Wave physicist
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Test YourselfTransverse waves, sound, the electromagnetic spectrum and seismic waves — with an explanation after every question and a link to exactly where to read more.
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The complete bank, grouped by topic. Useful for revision without taking the quiz — and the reason the whole thing still works with JavaScript turned off.
Amplitude is how far the medium is displaced from equilibrium at the peak of its oscillation. It sets the energy the wave carries, not its speed — the distance between crests is wavelength, and cycles per second is frequency.
Wave properties →Use the universal wave equation v = f × λ. Here 120 × 2.5 = 300 m/s. The equation applies to every wave in physics, transverse or longitudinal.
Wave calculator →Period and frequency are reciprocals: T = 1/f = 1/40 = 0.025 s. Each complete cycle takes twenty-five thousandths of a second.
Wave calculator →Energy is proportional to amplitude squared, so doubling the amplitude gives 2² = 4 times the energy. This is why a small rise in amplitude makes a sound noticeably louder.
Amplitude and energy →Particles of the medium oscillate about a fixed rest position and return to it. A floating leaf bobs as ripples pass but does not travel to shore. Only energy — and the pattern carrying it — moves forward.
How waves carry energy →Perpendicular motion is the defining feature. Shake a rope up and down and the wave runs along the rope while the rope itself only moves across the direction of travel.
Sound is longitudinal — air molecules oscillate back and forth along the direction the sound travels. The other three all oscillate perpendicular to their travel.
Transverse vs longitudinal →The highest point is the crest and the lowest is the trough. Rarefactions belong to longitudinal waves, and a node is a point of zero displacement on a standing wave.
A transverse mechanical wave works by shearing the medium sideways, which needs the material to resist that shear and spring back. A liquid flows instead, so its shear modulus is zero and the wave speed √(G/ρ) collapses to zero.
Why S-waves stop at the core →Use v = √(T/μ) = √(64 / 0.004) = √16,000 ≈ 126.5 m/s. Tightening a string raises the tension and therefore the speed, which is how tuning a guitar works.
String speed calculator →Compressions are the high-pressure, high-density regions; rarefactions are where the particles spread apart. Longitudinal waves have no crests or troughs at all.
Compressions and rarefactions →Speed depends on the ratio of stiffness to density, v = √(E/ρ). Steel is denser than air, which alone would slow sound down, but it is roughly a million times stiffer — and stiffness wins decisively.
The speed of sound →v = 331.3 + 0.606 × 30 = 331.3 + 18.18 = 349.5 m/s. Every degree Celsius adds roughly 0.6 m/s, which is why sound carries differently on a hot day.
Temperature and the speed of sound →Polarization works by admitting one direction of oscillation and blocking the rest. A longitudinal wave already vibrates in a single direction — along its own path — so a filter has nothing left to remove. The impossibility is structural, not technological.
Polarization: the decisive test →A longitudinal wave is a physical compression of matter. With almost no particles present there is nothing to squeeze together or spread apart, so the wave cannot exist. Light, being an oscillation of fields rather than matter, crosses a vacuum freely.
Radio waves have the longest wavelengths and gamma rays the shortest. Moving along that order, wavelength falls while frequency and photon energy both rise.
The seven bands →Photon energy is proportional to frequency (E = hf), and gamma rays have the highest frequency of any electromagnetic wave — above 30 exahertz. Radio waves, at the other end, carry the least.
Wavelength, frequency and energy →Every electromagnetic wave travels at c ≈ 299,792,458 m/s in a vacuum regardless of band. They differ in wavelength, frequency and energy — never in speed.
What is the electromagnetic spectrum? →The transition sits inside ultraviolet, at a photon energy of roughly 10 to 33 eV. UV's lower reaches merely cause sunburn; its upper reaches cross into genuinely cell-damaging territory, along with all X-rays and gamma rays.
Human vision runs from about 380 nm at the violet end to 700 nm at the red end. Just beyond those limits lie ultraviolet (10–400 nm) and infrared (700 nm – 1 mm), both invisible to us.
Both leave at the same instant through the same rock. The longitudinal P-wave travels at √((K + 4G/3)/ρ) while the transverse S-wave travels at √(G/ρ). The P-wave formula contains everything the S-wave formula has plus the bulk modulus term, so it is always faster — typically by about 1.7× in rock.
P-waves and S-waves →Transverse S-waves cannot cross liquid, because a fluid has no shear rigidity. Their disappearance beyond about 103° could only mean a liquid layer deep inside. Oldham inferred a core from this in 1906; Lehmann found the solid inner core in 1936.
Shadow zones and Earth's core →Surface waves combine both motions. Each water particle moves forward at the crest and backward in the trough while also rising and falling, tracing a near-circular orbit that shrinks rapidly with depth. Seismic Rayleigh waves do the same in rock.
Only a transverse wave has a plane of oscillation directions for a filter to select from. Reflection, refraction and a finite speed are shared by both wave types, but polarization is possible only for transverse waves — which is what settled the argument in the early 1800s.
They share far more than they differ by: the same wave equation, v = fλ, T = 1/f, E ∝ A², and every wave behaviour including reflection, refraction, diffraction and interference. Only transverse waves polarize, only longitudinal waves always need a medium, and only longitudinal waves form compressions.
Twenty-five multiple-choice questions, split evenly across five topics: wave basics, transverse waves, sound and longitudinal waves, the electromagnetic spectrum, and comparison and seismic waves. You can take all twenty-five or filter to a single topic.
Yes. Every question gives instant feedback the moment you answer, with a written explanation of why the correct option is right and a link to the page that covers it in depth. The complete question bank is also listed further down this page for revision without taking the quiz.
Secondary school through introductory undergraduate physics — GCSE, A-level, IB and first-year university. The wave basics and transverse sections suit earlier study; the comparison and seismic questions reach into elastic moduli and wave speeds in solids.
As many times as you like. Question order is shuffled on every attempt, and after finishing you can retry just the questions you got wrong rather than starting over.
The interactive version does. Without JavaScript, the full question bank, the correct answers and all the explanations are still readable further down the page, so nothing is lost.
Definition, labelled diagram, properties and polarization.
Compressions, rarefactions and the speed of sound.
Every difference and similarity, side by side.
All seven bands, from radio waves to gamma rays.
Solve v = fλ, period, string speed and photon energy.
Every wave term on this site, defined and cross-linked.