TY - JOUR
T1 - Strain, anisotropy of anhysteretic remanence, and anisotropy of magnetic susceptibility in a slaty tuff
AU - Nakamura, Norihiro
AU - Borradaile, Graham J.
N1 - Funding Information:
We thank R.T. Merril and B. Housen for their valuable comments. This work was funded by NSERC operating and equipment grants to Graham Borradaile. Norihiro Nakamura was supported by the JSPS postdoctoral fellowships for research abroad during his stay in Canada.
PY - 2001
Y1 - 2001
N2 - Finite strain data for the Borrowdale slaty tuffs compare variably with the anisotropy of magnetic susceptibility (AMS) and anisotropy of anhysteretic remanent magnetization (AARM). Finite strain, determined from lapilli-rims, shows that slaty cleavage was formed by coaxial flattening with X:Y:Z in the ratio 1.74:1.21 and 0.48. AARM was measured in different coercivity windows to isolate contributions from magnetite of different grain sizes: (a) 0-3 mT for multi-domain (MD), (b) 3-15 mT for pseudo-single-domain (PSD) and (c) 15-60 mT for single-domain (SD). AMS combines petrofabric contributions from silicates as well as magnetite. Magnetite grains may grow, recrystalize or rearrange domains after or during metamorphism and postdate or overlap with the silicate's fabric evolution. AMS foliation, defined by paramagnetic chlorites, is parallel to slaty cleavage. AARM foliation for SD magnetites is offset clockwise from AMS foliation, which may reflect late crystallization or domain-rearrangement of magnetites in response to a latter noncoaxial increment. AMS fabric-shape consistently corresponds to strain ellipsoids and indicates that the strain-induced AMS fabric is susceptible to the change of oblateness rather than strain intensity. Furthermore, investigation of the different AARM subfabrics and finite strain shows that only SD magnetite's AARM correlates with finite strain, and weakly at that.
AB - Finite strain data for the Borrowdale slaty tuffs compare variably with the anisotropy of magnetic susceptibility (AMS) and anisotropy of anhysteretic remanent magnetization (AARM). Finite strain, determined from lapilli-rims, shows that slaty cleavage was formed by coaxial flattening with X:Y:Z in the ratio 1.74:1.21 and 0.48. AARM was measured in different coercivity windows to isolate contributions from magnetite of different grain sizes: (a) 0-3 mT for multi-domain (MD), (b) 3-15 mT for pseudo-single-domain (PSD) and (c) 15-60 mT for single-domain (SD). AMS combines petrofabric contributions from silicates as well as magnetite. Magnetite grains may grow, recrystalize or rearrange domains after or during metamorphism and postdate or overlap with the silicate's fabric evolution. AMS foliation, defined by paramagnetic chlorites, is parallel to slaty cleavage. AARM foliation for SD magnetites is offset clockwise from AMS foliation, which may reflect late crystallization or domain-rearrangement of magnetites in response to a latter noncoaxial increment. AMS fabric-shape consistently corresponds to strain ellipsoids and indicates that the strain-induced AMS fabric is susceptible to the change of oblateness rather than strain intensity. Furthermore, investigation of the different AARM subfabrics and finite strain shows that only SD magnetite's AARM correlates with finite strain, and weakly at that.
KW - Anisotropy of anhysteretic remanence
KW - Anisotropy of magnetic susceptibility
KW - Coercive force
KW - Slate
UR - http://www.scopus.com/inward/record.url?scp=0034776895&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0034776895&partnerID=8YFLogxK
U2 - 10.1016/S0031-9201(01)00214-X
DO - 10.1016/S0031-9201(01)00214-X
M3 - Article
AN - SCOPUS:0034776895
SN - 0031-9201
VL - 125
SP - 85
EP - 93
JO - Physics of the Earth and Planetary Interiors
JF - Physics of the Earth and Planetary Interiors
IS - 1-4
ER -