Paleointensity estimates from ignimbrites: An evaluation of the Bishop Tuff
Paleointensity estimates from ignimbrites: An evaluation of the Bishop Tuff
复制标题
凝灰岩的古强度估计:主教凝灰岩的评估
DOI:
10.1029/2009gc002834
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发表时间:
2010
期刊:
影响因子:
3.7
通讯作者:
J. Bowles
中科院分区:
文献类型:
--
作者:
J. Gee;Yongjae Yu;J. Bowles
Ash flow tuffs, or ignimbrites, typically contain fine‐grained magnetite, spanning the superparamagnetic to single‐domain size range that should be suitable for estimating geomagnetic field intensity. However, ignimbrites may have a remanence of thermal and chemical origin as a result of the complex magnetic mineralogy and variations in the thermal and alteration history. We examined three stratigraphic sections through the ∼0.76 Ma Bishop Tuff, where independent information on postemplacement cooling and alteration is available, as a test of the suitability of ignimbrites for paleointensity studies. Thermomagnetic curves suggest that low‐Ti titanomagnetite (Tc = 560°C–580°C) is the dominant phase, with a minor contribution from a higher Tc phase(s). Significant remanence unblocking above 580°C suggests that maghemite and/or (titano)maghemite is an important contributor to the remanence in most samples. We obtained successful paleofield estimates from remanence unblocked between 440°C and 580°C for 46 of 89 specimens (15 sites at two of three total localities). These specimens represent a range of degrees of welding and have variable alteration histories and yet provide a consistent paleofield estimate of 43.0 μT (±3.2), equivalent to a VADM of 7.8 × 1022 Am2. The most densely welded sections of the tuff have emplacement temperatures inferred to be as high as ∼660°C, suggesting that the remanence may be primarily thermal in origin, though a contribution from thermochemical remanence cannot be excluded. These results suggest that ignimbrites may constitute a viable material for reliable paleointensity determinations.