Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Paleomagnetism and Geochronology of 2.68 Ga Dyke from Murmansk Craton, NE Fennoscandia: New Data for Earth’s Magnetic Field Regime in the Neoarchean. / Veselovskiy, R.V.; Samsonov, A.V.; Stepanova, A.V.; Larionova, Y.O.; Arzamastsev, A.A.; Travin, A.V.; Egorova, S.V.; Erofeeva, K.G.; Kosterov, A.A.; Shcherbakova, V.V.; Shcherbakov, V.P.; Zhidkov, G.V.; Zakharov, V.S.
в: Izvestiya, Physics of the Solid Earth, Том 60, № 4, 01.08.2024, стр. 772-794.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Paleomagnetism and Geochronology of 2.68 Ga Dyke from Murmansk Craton, NE Fennoscandia: New Data for Earth’s Magnetic Field Regime in the Neoarchean
AU - Veselovskiy, R.V.
AU - Samsonov, A.V.
AU - Stepanova, A.V.
AU - Larionova, Y.O.
AU - Arzamastsev, A.A.
AU - Travin, A.V.
AU - Egorova, S.V.
AU - Erofeeva, K.G.
AU - Kosterov, A.A.
AU - Shcherbakova, V.V.
AU - Shcherbakov, V.P.
AU - Zhidkov, G.V.
AU - Zakharov, V.S.
N1 - Export Date: 21 October 2024 Адрес для корреспонденции: Veselovskiy, R.V.; Faculty of Geology, Russian Federation; эл. почта: roman.veselovskiy@ya.ru Сведения о финансировании: Kazan Scientific Centre, Russian Academy of Sciences, KazSC RAS Сведения о финансировании: Moscow State University of Geodesy and Cartography, MIIGAiK Сведения о финансировании: Russian Foundation for Basic Research, RFBR, 17-05-01121, 19-05-00471, 19-05-00433 Сведения о финансировании: Ministry of Education and Science of the Russian Federation, Minobrnauka, MD-1116.2018.5 Сведения о финансировании: FMEN-2023-0009 Сведения о финансировании: Russian Science Foundation, RSF, 16-17-10260 Сведения о финансировании: 122041400171-5 Текст о финансировании 1: This work was supported by RSF, grant #16-17-10260. Paleointensity studies were supported by the Ministry of Education and Science (grant MD-1116.2018.5) and RFBR grant 19-05-00433; rock magnetic measurements were supported by the Russian Foundation for Basic Research (grants 17-05-01121 and 19-05-00471) and by the state assignment of GO \u201CBorok\u201D IPE RAS. Computer modeling was carried out using the equipment of the shared research facilities of HPC computing resources at Lomonosov Moscow State University (Voevodin et al., 2019). Geochemistry studies were supported by the state assignment of Institute of Geology Karelian Research Centre RAS, grant FMEN-2023-0009. Ar/Ar dating was carried out on government assignment to the V.S. Sobolev Institute of Geology and Mineralogy (project No. 122041400171-5). Our special thanks for help in the field works is addressed to the crew of the \u201CUdacha\u201D boat and to the colleagues from Murmansk Marine Biological Institute, Kola Scientific Center of the Russian Academy of Sciences. Paleomagnetic team thanks Vladimir Tselmovich (GO \u201CBorok\u201D) for invaluable help with rock magnetic studies. The authors are grateful to two anonymous reviewers from Precambrian Research for their valuable suggestions that greatly improved the initial version of the paper. The authors also acknowledge the helpful feedback provided by Alexey Didenko and Andrey Guzhikov on the current version of the paper. This study is dedicated in loving memory of our dear colleague and friend, Svetlana Bogdanova (1937\u20132019), whose invaluable contribution has greatly influenced the knowledge of Precambrian geology and tectonics on the East European Platform and beyond. Текст о финансировании 2: This work was supported by RSF, grant #16-17-10260. Paleointensity studies were supported by the Ministry of Education and Science (grant MD-1116.2018.5) and RFBR grant 19-05-00433; rock magnetic measurements were supported by the Russian Foundation for Basic Research (grants 17-05-01121 and 19-05-00471) and by the state assignment of GO \u201CBorok\u201D IPE RAS. Computer modeling was carried out using the equipment of the shared research facilities of HPC computing resources at Lomonosov Moscow State University (Voevodin et al., 2019). Geochemistry studies were supported by the state assignment of Institute of Geology Karelian Research Centre RAS, grant FMEN-2023-0009. Ar/Ar dating was carried out on government assignment to the V.S. Sobolev Institute of Geology and Mineralogy (project No. 122041400171-5).
