a) The pressure drop per 100 m of pipe is 5.07 kPa.
Pressure drop:
Pressure drop is given by the formula: ΔP = f * (L/d) * (ρ * v^2 / 2)
Where, f = friction factor, ρ = density of oil.
ρ = 1 kg/m^3 (density of oil)
We know that
Reynold's number, Re = (ρ * v * d) / μRe = (1 * 0.85 * 5) / 0.0814 = 41.5
Friction factor can be found using the Moody chart.
The values of friction factor and Reynold's number are plotted on the chart and the intersection of the two is obtained. From the intersection, we get the friction factor.
f = 0.0157 (approx.)
Putting the values in the formula,
ΔP = f * (L/d) * (ρ * v^2 / 2)ΔP
= 0.0157 * (100/5) * (1 * 0.85^2 / 2)ΔP
= 5.07 kPa
Thus, pressure drop per 100 m of pipe = 5.07 kPa
b) The power lost in kilowatts to friction is 0.0575 kW.
Power lost to friction:
Power lost to friction is given by the formula: P = ΔP * Q
Where, ΔP = Pressure drop, Q = Volume flow rate of oil
Volume flow rate can be calculated using the formula: Q = A * v
Where, A = area of the pipe
Q = π/4 * d^2 * vQ
= π/4 * 5^2 * 0.85Q
= 11.33 * 10^-3 m^3/s
Putting the values of ΔP and Q in the formula, we get,
P = ΔP * QP
= 5.07 * 11.33 * 10^-3P
= 57.52 * 10^-3 kJ/s
Power lost in kilowatts to friction = 57.52 * 10^-3 kW
= 0.0575 kW.
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A steady current of 590μA flows through the plane electrode separated by a distance of 0.55 cm when a voltage of 15.5kV is applied. Determine the first Townsend coefficient if a current of 60μA flows when the distance of separation is reduced to 0.15 cm and the field is kept constant at the previous value.
The first Townsend coefficient is approximately 0.3722.
Ionization energy refers to the amount of energy that's required to remove an electron from an atom that's isolated.
To determine the first Townsend coefficient, we can use the Townsend's ionization equation:
α = (I2 / I1) * (d1 / d2)
where:
α is the first Townsend coefficient
I1 is the initial current (590 μA)
I2 is the final current (60 μA)
d1 is the initial separation distance (0.55 cm)
d2 is the final separation distance (0.15 cm)
Plugging in the given values:
α = (60 μA / 590 μA) * (0.55 cm / 0.15 cm)
≈ 0.1017 * 3.6667
≈ 0.3722
Therefore, the first Townsend coefficient is approximately 0.3722.
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A 60Co source is labeled 4.35 mCi, but its present activity is found to be 2.0x107 Bq. (a) What is the present activity in mCi? mCi. (b) How long ago in years did it actually have a 4.00-mCi activity? years.
(a) The present activity of the 60Co source is approximately 0.054 mCi.
(b) The 60Co source had a 4.00-mCi activity approximately 39.20 years ago.
(a) To convert the present activity from becquerels (Bq) to millicuries (mCi), we'll use the conversion factor:
1 mCi = 3.7 × 10[tex]^10[/tex] Bq
Present activity in mCi = (2.0 × 10[tex]^7[/tex] Bq) / (3.7 × 10[tex]^10[/tex]Bq/mCi)
Present activity in mCi ≈ 0.054 mCi
Therefore, the present activity of the 60Co source is approximately 0.054 mCi.
(b) To calculate the time elapsed in years, we can use the concept of half-life. The half-life of 60Co is approximately 5.27 years.
We can use the formula:
t = (ln(N₀/N))/(λ)
where:
t = time elapsed
N₀ = initial activity (4.00 mCi)
N = present activity (0.054 mCi)
λ = decay constant (ln(2)/half-life)
Substituting the values:
t = (ln(4.00/0.054))/(ln(2)/5.27)
t ≈ 39.20 years
Therefore, the 60Co source had a 4.00-mCi activity approximately 39.20 years ago.
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1. The specific heat of ice is a = 2.09 * 10 ^ 3 * l / k * gl The specific heat of water is c_{w} = 4.19 * 10 ^ 3 * l / k * gl and its heat of fusion L_{f} = 3.33 * 10 ^ 3 1/kg The melting point of water is T_{m} = 273K Consider a 0.118 kg block of ice at 263 K. It is placed in a 0.815 kg bath of water initially at 288 K and perfectly isolated.
(a)How much heat is required to raise the temperature of the ice from 261 K to its melting point?
(b) If this heat is taken from the bath of water what will the new water temperature be?
(c) How much heat is required to melt the ice with its temperature at its melting point?
(d) If the heat required to melt the ice is again taken from the bath of water what will the new water temperature be?
(e)What is the final temperature of the combined water at thermal equilibrium?
(a) The heat required to raise the temperature of the ice from 261 K to its melting point is 1.97 kJ.
(b) If this heat is taken from the bath of water, the new water temperature will be 287.82 K.
(c) The heat required to melt the ice with its temperature at its melting point is 391.94 kJ.
(d) If the heat required to melt the ice is taken from the bath of water, the new water temperature will be 277.41 K.
(e) The final temperature of the combined water at thermal equilibrium is 277.41 K.
(a) To calculate the heat required to raise the temperature of the ice, we use the formula Q = mcΔT, where Q is the heat, m is the mass, c is the specific heat, and ΔT is the temperature change. Plugging in the values, we get Q = (0.118 kg) * (2.09 * 10^3 J/kg·K) * (273 K - 261 K) = 1.97 kJ.
(b) Since the heat taken from the bath of water is equal to the heat gained by the ice, we can use the formula Q = mcΔT to find the new water temperature. Rearranging the formula, we have ΔT = Q / (mc), and plugging in the values, we get ΔT = (1.97 kJ) / (0.815 kg * 4.19 * 10^3 J/kg·K) ≈ 0.64 K. Subtracting this temperature change from the initial temperature of the water, we get the new water temperature of 288 K - 0.64 K ≈ 287.82 K.
(c) The heat required to melt the ice at its melting point is given by Q = mLf, where Q is the heat, m is the mass, and Lf is the heat of fusion. Plugging in the values, we get Q = (0.118 kg) * (3.33 * 10^3 J/kg) = 391.94 kJ.
(d) Using the same principle as in (b), we can find the new water temperature by using the formula ΔT = Q / (mc). Plugging in the values, we get ΔT = (391.94 kJ) / (0.815 kg * 4.19 * 10^3 J/kg·K) ≈ 0.12 K. Subtracting this temperature change from the initial temperature of the water, we get the new water temperature of 288 K - 0.12 K ≈ 287.88 K.
(e) At thermal equilibrium, the final temperature of the combined water will be the same. Therefore, the final temperature of the combined water is 287.88 K.
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There is a 50-km, 220-5V, 60-Hz, three-phase overhead transmission line. The line has a per-phase resistance of 0.152/km, a per-phase inductance of 1.3263 mH/km. Shunt capacitance is neglected. Use the appropriate line model. The line is supplying a three-phase load of 381 MVA at 0.8 power factor lagging and at 220 kV. Find the series impedance per phase.
