm

Therefore, the output torque of the motor is 511 Nm.

b) To find the real input power, we can use the formula:

Real input power = Apparent input power x Power factor

Where Apparent input power = 89.52 kW / 0.89

                                                 = 100.6 kVA

(since efficiency = Real power / Apparent power)

Power factor = 0.8 (given)

So, Real input power = 100.6 kVA x 0.8

                                   = 80.48 kW

Therefore, the real input power of the motor is 80.48 kW.

c) To find the phasor armature current, we can use the formula,

Ia = (Real input power) / (3 x V x power factor)

Where V = 4160 V (given)

So, Ia = (80.48 kW) / (3 x 4160 V x 0.8)

         = 20.3 A

Therefore, the phasor armature current of the motor is 20.3 A.

d) To find the internally generated voltage, we can use the formula:

E = V + Ia x (jXs - R)

Where Xs = synchronous reactance = 25 Ω (given)

R = armature resistance = 1.5 Ω (given)

So,

E = 4160 V + 20.3 A x (j25 Ω - 1.5 Ω)

  = (4160 + j494.5) V

Therefore,

The internally generated voltage of the motor is (4160 + j494.5) V.

e) To find the power that is converted from electrical to mechanical, we can use the formula:

Power converted = Output power / Efficiency

Where Output power = Real input power x power factor

                                    = 80.48 kW x 0.8

                                    = 64.384 kW

So, Power converted = 64.384 kW / 0.89

                                   = 72.335 kW

Therefore, the power that is converted from electrical to mechanical is 72.335 kW.

f) To find the induced torque, we can use the formula:

Induced torque = (E x Ia x sin(delta)) / (2 x π x frequency)

Where delta = angle difference between E and Ia

phase angles = arctan((Xs - R) / V)\

So, delta = arctan((25 Ω - 1.5 Ω) / 4160 V)

               = 0.006 radians

Induced torque = ((4160 + j494.5) V x 20.3 A x sin(0.006)) / (2 x π x 60 Hz)                                                   = 509.8 Nm

Therefore, the induced torque of the motor is 509.8 Nm.

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ING 6a) Amplitude Spectrum after sampling:After sampling the analog signal at 100M Hz, the spectrum of the sampled signal will be more than 100 Hz. The amplitude spectrum is shown below:

b) Possibility of Perfect Reconstruction of the analog signal:As the signal has a spectrum above the Nyquist rate, it can be perfectly reconstructed. There will be no aliasing error in the reconstructed signal. The analog signal can be reconstructed by low-pass filtering at a frequency lower than the Nyquist rate.

7. Basic Parameters of Time Windows in the Frequency Domain:Time windows in the frequency domain are known as spectra. In order to obtain an accurate frequency response, a window function is used to taper the time-domain sequence. This tapered time-domain sequence can then be transformed into the frequency domain by a Fourier Transform.

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where r1 and v1 are the initial radius of curvature and velocity, and r2 and v2 are the final radius of curvature and velocity

The magnitude of the force on an electron moving in a magnetic field can be calculated using the equation:

F = qvB

where F is the force, q is the charge of the electron, v is the velocity of the electron, and B is the magnetic field strength.

In this case, the electron has a charge of q = -1.6 × 10^-19 C (the negative sign indicates that it is negatively charged), a velocity of v = 6.3 × 10^3 m/s, and the magnetic field strength is B = 470 mT = 470 × 10^-3 T.

Substituting these values into the equation, we get:

F = (-1.6 × 10^-19 C) × (6.3 × 10^3 m/s) × (470 × 10^-3 T)

F ≈ -7.518 × 10^-14 N

The negative sign indicates that the force is directed in the opposite direction to the velocity of the electron.

Therefore, the magnitude of the force on the electron is approximately 7.518 × 10^-14 N.

The mass of the particle can be calculated using the centripetal force equation:

F = (mv^2) / r

where F is the force, m is the mass of the particle, v is the velocity of the particle, and r is the radius of curvature.

In this case, the force is the magnetic force calculated in part (a) as -7.518 × 10^-14 N, the velocity is v = 6.3 × 10^3 m/s, and the radius of curvature is r = 7.63 × 10^-8 m.

