Optical constants
Refractive index of Al2O3 (Aluminium sesquioxide, Sapphire, Alumina)
Hagemann et al. 1974: n,k 0.000775–0.207 µm
- Data
- tabulated nk
- Range
- 0.0007749–0.2066 µm
- Points
- 100
- Licence
- CC0-1.0
Plot
Click the plot to set the calculator wavelength.
At one wavelength
- Refractive index n
- 0.96937
- Extinction coefficient k
- 0.0345074
- Permittivity ε1
- 0.938488
- Permittivity ε2
- 0.0669009
- Absorption coefficient α
- 341443 cm⁻¹
- Penetration depth δ = λ/(2πk)
- 58.5749 nm
- Abbe number Vd
- —
- Chromatic dispersion dn/dλ
- 7.40741 µm⁻¹
- Group index ng
- 0.875296
- Group velocity dispersion
- — fs²/mm
- Dispersion parameter D
- — ps/(nm·km)
- Photon energy
- 97.6254 eV
ε = (n + ik)², α = 4πk/λ, ng = n − λ dn/dλ, GVD = λ³/(2πc²) d²n/dλ², D = −(λ/c) d²n/dλ². Group-velocity dispersion is given for formula data only.
Use it in Lightsmith
Load this data in Python, simulate in one more line
pip install lightsmith
import lightsmith as ls
# Al2O3 (Aluminium sesquioxide, Sapphire, Alumina): Hagemann et al. 1974: n,k 0.000775–0.207 µm
al2o3 = ls.fetch_refractiveindex("main", "Al2O3", "Hagemann", ref="c5c2f188e848453def5970e347399d653df2ffc2")
print(al2o3.range_nm) # (0.7749, 206.6) nm
eps = al2o3.eps([12.7]) # complex permittivity
Downloads the original record once (pinned to the imported snapshot) and caches it.
import json, urllib.request
import lightsmith as ls
url = "https://materials.lightsmith.dev/v1/datasets/ds_db79fbbe66b5/lightsmith"
al2o3 = ls.Tabulated.model_validate(json.load(urllib.request.urlopen(url)))
print(al2o3.source) # citation and provenance travel with the data
Any dataset here, as the library's Tabulated material (al2o3/hagemann-1974).
# ... load al2o3 as above, then:
sim = ls.Simulation(
particles=[ls.Particle(shape=ls.Sphere(radius_nm=50), material=al2o3)],
medium_index=1.0,
wavelengths=ls.WavelengthRange(start_nm=1, stop_nm=206, num=81),
)
res = ls.solve(sim) # exact Mie for a sphere
print(res.q_ext) # extinction efficiency at each wavelength
Same spec runs with DDA, FDTD, BEM or T-matrix: ls.compare(sim, ["mie", "dda"]).
Lightsmith is open source (MIT): Mie, T-matrix, BEM, DDA, FDTD, RCWA, TMM, mode solvers and inverse design behind one spec, on CPU or GPU. GitHub.
References
2) H.-J. Hagemann, W. Gudat, C. Kunz. DESY report SR-74/7 (1974)
- doi:10.1364/josa.65.000742 Optical constants from the far infrared to the x-ray region: Mg, Al, Cu, Ag, Au, Bi, C, and Al_2O_3, Journal of the Optical Society of America (1975)
Cite
H.-J. Hagemann, W. Gudat and C. Kunz. Optical constants from the far infrared to the x-ray region: Mg, Al, Cu, Ag, Au, Bi, C, and Al_2O_3. Journal of the Optical Society of America, 65, 742 (1975), doi:10.1364/josa.65.000742; H.-J. Hagemann, W. Gudat, C. Kunz. DESY report SR-74/7 (1974); Data from the refractiveindex.info database (M. N. Polyanskiy, Sci. Data 11, 94 (2024), doi:10.1038/s41597-023-02898-2)
Data
100 rows as published| λ (µm) | n | k |
|---|---|---|
| 0.0007749 | 1.0 | 9.14e-05 |
| 0.0007999 | 1.0 | 2.97e-05 |
| 0.0008266 | 1.0 | 3.4e-05 |
