Physics 30 Lesson 24: Electromagnetic Waves

Page 1: Introduction to Electromagnetic Waves

  • Date and Event: On April 11, 1846, Michael Faraday was scheduled to introduce Sir Charles Wheatstone at a meeting of the Royal Society of London.

    • Wheatstone experienced severe stage fright and left before his lecture began.

    • Faraday had to deliver an unprepared lecture discussing theoretical concepts related to electromagnetic waves.

  • Faraday's Background:

    • Known for well-prepared lectures and spectacular demonstrations.

    • He had made a significant discovery in 1845 regarding polarization changes in light passing through heavy glass when exposed to external magnetic fields.

    • Speculated about the connection between light and magnetism but lacked mathematical skills to advance his ideas.

    • Faraday's focus was diverted to other interests, leaving the exploration of this idea unfinished.

  • James Clerk Maxwell:

    • Born (1831-1879), he began exploring Faraday's theories ten years after Faraday's initial speculation.

    • Graduated from Cambridge University in 1853 and began making significant contributions to physics and mathematics.

I. Principles of Electromagnetism

  • Foundational Discoveries:

    • Oersted and Ampere discovered that:

    • A constant electric current in a conductor induces a uniform magnetic field that circles the conductor, with both fields being perpendicular.

    • A direct relationship ties electric currents and magnetic fields.

    • Henry and Faraday established the converse where:

    • A conductor moving through a perpendicular magnetic field induces a uniform current in the conductor.

  • Conductors vs. Insulators:

    • Conductors: Allow the flow of electric current.

    • Insulators: Resist current flow; however, Maxwell found that a changing magnetic field momentarily shifts charges in insulators which quickly revert to their original position due to internal attractive forces.

    • This confirmed the hypothesis that changing magnetic fields can induce currents in various materials.

II. Maxwell's Extrapolations of Electromagnetism

  • Induction Principles:

    • Maxwell extended Ampere's principle, stating:

    • A changing electric field in space creates a perpendicular changing magnetic field.

    • He reformulated Faraday's inductive principle, which states:

    • A changing magnetic field generates a perpendicular changing electric field.

  • Interconnectedness of Fields:

    • Cycle: A changing electric field induces a changing magnetic field leading to another changing electric field, thus perpetuating the phenomenon.

III. Propagation of Electromagnetic Waves

  • Creation of Waves:

    • Maxwell theorized that oscillating electric fields create electromagnetic waves.

    • Illustrated with fields:

    • An increasing electric field $E1$ induces a magnetic field $B1$, which in turn induces another electric field $E_2$, continuing indefinitely.

  • Wave Characteristics:

    • Visualized as two perpendicular components:

    • Electric fields (denoted by $ε$) and magnetic fields (denoted by $β$).

    • The wave propagates perpendicularly to both fields and can travel through vacuum as it does not require a medium.

    • Electromagnetic radiation (EMR) displays transverse characteristics and can be polarized.

IV. Predictions by Maxwell

  • Predictions about EM Waves:

    • Origin: Accelerating electric charge causes the formation of electromagnetic waves as it oscillates, leading to the radiation of energy in electric and magnetic fields.

    • Correspondence: The frequency of oscillation directly corresponds to the frequency of generated EM waves.

    • Speed Consistency: EM waves travel at approximately 3.00imes108m/s3.00 imes 10^8 m/s, adhering to the universal wave equation for wave mechanics represented as:

    • c=fλc = fλ

    • Perpendicular Properties: Electric and magnetic fields remain perpendicular to each other and the wave's propagation direction.

    • Transverse Characteristics: Interference, diffraction, refraction, and polarization are observable phenomena.

    • Observable Pressure: EM waves exert pressure when interacting with surfaces.

V. Confirmation of Maxwell's Theories by Hertz

  • Hertz's Experiments:

    • In 1888, Heinrich Hertz aimed to experiment and validate Maxwell's theories regarding EM waves.

