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Parana Basalt

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Journal Article
Journal: Geology
Published: 02 June 2023
Geology (2023) 51 (8): 753–757.
... for the late Berriasian–Valanginian interval. These records document a possible rise in weathering and nutrient runoff during the latest Berriasian, followed by a switch to Paraná-Etendeka basalt erosion during the Valanginian. The high weatherability of LIP basalts enhanced global silicate weathering despite...
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HSE patterns for 1.27 Ga Coppermine CFB, ~130 Ma Parana basalts and ~61 Ma West Greenland picrites versus fractional crystallization models (grey-lines from 13 wt.% MgO, highest HSE concentrations to 4 wt.% MgO, lowest HSE concentrations) assuming an ‘average’ West Greenland picrite composition for model starting composition. Explanation of the model is provided in detail in Day et al. (2013). Data sources are: Woodland (2000), Rocha-Junior et al. (2012), and Day et al. (2013). CI-chondrite normalization from Horan et al. (2003).
Published: 01 January 2016
Figure 31 HSE patterns for 1.27 Ga Coppermine CFB, ~130 Ma Parana basalts and ~61 Ma West Greenland picrites versus fractional crystallization models (grey-lines from 13 wt.% MgO, highest HSE concentrations to 4 wt.% MgO, lowest HSE concentrations) assuming an ‘average’ West Greenland picrite
Series: AAPG Memoir
Publisher: The American Association of Petroleum Geologists and Brazilpetrostudies
Published: 01 January 2021
DOI: 10.1306/13722321MSB.9.1853
EISBN: 9781629812892
... margin, syn-tectonic volcanic flows (Paraná tholeiitic basalts) calibrated by wells, and a continental necking zone. The location of the exhumation point is not recognized, and SDR geometries are not observed east of the necking zone. Nevertheless, the assignment of structural domains A and A', crustal...
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Journal Article
Published: 01 April 2013
Mineralogical Magazine (2013) 77 (3): 227–248.
...T. Moxon; C. M. Petrone; S. J. B. Reed Abstract Characterization of Brazilian agates containing a lower horizontally banded section and an upper chamber with bands parallel to the walls shows that these agates formed much later than the 135 Ma Paraná basalt host rock. Age differentiation between...
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Map showing the igneous (basalt)–sedimentary interaction of the Paraná Basin (modified based on Rossetti et al., 2014).
Published: 01 March 2023
Figure 1. Map showing the igneous (basalt)–sedimentary interaction of the Paraná Basin (modified based on Rossetti et al., 2014 ).
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(a) CI chondrite normalised HSE data for the lunar basalt La Paz 02225,13 (Day et al., 2007) compared with data for Parana basalt KS624 from Brazil (Rocha-Júnior et al., 2012). With the exception of Re, the patterns for these two basalts are quite similar for such low HSE abundance rocks, suggesting similar partitioning of HSE between mantle and basaltic melt for both the Earth and Moon. (b) Data for additional lunar (coloured symbols) and terrestrial basalts (black symbols) show both similarities and differences. Lunar basalts plot systematically lower than terrestrial basalts by more than a factor of 20. Green, orange and blue symbols are from Apollo 15 and 17 landing sites, and the La Paz meteorites, respectively. Lunar basalt data are from Day et al. (2007). Terrestrial basalt data are from Rocha-Júnior et al. (2012).
Published: 01 April 2016
Figure 4.5 (a) CI chondrite normalised HSE data for the lunar basalt La Paz 02225,13 ( Day et al ., 2007 ) compared with data for Parana basalt KS624 from Brazil ( Rocha-Júnior et al ., 2012 ). With the exception of Re, the patterns for these two basalts are quite similar for such low HSE
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(a) CI chondrite normalised HSE data for the lunar basalt La Paz 02225,13 (Day et al., 2007) compared with data for Parana basalt KS624 from Brazil (Rocha-Júnior et al., 2012). With the exception of Re, the patterns for these two basalts are quite similar for such low HSE abundance rocks, suggesting similar partitioning of HSE between mantle and basaltic melt for both the Earth and Moon. (b) Data for additional lunar (coloured symbols) and terrestrial basalts (black symbols) show both similarities and differences. Lunar basalts plot systematically lower than terrestrial basalts by more than a factor of 20. Green, orange and blue symbols are from Apollo 15 and 17 landing sites, and the La Paz meteorites, respectively. Lunar basalt data are from Day et al. (2007). Terrestrial basalt data are from Rocha-Júnior et al. (2012).