PY - 2024/8/1
Y1 - 2024/8/1
N2 - Abstract: We present new results of geochronological, rock magnetic, paleomagnetic and paleointensity studies of the olivine gabbro dyke located at the northern part of the Murmansk craton, NE Fennoscandia (the Kola Peninsula). According to its geochemistry, petrographic and geochronology features, the dyke belongs to the 2.68 Ga dyke swarm, as confirmed by Sm-Nd mineral isochron. We find a significant difference in the rock magnetic and paleomagnetic characteristics of the central and marginal parts of the dyke, which is independently supported by petrography and geochemistry. It is shown that the rocks of the central part of the dyke retained not only their primary mineral composition, but also the primary component of the natural remanent magnetization. We use its direction to determine the 2.68 Ga virtual geomagnetic pole for the Murmansk craton: Slat = 68.64292° N, Slong = 37.7945° E, N = 41 specimens, Plat = –73.5°, Plong = 138.9°, dp/dm = 3.2°/3.4°, paleolat = –65.9°. We also obtain reliable estimates (17 samples) of the Earth’s magnetic field intensity at ca. 2.68 Ga: VDM value is found to be 1.85 × 1022 A m2 corresponding to the geomagnetic field several times weaker than the present-day field. © Pleiades Publishing, Ltd. 2024. ISSN 1069-3513, Izvestiya, Physics of the Solid Earth, 2024, Vol. 60, No. 4, pp. 772–794. Pleiades Publishing, Ltd., 2024.
AB - Abstract: We present new results of geochronological, rock magnetic, paleomagnetic and paleointensity studies of the olivine gabbro dyke located at the northern part of the Murmansk craton, NE Fennoscandia (the Kola Peninsula). According to its geochemistry, petrographic and geochronology features, the dyke belongs to the 2.68 Ga dyke swarm, as confirmed by Sm-Nd mineral isochron. We find a significant difference in the rock magnetic and paleomagnetic characteristics of the central and marginal parts of the dyke, which is independently supported by petrography and geochemistry. It is shown that the rocks of the central part of the dyke retained not only their primary mineral composition, but also the primary component of the natural remanent magnetization. We use its direction to determine the 2.68 Ga virtual geomagnetic pole for the Murmansk craton: Slat = 68.64292° N, Slong = 37.7945° E, N = 41 specimens, Plat = –73.5°, Plong = 138.9°, dp/dm = 3.2°/3.4°, paleolat = –65.9°. We also obtain reliable estimates (17 samples) of the Earth’s magnetic field intensity at ca. 2.68 Ga: VDM value is found to be 1.85 × 1022 A m2 corresponding to the geomagnetic field several times weaker than the present-day field. © Pleiades Publishing, Ltd. 2024. ISSN 1069-3513, Izvestiya, Physics of the Solid Earth, 2024, Vol. 60, No. 4, pp. 772–794. Pleiades Publishing, Ltd., 2024.
KW - dyke
KW - Fennoscandian Shield
KW - geochronology
KW - Murmansk craton
KW - Neoarchean
KW - paleointensity
KW - paleomagnetism
KW - rock magnetism
UR - https://www.mendeley.com/catalogue/2fa47836-8bcd-364a-9b12-23d302bf2209/
U2 - 10.1134/s1069351324700538
DO - 10.1134/s1069351324700538
M3 - статья
VL - 60
SP - 772
EP - 794
JO - Izvestiya, Physics of the Solid Earth
JF - Izvestiya, Physics of the Solid Earth
SN - 1069-3513
IS - 4
ER -
ID: 126219970