scholarly journals Cyclostratigraphy of the Middle to Upper Ordovician successions of the Armorican Massif (western France) using portable X-ray fluorescence

2022 ◽  
Author(s):  
Matthias Sinnesael ◽  
Alfredo Loi ◽  
Marie-Pierre Dabard ◽  
Thijs R. A. Vandenbroucke ◽  
Philippe Claeys

Abstract. To expand traditional cyclostratigraphic numerical methods beyond their common technical limitations and apply them to truly deep-time archives we need to reflect on the development of new approaches to sedimentary archives that traditionally are not targeted for cyclostratigraphic analysis, but that frequently occur in the impoverished deep-time record. Siliciclastic storm-dominated shelf environments are a good example of such records. Our case study focusses on the Middle to Upper Ordovician siliciclastic successions of the Armorican Massif (western France), which are well-studied in terms of sedimentology and sequence stratigraphy. In addition, these sections are protected geological heritage due to the extraordinary quality of the outcrops. We therefore tested the performance of non-destructive high-resolution (cm-scale) portable X-ray fluorescence and natural gamma-ray analyses on outcrop to obtain major and trace element compositions. Despite the challenging outcrop conditions in the tidal beach zone, our geochemical analyses provide useful information regarding general lithology and several specific sedimentary features such as the detection of paleoplacers, or the discrimination between different types of diagenetic concretions such as nodules. Secondly, these new high-resolution data are used to experiment the application of commonly used numerical cyclostratigraphic techniques on this siliciclastic storm-dominated shelf environment, a non-traditional sedimentological setting for cyclostratigraphic analysis. In the lithological relatively homogenous parts of the section spectral power analyses and bandpass filtering hint towards a potential astronomical imprint of some sedimentary cycles, but this needs further confirmation in the absence of more robust independent age constraints.

2009 ◽  
Vol 56 (4) ◽  
pp. 2299-2302 ◽  
Author(s):  
M. K. Bacrania ◽  
A. S. Hoover ◽  
P. J. Karpius ◽  
M. W. Rabin ◽  
C. R. Rudy ◽  
...  

2004 ◽  
Vol 60 (3) ◽  
pp. 272-281 ◽  
Author(s):  
Radovan Černý ◽  
Guillaume Renaudin ◽  
Vincent Favre-Nicolin ◽  
Viktor Hlukhyy ◽  
Rainer Pöttgen

The new binary compound Mg1 + x Ir1 − x (x = 0–0.054) was prepared by melting the elements in the Mg:Ir ratio 2:3 in a sealed tantalum tube under an argon atmosphere in an induction furnace (single crystals) or by annealing cold-pressed pellets of the starting composition Mg:Ir 1:1 in an autoclave under an argon atmosphere (powder sample). The structure was independently solved from high-resolution synchrotron powder and single-crystal X-ray data: Pearson symbol oC304, space group Cmca, lattice parameters from synchrotron powder data a = 18.46948 (6), b = 16.17450 (5), c = 16.82131 (5) Å. Mg1 + x Ir1 − x is a topologically close-packed phase, containing 13 Ir and 12 Mg atoms in the asymmetric unit, and has a narrow homogeneity range. Nearly all the atoms have Frank–Kasper-related coordination polyhedra, with the exception of two Ir atoms, and this compound contains the shortest Ir—Ir distances ever observed. The solution of a rather complex crystal structure from powder diffraction, which was fully confirmed by the single-crystal method, shows the power of powder diffraction in combination with the high-resolution data and the global optimization method.


1998 ◽  
Vol 21 (7) ◽  
pp. 1015-1018 ◽  
Author(s):  
S.E. Boggs ◽  
R.P. Lin ◽  
P.T. Feffer ◽  
S. Slassi-Sennou ◽  
S. McBride ◽  
...  

1983 ◽  
Vol 101 ◽  
pp. 573-577
Author(s):  
G. Pizzichini ◽  
T. L. Cline ◽  
U. D. Desai ◽  
B. J. Teegarden ◽  
W. D. Evans ◽  
...  

The error box of the unusual Gamma-Ray Burst of March 5, 1979 falls completely inside the optical and radio image of the Supernova Remnant N49 in the Large Magellanic Cloud. This region was observed twice in x-rays with the High Resolution Imager of the Einstein Observatory, six weeks and nearly two years after the Gamma-Ray Burst. We show the comparison between the two observations.


2000 ◽  
Vol 25 (3-4) ◽  
pp. 901-904
Author(s):  
S.I. Svertilov ◽  
V.G. Stolpovskii ◽  
V.V. Bogomolov ◽  
M.I. Kudryavtsev ◽  
I.G. Mitrofanov ◽  
...  

2014 ◽  
Vol 70 (a1) ◽  
pp. C1206-C1206
Author(s):  
Julian Chen ◽  
Bryant Hanson ◽  
S Fisher ◽  
Paul Langan ◽  
Andrey Kovalevsky ◽  
...  

Neutron diffraction data to 1.1 Å was collected on a crystal of the small protein crambin at the Protein Crystallography Station (PCS) at Los Alamos, the highest resolution neutron structure of a protein to date, and a technical benchmark for the instrument. 95 % of the hydrogen atoms in the protein structure were resolved. The data allowed for the refinement of anisotropic temperature factors for selected deuterium atoms within the protein. Hydrogen bonding networks ambiguous in room temperature, ultra-high resolution (0.84 Å) electron density maps are clarified in the nuclear density maps. The ultra-high resolution data also reveals unusual H/D exchange patterns and novel chemistry in the side chains and protein backbone. Complementary X-ray diffraction data was collected at 19-ID at the Advanced Photon Source, with extensive re-configuration of the beamline to allow for operation at higher energy settings.


Author(s):  
Tadayuki Takahashi ◽  
Biswajit Paul ◽  
Kazuyuki Hirose ◽  
Chiho Matsumoto ◽  
Ryouichi Ohno ◽  
...  

2009 ◽  
Vol 706 (2) ◽  
pp. 1269-1276 ◽  
Author(s):  
A. Lemiere ◽  
P. Slane ◽  
B. M. Gaensler ◽  
S. Murray
Keyword(s):  
X Ray ◽  

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