The series impedance per phase of the given transmission line is approximately 7,600 Ω (resistance) + j66.315 Ω (reactance).
The series impedance per phase of the given transmission line, we can calculate the total impedance using the per-phase resistance and inductance.
The total impedance (Z) per phase of the transmission line can be calculated using the following formula:
Z = R + jX
where R is the resistance and X is the reactance.
Length of the line (L) = 50 km
Resistance per phase (R) = 0.152 Ω/km
Inductance per phase (L) = 1.3263 mH/km
First, we need to convert the length and inductance units to consistent units:
Length in meters (L) = 50 km × 1000 m/km = 50,000 m
Inductance in ohms (X) = (1.3263 mH/km) × (50,000 m/km) × (1 H/1000 mH) = 66.315 Ω
Therefore, the series impedance per phase can be calculated as:
Z = 0.152 Ω/km × 50,000 m + j(66.315 Ω)
Z = 7,600 Ω + j(66.315 Ω)
Hence, the series impedance per phase of the transmission line is 7,600 Ω + j(66.315 Ω).
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"
48 In Fig. 5-35, three blocks are pulled to the right on a horizontal frictionless table by a force of magnitude T3 = 95.0 N. If m₁ = 10.0 kg, m₂ = 14.0 kg, and m3 = 23.0 kg, calculate (a) the mag
"
In the given problem, three blocks are pulled towards the right on a frictionless horizontal table with a force of magnitude T3 = 95 N. The tension T1 in the string between m₁ and m₂ is 9.9 N, and the tension T2 in the string between m₂ and m₃ is 8.8 N.
The masses of the three blocks are m₁ = 10 kg, m₂ = 14 kg, and m₃ = 23 kg. We need to find (a) the magnitude of the acceleration of the system, (b) the tension T1 in the string between m₁ and m₂, and (c) the tension T2 in the string between m₂ and m₃. We can apply Newton's second law of motion to find the acceleration of the system.
Substituting T3 = 95 N,
m₁ = 10 kg,
m₂ = 14 kg,
and m₃ = 23 kg in equations (1), (2), and (3):
T1 - 95 = 10aa
= (T1 - 95) / 10 ...(4)T2 - T1
= 14aT2 - T1 = 14(T1 - 95) / 10T2
= 1.4T1 - 133 ...(5)T3 - T2 = 23a95 - T2 = 23(T1 - 95) / 10Substituting equation (5) in equation (3):
95 - 23(T1 - 95) / 10 = 23(T1 - 95) / 10239.5 = 4.6T1T1 = 53.4 N ...(6)
Substituting equation (6) in equation (5):T2 = 1.4 × 53.4 - 133T2 = 8.80 N ...(7)
Substituting equation (4) in equations (1), (2), and (3):
a = (53.4 - 95) / 10a = -4.66 m/s²
T1 - 95 = 10 × (-4.66)T1 = 9.9 NT2 - T1 = 14 × (-4.66)T2 = 8.8 N
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Using filters, a photographer has created a beam of light consisting of three wavelengths: 400 nm (violet), 500 nm (green), and 650 nm (red). He aims the beam so that it passes through air and then enters a block of crown glass. The beam enters the glass at an incidence angle of θ1 = 26.6°.
The glass block has the following indices of refraction for the respective wavelengths in the light beam.
wavelength (nm) 400 500 650
index of refraction
n400 nm = 1.53
n500 nm = 1.52
n650 nm = 1.51
(a) Upon entering the glass, are all three wavelengths refracted equally, or is one bent more than the others?
400 nm light is bent the most
500 nm light is bent the most
650 nm light is bent the most
all colors are refracted alike
(b)What are the respective angles of refraction (in degrees) for the three wavelengths? (Enter each value to at least two decimal places.)
(i) θ400 nm
?°
(ii)θ500 nm
?°
(iii)θ650 nm
?°
400 nm light is bent the most. Upon entering the glass, all three wavelengths are not refracted equally.the violet light than for the green or red light. The angle of refraction decreases with increasing wavelength, and the 650 nm light bends the least, while the 400 nm light bends the most.
This indicates that the velocity of the light decreases more when passing from air to glass for violet light than for green or red light. Since the velocity of the light is less in glass than in air, the light is refracted or bent towards the normal to the boundary surface.
(b) The angle of incidence is θ1 = 26.6° and the indices of refraction are as follows;n400 nm = 1.53n500 nm = 1.52n650 nm = 1.51The angle of refraction for each color can be determined using Snell's law;n1sinθ1 = n2sinθ2(i) θ400 nm= 16.36°(ii) θ500 nm= 16.05°(iii) θ650 nm= 15.72°
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A later observation of the object from question 2 was made and it was discovered that the dark lines are shifted by 15 nm to longer wavelengths than expected.
a) What does the shift in the wavelength tell us about the motion of the object?
b) A second star is observed to have its lines shifted by 20 nm to shorter wavelengths. Which of these two stars is moving the fastest?
A) The shift in the wavelength towards longer wavelengths indicates that the object observed in question 2 is moving away from the observer.
This phenomenon is known as redshift. When an object moves away from an observer, the wavelengths of light emitted by the object appear stretched or shifted towards longer wavelengths. This shift can be explained by the Doppler effect, which occurs due to the relative motion between the source of light (the object) and the observer.
B) The second star, which has its lines shifted by 20 nm to shorter wavelengths, is moving faster compared to the object in question 2. This shift towards shorter wavelengths is known as blueshift.
When an object moves towards an observer, the wavelengths of light emitted by the object appear compressed or shifted towards shorter wavelengths. Similar to the redshift, this blueshift is also explained by the Doppler effect. The greater the blueshift, the faster the object is moving towards the observer. Therefore, the second star, with a blueshift of 20 nm, is moving faster than the object in question 2, which had a redshift of 15 nm.
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The following impedances are connected in series across a 50V, 18 kHz supply:
i. A 12 Ω resistor,
ii. A coil with a resistance of 2Ω and inductance of 150 µH.
a. Draw the circuit diagram,
b. Draw the phasor diagram and calculate the current flowing through the circuit,
c. Calculate the phase angle between the supply voltage and the current,
d. Calculate the voltage drop across the resistor,
e. Draw the phasor diagram and calculate the voltage drop across the coil and its phase angle with respect to the current.
Voltage in rectangular form = -6.6 + 40.1j
b. Phasor diagram and current calculation:
At first, we need to find out the reactance of the coil,
Xᵣ.L= 150 µH
= 150 × 10⁻⁶Hf
=18 kHzω
=2πfXᵣ
= ωL
= 2 × 3.14 × 18 × 10³ × 150 × 10⁻⁶Ω
=16.9Ω
Applying Ohm's law in the circuit,
I = V/ZᵀZᵀ
= R + jXᵣZᵀ
= 12 + j16.9 |Zᵀ|
= √(12² + 16.9²)
= 20.8Ωθ
= tan⁻¹(16.9/12)
= 53.13⁰
I = 50/20.8 ∠ -53.13
= 2.4 ∠ -53.13A (Current in polar form).
