We did not have the opportunity to calibrate the pyrgeometers prior to the start of PCAPS, and therefore used old thermopile calibration factors for the Kipp & Zonen CG4 and Eppley PIR pyrgeometers.  These were subsequently recalibrated in the NOAA black body on March 8 & 10, 2011.  The following table lists multiplicative correction factors for Rpile outputs during the PCAPS field program.

Sensor

Location

Position

Pre-ops

Post-ops

Correction

k*

 

 

 

uV-m^2/W

uV-m^2/W

pre/post

 

PIR 031980

Playa (1)

in

3.58

3.58

1.000

4.0

PIR 031976

Playa

out

3.93

3.74

1.051

3.5

PIR 031975

ABC (2)

in

3.97

3.98

0.997

3.5

PIR 031978

ABC

out

3.50

3.53

0.992

4.0

CG4 050824

Highland (3)

in

14.09

13.81

1.020

NA

CG4 040740

Highland

out

7.85

7.76

1.012

NA

CG4 030675

West Valley (4)

in

9.97

9.93

1.004

NA

CG4 040741

West Valley

out

8.82

8.76

1.007

NA

PIR 031979

East Slope (5)

in

3.99

3.81

1.047

4.5

PIR 031981

East Slope

out

3.69

3.66

1.008

3.5

CG4 100225

West Slope (6)

in

11.93

11.28

1.058

NA

CG4 100226

West Slope

out

11.51

10.81

1.065

NA

CG4 050823

Riverton (7)

in

9.32

9.21

1.012

NA

CG4 030676

Riverton

out

11.27

11.21

1.005

NA

*per Ellsworth Dutton, blackbody values for k have been increased by 0.3 and then rounded up to nearest 0.5