Published: 01 April 2016
Figure 4.5 (a) CI chondrite normalised HSE data for the lunar basalt La Paz 02225,13 ( Day et al ., 2007 ) compared with data for Parana basalt KS624 from Brazil ( Rocha-Júnior et al ., 2012 ). With the exception of Re, the patterns for these two basalts are quite similar for such low HSE
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Zr/Y vs. Nb/Y variation for lavas from three continental flood basalt provinces; lines and errors as for Fig. 2. (a) Siberian Traps, Russia, Formations (suites) shown in stratigraphic sequence. Rocks show no detectable plume component. (b) Parana basalts. Some lavas show a possible hot spot signature. (c) Columbia River Basalt, U.S.A., formations shown in stratigraphic sequence. Some lavas show a plume component (see text for details). Sources of data are Garland et al. (1996), Hooper and Hawkesworth (1993), Hooper et al. (1984) — Nb = 17 × Ta, Lightfoot et al. (1990b), Martin (1989), Peate and Hawkesworth (1996), Peate et al. (1999).
Published: 25 May 2001
Fig. 4. Zr/Y vs. Nb/Y variation for lavas from three continental flood basalt provinces; lines and errors as for Fig.  2 . ( a ) Siberian Traps, Russia, Formations (suites) shown in stratigraphic sequence. Rocks show no detectable plume component. ( b ) Parana basalts. Some lavas show a possible
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Comparison of the initial isotope ratios at 135 Ma in the central Moroccan margin sediments with Early Cretaceous large igneous provinces. References for the isotope ratios of the large igneous provinces (see also Supplementary Table): Paraná basalts (Hawkesworth et al. 1986; Peate and Hawkesworth 1996; Marques et al. 1999, 2018; Peate et al. 1999; Turner et al. 1999; Rocha-Júnior et al. 2013; Barreto et al. 2016; Rämö et al. 2016); Etendeka basalts (Ewart et al. 1998a, 2004a; Le Roex and Lanyon 1998; Mingram et al. 2000; Thompson et al. 2001); Etendeka silicic sequences (Ewart et al. 1998b, 2004b; Trumbull et al. 2004); Comei basalts (Zhu et al. 2008; Liu et al. 2015); and Bunbury basalt and silicic sequences (Ewart et al. 1992; Frey et al. 1996; Allen et al. 1997; Direen et al. 2017). LIP, large igneous province.
Published: 07 March 2023
Fig. 8. Comparison of the initial isotope ratios at 135 Ma in the central Moroccan margin sediments with Early Cretaceous large igneous provinces. References for the isotope ratios of the large igneous provinces (see also Supplementary Table ): Paraná basalts ( Hawkesworth et al. 1986 ; Peate
Journal Article
Journal: Geology
Published: 01 August 2010
Geology (2010) 38 (8): 747–750.
...David S. Thiede; Paulo M. Vasconcelos Abstract The duration of volcanism in the Paraná continental flood basalt (CFB) province, essential information to assess models of melt generation, eruption rates, continental breakup, and volcanism-driven extinction events, remains unresolved due...
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Mogánite content as a function of host-rock age. The numbers correspond to the agate-producing regions listed in Fig. 5 and are as follows: (1) Yucca Mountain, Nevada, USA; (2) Mount Warning, Queensland, Australia; (3) Cottonwood Springs, Texas, USA; (4) Chihuahua, Mexico; (5) Washington, USA; (6) Las Choyas, Mexico; (7) Khur, Iran; (8) Gonabad, Iran; (9) British Tertiary Volcanic Province, Scotland. The open circle shows the mean mogánite content of wall-lining Brazilian agate from the 135 Ma Paraná basalt; this data point is arbitrarily placed at 50 Ma. The mogánite data suggests a formation age of ~24 Ma for this wall-lining Brazilian agate. Gonabad is new data (for the host age see Fauvelet and Eftekhar-Nezhad, 1992); other data are after Moxon and Carpenter (2009).