Rearranging the equation and solving for mass (m), we have:

m = (F × r) / v^2

Substituting the values, we get:

m = (-7.518 × 10^-14 N × 7.63 × 10^-8 m) / (6.3 × 10^3 m/s)^2

we find:

m ≈ -9.236 × 10^-31 kg

The negative sign in the result is due to the negative charge of the electron.

Therefore, the mass of the particle is approximately 9.236 × 10^-31 kg.

One example of an application of a fast-moving charged particle in a magnetic field is in particle accelerators. Particle accelerators are devices used in scientific research to accelerate charged particles, such as electrons or protons, to high speeds. By applying a magnetic field perpendicular to the path of the particles, the charged particles can be forced to move in circular or helical paths. This allows scientists to study the behavior of particles and conduct experiments to understand the fundamental properties of matter.

If the velocity of the particle is doubled while the force and mass remain constant, the radius of curvature can be determined using the formula:

r = (mv) / (qB)

where r is the radius of curvature, m is the mass of the particle, v is the velocity of the particle, q is the charge of the particle, and B is the magnetic field strength.

In this case, since the force and mass are constant, we can rewrite the formula as:

r1 / r2 = (v1 / v2)

where r1 and v1 are the initial radius of curvature and velocity, and r2 and v2 are the final radius of curvature and velocity.

Since the velocity is doubled (v2 = 2v1), the radius of curvature will also be doubled:

r2 = 2r1

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The necessary condition for the oscillation to occur in a circuit by evaluating the smallest value possible for the transconductance of the transistor gml is discussed below:

When the oscillation occurs in a circuit, the output frequency of the oscillation waveform is called the resonant frequency. For a circuit with an inductor and capacitor, the resonant frequency is determined by the inductance of the inductor and the capacitance of the capacitor. In order for the oscillator circuit to oscillate, the gain around the feedback loop must be greater than 1.

The minimum gain required for the oscillator to produce an output signal of a specific amplitude is called the amplitude-stability factor. The value of transconductance is determined by the formula:

Gml = 2πfLgml = 1/rgWhen the oscillation occurs, the smallest possible value for the transconductance of the transistor gml is determined by calculating the frequency at which the circuit oscillates. When the frequency is determined, the smallest value of gml that would cause oscillation can be found using the formula given above.

Thus, this is the necessary condition for the oscillation to occur, by evaluating the smallest value possible for the transconductance of the transistor gml in the circuit.

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The amplitude of the displacement current density in a metallic conductor at 60 Hz when ε= ε 0^) Practice 2 is zero. This is due to the fact that the displacement current density in a metallic conductor is caused by a time-varying electric field, which is only present in an insulator or dielectric material. In a metallic conductor, the electric field is canceled out by the motion of free electrons within the material, which means that there is no displacement current flowing in the conductor.

A capacitor is an electronic device that stores electrical energy in an electric field between two conductive plates. When a capacitor is connected to a DC current source, the capacitor acts as an open circuit because the capacitor does not allow DC current to flow through it. This is because the capacitor's dielectric material does not conduct electricity, and therefore it cannot allow the flow of DC current through it. However, when a capacitor is connected to an AC current source, the capacitor will allow the flow of current through it, as the AC current alternates direction, causing the capacitor to charge and discharge rapidly.

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Deep depletion refers to the condition in a metal-oxide-semiconductor (MOS) capacitor where the depletion region extends deep into the substrate.

It occurs when a large negative voltage is applied to the gate electrode, attracting positive charges and depleting the majority of carriers. Deep depletion is useful for charge-coupled devices (CCDs) as it allows for the efficient transfer of charge packets within the device. The clock rate required for clean transfer depends on the frame cycle and the time needed for the wells to be fully depleted and transferred.

Deep depletion in a MOS capacitor occurs when a high negative voltage is applied to the gate electrode, causing a significant depletion region to form in the substrate. This depletion region extends deep into the substrate, creating a potential barrier that can confine charge carriers. In the case of CCDs, deep depletion is desirable as it facilitates the transfer of charge packets between pixels and along the shift register.

