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    <title>DSpace Colección :</title>
    <link>http://hdl.handle.net/11703/120177</link>
    <description />
    <pubDate>Fri, 06 Mar 2026 04:57:18 GMT</pubDate>
    <dc:date>2026-03-06T04:57:18Z</dc:date>
    <item>
      <title>La colección de macroforaminíferos Josep Serra Kiel: realzando la dimensión científica del patrimonio paleontológico mueble</title>
      <link>http://hdl.handle.net/11703/120685</link>
      <description>Título : La colección de macroforaminíferos Josep Serra Kiel: realzando la dimensión científica del patrimonio paleontológico mueble; The Josep Serra Kiel larger foraminifera collection: remarking the scientific dimension of the palaeontological heritage
Nota : Departamento de Paleontología del Museu de Ciències Naturals de Barcelona (MCNB) recibió el pasado 2018 parte de la colección personal micropaleontológica del Dr. Josep Serra Kiel, eminente investigador y profesor de la Universidad de Barcelona. Esta colección está compuesta de material geológico que contiene una gran diversidad de foraminíferos bentónicos complejos del Eoceno medio al Mioceno inferior de Dhofar (Omán) y de la Isla de Socotra (Yemen). Consta de 200 números de registros con material diverso, con más de 1.000 rocas, 456 láminas delgadas, y 32 levigados con los que se han realizado varios estudios científicos de impacto internacional y en los que se han llegado a identificar 92 especies distintas. El mayor exponente del valor científico de esta colección lo constituye el material tipo, ya que en dichos estudios se han descrito nueve especies nuevas y cinco géneros nuevos. La colección micropaleontológica del MCNB ha aumentado cualitativa y cuantitativamente con la donación J. Serra Kiel, reforzando su papel en el escenario del patrimonio paleontológico mueble por su gran utilidad en futuros estudios y proyectos geológicos y museológicos.     Palabras clave: colecciones, foraminíferos, J. Serra Kiel, micropaleontología, patrimonio paleontológico mueble.; In 2018 the Museu de Ciències Naturals de Barcelona received part of the personal micropalaeontological collection of Dr. Josep Serra-Kiel, who was an renowned researcher and professor at the Universitat de Barcelona (Spain). This collection is composed of geological material that contains a great diversity of larger foraminifera from the middle Eocene to the lower Miocene of Dhofar (Oman) and Socotra Island (Yemen). The collection has 200 register numbers of different type of materials, namely, 1000 rocks, 456 thin sections, and 32 levigated samples, that have been objective of several studies of international impact, which identified up to 92 different species. The most important and remarkable part of this collection is the type material, as 9 new species and 5 new genera have been described in those studies. The micropalaeontological collection of the MCNB has increased qualitatively and quantitativelu with the donation of the J. Serra Kiel collection, strengthening its role in the the paleontological heritage scenario because of its usefulness in future geological and museological studies and projects.      Keywords: collections, Foraminifera, J. Serra Kiel, micropalaeontology, movable palaeontological heritage.</description>
      <pubDate>Tue, 01 Jan 2019 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/11703/120685</guid>
      <dc:date>2019-01-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>The chronology and rotational kinematics in the South-Eastern Jaca Basin (Southern Pyrenees): Las Bellostas section</title>
      <link>http://hdl.handle.net/11703/127815</link>
      <description>Título : The chronology and rotational kinematics in the South-Eastern Jaca Basin (Southern Pyrenees): Las Bellostas section