Current in rectangular form = I ∠ θI
= 2.4(cos(-53.13) + jsin(-53.13))
=1.2-j1.9
c. Phase angle,θ = tan⁻¹((Reactance)/(Resistance))
θ = tan⁻¹((16.9)/(12))
θ = 53.13⁰
d. Voltage drop across resistor= IR
= (2.4)(12)
= 28.8 V
e. Phasor diagram and voltage across the coil calculation:
Applying Ohm's law,
V = IZᵢZᵢ
= R + jXᵢZᵢ
= 2 + j16.9 |Zᵢ|
= √(2² + 16.9²)
= 17Ω
θ = tan⁻¹(16.9/2)
= 83.35⁰
Vᵢ = IZᵢ
Vᵢ = 2.4(17)
= 40.8 V (Voltage in polar form)
Voltage in rectangular form = V ∠ θV
= 40.8(cos(83.35) + jsin(83.35))
= -6.6 + 40.1j
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Calculate the integral (v) = ſº vƒ(v)dv. The function f(v) describing the actual distribution of molecular speeds is called the Maxwell-Boltzmann 3/2 m distribution, ƒ(v) = 4π(. -) ³/² √²e-mv² /2kT . (Hint: Make the change of variable v² = x and use the tabulated integral ax 5.00 xne dx where n is a positive integer and a is a positive constant.) = (v) n an+1 Express your answer in terms of the variables T, m, and appropriate constants. 2πkT IVE ΑΣΦ ?
The solution is as follows:Given function is [tex]f(v) = 4π(. -) ³/² √²e-mv² /2kT[/tex]
Let x = v²
⇒[tex]v = √xdx/dv[/tex]
= 2v
Integrating by substitution[tex]ſº vƒ(v)dv,[/tex]
we get[tex]ƒ(x)dx/dv = 2vƒ(x) = 2π (. -) ³/² √²e-mx /2kT[/tex]
We know that[tex]∫x⁵eⁿᵉᵈx = (x⁶/6) eⁿᵉ + C[/tex] …(1)
Using the above equation (1), we can write the integral in the question as
[tex]∫ƒ(x)dx = ∫2π (. -) ³/² √²e-mx /2kT 2v dv[/tex]
= [tex]2π (. -) ³/² √²/2kT ∫eⁿᵉ /2kT x⁵/2 e⁻ᵐˣ ᵈx[/tex]
= [tex]2π (. -) ³/² √²/2kT n!(2m/kT)³/² [∫x⁵/2 e⁻ᵐˣ ᵈx][/tex]
= [tex]π (. -) ³/² √²n (2m/kT)³/² ∫x⁵/2 e⁻ᵐˣ ᵈx...[/tex]
∵ n is a positive integer.So, the given integral is[tex]π (. -) ³/² √²n (2m/kT)³/² ∫x⁵/2 e⁻ᵐˣ ᵈx[/tex]
= π[tex](. -) ³/² √²n (2m/kT)³/² (2√π/3) (kT/m)³/²[/tex]
= [tex]4π [(. -) (m/2πkT)]³/² (kT/m)²[/tex]
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Explain why the deformation of the water well screen in the photograph occurs.
The deformation of the water well screen in the photograph occurs due to several reasons such as the stress caused by water pressure is considered a primary factor, the quality of the well screen and its installation determine its durability, and environmental factors like soil composition,
Water flows into the well with a specific pressure that exerts stress on the well's screen, and the rate of water flow is directly proportional to the water pressure. The well screen is usually designed to withstand such pressure and last for a long time. If the well screen is poorly constructed or installed, it is more likely to deform due to various factors, including water pressure. Moreover, some well screens may be of poor quality or made from low-quality materials, making them susceptible to deformation.
Environmental factors like soil composition, temperature, and the acidity of water may cause the well screen to deform over time. Soil composition plays a significant role in the durability of the well screen because it can corrode or erode it. Water with a high acidity level can also corrode the well screen, leading to its deformation. In conclusion, several factors, such as water pressure, installation quality, and environmental factors, contribute to the deformation of the water well screen.
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0.IKB/Sill 3:40 PM (f) •76% Homework of Chapter 6 9. Single Choice As every amusement park fan knows, a Ferris. wheel is a ride consisting of seats mounted on a tall ring that rotates around a horizontal axis. When you ride in a Ferris wheel at constant speed, what are the directions of a FN your acceleration and the normal force on you (from the always upright seat) as you pass through (1) the highest point and (2) the lowest point of the ride? (3) How does the magnitude of the acceleration at the highest point compare with that at the lowest point? (4) How do the magnitudes of the normal force compare at those two points? A , (1) a downward, FN downward; (2) a and FN upward; (3) same; (4) greater at lowest point; , (1) a downward, FN upward; (2) a and FN upward; (3) same; (4) greater at lowest point; , (1) a downward, FN upward; (2) a and FN upward; (3) greater at lowest point; (4) तं
The highest point is a downward and the lowest point of the ride is FN upward, The magnitude of the acceleration at the highest point compare with that at the lowest point is the same, The magnitudes of the normal force compare at those two points is greater at the lowest point. The correct answer is option(a).
When the Ferris wheel is at the highest point, the direction of the normal force is down towards the center of the wheel and the direction of acceleration is down or towards the ground. The net force at this point is equal to the force of gravity acting downwards. So, the normal force is lesser than the weight of the person riding on the Ferris wheel.
On the other hand, when the Ferris wheel is at its lowest point, the direction of the normal force is upwards, and the direction of acceleration is also upwards. The net force at this point is equal to the weight of the person plus the force of gravity. Hence, the normal force is greater than the weight of the person.
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Finding the work done in stretching or compressing a spring.
Hooke's Law for Springs.
According to Hooke's law the force required to compress or stretch a spring from an equilibrium position is given by F(x)=k, for some constant & The value of (measured in force units per unit length) depends on the physical characteristics of the spring. The constant & is called the spring constant and is always positive
Part 1.
Suppose that it takes a force of 20 N to compress a spring 0.8 m from the equilibrium
The force function, F(x), for the spring described is:
F(x) = 16.67x, where x is the displacement from the equilibrium position and F(x) is the force required to compress or stretch the spring.
To find the force function, F(x), for the spring described, we can use the given information and Hooke's law equation, F(x) = kx.
Given:
Force required to compress the spring = 20 N
Compression of the spring = 1.2 m
We can plug these values into the equation and solve for the spring constant, k.
20 N = k * 1.2 m
Dividing both sides of the equation by 1.2 m:
k = 20 N / 1.2 m
k = 16.67 N/m (rounded to two decimal places)
Therefore, the force function, F(x), for the spring described is:
F(x) = 16.67x, where x is the displacement from the equilibrium position and F(x) is the force required to compress or stretch the spring.
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The complete question is :-
According to Hooke's law, the force required to compress or stretch a spring from an equilibrium position is given by F(x)=kx, for some constant k. The value of k (measured in force units per unit length) depends on the physical characteristics of the spring. The constant k is called the spring constant and is always positive.
Part 1. Suppose that it takes a force of 20 N to compress a spring 1.2 m from the equilibrium position. Find the force function, Fx, for the spring described.
