کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
8908652 | 1636675 | 2018 | 49 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
Paleorift structure constrained by gravity and stratigraphic data: The Statherian Araà rift case
دانلود مقاله + سفارش ترجمه
دانلود مقاله ISI انگلیسی
رایگان برای ایرانیان
موضوعات مرتبط
مهندسی و علوم پایه
علوم زمین و سیارات
فرآیندهای سطح زمین
پیش نمایش صفحه اول مقاله

چکیده انگلیسی
Gravimetric and stratigraphic data were used to investigate the Paleoproterozoic Araà Paleorift, a failed Statherian continental rift located in the western margin of the São Francisco Craton, where basement and cover were affected by the Neoproterozoic Brasiliano Orogeny. Euler deconvolution, tilt, total horizontal gradient amplitude and upward continuation technics were applied to terrestrial gravimetric data in order to investigate the rift's main faults location, direction and depth, allowing to identify its main horsts, grabens, volcanic and plutonic centers. We found that rift faults occur to a maximum depth of ca. 38â¯km, but major fault throw occurs from 4 to 8â¯km deep and attenuates from 8 to 12â¯km, probably the brittle-ductile transition zone at the time of rifting, practically disappearing at 20â¯km. Stratigraphic data and basement mapping were used in order to constraint gravimetric results. We classify the Araà Rift as a passive, three-armed failed rift, narrow to divergent type, that produced preferably anorogenic rapakivi-related magmas, most of it still lodged in the crust from surface down to ca. 19â¯km deep and subsidiary mafic magmatism. The results indicate the deep occurrence of low-density magmas beneath the rift's main axis, detected up to 20â¯km deep. Correlation to other global Statherian rifts show that the São Francisco Craton was strongly affected by taphrogenesis during the Statherian, together with Siberia, North America and North China cratons. Finally, by comparing our results to recent rifts we found that the Ethiopian rift's morphology is quite similar to the AraÃ. Surrounding the Tanzanian craton, the Cenozoic East Africa rift system morphology is compared to the AraÃ-Espinhaço rift system, which surrounds the São Francisco craton. The major contribution of this paper is the recognition of Araà Paleorift surface and subsurface morphology, up to now unknown, over an area of ca. 45.000â¯km2.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Tectonophysics - Volumes 738â739, 25 July 2018, Pages 64-82
Journal: Tectonophysics - Volumes 738â739, 25 July 2018, Pages 64-82
نویسندگان
Marco Antonio Caçador Martins-Ferreira, José Eloi Guimarães Campos, Monica Giannoccaro Von Huelsen, Brandow Lee Neri,