Nota : Despite  the  large  number  of  magnetostratigraphic  studies  in  the  South  Pyrenean  Basin  aiming  to  calibrate  the  basin  chronostratigraphy  and  the  biostratigraphic  scales,  the  South  Eastern  Jaca  Basin  remains  unexplored  from  this  perspective,  and  its  relation  with  the  Ainsa  Basin  is  not  fully  understood.  In  this  work  we  contribute  with  new  magnetostratigraphic  data  from  the  950m  thick  Las  Bellostas  section,  located  in  the  northern  hinge  of  the  Balzes anticline. Well-proven primary signal (positive fold test and two pseudo-antiparallel polarities) supported by  numerous  primary  data  in  the  surroundings  allow  us  building  a  reliable  local  polarity  sequence  of  eight  magnetozones (from R1 to N4). Additionally, seven new biostratigraphic samples (Nummulites and Assilina) in the lower part of the section (marine environment) allows tightening the section to the Geomagnetic Polarity Time Scale (GPTS) and proposing a refined age model for the southeastern Jaca Basin. The section starts in the Boltaña Fm.,  of  Cuisian  age  (Shallow  Benthic  Zone,  SBZ11),  is  followed  by  a  sedimentary  gap  from  C22n  to  C20n  as  witnessed by biostratigraphic data (SBZ11 underneath the hiatus and SBZ16 just atop). The deltaic Sobrarbe Fm can be tracked until the C19n (Late Lutetian). From this point (200m) until the top of the section (950m), at least, the entire C18n chron can be recognized within the molassic Campodarbe Fm (C18n.2n-C18n.1r and C18n.1n) (Bartonian)  equivalent  to  the  West  to  the  prodeltaic  Arguis  marls  Fm.  The  Middle  Cusian  (SBZ11)  to  Middle  Lutetian  (SBZ15)  stratigraphic  hiatus  is,  in  part,  enhanced  by  the  structural  position  at  the  hinge  of  the  Balzes  anticline. These new chronostratigraphic constraints help refining the W-E and N-S stratigraphic relationships in the eastern Jaca Basin and in the Ainsa Basin. This section also allows us to accurately refine the kinematics of the  rotational  activity  in  the  eastern  External  Sierras.  The  significant  difference  in  magnetic  declination  along  the section and neighboring paleomagnetic data from the Balzes anticline (from ≈70º clockwise at the base of the stratigraphic section to non-significant at the top) together with the new age model for the Eastern Jaca Basin help characterizing the rotational activity of the Balzes thrust sheet. The rotation took place between chrons C20r (Middle Lutetian; 45Ma) and C17 (Lower Priabonian 37-38Ma) in agreement to nearby structures (Boltaña, Pico del  Aguila  anticlines)  but  clearly  diachronic  to  western  ones  (Santo  Domingo  anticline).  Besides,  the  rotational activity seems to follow a linear and continuous pattern (velocity 9-11º/Ma, R: 0.83-0.96) in contrast to closer structures that show two distinct rotational velocities (i.e. Boltaña). These new data still let open the debate on the rotational kinematics along the South Pyrenean basal thrust.</description>
      <pubDate>Fri, 23 Sep 2022 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/11703/127815</guid>
      <dc:date>2022-09-23T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Los Hippurites del Barranc del Racó, microfacies y fauna asociada (Maastrichtiense Superior, sur de la provincia de Valencia)</title>
      <link>http://hdl.handle.net/11703/127808</link>
      <description>Título : Los Hippurites del Barranc del Racó, microfacies y fauna asociada (Maastrichtiense Superior, sur de la provincia de Valencia)
Nota : El Cretácico superior, en el flanco 5 de la Sierra de La Solana, en el Barranc
deis Albarcers y Barrane del Racó, cerca del Mas del Racó al W de Hocairent,
presenta un nivel formado por un thicket de rudistas con Hippurites
radiosas des Moulins y Hippurites cornucopiae Defrance, junto a equinidos,
como Pygopyrina darderí (Lambert), corales coloniales como Actinacis sp. y
Procladocora sp., y solitarios, en una matriz biomicrítica con abundantes foraminíferos,
ostrácodos y dasicladales (Neomeris sp.) y localmente siliciclastos.
La base del thicker está formada por una biosparita de foraminíferos que
presenta rellenos geopetales y «silto vadoso. El techo del thicket está formado
por una biomierosparita a biomicrita dc foraminíferos con abundante fauna
de bivalvos y equinidos, con ejemplares completos o muy fragmentados.
