2015
DOI: 10.1002/2015gl064678
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Grain growth and transformation of pedogenic magnetic particles in red Ferralsols

Abstract: Soil magnetism depends on the mineral composition and grain size distribution of magnetic particles. The accumulation of magnetic particles with different grain sizes has been found in the laboratory to precede the formation of hematite (Hm), which competes with goethite (Gt) in natural systems. To explore changes in the correlation between magnetic particles and Hm during pedogenesis, we focus on three representative red Ferrasol profiles with comparable total concentrations of iron oxides but different Hm/(H… Show more

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Cited by 26 publications
(16 citation statements)
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“…sequence. The grain growth of FM particles has also been observed in our previous studies on the climosequence with dramatic changes in Hm/(Hm + Gt) (Long et al, 2015). However, the Hm/ (Hm + Gt) values in the two sequences are comparable, and therefore, the difference in the accumulation efficiency of different FM particles should be controlled by the contrasting P/Fe ranges.…”
Section: 1029/2020gl090439supporting
confidence: 76%
See 1 more Smart Citation
“…sequence. The grain growth of FM particles has also been observed in our previous studies on the climosequence with dramatic changes in Hm/(Hm + Gt) (Long et al, 2015). However, the Hm/ (Hm + Gt) values in the two sequences are comparable, and therefore, the difference in the accumulation efficiency of different FM particles should be controlled by the contrasting P/Fe ranges.…”
Section: 1029/2020gl090439supporting
confidence: 76%
“…However, the relative formation efficiency of Mgh and Hm seems to be modulated by water activity (Long et al, 2016) and ligand adsorption of precursor iron oxides (Cabello et al, 2009) due to the similar thermodynamic stability of Mgh and Hm in nanometers (Navrotsky et al, 2008). Our previous study found significant grain growth of Mgh particles and their transformation to Hm in tropical Ferralsol, with a high formation efficiency estimated by Hm/(Hm + Gt) above 0.6 (Long et al, 2015). However, in some red soils and sediments with relatively high chemical weathering intensity formed in warm periods (Fang et al, 2003; Guo et al, 2002; Ren et al, 2020), the asynchronous change of redness and magnetism can also be frequently observed (Chen et al, 2019; Jiang et al, 2015; Nie et al, 2016; Walker et al, 1981), although the Hm/(Hm + Gt) fluctuates slightly below 0.6, and the positive correlation between redness and magnetism is still maintained in these soils and sediments (Balsam et al, 2004; Ding et al, 2001; Ji et al, 2004; Torrent et al, 2006).…”
Section: Introductionmentioning
confidence: 95%
“…In the LZ, SP and SD particles have a similar formation rate with magnetic enhancement, whereas in the UZ, the production rate of SP particles is higher than that of SD particles (Figure e). Long et al [] reported that χ FD / χ ARM ratios increase rapidly with low χ (~100–1000 × 10 −8 m 3 kg −1 ) but remain constant at high χ (~1000–3000 × 10 −8 m 3 kg −1 ) in red Ferralsols. However, the different formation rate between SP and SD particles is controlled mainly by water content, temperature, and Fe supply in the soil.…”
Section: Discussionmentioning
confidence: 99%
“…Although fine magnetic particles were formed, the topsoil had a lower χ than the parent basalt. Recently, Long et al [] investigated the magnetic properties of three red Ferralsols from localities with MAP from 1440 to 1650 mm/yr and noted that χ is generally 3–20 times higher than that of unweathered basalt and ferrimagnetic material becomes enriched as the hematite (Hm) content increases in the profile. Due to soil drainage and leaching processes, magnetic properties differ greatly among these red soils, despite their similar parent material.…”
Section: Introductionmentioning
confidence: 99%
“…The classic viewpoint (Schwertmann and Taylor, 1989) argues that the hematite forms by dehydrating ferrihydrites and thus high temperature and dry climate favor formation of hematite. on the other hand, some authors propose that the production of hematite results from the aging of maghemite grains that are in turn produced by the aging of ferrihydrites (Torrent et al, 2006;Liu et al, 2008Liu et al, , 2012Long et al, 2015). Therefore, future studies need to continue to focus on clarifying the formation mechanisms of hematite and goethite.…”
Section: Future Research Directionsmentioning
confidence: 99%