LIBS Info: Element Analysis

Title Authors Material Detector Spectrometer Software
Analysis of heavy metals in soils using laser-induced breakdown spectrometry combined with laser-induced fluorescence Frank Hilbk-Kortenbruck, Reinhard Noll, Peter Wintjens, Heinz Falk, Christoph Becker Soil Photomultiplier Spectrolab M
Laser: Nd:YAG
1064.0000nm
450.0000mJ
10.000Hz
Gate Delay: 1.000us
Gate Width: 20.000us
Use a commercial Paschen-Runge spectrometer with dedicated photomultipliers for each wavelength of interest. Calibration samples prepared by spiking a standard soil with different metal salts. This was then dried, ground and pressed (with wax binder) into pellets. In addition, Laser Induced Fluorescence of the LIBS plasma produced significantly lower detection limits (0.3ppm for Cd and 0.5ppm for Tl)
Element Detection Limit (ppm) Wavelength (nm) Other Wavelengths (nm) Calibration Method Calibration Range (ppm) Notes
As 3.3000 (Stated) 235.0000 N/A Univariate Calibration -10.0000--10.0000 Experiment conducted in Ar atmosphere. No normalisation/ratioing used as the same soil was the base for all samples, with the only difference being the metal salt spiking to produce the required concentration
Cd 6.0000 (Stated) 228.8000 N/A Univariate Calibration -10.0000--10.0000 Experiment conducted in Ar atmosphere. No normalisation/ratioing used as the same soil was the base for all samples, with the only difference being the metal salt spiking to produce the required concentration. Using LIF on the LIBS plasma realised a detection limit of 0.3ppm
Cr 2.5000 (Stated) 425.4000 N/A Univariate Calibration -10.0000--10.0000 Experiment conducted in Ar atmosphere. No normalisation/ratioing used as the same soil was the base for all samples, with the only difference being the metal salt spiking to produce the required concentration
Cu 3.3000 (Stated) 324.8000 N/A Univariate Calibration -10.0000--10.0000 Experiment conducted in Ar atmosphere. No normalisation/ratioing used as the same soil was the base for all samples, with the only difference being the metal salt spiking to produce the required concentration
Hg 84.0000 (Stated) 253.7000 N/A Univariate Calibration -10.0000--10.0000 Experiment conducted in Ar atmosphere. No normalisation/ratioing used as the same soil was the base for all samples, with the only difference being the metal salt spiking to produce the required concentration.
Ni 6.8000 (Stated) 231.6000 N/A Univariate Calibration -10.0000--10.0000 Experiment conducted in Ar atmosphere. No normalisation/ratioing used as the same soil was the base for all samples, with the only difference being the metal salt spiking to produce the required concentration
Pb 17.0000 (Stated) 405.8000 N/A Univariate Calibration -10.0000--10.0000 Experiment conducted in Ar atmosphere. No normalisation/ratioing used as the same soil was the base for all samples, with the only difference being the metal salt spiking to produce the required concentration
Tl 48.0000 (Stated) 351.9000 N/A Univariate Calibration -10.0000--10.0000 Experiment conducted in Ar atmosphere. No normalisation/ratioing used as the same soil was the base for all samples, with the only difference being the metal salt spiking to produce the required concentration. Using LIF on the LIBS plasma resulted in a LOD of 0.5ppm
Zn 98.0000 (Stated) 334.5000 N/A Univariate Calibration -10.0000--10.0000 Experiment conducted in Ar atmosphere. No normalisation/ratioing used as the same soil was the base for all samples, with the only difference being the metal salt spiking to produce the required concentration


Element RMSE (ppm) Wavelength (nm) Calibration Method Notes