Physics A Level با پاسخ Chapter 12: Waves 12.3 Wave energy
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Physics (9702)
- Chapter 1: Kinematics
- 1.1 Speed
- 1.2 Distance and displacement, scalar and vector
- 1.3 Speed and velocity
- 1.4 Displacement–time graphs
- 1.5 Combining displacements
- 1.6 Combining velocities
- 1.7 Subtracting vectors
- 1.8 Other examples of scalar and vector quantities
- Chapter 2: Accelerated motion
- 2.1 The meaning of acceleration
- 2.2 Calculating acceleration
- 2.3 Units of acceleration
- 2.4 Deducing acceleration
- 2.5 Deducing displacement
- 2.6 Measuring velocity and acceleration
- 2.7 Determining velocity and acceleration in the laboratory
- 2.8 The equations of motion
- 2.9 Deriving the equations of motion
- 2.10 Uniform and non-uniform acceleration
- 2.11 Acceleration caused by gravity
- 2.12 Determining g
- 2.13 Motion in two dimensions: projectiles
- 2.14 Understanding projectiles
- Chapter 3: Dynamics
- 3.1 Force, mass and acceleration
- 3.2 Identifying forces
- 3.3 Weight, friction and gravity
- 3.4 Mass and inertia
- 3.5 Moving through fluids
- 3.6 Newton’s third law of motion
- 3.7 Understanding SI units
- Chapter 4: Forces
- 4.1 Combining forces
- 4.2 Components of vectors
- 4.3 Centre of gravity
- 4.4 The turning effect of a force
- 4.5 The torque of a couple
- Chapter 5: Work, energy and power
- 5.1 Doing work, transferring energy
- 5.2 Gravitational potential energy
- 5.3 Kinetic energy
- 5.4 Gravitational potential to kinetic energy transformations
- 5.5 Down, up, down: energy changes
- 5.6 Energy transfers
- 5.7 Power
- Chapter 6: Momentum
- 6.1 The idea of momentum
- 6.2 Modelling collisions
- 6.3 Understanding collisions
- 6.4 Explosions and crash-landings
- 6.5 Collisions in two dimensions
- 6.6 Momentum and Newton’s laws
- 6.7 Understanding motion
- Chapter 7: Matter and materials
- 7.1 Density
- 7.2 Pressure
- 7.3 Archimedes’ principle
- 7.4 Compressive and tensile forces
- 7.5 Stretching materials
- 7.6 Elastic potential energy
- Chapter 8: Electric current
- 8.1 Circuit symbols and diagrams
- 8.2 Electric current
- 8.3 An equation for current
- 8.4 The meaning of voltage
- 8.5 Electrical resistance
- 8.6 Electrical power
- Chapter 9: Kirchhoff’s laws
- 9.1 Kirchhoff’s first law
- 9.2 Kirchhoff’s second law
- 9.3 Applying Kirchhoff’s laws
- 9.4 Resistor combinations
- Chapter 10: Resistance and resistivity
- 10.1 The I-V characteristic for a metallic conductor
- 10.2 Ohm’s law
- 10.3 Resistance and temperature
- 10.4 Resistivity
- Chapter 11: Practical circuits
- 11.1 Internal resistance
- 11.2 Potential dividers
- 11.3 Sensors
- 11.4 Potentiometer circuits
- Chapter 12: Waves
- 12.1 Describing waves
- 12.2 Longitudinal and transverse waves
- 12.3 Wave energy
- 12.4 Wave speed
- 12.5 The Doppler effect for sound waves
- 12.6 Electromagnetic waves
- 12.7 Electromagnetic radiation
- 12.8 Orders of magnitude
- 12.9 The nature of electromagnetic waves
- 12.10 Polarisation
- Chapter 13: Superposition of waves
- 13.1 The principle of superposition of waves
- 13.2 Diffraction of waves
- 13.3 Interference
- 13.4 The Young double-slit experiment
- 13.5 Diffraction gratings
- Chapter 14: Stationary waves
- 14.1 From moving to stationary
- 14.2 Nodes and antinodes
- 14.3 Formation of stationary waves
- 14.4 Determining the wavelength and speed of sound
- Chapter 15: Atomic structure
- 15.1 Looking inside the atom
- 15.2 Alpha-particle scattering and the nucleus
- 15.3 A simple model of the atom
- 15.4 Nucleons and electrons
- 15.5 Forces in the nucleus
- 15.6 Discovering radioactivity
- 15.7 Radiation from radioactive substances
- 15.8 Energies in α and β decay
- 15.9 Equations of radioactive decay
- 15.10 Fundamental particles
- 15.11 Families of particles
- 15.12 Another look at β decay
- 15.13 Another nuclear force
- P1 Practical skills at AS Level
- P1.1 Practical work in physics
- P1.2 Using apparatus and following instructions
- P1.3 Gathering evidence
- P1.4 Precision, accuracy, errors and uncertainties
- P1.5 Finding the value of an uncertainty
- P1.6 Percentage uncertainty
- P1.7 Recording results
- P1.8 Analysing results
- P1.9 Testing a relationship
- P1.10 Combining uncertainties
- P1.11 Identifying limitations in procedures and suggesting improvements
- Chapter 16: Circular motion
- 16.1 Describing circular motion
- 16.2 Angles in radians
- 16.3 Steady speed, changing velocity
- 16.4 Angular speed
- 16.5 Centripetal forces
- 16.6 Calculating acceleration and force
- 16.7 The origins of centripetal forces
- Chapter 17: Gravitational fields
- 17.1 Representing a gravitational field
- 17.2 Gravitational field strength g
- 17.3 Energy in a gravitational field
- 17.4 Gravitational potential
- 17.5 Orbiting under gravity
- 17.6 The orbital period
- 17.7 Orbiting the Earth
- Chapter 18: Oscillations
- 18.1 Free and forced oscillations
- 18.2 Observing oscillations
- 18.3 Describing oscillations
- 18.4 Simple harmonic motion
- 18.5 Representing s.h.m. graphically
- 18.6 Frequency and angular frequency
- 18.7 Equations of s.h.m.
