Electromagnetic Waves and Their Properties

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31 Terms

1

Electromagnetic Waves

Electromagnetic waves are transverse because their electric and magnetic fields oscillate perpendicular to the direction of wave propagation.

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2

Speed of Electromagnetic Waves

In a vacuum, electromagnetic waves travel at c = 3 × 10^8 m/s. In other media, their speed decreases due to interactions with atoms, but their frequency remains constant.

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3

Medium Requirement

Electromagnetic waves do not require a medium because they consist of oscillating electric and magnetic fields. Sound waves are mechanical waves that rely on particle vibrations in a medium.

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4

Wave Speed Calculation

A wave has a frequency of 50 Hz and a wavelength of 2 m. v = fλ = 50 × 2 = 100 m/s.

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5

Frequency from Period

If the period of a wave is 0.02 s, its frequency is f = 1/T = 1/0.02 = 50 Hz.

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6

Wavelength and Frequency Relationship

Wavelength is inversely proportional to frequency (λ = v/f), so doubling the frequency halves the wavelength.

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7

Frequency Calculation in Air

A wave travels at 340 m/s in air. If its wavelength is 17 m, its frequency is f = v/λ = 340/17 = 20 Hz.

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8

Electromagnetic Spectrum Order

The regions of the electromagnetic spectrum in order of increasing energy are: Radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, gamma rays.

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9

Harmful Effects of UV Radiation

UV radiation can damage skin cells, leading to sunburn, premature aging, and an increased risk of skin cancer.

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10

Microwaves vs Visible Light

Microwaves have longer wavelengths (1 mm to 1 m) compared to visible light (400-700 nm). Visible light has higher energy because energy increases with frequency (E = hf).

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11

Uses of Gamma Rays in Medicine

Gamma rays are used in radiation therapy to kill cancer cells and sterilize medical equipment.

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12

Refraction Calculation

Light travels from air (n = 1) into glass (n = 1.5). If the angle of incidence is 30°, using Snell's Law, θ2 = sin⁻¹(0.333) ≈ 19.5°.

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13

Critical Angle Calculation

For light travelling from water (n = 1.33) to air (n = 1), the critical angle θc = sin⁻¹(0.75) ≈ 48.6°.

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14

Prism and Spectrum

A prism splits white light into a spectrum of colours.

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15

Dispersion

Different wavelengths of light refract at different angles as they pass through the prism, causing dispersion.

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16

Refractive Index

The refractive index (n) is inversely proportional to the speed of light in the medium (v = c/n).

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17

Temperature Conversion

0 K = −273.15 °C.

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18

Thermal Energy Increase

Heating increases the kinetic energy of particles (they move faster) and their potential energy (interatomic forces change).

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19

Conduction vs Convection

In conduction, particles vibrate but do not move from their positions. In convection, particles move from one place to another, carrying heat with them.

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20

Evaporation Cooling

Evaporation removes the highest-energy molecules from the liquid, reducing the average kinetic energy (temperature) of the remaining molecules.

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21

Energy Calculation for Heating Water

Q = mcΔT = 2 × 4200 × (80 − 20) = 504,000 J.

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22

Energy to Melt Ice

Q = mL = 0.5 × 334,000 = 167,000 J.

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23

Specific Heat Capacity Calculation

If 2000 J of energy is added to 0.1 kg of a substance, and its temperature increases by 10°C, what is its specific heat capacity?

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24

Wien's Law Peak Wavelength

λmax = bT = 2.898 × 10−3 / 6000 = 4.83 × 10−7 m (483 nm, visible light).

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25

Energy Emission Comparison

Energy is proportional to T^4, so the object at 600 K emits 16 times more energy than the object at 300 K.

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26

Wien's Law and Wavelength

According to Wien's Law, λmax is inversely proportional to temperature. Hotter objects have more energy, leading to higher-frequency (shorter wavelength) radiation.

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27

Optical Fibres in Endoscopy

Optical fibres transmit light into the body, allowing doctors to see internal organs without invasive surgery.

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28

Microwaves in Communication

Microwaves can penetrate the atmosphere and travel long distances without significant signal loss.

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29

X-ray Production and Use

X-rays are produced by high-energy electron collisions. They penetrate soft tissues but are absorbed by dense materials like bones, creating contrast in images.

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30

Greenhouse Effect and Infrared Radiation

Greenhouse gases absorb and re-emit infrared radiation from the Earth's surface, trapping heat and warming the atmosphere.

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31

Kelvin Scale in Science

The Kelvin scale starts at absolute zero (0 K), where all molecular motion stops, making it ideal for thermodynamic calculations.

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