La asociación de foraminíferos, igual en el thicket que en su base y techo,
está formada por Siderolites calcitrapoides Lamarck, Acervulina aif. ogormani
(Douvdlé), Orbitoides media d’Orbigny, Orbitoides tissoti Schlumberger, Orbitoides
apiculata Schlumberger, Hellenocyclina beotica Reichel, Omphalocyclus
macroporus (Lamarck), miliólidos y rotálidos.
Las microfacies indican un medio marino protegido, más o menos restringido,
los tipos de procesos diagenéticos observados sugieren que este medio se vio rápidamente afectado por condiciones metedrico-vadosas y la fauna
determina una edad Maastrichtiense superior.; The Upper Cretaceous of the southern flank of Sierra de La Solana, at
Barrane deis Albarcers and Barranc del Racó, around Mas del Raed, west of
Bocairent, presents a level formed by a rudists thicket with hippurites radiosus
des Moulins and Hippurites cornucopiae Defrance, together with echinoids
like Pygopyrina darderi (Lambert), colonial corals like Actinacis sp. and
Procladocora sp. and solitary ones, in a biomicritic matrix containing abundant
foraminifera, ostracodes and dasycladaleans (Neorneris sp.) and sporadic
siliciclasts.
The base of the thieket is formed hy a foraminiferal biosparite presenting
geopetal infillings and vadose silt. The top of the thicket is formed by a foraminiferal
biomicrosparite-biomicrite with an abundant fauna of bivalves and
ecbinoids, complete or very fragmented.
The foraminiferal association, dic same in the thicket as in its base and
top, is formed by Siderolites calcitrapoides Lamarck, Acervulina aff. ogorman¡
(Douvillé), Orbitoides media d’Orbigny, Orbitoides tissoti Schlumberger, Qrbitoldes
apiculata Schlumberger, Ilellenocyclina beotica Reichel, Omphalocyclus
macroporus (Lamarck), miliolids and rotalids.
Microfacies indicate a protected, more or less restricted, marine environment,
the type of diagenetic processes suggest that this cnvironment quickly
undergone a meteoric-vadose condition and the fauna is charactcristic of Late
Maastrichtian age.</description>
      <pubDate>Sat, 01 Jan 1994 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/11703/127808</guid>
      <dc:date>1994-01-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Micropalaeontology, biostratigraphy, and depositional setting of the mid-Cretaceous Derdere Formation at Derik, Mardin, south-eastern Turkey</title>
      <link>http://hdl.handle.net/11703/120692</link>
      <description>Título : Micropalaeontology, biostratigraphy, and depositional setting of the mid-Cretaceous Derdere Formation at Derik, Mardin, south-eastern Turkey
Nota : The micropalaeontology of the mid-Cretaceous Derdere Formation (Mardin Group) from outcrops
close to the town of Derik in south-eastern Turkey is described here. In thin sections from the carbonates that
form the majority of this formation, rich and diverse micropalaeontological assemblages are present. These include larger benthonic foraminifera, planktonic foraminifera, and other microfossils, including calcareous algae.
Alveolinid foraminifera are particularly common and include a new species – Simplalveolina mardinensis. In
contrast to some previous studies, the majority of the section can be demonstrated to be Cenomanian (notably
middle Cenomanian) in age with no confirmation of extension into the Albian or Turonian. Deposition took
place on a carbonate ramp within a range of discrete deposition settings ranging from peritidal to outer ramp. A
notable feature is the small-scale (a few metres) shallowing-up cycles within the inner-ramp facies that may be
allocyclic or autocyclic in origin. Three major deepening events are recognised within the succession, characterised by more open marine microfauna and microfacies. These occur at the base of the formation, within the
mid-Cenomanian lower part, and towards the top of the formation. These may correlate with three Cenomanian
deepening phases seen in other parts of the Arabian Plate.</description>
      <pubDate>Thu, 05 Nov 2020 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://hdl.handle.net/11703/120692</guid>
      <dc:date>2020-11-05T00:00:00Z</dc:date>
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