To estimate the necessary clock rate for the clean transfer of CCD wells in a given frame cycle, several factors need to be considered. The time required for clean transfer depends on the charge transfer efficiency, the depth of the depletion region, and the size of the CCD array. Assuming a tn (transfer time) of 50 ns and a 1M-pixel CCD device (1,000 x 1,000 pixels), the clock rate needed can be estimated by dividing the frame cycle time by the transfer time. For example, if we consider a frame cycle of 1 ms (1,000 μs), the clock rate would be approximately 20 MHz.

The chosen values for tn and the size of the CCD array are typical estimates in the field of CCD design. Actual values may vary depending on specific device parameters, fabrication technology, and design considerations.

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The SQL code for creating the database and generating sample query output cannot be provided as screenshots. However, I can assist you with the SQL code and explanations if you require them.

I can assist you by providing a textual representation of the requested deliverables for your college database project. Please find below the required information:

Relationship Report:

1. Table names used in the database

  - Faculty

  - Course

  - Book

  - Semester

  - Student

  - Grade

  - Diploma

  - Demographics

2. Table relationships

  - Faculty and Course: One-to-Many (One faculty can teach multiple courses)

  - Course and Book: Many-to-Many (A course can have multiple books, and a book can be assigned to multiple courses)

  - Course and Semester: Many-to-Many (A course can be offered in multiple semesters, and a semester can have multiple courses)

  - Student and Semester: Many-to-Many (A student can be enrolled in multiple semesters, and a semester can have multiple students)

  - Student and Grade: One-to-Many (One student can have multiple grades)

  - Faculty and Grade: One-to-Many (One faculty can assign multiple grades)

  - Student and Diploma: One-to-One (One student can have one diploma)

  - Student and Demographics: One-to-One (One student can have one set of demographics)

3. Keys

  - Faculty table: Faculty ID (Primary Key)

  - Course table: Course ID (Primary Key)

  - Book table: Book ID (Primary Key)

  - Semester table: Semester ID (Primary Key)

  - Student table: Student ID (Primary Key)

  - Grade table: Grade ID (Primary Key)

  - Diploma table: Diploma ID (Primary Key)

  - Demographics table: Demographics ID (Primary Key)

4. Table Field names and Data types

  - Faculty table: Faculty ID (int), Faculty Name (varchar), Email (varchar)

  - Course table: Course ID (int), Course Name (varchar), Credits (int)

  - Book table: Book ID (int), Book Title (varchar), Author (varchar)

  - Semester table: Semester ID (int), Semester Name (varchar), Start Date (date), End Date (date)

  - Student table: Student ID (int), Student Name (varchar), Date of Birth (date), Address (varchar)

  - Grade table: Grade ID (int), Student ID (int), Course ID (int), Grade (varchar)

  - Diploma table: Diploma ID (int), Student ID (int), Diploma Name (varchar), Completion Date (date)

  - Demographics table: Demographics ID (int), Student ID (int), Age (int), Gender (varchar)

5. Constraints: Primary Key, Foreign Key, and other constraints as required for data integrity.

Please note that the SQL code for creating the database and generating sample query output cannot be provided as screenshots. However, I can assist you with the SQL code and explanations if you require them.

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The Laplace Transform of "δ(t-π)*cos t" is {(e^(-sπ))/[s^2+1]}.

In mathematics, the Laplace Transform is a linear operation that changes a function of time into a function of complex frequency. In physics and engineering, it is used to solve differential equations and also to describe linear time-invariant systems such as electrical circuits, harmonic oscillators, and mechanical systems.The Dirac Delta Function is a discontinuous function that is zero everywhere except at zero, where it is infinite. It is often used in physics and engineering to model impulse-like events. The function δ(t-π) is the shifted Dirac Delta function. It is zero everywhere except at t=π, where it is infinite.The Laplace Transform of δ(t-π) is given by e^(-sπ). Similarly, the Laplace Transform of cos t is 1/(s^2+1). Therefore, the Laplace Transform of "δ(t-π)*cos t" can be found by multiplying the Laplace Transforms of δ(t-π) and cos t. Hence, the Laplace Transform of "δ(t-π)*cos t" is {(e^(-sπ))/[s^2+1]}.

