EVASKY S87
1 dataset, together covering 0.25–2.5 µm. Default: Vogt et al. 2016: n,k 0.25–2.5 µm.
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Use it in Lightsmith
Load this data in Python, simulate in one more line
pip install lightsmith
import lightsmith as ls
# EVASKY S87: Vogt et al. 2016: n,k 0.25–2.5 µm
evasky_s87 = ls.fetch_refractiveindex("other", "EVASKY_S87", "Vogt", ref="c5c2f188e848453def5970e347399d653df2ffc2")
print(evasky_s87.range_nm) # (250, 2500) nm
eps = evasky_s87.eps([633]) # 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_f072e7533cb9/lightsmith"
evasky_s87 = ls.Tabulated.model_validate(json.load(urllib.request.urlopen(url)))
print(evasky_s87.source) # citation and provenance travel with the data
Any dataset here, as the library's Tabulated material (evasky-s87/vogt-2016).
# ... load evasky_s87 as above, then:
sim = ls.Simulation(
particles=[ls.Particle(shape=ls.Sphere(radius_nm=50), material=evasky_s87)],
medium_index=1.0,
wavelengths=ls.WavelengthRange(start_nm=400, stop_nm=1000, 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.
About EVASKY S87
Other names: EVASKY_S87
API: /v1/materials/mat_3513fa7f21c5 · slug evasky-s87