Fiber Optic Oxygen Sensors — How Do They Work?

For a given media, and at a constant total pressure and temperature, the partial pressure of oxygen is proportional to oxygen mole fraction.

The Stern-Volmer constant (k) is primarily dependent on the chemical composition of the sensor formulation. Our probes have shown excellent stability over time, and this value should be largely independent of the other parts of the measurement system. However, the Stern-Volmer constant (k) does vary among probes, and it is temperature dependent. All measurements should be made at the same temperature as the calibration experiments or temperature monitoring devices should be used.

If you decide to compensate for temperature, the relationship between the Stern-Volmer values and temperature is defined as:

I0 = a0 + b0 * T + c0 * T2
k = a + b * T + c * T2

The intensity of fluorescence at zero pressure of oxygen (I0) depends on details of the optical setup: the power of the LED, the optical fibers, loss of light at the probe due to fiber coupling, and backscattering from the sample. It is important to measure the intensity of fluorescence at zero pressure of oxygen (I0) for each experimental setup.

It is evident from the equation that the sensor will be most sensitive to low levels of oxygen. The photometric signal-tonoise ratio is roughly proportional to the square root of the signal intensity. The rate of change of signal intensity with oxygen concentration is greatest at low levels. Deviations from the Stern-Volmer relationship occur primarily at higher oxygen concentration levels. Using the second order polynomial algorithm when calibrating corrects these deviations.

Backscattering in the media can increase the collection efficiency of the probe, increasing the observed fluorescence. It is important to perform calibration procedures in the media of interest for highly scattering substances. For optically clear fluids and gases, this is unnecessary.

Second Order Polynomial Algorithm

The second order polynomial algorithm requires at least three standards of known oxygen concentration. The first standard must have 0% oxygen concentration and the last standard must have a concentration in the high end of the concentration range in which you will be working. The second order polynomial algorithm is considered to provide more accurate data because it requires at least three known concentration standards while the Linear (Stern- Volmer) algorithm requires a minimum of two known concentration standards. The second order polynomial algorithm is defined as:

I0 is the fluorescence intensity at zero concentration
I is the intensity of fluorescence at a pressure p of oxygen
K1 is the first coefficient
K2 is the second coefficient

If you decide to compensate for temperature, the relationship between the second order polynomial algorithm and temperature is defined as:

I0 = a0 + b0 * T + c0 * T2
K1 = a1 + b1 * T + c1 * T2
K2 = a2 + b2 * T + c2 * T2

Henry's Law

It is possible to calibrate the system in gas and then use the probe in liquid or vice versa. In theory, your sensor probe detects the partial pressure of oxygen. In order to convert partial pressure to concentration, you can use Henry's Law. When the temperature is constant, the weight of a gas that dissolves in a liquid is proportional to the pressure exerted by the gas on the liquid. Therefore, the pressure of the gas above a solution is proportional to the concentration of the gas in the solution. The concentration (mole %) can be calculated if the absolute pressure is known:

Oxygen mole fraction = oxygen partial pressure / absolute pressure

Since the sensor detects partial pressure of oxygen, the response in a gas environment is similar to a liquid environment in equilibrium with gas. Therefore, it is possible to calibrate the sensor in gas and then use the system with liquid samples and vice versa if you utilize Henry's Law.

However, Henry's Law does not apply to gases that are extremely soluble in water. The following information illustrates the solubility of oxygen in water at different temperatures.

ln(X)=a+b/T*+ cln (T*)

Temperature range: 0°C - 75°C
X=mole fraction
T* = T/100 in Kelvin
a = -66.7354
b = 87.4755
c = 24.4526

Scattering Media

Fluorescence emissions from the sensor formulation propagate in all directions. In clear media, only those emissions propagating toward the fiber within the acceptance angle of the probe are detected. If the probe tip is held near a reflecting surface, or immersed in a highly scattering media, the fluorescence signal will increase. The increase will be proportional for both the intensity of the fluorescence at a pressure of oxygen and the intensity of fluorescence at zero pressure of oxygen, but will not affect the Stern- Volmer constant. For this reason, it is necessary to measure the intensity of fluorescence at zero pressure of oxygen in the sample. Also, if you are measuring oxygen in highly scattering media, then the standards you use for your calibration procedure should be in the same media as your sample for the most accurate results.

This article was written by Monde Qhobosheane, Ph.D., Field Sales Engineer, Ocean Optics (Dunedin, FL). For more information, contact Dr. Qhobosheane at This email address is being protected from spambots. You need JavaScript enabled to view it., or visit http://info.hotims.com/40433-200.


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