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Towards FAIR Paleomagnetic Data Management Through Paleomagnetism.org 2.0
Published 2020-02-01Subjects: “…paleomagnetism…”
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Encyclopedia of Geomagnetism and Paleomagnetism [electronic resource]/
Published 2007Subjects: Get full text
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A paleomagnetic analysis of the Patagonian orocline
Published 2007-01-01Subjects: “…Paleomagnetism…”
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Paleomagnetic constraints on the volcanic history of Iztaccihuatl
Published 1985-01-01Get full text
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Paleomagnetism and rock magnetism as tools for volcanology
Published 2022Subjects: Get full text
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Paleomagnetism and paleomagnetic dating to large volcanic bombs: an example from the historical eruption of Azuma–Jododaira volcano, NE Japan
Published 2023-11-01Subjects: “…Paleomagnetic dating…”
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Paleomagnetic investigation of McMurdo volcanics, Antarctica
Published 1983-01-01“…A total of 212 paleomagnetic samples were collected from the Hut Point Peninsula, the Cape Royds and the Taylor Valley in the McMurdo Sound, Antarctica. …”
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On the earliest human occupation in Europe: Paleomagnetic constraints
Published 2001-07-01Get full text
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Paleomagnetism of the Amazonian Craton and its role in paleocontinents
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Pangea B: an artifact of incorrect paleomagnetic assumptions?
Published 2001-06-01Subjects: “…paleomagnetism…”
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History of the solar nebula from meteorite paleomagnetism
Published 2021“…We discuss the implications of theory, meteorite measurements, and astronomical observations for planetary formation and nebular evolution. Paleomagnetic measurements indicate the presence of fields of 0.54 ± 0.21 G at ~1 to 3 astronomical units (AU) from the Sun and ≳0.06 G at 3 to 7 AU until >1.22 and >2.51 million years (Ma) after solar system formation, respectively. …”
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History of the solar nebula from meteorite paleomagnetism
Published 2022“…We discuss the implications of theory, meteorite measurements, and astronomical observations for planetary formation and nebular evolution. Paleomagnetic measurements indicate the presence of fields of 0.54 ± 0.21 G at ~1 to 3 astronomical units (AU) from the Sun and ≳0.06 G at 3 to 7 AU until >1.22 and >2.51 million years (Ma) after solar system formation, respectively. …”
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Constraining Planetary Science Problems with Micro-Paleomagnetism
Published 2022“…With the development of micro-paleomagnetic techinques we can measure the magnetic field of micro-scale samples that have direct implications for problems in planetary science. …”
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Pallasite paleomagnetism: quiescence of a core dynamo
Published 2016“…Recent paleomagnetic studies of two Main Group pallasites, the Imilac and Esquel, have found evidence for a strong, late-stage magnetic field on the parent body. …”
Journal article