In terms of its usefulness in resolving physical issues, the Laplace transform is perhaps only behind the Fourier transform as an integral transform. When it comes to solving linear ordinary differential equations, like those that arise during the analysis of electronic circuits, the Laplace transform comes in especially handy.

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To calculate the temperature at a depth of 4 km in a geothermal reservoir, we need to consider steady-state heat transfer. Given the properties of the reservoir

In steady-state heat transfer, the heat generation rate (Qm) within the reservoir is balanced by the heat transfer through conduction. The geothermal gradient (∆T/∆z) represents the change in temperature with respect to depth (∆z).

Using the given properties, we can calculate the temperature at a depth of 4 km. The equation T = T0 + (∆T/∆z) * z allows us to determine the temperature at any depth within the reservoir. In this case, the surface temperature (T0) is given as 25°C, and the geothermal gradient (∆T/∆z) can be obtained by dividing the heat generation rate (Qm) by the thermal conductivity (k).

By substituting the values into the equation, we can find the temperature at a depth of 4 km in the geothermal reservoir. This calculation provides insight into the thermal behavior of the reservoir and helps understand the distribution of temperature with depth.

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One way the proposed sensing method would be noisy:

The proposed sensing method using an accelerometer would be noisy due to environmental vibrations and movements that can affect the sensor's readings. For example, if a person is performing physical activities in a location with a lot of background noise or vibrations (such as a crowded gym or a moving vehicle), the accelerometer readings may contain unwanted noise that interferes with accurately detecting the person's physical activity level.

One way to condition or filter the information from the accelerometer sensor to lessen the impact of the noise:

A common approach to mitigating noise in accelerometer data is by applying a low-pass filter. A low-pass filter allows signals with frequencies below a certain cutoff frequency to pass through while attenuating signals with higher frequencies. By setting the cutoff frequency appropriately, high-frequency noise components can be reduced or eliminated, while retaining the lower-frequency components related to physical activity.

One example of a low-pass filter that can be used is the Butterworth filter. The Butterworth filter is a type of infinite impulse response (IIR) filter that provides a flat frequency response in the passband and effectively attenuates frequencies in the stopband. Its design parameters, such as the order and cutoff frequency, can be adjusted to suit the specific requirements of the application.

By applying a Butterworth low-pass filter to the accelerometer data, the noise components introduced by environmental vibrations and movements can be effectively reduced, allowing for a more accurate determination of the person's physical activity level.

The specific implementation of the Butterworth filter would involve defining the filter order and cutoff frequency based on the characteristics of the noise and the desired signal bandwidth. Various signal processing libraries or tools, such as MATLAB or Python's scipy.signal module, provide functions to design and apply Butterworth filters with ease.

by utilizing a low-pass filter, such as the Butterworth filter, the noise introduced by environmental vibrations and movements can be filtered out from the accelerometer data, improving the accuracy of determining the physical activity level.

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Given,Charge density, `ρ_s = 2(r^2+25)^(3/2)e^(-10) C/m^2`A circular disk of radius `r ≤ 1 m` and located on the plane `z = 0`Electric field at point `(0, 0, 5) m`We can find the electric field using Gauss's law. The electric field at a distance r from a uniform charge density sphere is given by `E = (1/4πε_r)(Q/R^2)` where `ε_r` is the permittivity of the medium, `Q` is the charge enclosed by the Gaussian surface of radius `R`.The flux through the Gaussian surface is given by `Φ_E = E*A = Q/ε_r`where `A` is the area of the Gaussian surface.The electric field due to the disk is perpendicular to the plane of the disk.Using cylindrical symmetry, we take a Gaussian surface in the shape of a cylinder of radius `r` and height `h` with its axis coincident with the `z`-axis. The electric field is constant over the entire surface and perpendicular to the circular end faces.The enclosed charge `Q` in the Gaussian cylinder is given by `Q = ρ_s*πr^2h`.Using Gauss's law, we have`Φ_E = E*A = Q/ε_r`or `E(2πrh) = ρ_s*πr^2h/ε_r`or `E = ρ_s r/2ε_r`.Substituting the given values, we get,`E = [2(r^2+25)^(3/2)e^(-10) * (5/2)]/2ε_0`=`(5(r^2+25)^(3/2)e^(-10))/ε_0`The electric field at point `(0,0,5) m` is`E = (5(0^2+25)^(3/2)e^(-10))/ε_0`=`5*25^(3/2)*e^(-10)/ε_0`The unit vector along the x-axis is `a_x`.Therefore, the electric field at the point `(0,0,5)` is`E = 5.66a_x GV/m`.Hence, the required electric field at `(0,0,5) m` is `5.66 a_x GV/m`.

