The critical angle for n = 1.5 into n = 1
At its defaults it draws the critical angle for n = 1.5 into n = 1. Refracted angle against incident angle. It rises faster than the incident angle and reaches 90° at 41.8°, beyond which no refracted ray exists at all.
critical-angle is one function in lib/figures/optics.js —
rays, lenses, mirrors and what light does to a surface. Everything below came out
of it during this build, at parameters taken from the essays rather than invented for this
page. A figure here is the figure a reader meets in an essay, and if the generator changes,
this page changes with it.
At its defaults
Drawn even though every essay passes options, because a default nothing exercises is a trap for the next essay to call this with none — which has happened here twice.
Refracted angle against incident angle. It rises faster than the incident angle and reaches 90° at 41.8°, beyond which no refracted ray exists at all.
The angle at which a total reflection stops being total
The options are the ones The angle at which total reflection stops being total passes. A branch drawn at its own defaults instead would be a picture no essay asked for and no assertion has been run against.
Reflectance of light at 633 nm inside a BK7 prism whose face carries a 50 nm gold film with water beyond it, against the angle of incidence, for the two polarisations, from the three-layer Fresnel sum in complex arithmetic. Past the critical angle for glass and water, 61.62°, s-polarised light is reflected almost completely, as total internal reflection requires, apart from what the thin gold absorbs. p-polarised light is reflected too — except near one angle, where the reflectance falls to 0.014 at 71.52°. The dispersion relation of a surface plasmon on gold against water puts its resonance at 71.67°; the difference is the film's finite thickness and the prism on its other side pulling the resonance slightly.
How thick the gold has to be
The options are the ones The angle at which total reflection stops being total passes. A branch drawn at its own defaults instead would be a picture no essay asked for and no assertion has been run against.
The p-polarised reflectance of the glass | gold | water arrangement against angle for gold films of 30, 40, 50, 60, 70 nm. At 30 nm the dip reaches 0.367 at 71.05°; at 40 nm the dip reaches 0.075 at 71.28°; at 50 nm the dip reaches 0.014 at 71.52°; at 60 nm the dip reaches 0.209 at 71.70°; at 70 nm the dip reaches 0.472 at 71.80°. The deepest dip, found by scanning the thickness in half-nanometre steps, is at 47.0 nm, where it reaches zero to four decimal places: there the energy the plasmon loses by leaking back through the film into the prism equals what it loses by heating the gold, and the reflected wave cancels. Thinner films leak too much and give a broad, shallow dip; thicker ones let too little light reach the plasmon at all.
A dip that moves when anything touches the gold
The options are the ones The angle at which total reflection stops being total passes. A branch drawn at its own defaults instead would be a picture no essay asked for and no assertion has been run against.
The p reflectance of the glass | 50 nm gold | sample arrangement for samples of index 1.333 and 1.343, and the angle of the dip against the sample's index from 1.330 to 1.340. The dip moves from 71.52° to 72.99° for an index change of 0.010, and over the whole range at 144° per unit of index. A dip whose position is read to a thousandth of a degree therefore registers a change of index of 7.0 × 10⁻⁶, averaged over the thin layer next to the gold that the plasmon's field reaches — the scale on which molecules binding to the gold are detected.
Why the sharpest dip comes from the least lossy metal
The options are the ones The angle at which total reflection stops being total passes. A branch drawn at its own defaults instead would be a picture no essay asked for and no assertion has been run against.
The p reflectance against angle for films of silver, gold and aluminium between a BK7 prism and water at 633 nm, each at the thickness that gives it its deepest dip, with permittivities from tabulated values: silver, ε = −18.30 + 0.48i, 55 nm, dip at 67.82° and 0.79° wide at half depth; gold, ε = −12.45 + 1.29i, 47 nm, dip at 71.46° and 5.54° wide at half depth; aluminium, ε = −55.90 + 20.80i, 12 nm, dip at 64.78° and 18.38° wide at half depth. The width is set by how fast the plasmon loses energy into the metal, which grows with the imaginary part of the permittivity relative to the real: silver's resonance is the sharpest, aluminium's so broad it is barely a resonance. Gold is used anyway, because silver tarnishes and gold does not.
The field the plasmon piles up at the surface
The options are the ones The angle at which total reflection stops being total passes. A branch drawn at its own defaults instead would be a picture no essay asked for and no assertion has been run against.
The intensity of the magnetic field just beyond the gold, in the water, relative to the incident light's, against the angle of incidence, for the same 50 nm film. At the resonance, 71.03°, it is 12.6 times the incident intensity, although almost no light is reflected and none is transmitted into the water as a propagating wave: the energy is held in the plasmon and dissipated in the metal. Into the water the intensity falls by a factor of e in 96 nm — set, as for any evanescent wave, by the angle alone — so the resonance senses a layer of the order of a hundred nanometres thick and nothing beyond it.
What checks it
physicscheck asserts something about critical-angle that
could fail — it draws it and measures the result against a value reached some other
way.
Across the library: 100 interrogated, 2 exercised only, 1 untouched, of 103. Read out of the gate's source by the gate's own two patterns — and the gate's last claim fails the build if that read disagrees with what it was handed while running.
Where it is called
Changing this generator changes every figure on this list. That is what makes the list worth publishing rather than keeping in a check script.