1. How can you determine the terminal velocity at hindered gravitational settling in the zone settling regime of a solid particle in the fluid phase? What is hindered settling and the opposite of that? What can you say about the drag coefficient in these cases?
Terminal velocity at hindered gravitational settling in the zone settling regime of a solid particle in the fluid phase can be determined as follows: For hindered settling, there is an extensive inter-particle interaction that hinders the settling velocity of solid particles in fluid.
Hindered settling occurs at relatively high solids loading conditions. The hindered settling is the opposite of the ideal settling, which occurs under low solids loading conditions. Hindered settling can be further broken down into three categories, depending on the extent of hinderance they experience. The categories are "Z" factor, "F" factor, and "Q" factor.
For all three categories, the particles' settling speed decreases as the solids loading increases.For a particle that is settling through a fluid, the drag coefficient refers to the resistance it encounters from the fluid. The fluid's properties, such as its viscosity, density, and velocity, all have an impact on the drag coefficient. The drag coefficient is larger in cases where the particle is large and the fluid is viscous.
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A gas mixture (treated as ideal) is contained in a sealed flask at atmospheric pressure. After all the carbon dioxide is chemically removed from the sample at constant temperature, the final pressure is 67.89 kPa. Calculate what percentage of the molecules of the original sample was carbon dioxide.
The percentage of carbon dioxide molecules in the original gas mixture is approximately 13.3%.
When the carbon dioxide is chemically removed from the gas sample, the remaining gas molecules will contribute to the final pressure. Since the temperature is constant and the gas is treated as ideal, the final pressure is directly proportional to the number of moles of gas present.
In this case, the final pressure is given as 67.89 kPa. Let's assume that the original gas mixture contained a total of n moles of gas, with x moles of carbon dioxide. After the carbon dioxide is removed, the remaining gas molecules contribute to the final pressure, which means that the pressure is proportional to the number of moles of the remaining gas.
Therefore, we can set up a proportion:
(n - x) / n = 67.89 kPa / atmospheric pressure
Solving for x (moles of carbon dioxide) gives:
x = n - (67.89 kPa / atmospheric pressure) * n
To calculate the percentage of carbon dioxide molecules, we divide x by n and multiply by 100:
Percentage of carbon dioxide molecules = (x / n) * 100
Substituting the expression for x from the previous equation, we have:
Percentage of carbon dioxide molecules = [n - (67.89 kPa / atmospheric pressure) * n] / n * 100
Simplifying the equation further, we get:
Percentage of carbon dioxide molecules = (1 - 67.89 kPa / atmospheric pressure) * 100
Substituting the given values, assuming atmospheric pressure is 101.325 kPa:
Percentage of carbon dioxide molecules = (1 - 67.89 kPa / 101.325 kPa) * 100 = 13.3%
Therefore, approximately 13.3% of the molecules in the original gas sample were carbon dioxide.
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A telecommunications line is modelled as a series RLC circuit with R = 1 Ohm/km. = 1 H/km and C= 1 F/km. The input is a 1V sinusoid at 1kHz. The output is the voltage across the capacitor. At what distance (to the nearest km) will the system have lost half its power. A telecommunications line is modelled as a series RLC circuit with R = 1 Ohm/km, L = 1 H/km and C = 1 F/km. The input is a 1V sinusoid of varying frequency. The output is the voltage across the capacitor and the line is of 100km length. At what frequency (to the nearest Hz) will the system have lost half its power.
Part 1:Power loss occurs due to resistance. The distance at which the system loses half of its power can be determined as follows: Let the distance be x km. The power loss will be P/2, where P is the power transmitted.
The RLC circuit is a low pass filter with the cut off frequency given by:f = 1/2π√LCHere,
L = 1 H/km,
C = 1 F/km and
f = 1 kHz
∴ 1 kHz = 1000 Hz
f = 1/2π√LC
= 1/2π√(1 × 10³ × 1 × 10⁻⁹)
= 1/2π × 1 × 10⁻³
= 159.15 Hz
P/2 = P(x)/100, where P(x) is the power transmitted at a distance of x km.
P = V²/R, we have
P/2 = (V²/R) (x)/100
Solving for x, we get x = 69.3 km (approx.)
The system will have lost half its power at a distance of 69 km (approx.).
Part 2: Using the same formula for cut-off frequency as in Part 1, we get f = 1/2π√LC = 1/2π√(1 × 10³ × 1 × 10⁻⁹) = 159.15 Hz The system will have lost half its power at a frequency of 159 Hz (approx.).
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Using the component method, calculate the resultant (sum) of the following two vectors.
v
1
=175 m/s,70
∘
polar (positive)
v
4
=200 m/s,200
∘
polar (positive)
Calculate the components for r
v
1
Using the component method, calculate the resultant (sum) of the following two vectors.
v
1
=175 m/s,70
∘
polar (positive)
v
2
=200 m/s,200
∘
polar (positive)
Calculate the components for
v
2
Using the component method, calculate the resultant (sum) of the following two vectors.
v
1
=175 m/s,70
∘
polar (positive)
v
2
=200 m/s,200
∘
polar (positive)
Add the components of the resultant vector Using the component method, calculate the resultant (sum) of the following two vectors.
v
1
=175 m/s,70
∘
polar (positive)
v
2
=200 m/s,200
∘
polar (positive)
Calculate the resultant magnitude using the Pythagorean theorem. Using the component method, calculate the resultant (sum) of the following two vectors.
v
1
=175 m/s,70
∘
polar (positive)
v
2
=200 m/s,200
∘
polar (positive) Calculate the resultant direction using the tangent function. Express the direction in terms of the polar (positive) specification.
The components of v1 are 165.3 m. Component of v2 -68.3 m. The components of the resultant vector r are 97.0m. The resultant vector is 111.2 m/s at an angle of 59.9 degrees below the positive direction of the polar axis.
Components of v1:
Since v1 is 175 m/s at 70 degrees in the positive direction of the polar axis, its components in the x and y directions are:
x component: v1x=175
cos 70° = 56.5
my component:
v1y=175 sin 70° = 165.3 m
Component of v2:
Since v2 is 200 m/s at 200 degrees in the positive direction of the polar axis, its components in the x and y directions are:
x component: v2x=200
cos 200° = -112.7
my component:
v2y=200 sin 200° = -68.3 m
Addition of v1 and v2:
The components of the resultant vector r are:
rx=v1x+v2x=56.5−112.7
=-56.2mry
=v1y+v2y
=165.3−68.3
=97.0m
Magnitude of resultant vector:
The magnitude of the resultant vector r is:
|r| = √(rx² + ry²)=√((-56.2)² + 97.0²)=111.2m
The direction of the resultant vector:
The direction of the resultant vector r is given by:
tan θ = ry / rx= -97.0 / 56.2=-1.727θ = tan-1(-1.727) = -59.9°
Therefore, the resultant vector is 111.2 m/s at an angle of 59.9 degrees below the positive direction of the polar axis.
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A singly charged positive ion moving at 4.60 x 105 m/s leaves a circular track of radius 7.94 mm along a direction perpendicular to the 1.80 T magnetic field of a bubble chamber. Compute the mass (in atomic mass units) of this ion, and, from that value, identify it. .
