scholarly journals Monitoring Soil Surface Mineralogy at Different Moisture Conditions Using Visible Near-Infrared Spectroscopy Data

2019 ◽  
Vol 11 (21) ◽  
pp. 2526
Author(s):  
Irena Ymeti ◽  
Dhruba Pikha Shrestha ◽  
Freek van der Meer

The soil minerals determine essential soil properties such as the cation exchange capacity, texture, structure, and their capacity to form bonds with organic matter. Any alteration of these organo-mineral interactions due to the soil moisture variations needs attention. Visible near-infrared imaging spectroscopy is capable of assessing spectral soil constituents that are responsible for the organo-mineral interactions. In this study, we hypothesized that the alterations of the surface soil mineralogy occur due to the moisture variations. For eight weeks, under laboratory conditions, imaging spectroscopy data were collected on a 72 h basis for three Silty Loam soils varying in the organic matter (no, low and high) placed at the drying-field capacity, field capacity and waterlogging-field capacity treatments. Using the Spectral Information Divergence image classifier, the image area occupied by the Mg-clinochlore, goethite, quartz coated 50% by goethite, hematite dimorphous with maghemite was detected and quantified (percentage). Our results showed these minerals behaved differently, depending on the soil type and soil treatment. While for the soils with organic matter, the mineralogical alterations were evident at the field capacity state, for the one with no organic matter, these changes were insignificant. Using imaging spectroscopy data on the Silty Loam soil, we showed that the surface mineralogy changes over time due to the moisture conditions.

Author(s):  
Roger N. Clark ◽  
Carlé M. Pieters ◽  
Robert O. Green ◽  
J. W. Boardman ◽  
Noah E. Petro

2008 ◽  
Vol 56 (10) ◽  
pp. 1385-1390 ◽  
Author(s):  
Jeremy Bailey ◽  
S. Chamberlain ◽  
D. Crisp ◽  
V.S. Meadows

2013 ◽  
Vol 556 ◽  
pp. A136 ◽  
Author(s):  
C. Iserlohe ◽  
A. Krabbe ◽  
J. E. Larkin ◽  
M. Barczys ◽  
M. W. McElwain ◽  
...  

2001 ◽  
Vol 18 (1) ◽  
pp. 41-57 ◽  
Author(s):  
Peter J. McGregor ◽  
Michael Dopita ◽  
Peter Wood ◽  
Michael G. Burton

AbstractThe Near-infrared Integral Field Spectrograph (NIFS) will beAustralia’s first Gemini instrument. NIFS is a near-infrared, imaging spectrograph that will be used with the ALTAIR facility adaptive optics system on Gemini North to perform near-diffraction-limited imaging spectroscopy over a 3·0″ × 3·0″ field of view with 0·1″ wide slitlets and a spectral resolving power of ˜5300. NIFS will operate in the wavelength range from 0·94–2·50 µm where ALTAIR delivers its greatest gains. Its primary purpose is to study moderate-surface-brightness structures around discrete objects that are revealed at high spatial resolution by ALTAIR. NIFS will address a wide range of science from studies of Galactic star formation and the Galactic centre to the nature of disk galaxies at z ˜ 1. Studies of the demographics of massive black holes in galactic nuclei and studies of the excitation conditions in the inner narrow-line regions of Seyfert galaxies have been identified as two core NIFS programs. These and other science drivers for NIFS are discussed.


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