Critical angle (TIR)
API · /snell-api
Snell Refraction API
Snell's-law refraction optics as an API, computed locally and deterministically. The refraction endpoint applies Snell's law, n1·sin(θ1) = n2·sin(θ2): from the refractive indices of two media (given directly or by material — vacuum, air, water, glass, diamond and more) and the angle of incidence it returns the angle of refraction, or solves for the incidence angle from a refraction angle; when light passes into a less dense medium beyond the critical angle it reports total internal reflection instead of a refracted ray. The critical-angle endpoint gives the threshold for total internal reflection, θc = asin(n2/n1) for n1 > n2 — the principle behind optical fibres — defaulting the exit medium to air. The speed endpoint gives the speed of light in a medium, v = c/n, as a fraction of c, and — with a vacuum wavelength — the shorter wavelength inside the medium (the frequency is unchanged). Angles are in degrees, wavelengths in nanometres. Everything is computed locally and deterministically, so it is instant and private. Ideal for optics and photonics tools, fibre-optic and lens-design apps, photography and physics education, and AR/VR and rendering software. Pure local computation — no key, no third-party service, instant. Live, nothing stored. 3 endpoints. This is Snell's-law refraction; for camera depth of field and field of view use a photography API.
API salute
salutare- Tempo di attività
- 100.00%
- Sondaggi del server · 24 ore su 24
- Latenza media
- 71 ms
- Sondaggi del server · 24 ore su 24
- Abbonati
- 3,539
- attiva
- Chiamate totali
- 76
- ultimi 7 giorni
Prezzi
Scegli un livello: fatturazione mensile, annullamento in qualsiasi momento.
Free
Gratis
- 2,000 chiamate/mese
- 2 richieste/secondo
- Tetto rigido (429 sopra la quota, nessuna eccedenza)
- 15,635 calls/month
- 2 req/sec
- Refraction + critical angle + speed
- No credit card
Starter
€5.00 /mese
- 25,000 chiamate/mese
- 5 richieste/secondo
- Tetto rigido (429 sopra la quota, nessuna eccedenza)
- 26.55k calls/month
- 8 req/sec
- TIR detection, material library
- Email support
Pro
€15.00 /mese
- 150,000 chiamate/mese
- 15 richieste/secondo
- Tetto rigido (429 sopra la quota, nessuna eccedenza)
- 303.5k calls/month
- 20 req/sec
- Optics / photonics pipelines
- Priority support
Mega
€45.00 /mese
- 753,000 chiamate/mese
- 40 richieste/secondo
- Tetto rigido (429 sopra la quota, nessuna eccedenza)
- 1.56M calls/month
- 50 req/sec
- Platform scale
- Dedicated SLA
Costruito da
Correlato APIs
Altro APIs con tag sovrapposti.
Telescope Optics API
Teleskop-Optik-Mathematik als API, lokal und deterministisch berechnet – die Vergrößerungs-, Austrittspupillen- und Auflösungsleistungszahlen, mit denen ein Amateurastronom oder eine Sternenbeobachtungs-App Ausrüstung und Okulare auswählt. Der Vergrößerungs-Endpunkt liefert die Vergrößerung = Brennweite des Teleskops ÷ Brennweite des Okulars (ein 1000-mm-Fernrohr mit einem 10-mm-Okular ergibt 100×), das Öffnungsverhältnis und – aus der Apertur – den nutzbaren Bereich von etwa der Apertur in mm ÷ 7 (niedrigste nutzbare, ein 7-mm-Austrittspupille) bis etwa 2× der Apertur in mm, jenseits dessen das Bild nur dunkler und unscharf wird; übergibt man ein Okular-Sichtfeld, wird das wahre Gesichtsfeld zurückgegeben. Der Austrittspupillen-Endpunkt liefert Apertur ÷ Vergrößerung, die Breite des Lichtstrahls, der das Okular verlässt – eine große 4–7 mm Austrittspupille für helle, weite Ansichten von Nebeln, eine kleine 0,5–2 mm für den Mond und Planeten bei hoher Vergrößerung. Der Auflösungs-Endpunkt liefert das Dawes-Limit ≈ 116 ÷ Apertur(mm) und das etwas strengere Rayleigh-Limit ≈ 138 ÷ Apertur in Bogensekunden, plus die Grenzhelligkeit ≈ 2,7 + 5·log₁₀(Apertur mm) – größeres Glas spaltet feinere Doppelsterne und erreicht schwächere Sterne, obwohl Seeing die reale Auflösung normalerweise auf etwa 1 Bogensekunde begrenzt. Alles wird lokal und deterministisch berechnet, daher ist es sofort und privat. Ideal für Astronomie- und Sternenbeobachtungs-Apps, Teleskop-Shop- und Okularrechner-Tools sowie Beobachtungsplaner-Hilfsprogramme. Reine lokale Berechnung – kein Key, kein Drittanbieter-Service, sofort. 3 Compute-Endpunkte. Für Kamera-/Dünnlinsen-Bildgebung verwenden Sie eine Lens-API; für Sternhelligkeiten eine Star-Magnitude-API.
