Masters Thesis - Phenolics in Australian Grain Crops

Published: 17 February 2022| Version 1 | DOI: 10.17632/8bb2d725sd.1
Contributor:
Joel Johnson

Description

The NIR and MIR datasets contain sample information, chemical reference data and the mean NIR/MIR spectra for each sample. The x-axis variables across the top of the NIR datasets are provided in nm; MIR data in cm-1. CUPRAC, FRAP, TP and TMA values are given as mg/100 g. Moisture and protein are in % w/w. Starch, amylose, amylopectin, vicine, convicine and total VC are in mg/g. The phenolic_contents datasets show the results from HPLC analysis of individual phenolic compounds present in each sample. The content of individual phenolic acids are given in mg/kg. All measurements are expressed on an oven-dried weight basis. Abbreviations used: HKW = hundred kernel weight CUPRAC = cupric reducing antioxidant capacity FRAP = ferric reducing antioxidant potential TP = total phenolic content TMA = total monomeric anthocyanin content Total_VC = sum of vicine and convicine contents

Files

Steps to reproduce

Chemical analysis was conducted following protocols previously published by our laboratory (DOI: 10.1002/leg3.28). Near-infrared spectra were collected from the flour samples using an Antaris II FT-NIR Analyzer (Thermo Scientific; USA). The instrument was operated in reflectance mode, using the integrating sphere with a rotating sample cup (30 mm diameter). Spectra were collected between 1000-2500 nm (10,000-4,000 cm-1), as the mean of 32 scans (resolution of 8 cm-1). Spectra were collected in triplicate, repacking the sample cup with fresh flour each time. Spectra were exported in *.csv format, with the mean of the triplicate spectra for each sample used in subsequent analysis. Mid-infrared spectra were collected from the flour samples using a Bruker Alpha FTIR (Fourier transform infrared) spectrophotometer (Bruker Optics Gmbh, Ettlingen, Germany) fitted with a platinum diamond ATR single reflection module. Air was used as a reference background; the background measurement was performed every 10 samples. MIR spectra were recorded between 4000 and 400 cm-1 using the OPUS software version 7.5 (Bruker Optics Gmbh, Ettlingen, Germany) as the average of 24 scans at a resolution of 4 cm-1. Replicate spectra were collected from each sample (3 for mungbean and chickpea and 5 for faba bean and wheat), repacking the instrument with fresh flour each time. The mean of these replicate scans were used in subsequent analysis.

Institutions

Central Queensland University

Categories

Wheat, Fourier Transform Infrared Spectroscopy, Near Infrared Spectroscopy, Phenolic Acids, Grain Science, Grain Legume

Licence