AbstractX-ray photoemission electron microscopy (XPEEM) enables natural remanent magnetisation to be imaged with ∼30 nm resolution across a field of view of 5–20 μm. The method is applied to structural features typical of the Widmanstätten microstructure (kamacite – tetrataenite rim – cloudy zone – plessite) in the Tazewell IIICD iron meteorite. Kamacite lamellae and the tetrataenite rim are multidomain, whereas plessite consists of laths of different phases displaying a range of stable magnetisation directions. The cloudy zone (CZ) displays a complex interlocking domain pattern resulting from nanoscale islands of tetrataenite with easy axes distributed along three possible crystallographic directions. Quantitative analysis of the coarse an...
Stable paleomagnetic information in meteoritic metal is carried by the “cloudy zone”: ~1–10 μm-wide ...
Nanoscale intergrowths unique to the cloudy zones (CZs) of meteoritic metal display novel magnetic b...
International audienceRecent paleomagnetic studies have constrained the strength and longevity of th...
X-ray photoemission electron microscopy (XPEEM) enables natural remanent magnetisation to be imaged ...
AbstractX-ray photoemission electron microscopy (XPEEM) enables natural remanent magnetisation to be...
AbstractNanoscale intergrowths unique to the cloudy zones (CZs) of meteoritic metal display novel ma...
Meteorites contain a record of their thermal and magnetic history, written in the intergrowths of ir...
Meteorites contain a record of their thermal and magnetic history, written in the intergrowths of ir...
Iron and stony‐iron meteorites form the Widmanstätten pattern during slow cooling. This pattern is c...
Stable paleomagnetic information in meteoritic metal is carried by the “cloudy zone”: ~1–10 μm‐wide ...
International audienceMeteorites are a primary source of information about past magnetic field in th...
Dusty olivine (olivine containing multiple sub-micrometer inclusions of metallic iron) in chondritic...
Iron and stony-iron meteorites form the Widmanstätten pattern during slow cooling. Thispattern is co...
Stable paleomagnetic information in meteoritic metal is carried by the “cloudy zone”: ~1–10 μm-wide ...
Nanoscale intergrowths unique to the cloudy zones (CZs) of meteoritic metal display novel magnetic b...
International audienceRecent paleomagnetic studies have constrained the strength and longevity of th...
X-ray photoemission electron microscopy (XPEEM) enables natural remanent magnetisation to be imaged ...
AbstractX-ray photoemission electron microscopy (XPEEM) enables natural remanent magnetisation to be...
AbstractNanoscale intergrowths unique to the cloudy zones (CZs) of meteoritic metal display novel ma...
Meteorites contain a record of their thermal and magnetic history, written in the intergrowths of ir...
Meteorites contain a record of their thermal and magnetic history, written in the intergrowths of ir...
Iron and stony‐iron meteorites form the Widmanstätten pattern during slow cooling. This pattern is c...
Stable paleomagnetic information in meteoritic metal is carried by the “cloudy zone”: ~1–10 μm‐wide ...
International audienceMeteorites are a primary source of information about past magnetic field in th...
Dusty olivine (olivine containing multiple sub-micrometer inclusions of metallic iron) in chondritic...
Iron and stony-iron meteorites form the Widmanstätten pattern during slow cooling. Thispattern is co...
Stable paleomagnetic information in meteoritic metal is carried by the “cloudy zone”: ~1–10 μm-wide ...
Nanoscale intergrowths unique to the cloudy zones (CZs) of meteoritic metal display novel magnetic b...
International audienceRecent paleomagnetic studies have constrained the strength and longevity of th...