api.oanor.com/telescope-api
Prism Optics API
Optical-prism geometry as an API, computed locally and deterministically. The deviation endpoint computes the minimum deviation angle of a light ray passing through a prism of apex angle A and refractive index n, δ_min = 2·arcsin(n·sin(A/2)) − A, together with the symmetric angle of incidence and the internal refraction angle A/2 on each face — an equilateral prism (A = 60°) of crown glass (n = 1.5) deviates light by about 37.2°. The refractive-index endpoint inverts the spectrometer formula n = sin((A + δ_min)/2) / sin(A/2), the standard way a refractive index is measured from a prism’s apex angle and its measured minimum deviation. The dispersion endpoint computes the angular dispersion between two wavelengths from their refractive indices and the apex angle, and, given the three Fraunhofer indices n_F, n_C and n_D, the dispersive power ω = (n_F − n_C)/(n_D − 1) and the Abbe number V = 1/ω that quantify how strongly a glass spreads colours — crown glass has ω ≈ 0.017 and V ≈ 59. All angles are in degrees. Everything is computed locally and deterministically, so it is instant and private. Ideal for optics, spectroscopy, refractometry, photonics and physics-education app developers, lens-and-prism design tools, and lab software. Pure local computation — no key, no third-party service, instant. Live, nothing stored. 3 endpoints. This is prism geometry; for a single flat-surface refraction use a Snell’s-law API and for thin lenses a lens API.
api.oanor.com/prism-api
Angular Size API
Angular-size astronomy and optics maths as an API, computed locally and deterministically. The angular-size endpoint computes the angular diameter an object subtends, δ = 2·arctan(d/(2D)), from its physical size and its distance, returning the angle in radians, degrees, arcminutes and arcseconds, along with the small-angle approximation δ ≈ d/D — the Sun and Moon are each about half a degree (31 arcminutes) across. The distance endpoint inverts the relation, D = d/(2·tan(δ/2)), to give an object's distance from its known true size and its measured angular size, the basis of the standard-ruler distance method. The object-size endpoint computes an object's physical diameter, d = 2·D·tan(δ/2), from its distance and angular size. Size and distance use any one consistent unit, and angles may be given in radians, degrees, arcminutes or arcseconds. Everything is computed locally and deterministically, so it is instant and private. Ideal for astronomy, telescope, astrophotography, surveying and optics app developers, field-of-view and rangefinding tools, and physics education. Pure local computation — no key, no third-party service, instant. Live, nothing stored. 3 endpoints. This is angular size; for stellar magnitude and parallax distance use a star-magnitude API and for sidereal time a sidereal API.
api.oanor.com/angularsize-api
Optical Fiber API
Optical-fibre photonics maths as an API, computed locally and deterministically. The numerical-aperture endpoint computes a step-index fibre's numerical aperture NA = √(n1² − n2²) from the core and cladding refractive indices, the acceptance angle θa = arcsin(NA) — the half-angle of the cone of light the fibre can capture — the full acceptance cone and the relative index difference Δ = (n1 − n2)/n1. The v-number endpoint computes the normalized frequency V = 2π·a·NA/λ from the core radius, the numerical aperture (or the indices) and the wavelength, classifies the fibre as single-mode when V is below the 2.405 cutoff or multimode above it, and gives the cutoff wavelength for single-mode operation. The modes endpoint estimates the number of guided modes — about V²/2 for a step-index fibre and V²/4 for a graded-index one — and confirms single-mode operation below the cutoff. Core radius and wavelength are in metres (1310 nm = 1.31×10⁻⁶ m) and refractive indices are dimensionless. Everything is computed locally and deterministically, so it is instant and private. Ideal for telecom, photonics, datacenter, sensor and laser app developers, fibre-link and waveguide-design tools, and optics education. Pure local computation — no key, no third-party service, instant. Live, nothing stored. 3 endpoints. This is optical-fibre guiding; for thin lenses and mirrors use a lens API and for refraction at a surface a Snell API.
api.oanor.com/fiber-api
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curl https://api.oanor.com/snell-api/SOME_PATH \
-H "x-oanor-key: oanor_test_..."
const res = await fetch("https://api.oanor.com/snell-api/SOME_PATH", {
headers: { "x-oanor-key": "oanor_test_..." }
});
const data = await res.json();
$ch = curl_init("https://api.oanor.com/snell-api/SOME_PATH");
curl_setopt($ch, CURLOPT_RETURNTRANSFER, true);
curl_setopt($ch, CURLOPT_HTTPHEADER, ["x-oanor-key: oanor_test_..."]);
$response = curl_exec($ch);
import requests
r = requests.get(
"https://api.oanor.com/snell-api/SOME_PATH",
headers={"x-oanor-key": "oanor_test_..."},
)
print(r.json())
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