Published: 01 April 2013
) Washington, USA; (6) Las Choyas, Mexico; (7) Khur, Iran; (8) Gonabad, Iran; (9) British Tertiary Volcanic Province, Scotland. The open circle shows the mean mogánite content of wall-lining Brazilian agate from the 135 Ma Paraná basalt; this data point is arbitrarily placed at 50 Ma. The mogánite data
Journal Article
Journal: Geology
Published: 01 October 2014
Geology (2014) 42 (10): 895–898.
... the third, the Paraná-Etendeka (P-E), is not ( Peate, 1997 ; Thiede and Vasconcelos, 2010 ). Our results, besides being the first sulfur measurements for CAMP and Paraná basalts, will be of use for the development of future models of global climate change during LIP eruptions and strengthen...
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Journal Article
Published: 08 March 2021
Petroleum Geoscience (2021) 27 (2): petgeo2020-036.
... in volcano-sedimentary successions. The interbedded nature of the continental flood basalts and aeolian erg deposits from the Cretaceous interval of the Paraná Basin, Brazil, provide an excellent opportunity to evaluate the impact and magnitude of the diagenetic effects in sandstones associated...
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Paraná-Etendeka continental flood basalts erupted 137–127 Ma (Turner et al. 1994) and are contemporaneous with the main phase rifting and are evidence for deep-seated mantle plume (note asymmetry as most of the volcanics reside on the Brazilian side). NW–SE orientation of Ponta Grossa dyke swarm (yellow line) suggests that early-rifting orientation differs from the main phase of rifting and ultimately drift of the South Atlantic. This could be related to far-field stresses associated with Neo-Tethys ‘slab pull’/subduction below the Ladakh Arc once the spreading ridge began subducting (reconstruction from Paleomap Project, Scotese 2008).
Published: 01 August 2010
Fig 3 Paraná-Etendeka continental flood basalts erupted 137–127 Ma ( Turner et al . 1994 ) and are contemporaneous with the main phase rifting and are evidence for deep-seated mantle plume (note asymmetry as most of the volcanics reside on the Brazilian side). NW–SE orientation of Ponta Grossa
Journal Article
Published: 19 July 2010
Geological Magazine (2010) 147 (6): 954–970.
... University Press basalt geochemistry scintillometry correlation Paraná Brazil Uruguay The geochemical analyses of basaltic rocks, integrated with a gamma-spectrometric (scintillometric) survey, yield significant information regarding the stratigraphy and correlation of lavas in continental...
Series: Geological Society, London, Special Publications
Published: 13 April 2023
DOI: 10.1144/SP520-2020-176
EISBN: 9781786209535
... with volcanism, provide an important rock record to understand palaeoenvironments in volcanic settings. The Paraná–Etendeka Igneous Province is a well-known example of a continental flood basalt emplaced on a dry desert environment, but evidence has also shown the existence of humid conditions during...
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Journal Article
Published: 01 December 1991
Journal of the Geological Society (1991) 148 (6): 973–977.
... P. Silver P. G. Carlson R. W. The large-scale structure of convection in the Earth's mantle Nature 1990 344 209 215 Peate D. W. Hawkesworth C. J. Mantovani M. S. M. Shukowsky W. Mantle plumes and flood basalt stratigraphy in the Parana, South America Geology...
Journal Article
Journal: AAPG Bulletin
Published: 01 March 1985
AAPG Bulletin (1985) 69 (3): 346–360.
... over portions of Brazil, Paraguay, Uruguay, Argentina, and Bolivia. The Paleozoic marine sedimentary rocks in the Paraná basin are covered by the world’s most extensive flood basalt complex, making geophysical exploration extremely difficult, although modern seismic techniques recently applied...
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Journal Article
Journal: AAPG Bulletin
Published: 01 April 1984
AAPG Bulletin (1984) 68 (4): 531.
... the basalt and underlying sediments to provide scattered signals containing critical information on thicknesses and resistivities of the geologic units. The MT method has been utilized in a multidisciplinary exploration program recently completed in the Parana basin by the State of Sao Paulo. In the deeper...
Journal Article
Journal: AAPG Bulletin
Published: 01 August 1960
AAPG Bulletin (1960) 44 (8): 1316–1370.
.... The present-day structural basin of Paraná occupies about 1,200,000 sq. km. Of this area, about 800,000 sq. km. are covered by outcropping basaltic lava flows. This lava at once renders most of the normal exploration tools of oil geology impractical and ineffective. Since the nation-wide oil development...
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