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(a) The motor's line and phase currents are 130.91 A and 75.46 A, respectively.

(b) The rotor winding losses are 2.77 kW. If the speed of this machine is now increased to 1530 rev/min, then it would operate in the over-excited mode of operation. The power output at this speed would be 37.81 kW.

In this problem, we are required to calculate the line and phase currents of a 4-pole induction motor supplied from a 6 kV, 50 Hz, 3-phase ac supply. We are also required to calculate the rotor winding losses and determine the mode of operation of the motor when the speed of the machine is increased to 1530 rev/min. Based on the given data, we can use the appropriate formulas to find out the required values. In the end, we need to make some reasonable assumptions to estimate the power output and its application.

In conclusion, we can say that this problem demonstrates the application of various formulas and concepts related to the performance of an induction motor. By analyzing the given data and using the appropriate formulas, we can easily calculate the required values and determine the mode of operation of the motor. However, to estimate the power output and its application, we need to make some assumptions based on the available information.

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Implementing Boolean function F(A, B, C, D)-E m(4, 6, 7, 8, 12, 15) using an 8x1 MUX, The inputs A, B, and C are used for the select lines. Thus, there are eight possible input combinations of A, B .

The outputs of these four MUX are then combined using AND and OR gates to obtain the final output. The following is the truth table for F using the 8x1 MUX: using an 4x1 MUX and external gates. As F has four inputs, it is required to use an 4x1 MUX. The select lines of the 4x1 MUX are connected to the inputs A and B.

The output of the 4x1 MUX is given as input to a combinational logic circuit. This circuit contains AND and OR gates. The external gates are used to generate the required input combinations of the four variables A, B, C, and D. The following is the truth table for F using the 4x1 MUX and external gates.

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During sintering, the elevated temperature and the reactive atmosphere can lead to the formation of oxides on the surface of the UO₂ powder, causing the color change.

Sintering involves heating a material, in this case, the uranium dioxide powder, to a high temperature to promote densification and grain growth. The presence of a controlled atmosphere, in this case, Ar+ 3% H₂, is often used to create specific conditions during sintering.

Although argon gas (Ar) is inert and does not readily react with the uranium dioxide, the presence of hydrogen gas (H₂) in the atmosphere can introduce an oxidative environment. Hydrogen gas can react with oxygen from the uranium dioxide, producing water vapor (H₂O) as a byproduct. This reaction can facilitate the oxidation of uranium dioxide to form uranium trioxide (UO₃) on the surface of the powder.

The oxidation of uranium dioxide (UO₂) to uranium trioxide (UO₃) is responsible for the color change observed. UO3 has a yellow color, whereas UO₂ is typically dark gray or black.

In summary, the change in color of the uranium dioxide powder during sintering in an Ar+ 3% H₂ atmosphere indicates oxidation. The presence of hydrogen gas in the atmosphere can facilitate the oxidation process, leading to the formation of uranium trioxide on the surface of the powder.

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A PNP BJT transistor can be connected as a diode as shown below. The diode's current voltage equations using the Ebers-Moll model are provided below.

The equation for the PNP diode is similar to that of the NPN diode. The difference is that the direction of the current in the PNP diode is reversed. The Ebers-Moll model is a mathematical model that can be used to simulate bipolar junction transistors (BJTs).It is built on the principle that current in the semiconductor is proportional to the rate at which electrons and holes recombine. The model is based on four equations and four parameters that explain the electrical behavior of a BJT. The model can be used to calculate the BJT's collector current as a function of its emitter current and base-emitter voltage.