The angle at which total reflection stops being total
Coat the back face of a glass prism with fifty nanometres of gold and total internal reflection still returns almost all the light — except at one angle, where the reflection of one polarisation falls nearly to zero. The light has gone into an electron wave bound to the far surface of the gold, and because that wave's angle depends on whatever touches the gold, the missing reflection has become one of the most sensitive balances in biochemistry.
OpticsThe angle past which light cannot leave
Snell's law asks for the sine of an angle greater than one, and no such angle exists. What happens instead is a perfect mirror made out of nothing but a change of speed.
OpticsThe angle that is two angles
Snell's law survives a complex index by giving a complex answer, and a complex angle is not an angle. What the phase-matching argument actually fixes is the tangential wavenumber, and when the medium absorbs, the surfaces of constant phase and the surfaces of constant amplitude stop being parallel. In silver at 550 nanometres the phase fronts run within four degrees of the surface while the amplitude decays straight into it.
OpticsThe bend at the boundary, and what it is really about
Light changes direction when it changes speed. Snell's law is the geometry of that statement, and it can be derived without knowing anything about light at all.
WavesThe channel with no walls
A pipe will not carry a note below its cutoff, and no length of pipe helps. Replace the walls with nothing but a region where the wave travels slightly slower, and the cutoff disappears — however weak the contrast and however thin the channel, at least one mode is bound. The difference is not a matter of degree; it is the difference between a boundary condition and a potential well.
OpticsThe corner that sends light home
Three mirrors at right angles send light straight back the way it came, from any direction they can see, because each one reverses one component of its direction. Made from solid glass, a corner reflects by total internal reflection and needs no silver — which is why the reflectors left on the Moon are bare glass — but each of its six sectors then returns a different polarisation, and the returned spot loses three-quarters of its peak.
OpticsThe drop that cannot hold the light it lets in
Light inside water meeting the surface at more than 48.6° is totally reflected, and every raindrop is made of water. Yet no ray of sunlight that enters a raindrop is ever totally reflected inside it. A sphere's geometry forbids it: a ray refracted on the way in meets the inside of the surface at its refraction angle, and keeps meeting it at that same angle every time it bounces, and that angle is always smaller than the critical one. The light leaks out a little at every bounce, which is why there are rainbows at all. Light born inside the drop is another matter, and a sphere can keep it for ever.
OpticsThe index that falls below one
Glass bends light because light is slower in it. X-rays are not slower in glass, or in anything: every material's refractive index for them is slightly less than one, by a few parts in a million. Everything about X-ray optics follows from that small number with the wrong sign. A lens that focuses them must be thinner in the middle than at the edges, and so weak that dozens are stacked in a row. A mirror reflects them only if they arrive at a glancing angle of less than a degree — totally, from the outside, the reverse of the way a diamond traps light — which is why the mirrors of an X-ray telescope are long, nested barrels rather than dishes.
OpticsThe mirror that lights a tenth of a micrometre
Total internal reflection sends back every photon, and it leaves behind a field in the medium beyond that dies away within a fraction of a wavelength. Put a living cell on a coverslip and reflect a laser inside the glass, and that field lights only the hundred nanometres of the cell pressed against the glass: the membrane, and the proteins moving in it. Nothing else glows. The same field works in reverse. A molecule close to the glass sends part of its own light into angles no ray from the water could reach, and how much it sends there says how close it is.
OpticsThe reflection that happens where the glass is not
Total internal reflection sends back every photon, which is why it is called total. It does not send them back from where they arrived — the beam re-emerges displaced along the surface, by a fraction of a wavelength, and a displacement is only possible if the light spent time on the far side of a boundary it never crossed.
OpticsThe roof that splits a binocular's image
A slim, straight binocular turns its image upright with a roof — two glass faces meeting at a right angle, which reflect every ray twice by total internal reflection and lose no light at all. They lose sharpness instead. Total reflection shifts the phases of the two polarisations of light by different amounts, and the half of the beam on one side of the roof's edge meets the two faces in the opposite order from the other half. The halves leave in different polarisations, interfere only partly at the focus, and every star becomes a slightly doubled smudge — unless a coating a fraction of a micrometre thick makes the glass behave like a mirror.
OpticsThe window a diamond is cut inside
A well-cut diamond sends back out of its top most of the light that falls on it, and it does so without a single silvered surface. Light entering the top is totally reflected at one sloping face of the pavilion below, again at the opposite face, and then has to leave through the top — where it must not be totally reflected. Each of those three is a condition on one angle, and together they leave a window a dozen degrees wide inside which a stone looks bright and outside which it looks glassy. The window is wide for diamond and nearly closed for glass, which is why a cutter's skill cannot make glass sparkle.
OpticsThe windscreen that feels the rain
Behind the rear-view mirror of most modern cars a small box decides when the wipers should run, and it does so without looking at the rain. It shines infrared light into the windscreen at forty-five degrees, steep enough to be trapped inside the glass by total internal reflection, and counts how much comes back out of the far end of the glass a few centimetres away. A raindrop on the outside changes the medium the glass is touching from air to water, and water's critical angle against glass is sixty-one degrees, not forty-one: at forty-five the light is no longer trapped, and nearly all of it leaves into the drop. The sensor measures the area the rain is touching, and the rain rate from how fast that area grows.