Precise Yield Estimation through Improvised CASA Model by Development of Soil and Atmospheric Constants (Sᵮ) and (Aþ)
Rao Mansor Ali Khan* and Syed Amer Mahmood
Department of Space Science, University of the Punjab, Lahore, Pakistan.
*Correspondence | Rao Mansor Ali Khan, Department of Space Science, University of the Punjab, Lahore, Pakistan; Email:
[email protected]
Figure 1:
(a) Map of Punjab, Pakistan; (b) Investigation site (c) Spatial extent of the study area.
Figure 2:
Flowchart of methodology.
Figure 3:
Variations recorded in LAI on various dates with a temporal resolution of five days throughout the WGP.
Figure 5:
Variations in (n/N) throughout the WGP.
Figure 6:
Variations in Go for the complete WGP.
Figure 7:
Variation in λE and H throughout WGP.
Figure 8: Variation in W throughout the WGP.
Figure 9: Variations in LUE throughout the WGP.
Figure 10:
Variations in ‘f’ throughout the WGP.
Figure 11:
Variation in biomass throughout the WGP.
Figure 12:
Spatio temporal variations in PAR (Wm−2), NDVI, APAR (Wm−2) and biomass generation (g/m2).
Figure 13: Variation in BC values throughout WGP.
Figure 14: Variation in CO values throughout WGP.
Figure 15: Variation in NO2 values of different atmospheric pollutants.
Figure 16: Variation in O3 values throughout WGP.
Figure 18:
(A) Wheat yields spatial distribution; (B) Wheat cultivation mask; (C) Integration of yield distribution with wheat cultivation mask.
Figure 4:
Variations in extraterrestrial radiation (Ra); clear sky radiation (Rso); actual incoming radiation (Rs); net radiation (Rn); net longwave radiation (Rnl) and net shortwave radiation (Rns) throughout the WGP.
Figure 17:
Variation in SO2 values throughout WGP.