Contents

Title: Mayberry - NDVI (SRS, Planet)
Date:2017-06-06 - 2021-04-15
Data File: MB_NDVI.csv
Refers to:MB,2046503376,2046503354

Various sensors measuring NDVI have been installed across the Delta sites over the last several years. At some sites, the SRS sensors from Decagon/METER have been drifting low, so I wanted to compare them with other NDVI measurements.

  • SRS sensor (Decagon/METER): A pair of photodiodes with cosine correcting Teflon diffuser and hemispherical view. Red band is measured at 650nm and NIR band is measured at 810nm.
  • SR-411 sensor (Apogee): A pair of photodiodes with acrylic diffuser and hemispherical view. Red band is measured at 650nm and NIR band is measured at 810nm.
  • Planet Labs data: L3H (CESTEM) alpha data product. Pixel size is 3m, and there are daily gap-filled images from 2018-2020. Gap fills are done with Planet imagery from the day before and after, combined with daily MODIS data. From the full image, Joe cut out a 730mx730m tile for each site, centered on the tower. Product includes NDVI, GCC, ECI, and the following reflectances: red, NIR, green, blue. For more information, see Box/Biometlab/Remote_Sensing/PlanetLabs/L3H_distribution_lodi_islands_readme.pdf.
  • Broadband NDVI: NDVI calculated using reflected SW and PAR data from the tower, called "broadband" because it uses the broader bands of shortwave and PAR radiation rather than the narrow bands of the SRS and Apogee sensors. See Huemmrich et al., 1999 in Journal of Geophysical Research: Atmospheres and Tittebrand et al., 2009 in Theoretical and Applied Climatology.

For some sites with I also compared GCC with the various NDVI values to see how much GCC values varied year over year. Photos were taken by a variety of cameras: Netcam Stardot cameras (the official camera of the Phenocam Network®), Canon point-and-shoot cameras with custom firmware, or a Raspberry Pi camera.

I used Joe's datafetch tool to calculate daily average mid-day values of NDVI and GCC from the various sensors. Mid-day values included data from 11:00 to 13:00, 5 values a day. I despiked the data in Excel.

  • NDVI = (NIR-Red)/(NIR+Red)
  • GCC = (Green)/(Red + Green + Blue)
  • Broadband NDVI = (rho_NIR-rho_PAR)/(rho_NIR+rho_PAR)
    • rho_NIR= (SWout-PARout)/(SWin-PARin)
    • rho_PAR=(PARout/PARin)
    • Units of both SW and PAR should be in W/m2. Use the conversion 4.6 umol/m2/s = 1 W/m2 to convert the usual PAR units (umol/m2/s) to W/m2.

See reports for other Delta sites here:

Bouldin Alfalfa

Bouldin Corn

East End

East Pond / Sherman Wetland Temp Tower (both sites had same set of SRS sensors)

Mayberry

Sherman Wetland

Twitchell Alfalfa / Sherman Barn (both sites had same set of SRS sensors)

 West Pond

 

Site SRS sensor (incoming/outgoing) Conclusion
Mayberry sn 2046503376 / sn 2046503354

At Mayberry, SRS NDVI data looks ok. No correction needed.

 

Figure 1. Time series of NDVI data at Mayberry. SRS values do not have any obvious decay, although it has NDVI values that are consistently about 0.3 lower than PL or broadband NDVI.

 

Figure 2. Time series of individual SRS bands. Seasonal maxes seem reasonable; no obvious decay.

 

Figure 3. Red reflectance. SRS has a consistently higher red reflectance than PL reflectance. Maybe SRS reflectance is increasing year after year.

 

Figure 4. NIR reflectance. Very similar magnitude for SRS and PL data.

 

Regression Data

Residuals

Figure 5. NDVI linear regression. PL and broadband NDVI have similar fits with R2 from 0.85 to 0.87.

 

Figure 6.  Mayberry GCC data compared with SRS data. GCC_13-15 is the average GCC from 13:00 to 15:00, and GCC_11-13 is the average GCC from 11:00 to 13:00. They both match well with the SRS NDVI data over the last 4 years, although GCC seems to peak in June/July while the SRS NDVI seems to peak a little later in September.

 

Regression Data

Residuals

Figure 7. NDVI-GCC regression with GCC 11:00-13:00. R2 ranges from 0.64 to 0.78; PL has the best fit with R2=0.78.

 

Figure 8. NDVI-GCC regression with GCC 13:00-15:00. All 3 NDVI series have similar R2 values (ranging from 0.77 to 0.80; PL has the best fit with R2=0.80). There is a larger difference than I expected in R2 between the sets of GCC data. GCC_13-15 has more points at the upper end of the GCC range (and it also has more points overall), which may explain its higher R2 value