2001
DOI: 10.1046/j.0956-540x.2001.01443.x
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Low-temperature behaviour of haematite: susceptibility and magnetization increase on cycling through the Morin transition

Abstract: Summary It has been realized previously (e.g. Borradaile 1994) that cycling through the Morin transition (Tm, occurring in ideal α‐Fe2O3 at −10 °C) may have implications for the NRM of some haematite‐bearing rocks. We investigate the behaviour of the low‐field susceptibility (χlf), several magnetizations (in fields of 5, 25, 100 and 1600 mT) and SIRM on cycling through Tm of several well‐characterized haematite types of varying crystallinity and particle shape. Before low‐temperature treatment, χlf of the haem… Show more

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Cited by 52 publications
(38 citation statements)
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“…smaller than 25-30 nm [20]. In contrast, M1 yields particles which are less affected by the silica coating due to their larger size and more compact structure, and show only an increased H C that can result from higher lattice strain [37] or a changed grain size distribution [42,43].…”
Section: Resultsmentioning
confidence: 99%
“…smaller than 25-30 nm [20]. In contrast, M1 yields particles which are less affected by the silica coating due to their larger size and more compact structure, and show only an increased H C that can result from higher lattice strain [37] or a changed grain size distribution [42,43].…”
Section: Resultsmentioning
confidence: 99%
“…The magnetic behavior of nanocrystalline hematite has also been shown to deviate from that of bulk hematite. At room temperature bulk hematite is weakly ferromagnetic, but below 260 K (T M ) hematite undergoes a first order spin reorientation called the Morin transition [12][13][14][15]. The net magnetic moment is lost in this process, and bulk hematite transforms into an antiferromagnet.…”
Section: Introductionmentioning
confidence: 97%
“…Such martian hematite may preserve weak magnetic remanence. Above the so-called Morin transition temperature, T M = −10 • C, crystalline hematite possesses a weak spin-canted magnetic moment with electron spins in the c-planes (perpendicular to the axis of symmetry), while below T M hematite is perfectly antiferromagnetic with electron spins precisely antiparallel-aligned along the c-axis so that the only magnetism is that due to defects (Parkinson, 1983, p. 145); however, for reasons that are currently unknown, heating hematite above T M can make it "remember" a previous field (De Boer et al, 2001). Sinus Meridiani is the largest hematite region (Christensen et al, 2001) and is the landing site of one of NASA's Mars Exploration Rovers (MERs), called MER-B or "Opportunity," launched in July, 2003 (Golombek et al, 2002).…”
Section: Introductionmentioning
confidence: 99%