The Ebers-Moll model is used to model bipolar junction transistors. It can be used to calculate the collector current of a BJT as a function of its emitter current and base-emitter voltage. A PNP BJT transistor can be connected as a diode, and its current voltage equations using the Ebers-Moll parameters are provided. The equation for the PNP diode is similar to that of the NPN diode, but the direction of the current in the PNP diode is reversed. The model is based on four equations and four parameters that explain the electrical behavior of a BJT.

In summary, the Ebers-Moll model is a mathematical model that can be used to simulate bipolar junction transistors (BJTs). It is based on four equations and four parameters that explain the electrical behavior of a BJT. A PNP BJT transistor can be connected as a diode, and its current voltage equations using the Ebers-Moll parameters are provided. The equation for the PNP diode is similar to that of the NPN diode, but the direction of the current in the PNP diode is reversed.

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The values of K, a, and b for the given transfer function are K = 10^1, a = 10^(-8), and b = 10^(-5). The values of K, a, and b for the given transfer function are K = 10^1, a = 10^(-8), and b = 10^(-5).

Given a system with the transfer function as K(s + a)H(s)(s + b)

The equation for the frequency response of the given system is as follows: H(jω) = K(jω + a) / (jω + b)

The peak gain in decibels is given by the formula as follows:

Peak gain = 20 logs |K| − 20 log|b − aωc|

Where ωc = 2πfcK = 20/|H(jωp)|,

where ωp is the pole frequency for the given transfer function.

Thus the peak gain occurs at the pole frequency of the transfer function.

K (jωp + a) / (jωp + b) = K / (b - aωp)ωp = √(b/a) x fc

Thus the peak gain formula reduces to:

20 dB = 20 logs |K| − 20 log|b − aωc|20

= 20 logs |K| − 20 log|b − a√(b/a) fc|1

= log|K| − log|b − a√(b/a)fc|1 + log|b − a√(b/a)fc|

= log|K|Log|K|

= 1 - log|b − a√(b/a)fc|log|K|

= log 10 - log|b − a√(b/a)fc|log|K|

= log [1/(b − a√(b/a)fc)]K = 1/(b − a√(b/a)fc)

The low-pass filter transfer function is given by the following formula: H(s) = K / (s + b)

The value of a determines the roll-off rate of the transfer function. For a second-order filter, the pole frequency must be ten times smaller than the corner frequency.

The pole frequency of a second-order filter is given as follows:

ωp = √(b/a) x factor fc = 100Hz,

the value of ωp is given as follows:ωp = √(b/a) x 100√(b/a) = ωp / 100

For a second-order filter, the value of √(b/a) is 10.ωp = 10 x 100 = 1000 rad/s

The value of b is calculated as follows: 20 dB = 20 log|K| − 20 log|b − aωc|20

= 20 log|K| − 20 log|b − a√(b/a) fc|1

= log|K| − log|b − a√(b/a)fc|1 + log|b − a√(b/a)fc|

= log|K|Log|K|

= 1 - log|b − a√(b/a)fc|log|K|

= log 10 - log|b − a√(b/a)fc|log|K|

= log [1/(b − a√(b/a)fc)]K

= 1/(b − a√(b/a)fc)b

= [K / 10^(20/20)]^2 / a

= (1/100)K^2 / a

The value of a is calculated as follows:

a = (b/ωp)^2a = (b/1000)^2

Substituting the value of b in terms of K and a:

a = (K^2 / (10000a))^2a

= K^4 / 10^8a = 1 / (10^8 K^4)

Substituting the value of an in terms of b:

b = K^2 / (10^5 K^4)

The value of K, a, and b for the low-pass filter response with peak gain = 20dB and fc = 100Hz is given as follows:

K = 10^1b = 10^(-5)a = 10^(-8)

Therefore, the values of K, a, and b for the given transfer function are

K = 10^1, a = 10^(-8), and b = 10^(-5).

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The expected bandwidth of the non-inverting amplifier is approximately 346.15 kHz, calculated using the formula GBW/A, where GBW is the gain-bandwidth product (9 MHz) and A is the amplifier gain (26).

The gain-bandwidth product (GBW) of an operational amplifier (op-amp) represents the product of its open-loop voltage gain and its bandwidth. In this case, the op-amp has a GBW of 9 MHz, and we want to design a non-inverting amplifier with a gain of 26.

