Disclaimer: use at your own risk. Help available at the bottom of this page.
Extinction and scattering spectra for a core-shell particle are calculated
using the Mie theory.
The core and the shell of the spherical particle are defined by their
external radii and compositions (or refractive indices if material
n
is chosen).
The embedding medium is defined by its
refractive index.
Qext, Qabs and Qsca are calculated and
are respectively the extinction, absorption and scattering cross-sections divided by
πR2 where R is the external radius of the core-shell sphere.
You can zoom the plot by selecting a rectangle and zoom out using
the lower left icon. The plot can also be resized using the lower
right icon. The calculated values are available when clicking the
DAT
icon.
Some optical constants are pre-defined but you can enter your own ones. For example, you can visit refractiveindex.info, choose the material you are interested in and download the data by using the “Full database record” link. Then select the “table” option of the “user-defined” group in the drop-down list for the core or the shell and import the file or paste the data in the text area. Finally select the correct unit for the first column and click the “Apply” button.
Interpolation of the optical constants is accomplished using the monotone cubic interpolation method.
The refractive indices (n and k) may depend on the wavelength l in
micrometer. For example, according to
doi:10.1364/AO.46.003811
for water at 24°C you may use:
sqrt(1+5.66695982e-1*l*l/(l*l-5.084151894e-3)+1.731900098e-1*l*l/(l*l-1.818488474e-2)+2.095951857e-2*l*l/(l*l-2.625439472e-2)+1.125228406e-1*l*l/(l*l-1.073842352e1))
and according to
doi:10.1039/C7NR02952G
for PVA you may use:
1.460+0.00665/l/l