2
4
He
+
1
1
H
+
3
2
He
+
1
2
H
+
We identify the particle whose mass is 182.70 amu to be 4He²⁺. We have to compute the mass (in atomic mass units) of the ion. We shall use the following formula to solve the problem: mv²r = q B
We are given the following data: Speed of the singly charged positive ion = v = 4.60 x 10⁵ m/s, Radius of the circular track along which the ion travels = r = 7.94 mm = 7.94 x 10⁻³ m, Magnetic field = B = 1.80 T
We have to compute the mass (in atomic mass units) of the ion. We shall use the following formula to solve the problem: mv²r=qB
From the given data, we know the value of qBmv²r=qBmv²r
= qB
Because the particle is positively charged, we have q = +1.6 x 10⁻¹⁹ C
Substituting the values, we get
m(4.60 x 10⁵)2(7.94 x 10⁻³)= (1.6 x 10⁻¹⁹)(1.80)m = (1.6 x 10-19)(1.80)(7.94 x 10⁻³)(4.60 x 10⁵)2m
= 3.038 x 10⁻²² kg
We can now compute the mass of the ion in atomic mass units.1 atomic mass unit (amu) = 1.661 x 10⁻²⁷ kg
Therefore, the mass of the ion is: m = (3.038 x 10⁻²²)/(1.661 x 10⁻²⁷)
= 182.70 amu
We identify the particle whose mass is 182.70 amu to be 4He²⁺.
Hence, the answer is: 4He²⁺.
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The length of a day increases by 1 ms per century. Find the angular acceleration of the Earth in rad/s
1. The angular acceleration of the Earth is approximately 1.745 × 10⁽⁻⁷⁾ rad/s².
The angular acceleration of the Earth, we can use the relationship between the change in time (Δt) and the change in angular displacement (Δθ).
Change in time, Δt = 1 ms per century = 1 × 10⁽⁻³⁾ s / 100 years
360 degrees = 2π radians
The angular acceleration (α) is defined as the rate of change of angular velocity (ω) over time (t):
α = Δω / Δt
We know that angular velocity is the change in angular displacement (θ) over time (t):
ω = Δθ / Δt
Rearranging the equation, we get:
Δθ = ω * Δt
Substituting the values, we have:
Δθ = (1 × 10⁽⁻³⁾) s / 100 years) * (2π radians / 360 degrees)
Calculating the value, we find:
Δθ ≈ 1.745 × 10⁽⁻⁹⁾ radians
Now, we can calculate the angular acceleration using the equation:
α = Δθ / Δt
Substituting the values:
α = (1.745 × 10⁽⁻⁹⁾ radians) / (1 × 10⁽⁻³⁾ s / 100 years)
Simplifying the equation, we have:
α ≈ 1.745 × 10⁽⁻⁷⁾ radians per second squared
Therefore, the angular acceleration of the Earth is approximately 1.745 × 10⁽⁻⁷⁾ rad/s².
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Q1. A lawn sprinkler sprays water from an array of 12 holes, each 0.40 cm in diameter. The sprinkler is fed by a garden hose 3.5 cm in diameter, which is supplied by a tap. a) If the tap can supply 15 litres of water every minute, calculate the speed at which water moves through the garden hose. (4) b) Calculate the velocity with which the water leaves one hole in the sprinkler array. (4)
(a) The speed at which water moves through the garden hose is 25.97 cm/s. (b) The velocity with which the water leaves one hole in the sprinkler array is 2.57 m/s.
a) To calculate the speed at which water moves through the garden hose, we'll use the formula for the volume rate of flow, which is given by
Q = A×v, where A is the cross-sectional area of the hose and v is the velocity of the water. We have the diameter of the hose, which we'll use to find its radius.
r = d/2 = 3.5/2 = 1.75 cmA = πr² = π(1.75)² = 9.625 cm²
To convert the flow rate from L/min to cm³/s, we'll multiply by 1000/60, because 1 L = 1000 cm³ and 1 min = 60 s.Q = 15 × 1000/60 = 250 cm³/s
Q = A × v ⇒ v = Q/A
= 250/9.625
= 25.97 cm/s
(b)The velocity with which the water leaves one hole in the sprinkler array can be found using Bernoulli's equation, which relates the pressure of the fluid to its velocity.
p1 + (1/2)ρv1² = p2 + (1/2)ρv2²
where p1 and v1 are the pressure and velocity of the water as it enters the sprinkler array, and p2 and v2 are the pressure and velocity of the water as it leaves the hole in the sprinkler.
We'll assume that the pressure remains constant throughout, so p1 = p2. Let's start by finding the velocity of the water as it enters the sprinkler array. Since the cross-sectional area of the hose is much larger than the combined areas of the holes in the sprinkler array, we can assume that the velocity of the water remains constant as it passes through the array. We'll use the equation of continuity to relate the velocity of the water in the hose to the velocity of the water in the sprinkler. A1v1 = A2v2
where A1 and v1 are the cross-sectional area and velocity of the hose, and A2 and v2 are the cross-sectional area and velocity of the water as it passes through one hole in the sprinkler.
We have already found
A1 and v1.v2 = A1v1/A2 = (9.625 × 25.97)/(12 × (0.4/2)² × π) = 2.57 m/s
The velocity of the water as it leaves the hole in the sprinkler is 2.57 m/s.
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A thin hoop of negligible width is rolling on a horizontal surface at speed v=3.6 m/s when it reaches a 17
∘
incline. How far up the incline will it go? Express your answer using three significant figures and include the ap, Part B How long will it be on the incline before it arrives back at the bottom? Express your answer using three significant figures and include the apprc
1). The hoop will go up the incline approximately 0.656 m when rolling with a speed of 3.6 m/s. 2). It will take approximately 0.322 s for the hoop to arrive back at the bottom of the incline.
To determine how far up the incline the hoop will go, we can analyze the energy conservation in the system. When the hoop reaches the incline, its initial kinetic energy is converted into potential energy as it moves up the incline. The total mechanical energy of the system is conserved, neglecting any energy losses due to friction.
Initial speed, v = 3.6 m/s
Incline angle, θ = 17°
The height the hoop will reach on the incline, we need to equate the initial kinetic energy to the potential energy at the highest point:
1/2 * I * ω² = m * g * h
The moment of inertia (I) for a thin hoop of mass m and radius r is I = m * r².
The linear velocity v of the hoop is related to the angular velocity ω by v = r * ω.
Plugging these values into the equation, we have:
1/2 * m * r² * (v / r)² = m * g * h
Simplifying the equation, we get:
1/2 * v² = g * h
Solving for h, we have:
h = (1/2 * v²) / g
Substituting the given values:
h = (1/2 * 3.6²) / g
The acceleration due to gravity, g, is approximately 9.8 m/s².
h = (1/2 * 3.6²) / 9.8
Calculating the value, we find:
h ≈ 0.656 m (rounded to three significant figures)
Therefore, the hoop will go up the incline approximately 0.656 m.
Now, let's move on to Part B, which asks for the time it takes for the hoop to arrive back at the bottom of the incline.
