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  • 1
    Call number: SR 92.0157(101)
    In: Geologica Bavarica
    Type of Medium: Series available for loan
    Pages: 333 S.
    Series Statement: Geologica Bavarica 101
    Language: German
    Location: Lower compact magazine
    Branch Library: GFZ Library
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  • 2
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 116 (1994), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: Apparently conflicting data within the palaeomagnetic database suggest that Bohemia was at much shallower palaeolatitudes than the Armorican and Iberian massifs in Ordovician times. In order to resolve this controversy a palaeomagnetic study of Arenig and Llanvirn volcanic and sedimentary rocks from the Barrandian Basin, Central Bohemia has been carried out. This basin comprises a sequence of unmetamorphosed Lower Palaeozoic rocks, the main folding of which occurred in Late Devonian to Early Carboniferous times. The samples collected (17 sites, 153 samples) were subjected to stepwise thermal and alternating field treatment. Eleven sites yielded reliable magnetic directions, with analysis of the results using standard principal component and great circle analyses. Up to three directions of magnetization can be identified in these rocks. The first, termed A, is generally removed below 200°C, although in some cases it persists up to 450°C in the volcanic rocks. It is approximately parallel to the present-day Earth's magnetic field in the study area (Dec/Inc 360°/67°) and is thus thought to be of recent origin. The second direction identified, termed B, is isolated at intermediate blocking temperatures (150–350°C), and yields an overall in situ mean direction of 195°/8°, k= 22.3, α95= 13.1° (seven sites). These directions fail the fold test of McFadden (1990), and correspond to a palaeopole position of 34°S; 356°E. This coincides with the Late Carboniferous sector of the European apparent polar wander path, and thus the B direction is interpreted as being a secondary overprint of this age. The highest blocking temperature direction, termed C, is identified at temperatures between 350° and 450–600°C. It passes the fold test, resulting in an overall mean direction of 312°/83°, k= 21.9, α95= 14.6° (six sites) after bedding correction. This direction is interpreted as being representative of the Early Ordovician palaeomagnetic field direction in the Bohemian Massif and yields a palaeopole position of 58°N; 355°E. This translates into palaeolatitudes of 76°S for Bohemia, thus demonstrating that the Bohemian Massif was at similar peri-polar latitudes to the rest of Armorica during Early Mid-Ordovician times, and formed part of the northern margin of Gondwana.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 99 (1989), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: Palaeomagnetic samples were collected from the Early to Mid-Ordovician igneous ring complex at Salala, northern Red Sea Hills, Sudan. Detailed demagnetization experiments on 114 samples from 17 sites yield two distinct groups of characteristic directions of the natural remanent magnetization. Component ‘A’, predominant in samples from the quartz syenitic central part and minor ring dyke of the complex, displays rather high blocking temperatures, well above 600°C and is presumably carried by haematite. The direction of this component (Dec/Inc = 1°/+37°) is virtually identical with the direction of the present day Earth's magnetic field at the sampling locality (Dec/Inc = 0°/ +37°). Mixed polarities of ‘A’ magnetization strongly suggest a Recent/pre-Brunhes age of this component, and the effects of long-term weathering and low-temperature oxidation. Component ‘B’, pointing to the southeast and upward, has been identified in seven sites from the major ring dyke, composed of aegirine syenite. Maximum blocking temperatures of this component do not exceed 580°C and, together with the results of rock magnetic and optical examinations, are indicative of primary magnetite as the carrier of the characteristic magnetization. The mean direction (Dec/Inc = 124°/-50°, α95 = 9.2, k= 44.1) differs significantly from component ‘A’ and is thought to be primary and representative for the direction of the Earth's magnetic field during emplacement and cooling of the ring complex in Mid-Ordovician times. The resulting palaeomagnetic pole (40°N, 30°W, dp= 8, dm= 12), situated off the coast of West Africa, plots very close to a cluster of Ordovician palaeomagnetic poles from Africa. These poles have not been integrated into the majority of the various apparent polar wander paths for Gondwana but this new result re-enforces their correctness. The application of recently revised rotation parameters for eastern Gondwana significantly reduces the longitudinal gap between the African data and that from eastern Gondwana (particularly Australia) for the Ordovician.