| 0.0008856 | 1.0 | 4.5e-05 |
| 0.001033 | 1.0 | 8.1e-05 |
| 0.00124 | 0.999 | 0.000161 |
| 0.00155 | 0.999 | 0.000349 |
| 0.002066 | 0.999 | 0.000977 |
| 0.002254 | 0.999 | 0.000809 |
| 0.00248 | 0.998 | 0.000402 |
| 0.0031 | 0.997 | 0.000729 |
| 0.003542 | 0.995 | 0.00124 |
| 0.004133 | 0.994 | 0.00181 |
| 0.004959 | 0.991 | 0.00326 |
| 0.006199 | 0.987 | 0.00533 |
| 0.006888 | 0.985 | 0.00709 |
| 0.007749 | 0.982 | 0.00977 |
| 0.008266 | 0.98 | 0.0113 |
| 0.008856 | 0.978 | 0.0133 |
| 0.008984 | 0.978 | 0.0135 |
| 0.009116 | 0.977 | 0.0139 |
| 0.009253 | 0.976 | 0.0143 |
| 0.009537 | 0.975 | 0.0156 |
| 0.00984 | 0.974 | 0.0171 |
| 0.009999 | 0.974 | 0.0181 |
| 0.01016 | 0.973 | 0.0183 |
| 0.01033 | 0.973 | 0.0185 |
| 0.01078 | 0.97 | 0.0204 |
| 0.01127 | 0.968 | 0.0233 |
| 0.01181 | 0.966 | 0.0275 |
| 0.0124 | 0.966 | 0.0332 |
| 0.01265 | 0.969 | 0.0346 |
| 0.01292 | 0.971 | 0.0341 |
| 0.01319 | 0.972 | 0.0314 |
| 0.01348 | 0.97 | 0.0291 |
| 0.01362 | 0.968 | 0.0284 |
| 0.01378 | 0.966 | 0.0286 |
| 0.01393 | 0.964 | 0.0295 |
| 0.01409 | 0.963 | 0.0307 |
| 0.01425 | 0.962 | 0.032 |
| 0.01442 | 0.962 | 0.033 |
| 0.01459 | 0.961 | 0.0337 |
| 0.01476 | 0.96 | 0.0343 |
| 0.01494 | 0.959 | 0.035 |
| 0.01512 | 0.957 | 0.0365 |
| 0.01531 | 0.956 | 0.0404 |
| 0.0154 | 0.958 | 0.0431 |
| 0.0155 | 0.961 | 0.0445 |
| 0.0156 | 0.965 | 0.043 |
| 0.01569 | 0.966 | 0.0398 |
| 0.01579 | 0.965 | 0.0372 |
| 0.0159 | 0.963 | 0.0363 |
| 0.016 | 0.963 | 0.0392 |
| 0.0161 | 0.967 | 0.0372 |
| 0.01621 | 0.966 | 0.0305 |
| 0.01631 | 0.961 | 0.0298 |
| 0.01642 | 0.958 | 0.0302 |
| 0.01653 | 0.957 | 0.0306 |
| 0.01664 | 0.955 | 0.0311 |
| 0.01675 | 0.953 | 0.0317 |
| 0.01698 | 0.951 | 0.0329 |
| 0.01722 | 0.948 | 0.0341 |
| 0.01771 | 0.944 | 0.0365 |
| 0.01907 | 0.933 | 0.0438 |
| 0.02066 | 0.92 | 0.0541 |
| 0.02254 | 0.907 | 0.0686 |
| 0.0248 | 0.892 | 0.0864 |
| 0.02755 | 0.872 | 0.111 |
| 0.031 | 0.848 | 0.148 |
| 0.03542 | 0.823 | 0.203 |
| 0.04133 | 0.794 | 0.282 |
| 0.04428 | 0.774 | 0.327 |
| 0.04769 | 0.748 | 0.393 |
| 0.05166 | 0.722 | 0.502 |
| 0.05636 | 0.765 | 0.651 |
| 0.05904 | 0.812 | 0.723 |
| 0.06048 | 0.841 | 0.747 |
| 0.06199 | 0.862 | 0.769 |
| 0.06358 | 0.88 | 0.794 |
| 0.06525 | 0.896 | 0.825 |
| 0.06888 | 0.947 | 0.912 |
| 0.07293 | 1.035 | 0.997 |
| 0.07749 | 1.148 | 1.07 |
| 0.08266 | 1.293 | 1.14 |
| 0.08551 | 1.379 | 1.16 |
| 0.08856 | 1.471 | 1.16 |
| 0.09184 | 1.555 | 1.17 |
| 0.09537 | 1.649 | 1.17 |
| 0.09919 | 1.753 | 1.17 |
| 0.1033 | 1.868 | 1.17 |
| 0.1078 | 2.017 | 1.16 |
| 0.1127 | 2.218 | 1.11 |
| 0.1181 | 2.484 | 0.951 |
| 0.124 | 2.582 | 0.597 |
| 0.1305 | 2.524 | 0.253 |
| 0.1378 | 2.297 | 0.0895 |
| 0.1459 | 2.153 | 0.0478 |
| 0.155 | 2.058 | 0.028 |
| 0.1771 | 1.924 | 0.00824 |
| 0.2066 | 1.774 | 0.0022 |
Optical transmission calculator
Free-standing sample in vacuum, normal incidence- Transmittance T
- —
- Reflectance R
- —
Fresnel reflection calculator
- Rp
- —
- Rs
- —
- R = (Rp+Rs)/2
- —
- Phase φp
- —
- Phase φs
- —
- Brewster angle θB
- —
- Critical angle θC
- —