We can find the time using the kinematic equation:
s = ut + (1/2)at²
where:
s = displacement (height of the incline)
u = initial velocity (0 since the hoop starts from rest at the top)
a = acceleration (due to gravity, -9.8 m/s²)
t = time
Rearranging the equation, we have:
t = [tex]\sqrt{(2s)/a}[/tex]
Substituting the known values:
t = sqrt([tex]\sqrt{(2 * 0.656) / 9.8}[/tex])
Calculating the value, we find:
t ≈ 0.322 s (rounded to three significant figures)
Therefore, the hoop will take approximately 0.322 s to arrive back at the bottom of the incline.
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Question 11 The electric field of a plane wave propagating in a nonmagnetic material is given by E=(3y^+4z^)cos(1.0π×108t−1.34πx)(V/m). Find the relative permittivity of the material εr. εr= Your Answer: Answer Question 12 A 3.0MHz frequency plane wave propagates in a medium characterized by εT=3.0. μr=1.5, and σ=5.0( S/m). Calculate α. α= Your Answer: Answer Question 13 A parallel-polarized ( p-wave) plane wave is incident from air onto a dielectric medium with εr=4. At what incident angle θi there will be no reflection? Answer to the 4th digit precision after the decimal place (eg. 1.2345). θi=(rad). Your Answer: Answer Question 14 A plane wave with a frequency of f=1.5MHz and electric field amplitude of 9 (V/m) is normally incident in air onto the plane surface of a semi-infinite conducting material with a relative permittivity εr=7.3, relative permeability μr=1, and conductivity σ=110(5/m). Determine the transmitted power per unit cross sectional area in a 2.2 mm penetration of the conducting medium. Answer to the 4 th digit precision after the decimal place (eg. 1.2345). Your Answer: Answer
Question 11
The electric field of a plane wave propagating in a non-magnetic material is given by the following equation;
E=(3y^+4z^)cos(1.0π×108t−1.34πx)(V/m)
The relative permittivity of the material εr is;
εr=1+(1/3.0)[(3y^+4z^)cos(1.0π×108t−1.34πx)/E0]^2
εr=1+(1/3.0)[(3^2+4^2)cos^2(1.0π×108t−1.34πx)/E0]^2
εr=1+(1/3.0)[25cos^2(1.0π×108t−1.34πx)/E0]^2
εr=1+(1/3.0)(25/81)
εr=1.31
Question 12
The propagation constant, α is given by the following equation;
α=ω√(μrεr(1+jσ/ωεr))
Where;
σ = 5.0 S/m; εr=3.0; μr=1.5; and f = 3.0 MHz
The angular frequency, ω is given by;
ω=2πf = 2 x π x 3.0 x 10^6 rad/s
Substituting the given parameters;
α=2π x 3.0 x 10^6 √(1.5 x 3.0(1+j5.0 x 10^-6 x 3.0)/(3.0))
α=2.502 x 10^5 Np/m
Question 13
The critical angle of incidence, θc is given by the equation;
sinθc=1/εr
sinθc=1/4θ
c=asin(1/4)
= 14.48 degrees
For total internal reflection to occur, the incident angle, θi must be greater than the critical angle of incidence, θc;θi>θcθi>14.48 degrees
Question 14
The power of the transmitted wave through a given depth, z is given by the equation;
P(z)=E2/2ρcT
Where;E = 9 V/m;ρc = μrμo/εrεo = 3 x 10^8 m/s; εo = 8.85 x 10^-12 F/m; z = 2.2 mm
The wave impedance is given by;
η = sqrt(μrμo/εrεo)
= sqrt(1 x 4π x 10^-7/7.3 x 8.85 x 10^-12)
= 226.46 Ω
The transmitted power per unit cross-sectional area in a 2.2 mm penetration of the conducting medium is given by;
P(z)=E2/2ρcT
= (9/2 x 226.46 x 3 x 10^8) x e^(-2σz)P(z)
=6.14 x 10^-9 W/m^2
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A rectangular waveguide has dimensions a = 0.12 cm and b = 0.06 cm
a) Determine the first three TE modes of operation and their cutoff frequencies.
b) Write the expressions for the E, and E, electric field components when you are above the cutoff frequency for 2nd order mode and below the cutoff frequency for the 3rd order mode. Leave the answer in terms of unknown variables.
a) The cutoff frequency is the frequency above which the mode propagates in the waveguide. For a rectangular waveguide, the cutoff frequency is given by the formula
fco = c / 2√(a² + b²),
where c is the speed of light in free space.
Substituting the given values, we get:
fc1 = 3.29 GHz
fc2 = 9.87 GHz
fc3 = 19.83 GHz
The first three TE modes are:
TE101, with fc1 as the cutoff frequency
TE201, with fc2 as the cutoff frequency
TE301, with fc3 as the cutoff frequency
b) The expression for the E field components for the TE201 mode are:
Ez = E0 cos(πy/b) sin(πx/a)
Ey = 0Ex = 0
where E0 is the amplitude of the electric field, and x and y are the dimensions of the waveguide.
For a frequency above the cutoff frequency of the TE201 mode but below the cutoff frequency of the TE301 mode, the waveguide would support only the TE201 mode.
The expression for the E field components in this case would be:
Ez = E0 cos(πy/b) sin(πx/a)
Ey = 0Ex = 0
For a frequency below the cutoff frequency of the TE301 mode, the waveguide would not support any mode of operation.
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Assignment: 1. Determine the internal normal force at section \( A \) if the rod is subjected to the external uniformally distributed loading along its length. 2. Determine the internal normal force o
1. Internal normal force at section A:Let's consider a rod subjected to a uniformly distributed load. We can see that the section will be in the state of the internal force if it is cut from this rod by the plane section at point A.The internal normal force of the rod can be determined by using the free body diagram as shown below:
Let the internal normal force at section A be N, and the external distributed load be w per unit length. Now, consider an infinitesimal section of the rod of length dx at a distance x from point A. The free body diagram of this section can be drawn as:Applying the equation of equilibrium in the vertical direction, we can get:N(x) − N(x+dx) − wdx = 0Since the rod is in a state of static equilibrium, the internal normal force must be constant throughout the length of the rod. Thus, we can write:N − N − wl = 0N = wl
Therefore, the internal normal force at section A is wL.2. Internal normal force of the rod:Let's consider a rod of length L subjected to a uniformly distributed load. We can find the internal normal force of the rod using the free body diagram as shown below:Let the internal normal force at the left end be N1 and that at the right end be N2. Now, consider an infinitesimal section of the rod of length dx at a distance x from the left end.
The free body diagram of this section can be drawn as:Applying the equation of equilibrium in the vertical direction, we can get:N(x) − N(x+dx) − wdx = 0Since the rod is in a state of static equilibrium, the internal normal force must be constant throughout the length of the rod. Thus, we can write:N1 − N2 = ∫₀ᴸwdxN1 − N2 = (wL²)/2Therefore, the internal normal force of the rod is (wL²)/2.
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A lawn sprinkler is made of a 1.0 cm diameter garden hose with one end closed and 25 holes, each with a diameter of 0.050 cm, cut near the closed end if water flows at 2.0 m/s in the hose,find the speed of the water leaving a hole.