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 102 (1990), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: The isotopically dated Lower to Middle Devonian Sabaloka complex (16.3d̀N, 32.6d̀E) in Northern Sudan, for which a palaeomagnetic pole position close to the present geomagnetic pole had been derived in a previous investigation, has been revisited. The formerly determined direction of remanence is shown to be of secondary origin (possibly due to recent or Pleistocene weathering, as shown by ore microscopy and a negative conglomerate test) and a further component of magnetization is detected at several sites. Rockmagnetic studies give strong arguments in favour of a primary origin of the newly found remanence direction. In this paper the palaeomagnetic results (site means) of the two laboratories (Munich and Leeds) for the Sabaloka complex have been combined yielding D= 340.1d̀, I=- 43.9d̀, N= 15, k= 20.6, α95= 8.0d̀. This gives a palaeomagnetic South Pole position (site mean) at 42.0d̀S and 55.7d̀E which is discussed in the context of other Palaeozoic pole positions of Gondwana.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 122 (1995), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: The palaeogeographic position of Armorica in the upper Ordovician is still rather unclear, due mainly to the lack of reliable palaeomagnetic data. To help resolve this, a palaeomagnetic study of Caradocian and Ashgillian sediments and volcanics of the Barrandian Basin in the central Bohemian Massif (Czech Republic) has been carried out. A total of 29 sites were sampled, including four from a diabase sill intruded into Hirnantian-age sediments, thus providing a baked contact test. Three components of magnetization, labelled A, B and C, have been resolved, in addition to a low-temperature component which corresponds to the present-day direction of the local geomagnetic field (D/I= 360°/67°). Component A (southerly and shallow before bedding correction) is only sporadically present, and corresponds to a remagnetization event of Permo-Carboniferous age which is well known throughout Hercynian Europe. Component B, present as stable endpoints in the sill, and as a secondary component in the host-rock sandstones, yields an overall mean direction of 360°/39°, α95= 9.3°, k= 52.3 in situ, and 355°/21°, α95= 9.3°, k= 52.3 after bedding correction. Component C, identified as stable endpoints in sedimentary and volcanic rocks, passes both a fold test and a baked contact test and is interpreted as being the primary direction of magnetization. The overall mean direction for C is 183°/−59°, α95= 9.5°, k= 30.3 (nine sites) after bedding correction which corresponds to a palaeopole position of 80°S; 360°E. This translates into palaeolatitudes of 40°S for the area studied in latest Ordovician times, but indicates large amounts of rotation (up to 170°) of the Bohemian Massif before final consolidation of Hercynian Europe. Although such large amounts of rotation are difficult to accommodate, they are consistent with palaeomagnetic results obtained from lower Ordovician and upper Silurian rocks elsewhere in the Barrandian Basin.If the Bohemian Massif is interpreted as being an integral part of the Armorican microplate, then these results indicate that prior to Caradoc times, Armorica rifted away from the northern margin of Gondwana, and that by Ashgillian times it was located at intermediate palaeolatitudes.
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 104 (1991), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: The approach of Gondwana, and/or microplates derived from its northern margins, towards Laurentia and the closure of the intervening Palaeo-Tethys is a controlling factor in the geodynamic evolution of the Atlantic bordering continents during the early and mid-Palaeozoic. However the currently available palaeomagnetic data for Gondwana, especially for the geodynamically critical Silurian to Devonian interval are still rather sparse and are compatible with a number of palaeogeographic scenarios. In order to address this issue 114 samples (18 sites) have been collected from a series of high level acidic intrusive rocks, rhyolitic lavas and tuffs of mid-Devonian age (377 ± 5 Ma, Rb/Sr) along the southern escarpment of the Gilif Hills, Sudan (17.83°N, 32.67°E). Detailed demagnetization experiments revealed the presence of three directionally distinct components of magnetization, labelled A, B and C. The overall mean direction of component A (Dec. 0.9°, Inc. 29.8°, α95= 4.6°, k= 91.1, N= 12 sites) is indistinguishable from either the direction of the present field or the geocentric axial dipole field in northern Sudan. Mixed polarities suggest a Recent or Pleistocene age of this component. Component B also displays mixed polarities. The site mean directions for this component average to 6.5° declination, -40.2° inclination with α95= 7.0° and k= 48.1 (based on 10 sites) and yield a palaeomagnetic pole at 48.8°S, 23.5°E (dp= 5.1°1, dm= 8.4°). Maghaemite and haematite have been identified to be the predominant magnetic phases in samples which carry component A and/or B. Both A and B are the probable results of low-temperature oxidation of magnetite. Although the age of component B can not be directly determined, it is inferred by correlation with published data to reflect a late Carboniferous overprint. Component C, identified in 11 sites (39 samples), is characterized by a very steep downward magnetization (Dec. 296.2°, Inc. 79.3°, α95= 10.8°, k= 18.7, n= 11 sites) which corresponds to a palaeomagnetic pole position in the southwestern corner of Libya (25.9°N, 11.6°E, dp= 19.6°, dm= 20.6°). Maximum blocking temperatures of component C, generally below 580°C, are indicative of magnetite as carrier of this remanence. The results of thermal remanent magnetization experiments demonstrate that component C is a thermo-remanent magnetization, probably primary, and suggest this component to be representative for the direction of the Earth's magnetic field during emplacement of the Gilif Hills volcanic rocks in mid-Devonian times. The position of the resulting palaeomagnetic pole lends new support to geodynamic scenarios advocating the existence of a wide (approx. 