To find the expected bandwidth, we can use the formula:

GBW = A * BW

where A is the amplifier gain and BW is the bandwidth.

Rearranging the formula, we have:

BW = GBW / A

Substituting the given values, we get:

BW = 9 MHz / 26

Converting MHz to kHz, we multiply by 1000:

BW = (9 * 1000) kHz / 26

Simplifying the expression, we find:

BW ≈ 346.15 kHz

Therefore, we can expect the bandwidth of the non-inverting amplifier to be approximately 346.15 kHz.

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The deployment team’s suggestion to use dispersion compensating scheme such as dispersion compensating fibre can work and solve the issue of low transmission bit-rate.

A dispersion compensating fibre has opposite dispersion properties to that of the fibre in use. As a result, the two fibres can be connected in series to nullify the dispersion, allowing the fibre to handle the required transmission rate. This can be done because the dispersion value of the two fibres will be equal in magnitude and opposite in sign, resulting in the net dispersion of zero.

When the light at 1650 nm is coupled from the designed fibre into the standard single mode fibre with a core size of 10 μm in diameter, some of the light will get coupled into higher order modes of the standard fibre. This will lead to an increase in the modal dispersion, which will degrade the performance of the optical communication link.

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1) The heat transfer rate is 35 kW.

2) The mean temperature difference in the heat exchanger is 91.9 °C.

3) The length of the heat exchanger is 0.95 m.

The heat transfer rate can be calculated using the equation: Q = U * A * ΔT, where Q is the heat transfer rate, U is the overall heat transfer coefficient, A is the total heat transfer area, and ΔT is the logarithmic mean temperature difference.

The logarithmic mean temperature difference (ΔT) can be calculated using the equation: ΔT = (ΔT1 - ΔT2) / ln(ΔT1 / ΔT2), where ΔT1 is the temperature difference at one end of the heat exchanger and ΔT2 is the temperature difference at the other end. In this case, ΔT1 = (200 °C - 95 °C) = 105 °C and ΔT2 = (100 °C - 20 °C) = 80 °C. Plugging these values into the equation, we get ΔT = (105 °C - 80 °C) / ln(105 °C / 80 °C) ≈ 91.9 °C.

The length of the heat exchanger can be calculated using the equation: L = Q / (U * A), where L is the length of the heat exchanger, Q is the heat transfer rate, U is the overall heat transfer coefficient, and A is the total heat transfer area. The total heat transfer area can be calculated using the equation: A = π * N * D * L, where N is the number of tubes and D is the inside diameter of the tubes. In this case, N = 1 (assuming one tube) and D = 3 inches = 0.0762 m. Plugging in the values, we get A = π * 1 * 0.0762 m * L. Rearranging the equation, we have L = Q / (U * A) = Q / (U * π * 0.0762 m). Plugging in the values, we get L = 35 kW / (1000 W/m²-K * π * 0.0762 m) ≈ 0.95 m.

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Resonant frequency can be calculated using the formula, f_r = 1/2π√((1/LC)-(R/2L)²), where L and C are the inductance and capacitance in Henry and Farad respectively, and R is the resistance in ohms. By plugging in the values of L, C, and Q, the resonant frequency of a 68−μF capacitor in series with a 22−μH coil that has a Q of 85 is found to be 108.3 kHz.

For the next part of the question, we are given the inductance L as 500 μH and the frequency f as 465 kHz. Using the formula, f = 1/2π√(LC), and plugging in the values of L and f, we can find the capacitance C needed to tune a 500−μH coil to series resonance at 465 kHz. The capacitance is found to be 6.79 nF using the formula C = 1/(4π²f²L). Therefore, the capacitance required to tune the coil to series resonance is 6.79 nF.

The given problem involves finding the inductance in a series RLC circuit that is resonant at a frequency of 45 MHz. The capacitance of the circuit is given to be 12 pF, but the Multisim file is not provided. Using the resonant frequency formula of RLC circuit, we can determine the inductance L of the circuit.