Hint:(ch 14, Fundementals of physic 8th edi)
The speed of the water leaving a hole is 318 m/s. Answer: 318 m/s
The problem states that the diameter of the garden hose is 1.0 cm with one end closed and 25 holes, each with a diameter of 0.050 cm, cut near the closed end. Given that water flows at 2.0 m/s in the hose, we need to find the speed of the water leaving a hole.To solve the problem, we need to use the principle of continuity. According to this principle, the mass of fluid that passes a given point per unit time is constant if the fluid is incompressible, i.e., the mass flow rate is constant. Since the density of water is constant, the mass flow rate can be expressed as
ρAv
where ρ is the density of water, A is the area of the hose, and v is the velocity of the water. If we assume that the water is incompressible, the mass flow rate is constant at all points along the hose, so
ρAv = constant
We can use this principle to relate the velocity of the water in the hose to the velocity of the water leaving a hole. Since the mass flow rate is constant, we have
ρAv = ρaυ
where a is the area of one of the holes, andυ is the velocity of the water leaving the hole. We can solve this equation forυ:υ = Av/a
Using the given values, we can calculate the area of the hose and the area of one of the holes:
A_hose = πr²
= π(0.5 cm)²
= 0.785 cm²A_hole
= πr²
= π(0.025 cm)²
= 0.00196 cm²
Now we can substitute these values into the equation forυ:
υ = (0.785 cm²)(2.0 m/s) / (0.00196 cm²)
υ ≈ 318 m/s
Therefore, the speed of the water leaving a hole is 318 m/s. Answer: 318 m/s
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1. If the centrifugal switch fails to open as a split-phase motor accelerates to its rated speed, what happens to the starting winding?
2. Describe one limitation of a capacitor-start, induction-run motor.
1. If the centrifugal switch fails to open as a split-phase motor accelerates to its rated speed, the starting winding will continue to be energized. This results in overheating of the winding and can cause damage to the motor. This is because the starting winding is designed to be used only during the starting process, and not continuously.
If the centrifugal switch fails to open, it means that the starting winding will be in use for too long, causing overheating, which will damage the motor.
2. One limitation of a capacitor-start, induction-run motor is that it has low power factor. This is because the capacitor is designed to be used only during the starting process, and not during the running process. Therefore, during the running process, the motor will have a low power factor, which means that it will consume more energy from the power supply than is actually required. This results in wastage of energy and higher electricity bills. Additionally, the motor may not be suitable for use in applications where high power factor is required, such as in industrial processes that require high efficiency and low energy consumption.
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[20 Points] Four very long straight wires located on the corners of a rectangle of width a=2[ m] and length b=10[ m]. Point A is located at the center of the rectangle, as shown in the figure. - Wire-1 is carrying a current I
1
=3 [A] directed into the page. - Wire-2 is carrying a current I
2
=10 [A] directed into the page. - Wire-3 is carrying a current I
3
=4[ A] directed out of the page. - Wire-4 is carrying a current I
4
=7[ A] directed out of the page. a) [4 Points] Find the magnetic field vector created by wire-1 at point A.
B
1
=∣
i
^
+∣∣
j
^
[T] b) [4 Points] Find the magnetic field vector created by wire-2 at point A.
B
2
=∣
i
^
+∣
j
^
[T] c) [4 Points] Find the magnetic field vector created by wire-3 at point A.
B
3
=∣
i
^
+ d) [4 Points] Find the magnetic field vector created by wire-4 at point A.
B
4
=∣
i
^
+∣
j
^
[T] e) [4 Points] Find the net magnetic field vector created by the 4 wires at point A.
B
net
=
i
^
+
j
^
[T]
Magnetic field vector (B) created by wire-4 at point A is 9.34 × 10^-9 i + 0 j T.(e) Net magnetic field(B net) vector created by the 4 wires at point A is; B net = B1 + B2 + B3 + B4Putting the calculated values, we get; B net = 0 + 4.02 × 10^-9 j + 1.34 × 10^-8 i + (-5.36 × 10^-9) i + 9.34 × 10^-9 i + 0 j T. On simplifying, we get; B net = 1.81 × 10^-8 i + 4.02 × 10^-9 j T. Therefore, the net B created by the 4 wires at point A is 1.81 × 10^-8 i + 4.02 × 10^-9 j T.
Given, The four very long straight wires are located on the corners of a rectangle of width (a)=2[m] and length (b)=10[m]. Point A is located at the center of the rectangle as shown in the figure. Wire-1 is carrying a current I1=3[Ampere(A)] directed into the page. Wire-2 is carrying a current I2=10[A] directed into the page. Wire-3 is carrying a current I3=4[A] directed out of the page. Wire-4 is carrying a current I4=7[A] directed out of the page.(a) Magnetic field vector created by wire-1 at point A is given as; B1=μ0I1/(4πr1) * sin90° From the right-hand rule(RHR), the magnetic field vector is along the positive i direction so it will be written as;B1 = 0 + (μ0I1/(4πr1) * 1) j . Here, r1 is the distance between wire-1 and point A which is (a^2+b^2)^0.5/2.Magnetic field at point A due to wire-1 is given as;B1 = 0 + (μ0I1/(4π(a^2+b^2)^0.5/2)) j. Putting the given values, we get;B1 = 0 + (4π × 10^-7 × 3/(4π(10^2+2^2)^0.5/2)) jB1 = 4.02 x 10^-9 j T.
Therefore, magnetic field vector created by wire-1 at point A is 0 + 4.02 x 10^-9 j T.(b) Magnetic field vector created by wire-2 at point A is given as;B2=μ0I2/(4πr2) * sin90°From the right-hand rule, the magnetic field vector is along the positive i direction so it will be written as; B2 = μ0I2/(4πr2) * (-1) j. Here, r2 is the distance between wire-2 and point A which is (a^2+b^2)^0.5/2. Magnetic field at point A due to wire-2 is given as; B2 = μ0I2/(4π(a^2+b^2)^0.5/2) * (-1) j. Putting the given values, we get;B2 = 4π × 10^-7 × 10/(4π(10^2+2^2)^0.5/2) * (-1) jB2 = -1.34 × 10^-8 j T. Therefore, magnetic field vector created by wire-2 at point A is 1.34 x 10^-8 i + 0 j T.(c) Magnetic field vector created by wire-3 at point A is given as; B3=μ0I3/(4πr3) * sin90° From the RHR, the magnetic field vector is along the negative j direction so it will be written as;B3 = μ0I3/(4πr3) * (-1) i. Here, r3 is the distance between wire-3 and point A which is (a^2+b^2)^0.5/2. Magnetic field at point A due to wire-3 is given as;B3 = μ0I3/(4π(a^2+b^2)^0.5/2) * (-1) i. Putting the given values, we get;B3 = 4π × 10^-7 × 4/(4π(10^2+2^2)^0.5/2) * (-1) iB3 = -5.36 × 10^-9 i T.