5000 km) Pre-Hercynian ocean during Devonian times. The simplest reconciliation of component B with the reference apparent polar wander path is achieved by assuming it to be of Carboniferous age and by invoking a westward cusp in the Carboniferous part of the apparent polar wander path. Taken at face value, the age of this cusp coincides with large-scale post-orogenic right lateral strike slip movements in Hercynian Europe and North Africa. This interpretation does not require the apparent polar wander (APW) loop and very high rates of plate motion implied by some alternative models. However, if it is valid it will require reinterpretation of the remanence-age of one West African intrusive suite and of some eastern Australian Palaeozoic rocks.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Earth and Planetary Science Letters 114 (1992), S. 1-15 
    ISSN: 0012-821X
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Earth and Planetary Science Letters 84 (1987), S. 487-499 
    ISSN: 0012-821X
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
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  • 9
    ISSN: 0016-7835
    Keywords: Key words Variscan fold belt ; Armorica ; Avalonia ; Palaeomagnetism ; Palaeogeography
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Notes: Abstract  The Variscan fold belt of Europe resulted from the collision of Africa, Baltica, Laurentia and the intervening microplates in early Paleozoic times. Over the past few years, many geological, palaeobiogeographic and palaeomagnetic studies have led to significant improvements in our understanding of this orogenic belt. Whereas it is now fairly well established that Avalonia drifted from the northern margin of Gondwana in Early Ordovician times and collided with Baltica in the late Ordovician/early Silurian, the nature of the Gondwana derived Armorican microplate is more enigmatic. Geological and new palaeomagnetic data suggest Armorica comprises an assemblage of terranes or microblocks. Palaeobiogeographic data indicate that these terranes had similar drift histories, and the Rheic Ocean separating Avalonia from the Armorican Terrane Assemblage closed in late Silurian/early Devonian times. An early to mid Devonian phase of extensional tectonics along this suture zone resulted in formation of the relatively narrow Rhenohercynian basin which closed progressively between the late Devonian and early Carboniferous. In this contribution, we review the constraints provided by palaeomagnetic data, compare these with geological and palaeobiogeographic evidence, and present a sequence of palaeogeographic reconstructions for these circum-Atlantic plates and microplates from Ordovician through to Devonian times.
    Type of Medium: Electronic Resource
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  • 10
    Publication Date: 2015-04-25
    Description: The Mead Stream section (South Island, New Zealand) consists of a 650-m-thick series of continuous, well-exposed strata deposited on a South Pacific continental slope from the Late Cretaceous to the middle Eocene. We examined the uppermost Paleocene–middle Eocene part of the section, which consists of ~360 m of limestone and marl, for detailed magnetic polarity stratigraphy and calcareous nannofossil and foraminifera biostratigraphy. Magneto-biostratigraphic data indicate that the section straddles magnetic polarity chrons from C24r to C18n, calcareous nannofossil zones from NP9a to NP17 (CNP11–CNE15, following a recently revised Paleogene zonation), and from the Waipawan to the Bortonian New Zealand stages (i.e., from the base of the Ypresian to the Bartonian international stages). The Mead Stream section thus encompasses 17 m.y. (56–39 Ma) of southwest Pacific Ocean history. The ages of calcareous nannofossil biohorizons are consistent with low- to midlatitude data from the literature, indicating that during the early–middle Eocene, the low- to midlatitude calcareous nannofossil domain extended at least to ~50°S–55°S in the South Pacific. Correlation of the magnetic polarity stratigraphy from the Mead Stream section with the geomagnetic polarity time scale allows us to derive sediment accumulation rates (SAR), which range between 8 and 44 m/m.y. Comparing the SAR with paleotemperature proxy records, we found that two intervals of increased SAR occurred during the early Eocene climatic optimum (52–50 Ma) and during the transient warming event peaking with the middle Eocene climatic optimum (40.5 Ma). This correlation indicates that, at Mead Stream, the climate evolution of the early–middle Eocene is recorded in a sedimentation pattern whereby, on a million-year time scale, warmer climate promoted continental weathering, transportation, and accumulation of terrigenous sediments.
    Print ISSN: 0016-7606
    Electronic ISSN: 1943-2674
    Topics: Geosciences
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