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Article
SMOS Optical Thickness Changes in Response to the Growth and Development of Crops, Crop Management, and Weather
Remote Sensing of Environment
  • Brian K. Hornbuckle, Iowa State University
  • Jason C. Patton, Iowa State University
  • Andy VanLoocke, Iowa State University
  • Andrew E. Suyker, University of Nebraska - Lincoln
  • Matthew C. Roby, Iowa State University
  • Victoria A. Walker, Iowa State University
  • Eswar R. Iyer, Iowa State University
  • Daryl E. Herzmann, Iowa State University
  • Erik A. Endacott, Iowa State University
Document Type
Article
Publication Version
Submitted Manuscript
Publication Date
7-1-2016
DOI
10.1016/j.rse.2016.02.043
Abstract
The Soil Moisture and Ocean Salinity (SMOS) remote sensing satellite was launched by the European Space Agency in 2009. The L-band brightness temperature observed by SMOS has been used to produce estimates of both soil moisture and τ, the optical thickness of the land surface. Although τ should theoretically be proportional to the amount of vegetation present within a SMOS pixel, several initial investigations have not been able to confirm this expected behavior. However, when the noise in the SMOS τ product is removed, τ in the U.S. Corn Belt, a region of extensive row-crop agriculture, has a distinct shape that mirrors the growth and development of crops. We find that the peak value of SMOS τ occurs at approximately 1000 °C day (base 10 °C) growing degree days after the mean planting date of maize (corn). We can explain this finding in the following way: τ is directly proportional to the water column density of vegetation; maize contributes the most to growing season changes in τ in the Corn Belt; and maize reaches its maximum water column density at its third reproductive stage of development, at about 1000 °C day growing degree days. Consequently, SMOS τ could be used to monitor the phenology of crops in the Corn Belt at a spatial resolution similar to a U.S. county and a temporal frequency on the order of days. We also examined the magnitude of the change in SMOS τ over the growing season and hypothesized it would be related to the amount of accumulated solar radiation, but found this not to be the case. On the other hand, the change in magnitude was smallest for the year in which the most precipitation fell. These findings are rational since SMOS τ at the satellite scale is in fact a function of both vegetation and soil surface roughness, and soil surface roughness is reduced by precipitation. To fully explain changes in SMOS τ in the Corn Belt it appears that it will be necessary to use in situ and remotely-sensed observations along with agro-ecosystem models to account for land management decisions made by farmers that affect changes in soil surface roughness and all of the relevant biophysical processes that affect the growth and development of crops.
Comments

This is a manuscript of an article from Remote Sensing of Environment 180 (2016): 320, doi: 10.1016/j.rse.2016.02.043. Posted with permission.

Rights
This manuscript version is made available under the CC-BY-NC-ND 4.0 license http://creativecommons.org/licenses/by-nc-nd/4.0/
Copyright Owner
Elsevier Inc.
Language
en
File Format
application/pdf
Citation Information
Brian K. Hornbuckle, Jason C. Patton, Andy VanLoocke, Andrew E. Suyker, et al.. "SMOS Optical Thickness Changes in Response to the Growth and Development of Crops, Crop Management, and Weather" Remote Sensing of Environment Vol. 180 (2016) p. 320 - 333
Available at: http://works.bepress.com/andy_vanloocke/23/