Therefore, magnetic field vector created by wire-3 at point A is -5.36 × 10^-9 i + 0 j T.(d) Magnetic field vector created by wire-4 at point A is given as;B4=μ0I4/(4πr4) * sin90° From the RHR, the magnetic field vector is along the positive j direction so it will be written as; B4 = μ0I4/(4πr4) * 1 i. Here, r4 is the distance between wire-4 and point A which is (a^2+b^2)^0.5/2. Magnetic field at point A due to wire-4 is given as;B4 = μ0I4/(4π(a^2+b^2)^0.5/2) * 1 i. Putting the given values, we get; B4 = 4π × 10^-7 × 7/(4π(10^2+2^2)^0.5/2) * 1 iB4 = 9.34 × 10^-9 i T.
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An ideal gas at 23.7°C and a pressure of 1.42×105 Pa occupies a volume of 2.08 m3. Let R = 8.314 J/K mol (a) How many moles of gas are present? Number: __________ mol (b) If the volume is raised to 3.79 m2 and the temperature raised to 37.1°C, what will be the pressure of the gas?
b) the pressure of the gas after the change in volume and temperature will be approximately 1.31 × 105 Pa.
(a) To calculate the number of moles of gas present, we can use the ideal gas law equation:
PV = nRT
Where:
P = Pressure of the gas
V = Volume of the gas
n = Number of moles of the gas
R = Ideal gas constant
T = Temperature of the gas
Given:
Pressure (P) = 1.42 × 105 Pa
Volume (V) = 2.08 m³
Temperature (T) = 23.7°C = 23.7 + 273.15 = 296.85 K (converted to Kelvin)
Ideal gas constant (R) = 8.314 J/K mol
Now, let's solve for the number of moles (n):
n = PV / RT
n = (1.42 × 105 Pa * 2.08 m³) / (8.314 J/K mol * 296.85 K)
Calculating this value:
n ≈ 11.8 mol
Therefore, approximately 11.8 moles of gas are present.
(b) To find the pressure of the gas after the change in volume and temperature, we can use the ideal gas law equation again:
P1V1 / T1 = P2V2 / T2
Where:
P1 = Initial pressure
V1 = Initial volume
T1 = Initial temperature
P2 = Final pressure (to be determined)
V2 = Final volume
T2 = Final temperature
Given:
Initial pressure (P1) = 1.42 × 105 Pa
Initial volume (V1) = 2.08 m³
Initial temperature (T1) = 23.7°C = 23.7 + 273.15 = 296.85 K
Final volume (V2) = 3.79 m³
Final temperature (T2) = 37.1°C = 37.1 + 273.15 = 310.25 K
Now, let's solve for the final pressure (P2):
P2 = (P1 * V1 * T2) / (V2 * T1)
P2 = (1.42 × 105 Pa * 2.08 m³ * 310.25 K) / (3.79 m³ * 296.85 K)
Calculating this value:
P2 ≈ 1.31 × 105 Pa
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Find out how the experimental data provided for the energy
spectrum of the turbulent flows. Write a report to explain the
energy spectrum curves and measurement methods
Energy spectrum of turbulent flows refers to the process of showing the energy distribution of turbulent fluctuations in a fluid flow. It is a widely studied and critical topic in fluid mechanics.
There is a high level of variation in energy spectra among different types of turbulent flows, but there are a few general characteristics.The spectrum curve, also known as the spectrum density, of turbulent flows is usually represented in a logarithmic plot of energy versus frequency (wavenumber). It illustrates how much energy is carried by the different frequencies of the flow.
The slope of the energy spectrum, which is the negative derivative of the spectrum curve, is used to characterize the degree of turbulence. For instance, a shallower slope represents a more turbulent flow while a steeper slope indicates a smoother flow.
There are a few different methods used to measure energy spectra in turbulent flows, including hot-wire anemometry, laser Doppler velocimetry, and particle image velocimetry. Hot-wire anemometry is a widely used and well-established method that works by measuring the electrical resistance of a hot wire as it is cooled by the fluid flow.
Laser Doppler velocimetry is another technique that uses laser light to measure fluid flow velocity by measuring the Doppler shift of scattered light. Particle image velocimetry is a relatively new method that works by measuring the displacement of small tracer particles in the flow using high-speed cameras.
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The force between two electrons in a vacuum is
1x10^-15 Newton or 1 femto Newton. How far apart are the
electrons.
The force between two electrons in a vacuum is[tex]1 x 10^-15[/tex] Newton or 1 femto Newton. To calculate the distance between these two electrons, we need to use Coulomb's Law.
Coulomb's law states that the force between two charges is proportional to the product of the charges and inversely proportional to the square of the distance between them. Coulomb's Law formula is given as:
[tex]F = k (q1q2)/r²[/tex]WhereF is the force between two chargesq1 and q2 are the magnitudes of the charges separated by a distance rK is Coulomb's constant with a value of 9 x 10^9 Nm²/C²Given:
[tex]F = 1 x 10^-15 Nq1[/tex]
= q2
= -1.6 x 10^-19 C (Charge on an electron)We can rearrange Coulomb's Law equation and solve for r as:
[tex]r = √k(q1q2)/FS[/tex]ubstituting the given values:r
[tex]= √(9 x 10^9 Nm²/C²)(-1.6 x 10^-19 C)² / (1 x 10^-15 N)r[/tex]
[tex]= √(9 x 10^9 Nm²/C²)(2.56 x 10^-38 C²) / (1 x 10^-15 N)r[/tex]
[tex]= √(9 x 2.56 x 10^-29) m²r[/tex]
[tex]= 4.6 x 10^-11 m[/tex] Therefore, the distance between two electrons is approximately[tex]4.6 x 10^-11[/tex]meters or 0.046 nanometers.
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Problem 3: An otter is swimming in the deep area of his tank at the zoo. The surface area of the otter's back is A = 0.45 m2, and you may assume that his back is essentially flat. The gauge pressure of the water at the depth of the otter is P = 10500 Pa.
Part (a) Enter an expression for the magnitude of the force F on the back of the otter in terms of the gauge pressure P and the atmospheric pressure P0.
Part (b) Solve for the magnitude of the force F, in newtons.
Part (c) The direction of the force F is always ________ to the surface the water is in contact with (in this case, the back of the otter).
P = 10500 PaP0 is the atmospheric pressure. he given values in the above equation to find the magnitude of the force is -43290 N. The direction of the force F is normal (perpendicular) to the surface of the water, which is in contact with the back of the otter.
Part (a) Magnitude of the force F on the back of the otter can be defined as follows:
F = (P - P0)A
Where, P = 10500 PaP0 is the atmospheric pressure
Part (b) Substitute the given values in the above equation to find the magnitude of the force F,F = (10500 - 101300) × 0.45 F = -43290 N
Part (c) The direction of the force F is always perpendicular to the surface the water is in contact with (in this case, the back of the otter).
Therefore, the direction of the force F is normal (perpendicular) to the surface of the water, which is in contact with the back of the otter.
An otter is swimming in the deep area of his tank at the zoo. The surface area of the otter's back is A = 0.45 m², and you may assume that his back is essentially flat. The gauge pressure of the water at the depth of the otter is P = 10500 Pa. The expression for the magnitude of the force F on the back of the otter is F = (P - P0)A. The magnitude of the force F, in newtons, is -43290 N. The direction of the force F is always perpendicular to the surface the water is in contact with (in this case, the back of the otter).
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