Skip to main content

ri_ammonium_sulfate

Constants

Ammonium sulfate aerosol ("(NH4)2SO4") complex refractive index m = n + i k, wavelength in nm. Assumptions: dry crystalline aerosol surrogate for continental haze; ~300 K; morphology not modeled. Guidance/sources (composite, smoothed for Mie with linear interpolation):

  • Toon, Pollack & Khare (1976); d'Almeida et al. (1991); Hess et al. (1998, OPAC) — visible/NIR anchors (n≈1.52, k≈0).
  • Palmer & Williams (1975) optical constants compendium; Querry (1985/1991) — UV and MIR/LWIR band behavior. Notes:
  • In the visible, k is extremely small (≈1e-6–1e-5). We use small nonzero values to avoid divide-by-zero corner cases.
  • MIR bands associated with sulfate and ammonium groups raise k around ~3 µm (weak) and ~7–10 µm (stronger).
  • Coverage: 200–20,000 nm; denser sampling near MIR bands.

Functions

🌫️ Ammonium sulfate (continental haze surrogate)

AMMONIUM_SULFATE_REFRACTION_INDEX_LUT

Ammonium sulfate aerosol ("(NH4)2SO4") complex refractive index m = n + i k, wavelength in nm. Assumptions: dry crystalline aerosol surrogate for continental haze; ~300 K; morphology not modeled. Guidance/sources (composite, smoothed for Mie with linear interpolation):

  • Toon, Pollack & Khare (1976); d'Almeida et al. (1991); Hess et al. (1998, OPAC) — visible/NIR anchors (n≈1.52, k≈0).
  • Palmer & Williams (1975) optical constants compendium; Querry (1985/1991) — UV and MIR/LWIR band behavior. Notes:
  • In the visible, k is extremely small (≈1e-6–1e-5). We use small nonzero values to avoid divide-by-zero corner cases.
  • MIR bands associated with sulfate and ammonium groups raise k around ~3 µm (weak) and ~7–10 µm (stronger).
  • Coverage: 200–20,000 nm; denser sampling near MIR bands.

Kind: global constant

ri_ammonium_sulfate(result, wavelength_nm)

🌫️ Ammonium sulfate (continental haze surrogate)

Kind: global function

ParamTypeDescription
resultArray.<number>complex number, refraction index
wavelength_nmnumberin nanometers