    • Hertz utilized an induction coil to create a spark and successfully detected induced sparks across a room, demonstrating the presence of EM waves.

  • Findings:

    • The speed of the electromagnetic wave measured around 3.0imes108m/s3.0 imes 10^8 m/s, confirming Maxwell's prediction.

    • Hertz's observations indicated that spark generation only occurs when the receiving apparatus aligns appropriately concerning the electric and magnetic fields of the EM wave, proving polarization behavior.

    • Subsequent tests for reflection, diffraction, interference, and refraction supported the behavior of EM radiation matching that of light.

  • Impact on Science:

    • Hertz's insights both confirmed Maxwell and inspired further studies, such as Marconi's work on radio transmission, establishing him as the father of radio communication.

VI. The Electromagnetic Spectrum

  • Definition: EM waves exist across various frequencies classified as the electromagnetic spectrum.

  • Spectrum Details:

    • The only distinction among EM waves is the frequency and wavelength.

    • Categories:

    • Low Frequency AC: ~60 Hz (used in AC power lines, creates interference).

    • Radio Waves: 1041010Hz10^{4} – 10^{10} Hz (from circuits, enables communication and navigation).

    • Microwaves: 1091012Hz10^{9} – 10^{12} Hz (applied in telecommunications and cooking).

    • Infrared Radiation: 10114×1014Hz10^{11} – 4 × 10^{14} Hz (relevant for thermography).

    • Visible Light: 4×10147.5×1014Hz4 × 10^{14} – 7.5 × 10^{14} Hz (detected by human eyes).

    • Ultraviolet Radiation: 7.5×10141017Hz7.5 × 10^{14} – 10^{17} Hz (causes tanning and fluorescence).

    • X-rays: 10171020Hz10^{17} – 10^{20} Hz (for medical imaging).

    • Gamma Rays: 10191024Hz10^{19} – 10^{24} Hz (from atomic nuclei and particle accelerators).

    • Cosmic Rays: > 1024Hz10^{24} Hz (from cosmic phenomena).

  • Memorization Aids:

    • Remember the range of visible light: 700 nm (red) to 400 nm (violet).

    • Acronym ROYGBIV for colors.

    • Categorization of frequencies:

    • Electromagnetic Types (TV, Microwave, Infrared, Visible, UV, X-rays, Gamma): 108,1010,1012,1014,1016,1018,1020Hz10^{8}, 10^{10}, 10^{12}, 10^{14}, 10^{16}, 10^{18}, 10^{20} Hz with frequency increments by a factor of 10.

  • Calculation: Use the universal wave equation c=λfc = λ f for wavelengths and frequencies.

VII. Assignment Questions

  1. Fundamentals:

    • A. What is the fundamental origin of all EMR?

    • B. Relationship of frequency in harmonic oscillators to EMR produced.

    • C. Speed of all EMR?

    • D. Sketch an EM wave.

  2. Differences Between Radiation Types:

    • Analyze similarities and differences among various radiation forms (radio, visible light, X-rays).

  3. Type of Radiation by Cause:

    • Classify types of radiation based on oscillation sources and transitions of electrons.

  4. Wave Penetration: X-rays or gamma rays comparison.

  5. Applications of Microwaves: Cooking processes and usage in technology.

  6. Camera Sensitivity: Required light type for nighttime visibility.

  7. Floral Perception: Sensitivity of honey bees in light spectrum.

  8. X-ray Functionality: Mechanism of using X-rays for imaging.

  9. EM Signaling: Calculate travel times for radio signals over distances and analyze frequency-related phenomena.

VIII. Calculations and Responses

  • Various tasks: Engage in mathematical problems resolving frequency and wavelength scenarios for EMR across various mediums.

    • E.g. Calculate the frequency of a 1.8 cm microwave. (Answer: $1.7 imes 10^{10} Hz$)

    • Determine $ ext{wavelength}$ and $ ext{periods}$ in different materials as indicated throughout the assignment tasks such as the period in Lucite or time taken for signals over astronomical distances.