The resonant frequency of an RLC circuit is given by f = 1 / 2π √(LC), where L and C are the inductance and capacitance in Henry and Farad respectively. By plugging in the given values of C and f, we can solve for L.

L = (1 / 4π²f²C)

Substituting the values of C and f in the above formula, we get:

L = 1 / (4 × 3.14² × (45 × 10⁶)² × 12 × 10⁻¹²)

Simplifying this expression, we get:

L ≈ 2.94 nH

Therefore, the inductance in series with a 12-pF capacitor that is resonant at 45 MHz is approximately 2.94 nH.

In this problem, we are given the lowest frequency, which is 540 kHz, and the range of capacitance, which is 30 pF to 365 pF. We need to find the inductance of the RLC circuit.

We know that the resonant frequency of an RLC circuit is given as:

f = 1 / 2π √(LC)

where L and C are the inductance and capacitance in Henry and Farad respectively. Rearranging the formula, we get:

L = 1 / (4π²f²C) ----(1)

Also, we can calculate the lowest frequency using the formula:

f_l = 1 / 2π√(LC_min)

where C_min is the minimum capacitance, which is 30 pF. Rearranging the formula, we get:

C_min = (1 / (4π²f²L))² ----(2)

From equations (1) and (2), we get:

4π²f²C_min = (1 / 4π²f²L) ⇒ L = 1 / (4π²f²C_min)

Putting the values of C_min and f, we get:

4π² × (540 × 10³)² × (30 × 10⁻¹²) = 1 / L ⇒ L = 27.84 μH

Therefore, the inductance needed is 27.84 μH.

We can also find the highest frequency to which the circuit can be tuned using the formula:

f_h = 1 / 2π √(L (C_max))

where C_max is the maximum capacitance, which is 365 pF. By plugging in the values of L and C_max, we get:

f_h = 1 / (2π) √(27.84 × 10⁻⁶ × 365 × 10⁻¹²) ≈ 371.6 kHz

Therefore, the highest frequency to which the circuit can be tuned is approximately 371.6 kHz.

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Discrete Fourier Transform (DFT) can be expressed by the following formula ; W4 WA = W4 + jW4₂ = (1/2)[W4 + (jW4₂)] + (1/2)[W4 - (jW4₂)]

Where, W4 = e^-j2π/4W4₂ = e^-j2π/4 * 2 = e^-jπ/2= -j .

Now, we find the element (0, 2) of the 4-point matrix W4 by using the OFT of the 4-point sequence oc[n].  

That is ; x[k] = 28[X-a₂]+8[X-b₂] 0≤k≤3OFT (Discrete Fourier Transform) is given by ; X[n] = ∑_(k=0)^{N-1}▒〖x[k]e^((-j2πkn)/N) 〗where, N is the number of samples in the sequence x[k].N = 4x[0] = 28, x[1] = x[2] = x[3] = 8 .

Therefore x[k] = 28[X-a₂]+8[X-b₂]⇒x[0] = 28[X-2]+8[X-1] . Putting k=0;x[0] = X[0]*1 + X[1]*1 + X[2]*1 + X[3]*1 = 28 Simplifying and solving for X[2];X[2] = (x[0] + x[2]) - (x[1] + x[3])= (28 + 8) - (8 + 8)= 20 .

Here, we find W4 and W4' when k=0,W4 = e^-j2π/4 = e^-jπ/2 = -jW4' = e^j2π/4 = e^jπ/2 = j .

The 6 properties of DFT matrix are :

1. Linearity : If x[n] and y[n] are two sequences then ; DFT(ax[n] + by[n]) = aDFT(x[n]) + bDFT(y[n])  where, a and b are constants.

2. Shifting: If x[n] is a sequence then ; DFT(x[n-k]) = e^(-j2πnk/N) X[k] where, k is an integer.

3. Circular shifting: If x[n] is a sequence then ; DFT(x[n-k]_N) = e^(-j2πnk/N) X[k] where, k is an integer.

4. Time reversal : If x[n] is a sequence then ; DFT(x[N-n-1]) = X[N-k]

5. Conjugate symmetry: If x[n] is a real sequence then;X[N-k] = X[k]*

6. Periodicity : If x[n] is a periodic sequence then X[k] is also periodic.

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