User's Manual
®
Ocean Optics with Xplorer GLX Measurements
8
Absorbance
The GLX uses this equation to evaluate each pixel on the detector and
produce the absorbance spectrum:
Where:
S
λ
= Sample intensity at wavelength λ
D
λ
= Dark intensity at wavelength λ
R
λ
= Reference intensity at wavelength λ (acquired with a blank
cuvette in place)
Absorbance is not a valid quantity if either or is
less than zero. This condition may occur if the test solution or the refer-
ence solution is very dark.
Transmission
The GLX calculates the transmission of a solution using this equation:
Rel. Irradiance
Relative irradiance is a comparison of the fraction of energy a sample
emits and the energy the spectrometer collects from a lamp with a black-
body energy distribution (normalized to 1 at the energy maximum).
To measure the relative irradiance of a sample, you must save the refer-
ence scan using a lamp of known color temperature and enter the color
temperature under the Lamp tab of the configuration screen.
The GLX calculates relative irradiance with this equation:
Where:
B
λ
= Relative energy of the reference (calculated from the color
temperature) at wavelength λ
S
λ
= Sample intensity at wavelength λ
D
λ
= Dark intensity at wavelength λ
R
λ
= Reference intensity at wavelength λ
A
λ
log
10
–
S
λ
D
λ
–
R
λ
D
λ
–
-------------------
=
S
λ
D
λ
–()R
λ
D
λ
–()
%T
λ
S
λ
D
λ
–
R
λ
D
λ
–
-------------------
100%×=
I
λ
B
λ
S
λ
D
λ
–
R
λ
D
λ
–
-------------------
=