- 18.8 Energy changes in s.h.m.
- 18.9 Damped oscillations
- 18.10 Resonance
- Chapter 19: Thermal physics
- 19.1 Changes of state
- 19.2 Energy changes
- 19.3 Internal energy
- 19.4 The meaning of temperature
- 19.5 Thermometers
- 19.6 Calculating energy changes
- Chapter 20: Ideal gases
- 20.1 Particles of a gas
- 20.2 Explaining pressure
- 20.3 Measuring gases
- 20.4 Boyle’s law
- 20.5 Changing temperature
- 20.6 Ideal gas equation
- 20.7 Modelling gases: the kinetic model
- 20.8 Temperature and molecular kinetic energy
- Chapter 21: Uniform electric fields
- 21.1 Attraction and repulsion
- 21.2 The concept of an electric field
- 21.3 Electric field strength
- 21.4 Force on a charge
- Chapter 22: Coulomb’s law
- 22.1 Electric fields
- 22.2 Coulomb’s law
- 22.3 Electric field strength for a radial field
- 22.4 Electric potential
- 22.5 Gravitational and electric fields
- Chapter 23: Capacitance
- 23.1 Capacitors in use
- 23.2 Energy stored in a capacitor
- 23.3 Capacitors in parallel
- 23.4 Capacitors in series
- 23.5 Comparing capacitors and resistors
- 23.6 Capacitor networks
- 23.7 Charge and discharge of capacitors
- Chapter 24: Magnetic fields and electromagnetism
- 24.1 Producing and representing magnetic fields
- 24.2 Magnetic force
- 24.3 Magnetic flux density
- 24.4 Measuring magnetic flux density
- 24.5 Currents crossing fields
- 24.6 Forces between currents
- 24.7 Relating SI units
- 24.8 Comparing forces in magnetic, electric and gravitational fields
- Chapter 25: Motion of charged particles
- 25.1 Observing the force
- 25.2 Orbiting charged particles
- 25.3 Electric and magnetic fields
- 25.4 The Hall effect
- 25.5 Discovering the electron
- Chapter 26: Electromagnetic induction
- 26.1 Observing induction
- 26.2 Explaining electromagnetic induction
- 26.3 Faraday’s law of electromagnetic induction
- 26.4 Lenz’s law
- 26.5 Everyday examples of electromagnetic induction
- Chapter 27: Alternating currents
- 27.1 Sinusoidal current
- 27.2 Alternating voltages
- 27.3 Power and alternating current
- 27.4 Rectification
It is important to realise that, for both types of mechanical wave, the particles that make up the material through which the wave is travelling do not move along – they only oscillate about a fixed point. It is energy that is transmitted by the wave. Each particle vibrates; as it does so, it pushes its neighbour, transferring energy to it. Then that particle pushes its neighbour, which pushes its neighbour. In this way, energy is transmitted from one particle to the next, to the next and so on down the line.
Intensity
The term intensity has a very precise meaning in physics. The intensity of a wave is defined as the rate of energy transmitted (power) per unit area at right angles to the wave velocity.
${\mathop{\rm int}} ensity = \frac{{power}}{{area}}$
Intensity is measured in watts per square metre ($W\,{m^{ - 2}}$). For example, when the Sun is directly overhead, the intensity of its radiation is about $1.0\,kW\,{m^{ - 2}}$ (1 kilowatt per square metre). This means that energy arrives at the rate of about $1 kW$ ($1000\,J\,{s^{ - 1}}$) on each square metre of the surface of the Earth. At the top of the atmosphere, the intensity of sunlight is greater, about $1.4\,kW\,{m^{ - 2}}$.
KEY EQUATION
${\mathop{\rm int}} ensity = \frac{{power}}{{area}}$
Question
4) A $100 W$ lamp emits electromagnetic radiation in all directions. Assuming the lamp to be a point source, calculate the intensity of the radiation:
a: at a distance of $1.0 m$ from the lamp
b: at a distance of $2.0 m$ from the lamp.
Hint: Think of the area of a sphere at each of the two radii.
Intensity and amplitude
- The intensity of a wave generally decreases as it travels along. There are two reasons for this:
- The wave may ‘spread out’ (as in the example of light spreading out from a lamp in Question 4).
The wave may be absorbed or scattered (as when light passes through the Earth’s atmosphere).
As a wave spreads out, its amplitude decreases. This suggests that the intensity I of a wave is related to its amplitude A.
In fact, intensity I is directly proportional to the square of the amplitude A:
${\mathop{\rm int}} ensity\, \propto \,amplitud{e^2}$ or $I\, \propto \,{A^2}$
KEY EQUATION
${\mathop{\rm int}} ensity\, \propto \,amplitud{e^2}$ or $I\, \propto \,{A^2}$
The relationship also implies that, for a particular wave:
$\frac{{{\mathop{\rm int}} ensity}}{{amplitud{e^2}}} = constant$
So, if one wave has twice the amplitude of another, it has four times the intensity. This means that the wave is transmitting four times the power per unit area at right angles to the wave velocity.
Question
5) A wave from a source has an amplitude of $5.0 cm$ and an intensity of $400\,W\,{m^{ - 2}}$.
a: The amplitude of the wave is increased to $10.0 cm$. Calculate the intensity now.
b: The intensity of the wave is decreased to $100\,W\,{m^{ - 2}}$. Calculate the amplitude now.