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APPLICATION NOTE NO. 11QSP-PD
Calculating Calibration Coefficients for Biospherical Instruments PAR Light Sensor without Built-In Log Amplifier
Revised February 2010

Print version

This application note applies to the following current output Biospherical Instruments PAR light sensors:

* Note: Biospherical’s 2200 series includes other instruments which are not compatible with Sea-Bird CTDs. Only the 2200 (PD) sensors can be integrated with Sea-Bird CTDs.

These PAR sensors are compatible with the following Sea-Bird CTDs:

The current output of these sensors is measured through a log amplifier in your CTD (or through the PN 90310 Log Amp Module) to obtain adequate resolution over the measurement range. SEASOFT computes PAR using the following equation:

PAR = [multiplier * (109 * 10(V-B) / M) / calibration constant] + offset

Enter the following coefficients in the CTD configuration file:

M = slope of log amplifier   (Note 2)

B = offset of log amplifier   (Note 2)

calibration constant CS = 6.022 x 10 13 / CW   (Note 3)

multiplier = 1.0 for output units of microEinsteins/m2 sec   (Note 4)

offset = 0, typically   (Note 5)

Notes:

  1. In our SEASOFT V2 suite of programs, edit the CTD configuration (.con or .xmlcon) file using the Configure Inputs menu in Seasave V7 (real-time data acquisition software) or the Configure menu in SBE Data Processing (data processing software).
  2. Sea-Bird provides two calibration sheets for the PAR sensor in the CTD manual:
  1. For calculation of CW and CS, see Mathematical Derivation below.
  2. The multiplier can be used to calculate irradiance in units other than μEinsteins/m2.sec. See Application Note 11General for multiplier values for other units.
    The multiplier can also be used to scale the data, for purposes of comparing the shape of data sets taken at disparate light levels. For example, a multiplier of 10 would make a 10 μEinsteins/m2.sec light level plot as 100 μEinsteins/m2.sec.
  3. Offset may be used to offset the data by a constant, if field data indicates a drift in the sensor. To calculate the offset:
    Enter M, B, calibration constant, and multiplier, and set offset = 0 in the configuration (.con or .xmlcon) file. With the sensor dark (covered), display the calculated PAR output in Seasave V7; then enter the negative of this reading as the offset in the configuration file.

 

Mathematical Derivation

CW = Biospherical wet calibration factor from Biospherical calibration sheet [(quanta/cm2.sec) / nAmp]

Output in water from Biospherical calibration sheet (quanta/cm2.sec) = CW * probe output (nAmp)

Output in water (quanta/cm2.sec) = CW * 10 9 * probe output (Amp)

I = probe output (Amp)

Output in water (quanta/cm2.sec) = CW * 10 9 * I

Output in water (quanta/m2.sec) = CW * 10 9 * I * 10 4 = CW * 10 13 * I

Output in water (μEinsteins/ m2.sec) = CW * 10 13 * I / 6.022 x 10 17
(see Application Note 11General for conversion from quanta to μEinsteins)

SEASOFT calculates: Light (μEinsteins/ m2.sec) = I x 10 9 / CS
where CS = calibration constant

Equating the Biospherical and SEASOFT relationships:

CW * 10 13 * I / 6.022 x 10 17 = I x 109 / CS
CW / 6.022 x 10 13 = 1 / CS
CS = 6.022 x 10 13 / CW

 

Example:

CW = Biospherical wet calibration factor from Biospherical calibration sheet = 4.77 x 10 14 (quanta/cm2.sec) / nAmp

Calibration constant CS = 6.022 x 10 13 / CW = 6.022 x 10 13 / 4.77 x 10 14 = 0.126 (for entry into .con or .xmlcon file)

Notes:

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Last modified: 05-May-2010

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