Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/10655
DC FieldValueLanguage
dc.date.accessioned2017-12-20T11:53:29Zen
dc.date.available2017-12-20T11:53:29Zen
dc.date.issued2017en
dc.identifier.urihttp://hdl.handle.net/2122/10655en
dc.description.abstractPoland is considered the most prospective country for shale gas production in Europe. Hydrocarbon generation/expulsion scenarios, drawn in the latest intensive exploration phases, tend to overestimate maturation levels when compared with brand new data acquired after recent drillings. We tested an integrated workflow to correlate published and original thermal maturity datasets for the Paleozoic to Jurassic successions cropping out in the Holy Cross Mountains. These successions, when preserved in subsurface, host the major source rocks in the area. The application of the workflow allowed us to highlight the burial and thermal evolutionary scenarios of the two tectono-stratigraphic blocks of the Holy Cross Mountains (Łysog ory and Kielce blocks) and to propose this approach as a tool for reducing levels of uncertainty in thermal maturity assessment of Paleozoic successions worldwide. In particular, published datasets including colour alteration indexes of Paleozoic microfossils (conodont, acritarchs) and vitrinite and graptolite reflectance data, show differences in levels of thermal maturity for the Łysog ory (mid mature to overmature) and Kielce (immature to late mature) blocks. Original data, derived from optical analysis, pyrolysis, and Raman spectroscopy on kerogen, and X-Ray diffraction on finegrained sediments, mostly confirm and integrate published data distribution. 1D thermal models, constrained by these data, show burial and exhumation events of different magnitude, during the Late Cretaceous, for the Łysog ory (maximum burial depths of 9 km) and Kielce (burial depths of 6 km) blocks that have been related to the Holy Cross Fault polyphase activity. In the end, Palynomorph Darkness Index and Raman spectroscopy on kerogen, for Llandoverian and Cambrian rocks, turned out to be promising tools for assessing thermal maturity of Paleozoic organic facies devoid of vitrinite macerals.en
dc.language.isoEnglishen
dc.relation.ispartofMarine and Petroleum Geologyen
dc.relation.ispartofseries/80(2017)en
dc.rightsCC0 1.0 Universalen
dc.rights.urihttp://creativecommons.org/publicdomain/zero/1.0/en
dc.subjectPaleozoic source rocksen
dc.subjectThermal maturityen
dc.subjectVitrinite and organoclast reflectanceen
dc.subjectClay mineralogyen
dc.subjectRaman spectroscopyen
dc.subjectPalynomorph darkness indexen
dc.subjectHoly Cross Mountainsen
dc.titleAssessment of thermal evolution of Paleozoic successions of the Holy Cross Mountains (Poland)en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber112-132en
dc.subject.INGV04.04. Geologyen
dc.subject.INGVBasin analysisen
dc.subject.INGVThermal evolutionen
dc.identifier.doi10.1016/j.marpetgeo.2016.11.016en
dc.description.obiettivoSpecifico1TR. Studi per le Georisorseen
dc.description.journalTypeJCR Journalen
dc.contributor.authorSchito, Andreaen
dc.contributor.authorCorrado, Svevaen
dc.contributor.authorTrolese, Matteoen
dc.contributor.authorAldega, Lucaen
dc.contributor.authorCaricchi, Chiaraen
dc.contributor.authorCirilli, Simonettaen
dc.contributor.authorGrigo, Domenicoen
dc.contributor.authorGuedes, Alexandraen
dc.contributor.authorRomano, Claudiaen
dc.contributor.authorSpina, Amaliaen
dc.contributor.authorValentim, Brunoen
dc.contributor.departmentUniversità degli studi di Roma Tre, Dipartimento di Scienzeen
dc.contributor.departmentUniversità degli studi di Roma Tre, Dipartimento di Scienzeen
dc.contributor.departmentUniversità degli studi di Roma Tre, Dipartimento di Scienzeen
dc.contributor.departmentUniversità degli Studi La Sapienza, Dipartimento di Scienza della Terraen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italiaen
dc.contributor.departmentUniversità degli Studi di Perugia, Dipartimento di Fisica e geologiaen
dc.contributor.departmentEni SpA - Exploration & Production Divisionen
dc.contributor.departmentIstituto de Ciencias della Terra (polo da FCUP), departamento de Geocienciaen
dc.contributor.departmentUniversità degli Studi di Roma Tre, Dipartimento di Scienzeen
dc.contributor.departmentUniversità degli Studi di Perugia, Dipartimento di Fisica e geologiaen
dc.contributor.departmentIstituto de Ciencias della Terra (polo da FCUP), departamento de Geocienciaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptUniversità degli studi di Roma Tre, Dipartimento di Scienze-
crisitem.author.deptUniversità degli studi di Roma Tre, Dipartimento di Scienze-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptUniversità degli Studi di Perugia, Dipartimento di Fisica e geologia-
crisitem.author.deptIstituto de Ciencias della Terra (polo da FCUP), departamento de Geociencia-
crisitem.author.deptUniversità degli Studi di Roma Tre, Dipartimento di Scienze-
crisitem.author.deptUniversità degli Studi di Perugia, Dipartimento di Fisica e geologia-
crisitem.author.deptIstituto de Ciencias della Terra (polo da FCUP), departamento de Geociencia-
crisitem.author.orcid0000-0003-0760-9321-
crisitem.author.orcid0000-0003-4356-4132-
crisitem.author.orcid0000-0001-9391-1484-
crisitem.author.orcid0000-0003-4100-7404-
crisitem.author.orcid0000-0001-6397-3713-
crisitem.author.orcid0000-0003-1442-7729-
crisitem.author.orcid0000-0003-1284-2574-
crisitem.author.orcid0000-0002-1463-9126-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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