Zobrazeno 1 - 10
of 54
pro vyhledávání: '"W. Hieke"'
Autor:
W. Hieke
Publikováno v:
Marine Geology. 207:259-265
The 1960 bathymetric map of Pfannenstiel showed a submarine volcano west of the Peloponnesus which could not be confirmed by modern bathymetric surveys. Pfannenstiel's interpretation was supported by a report of flames on the sea in 1886. It is most
Publikováno v:
Marine Geophysical Researches. 24:279-310
In order to understand the structure and evolution of the Mediterranean Ridge accretionary complex, it is necessary to understand the structure and history of its foreland. The Ionian Abyssal Plain is one of the varying types of foreland. The state o
Autor:
Friedrich Werner, W. Hieke
Publikováno v:
Sedimentary Geology. 135:205-218
A thick mud turbidite, up to 24 m in thickness (termed the “Augias turbidite”) is decribed from the Ionian and Sirte Abyssal Plains and the adjacent slopes of the Calabrian Rise and the Mediterranean Ridge. The material of the megaturbidite is de
Autor:
W. Hieke
Publikováno v:
Sedimentary Geology. 135:89-98
Echosounding and SCS records from the Ionian and Sirte Abyssal Plains show, below the Holocene Augias megaturbidite, two additional thick transparent layers which by analogy are interpreted as turbidites. Estimated thicknesses are 10 and 35 m (upper
Publikováno v:
Marine Geology. 132:113-129
This paper presents a “state of knowledge” of the Antaeus/Pan di Zucchero field (the summit area of the Mediterranean Ridge) including morphological, geological, geophysical and micropaleontological data. The area is characterized by elongated el
Publikováno v:
Marine Geology. 132:63-93
During Meteor Cruise 25 4 in 1993, a multibeam bathymetric (Hydrosweep) survey was carried out on the Mediterranean Ridge in an area south of Crete (comprising the original Olimpi and Prometheus-2 mud diapir fields). The morphology is characterized b
Publikováno v:
Earth and Planetary Science Letters. 109:493-504
A mud breccia has been repeatedly cored from four mud diapir fields located on the crest of the Mediterranean Ridge. This breccia is composed of subrounded clasts supported by a clay-rich matrix and ranges in age from Cretaceous to early Miocene. Sed
Autor:
C. Müller, Alina Polonia, W. Hieke, G. A. Dehghani, Maria Bianca Cita, Angelo Camerlenghi, L. Mirabile, Nicoletta Fusi, H. B. Hirschleber
In previous publications, the relationship between the Sirte Abyssal Plain as foreland and the Mediterranean Ridge as accretionary complex was considered to be simple: the foreland is undeformed, the accretionary complex consumes the foreland, the Me
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::127be2d76ed6c229437482ecfb9be4f3
http://hdl.handle.net/10281/12481
http://hdl.handle.net/10281/12481
Autor:
Judith A McKenzie, Alastair H. F. Robertson, R. Sartori, W. Hieke, Floyd W. McCoy, Georges Mascle, Jean-Pierre Réhault
Publikováno v:
Proceedings of the Ocean Drilling Program, 107 Scientific Results
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3266b3a8de2bdd29c06f0eb0151f3dc4
https://doi.org/10.2973/odp.proc.sr.107.179.1990
https://doi.org/10.2973/odp.proc.sr.107.179.1990