“…If the later calpionellid zonation scheme of Remane [35] is used, the Valanginian/Berriasian boundary would fall in or just younger than M15. This revision is consistent with the results from the Berriasian stratotype section [20], where the boundary was in a covered interval above a negative magnetozone which may correspond to M15. In view of these observations we place this boundary just younger than M15 which gives it an estimated age of 131 Ma.…”
Section: Stage Boundary Age Estimates From Magnetostratigraphic Corresupporting
confidence: 90%
“…Although this correlation may be associated with a hiatus it agrees favourably with a correlation near M22 found in the magnetostratigraphy of DSDP site 534 [19]. Comparison with the magnetic polarity time scale suggests an age of 143 Ma for this boundary, reasonably close to the 141 Ma age proposed by Van Hinte [30] on the assumption of equal biozone durations.…”
Section: Stage Boundary Age Estimates From Magnetostratigraphic Corresupporting
confidence: 86%
“…However, a different correlation of the boundary close to M18 was found in limestones from the southern Alps [17] and in DSDP sediments from the northern Atlantic [18]. Investigations of the magnetic polarity sequence in the Berriasian type section in southern France [19,20] imply a Cretaceous/Jurassic boundary location older than that found in Umbria, but the stratotype section does not extend completely to the boundary. Discrepancies in the boundary correlation result in part from the use of different biostratigraphic schemes [21,22] and the lack of paleontological unity of the definition of the boundary.…”
Section: Magnetostratigraphic Correlation Of M-sequence Tie-levelsmentioning
The ages of polarity chrons in previous M-sequence magnetic polarity time scales were interpolated using basal sediment ages in suitably drilled DSDP holes. This method is subject to several sources of error, including often large paleontological age ranges. Magnetostratigraphic results have now tied the Early Cretaceous and Late Jurassic paleontological stage boundaries to the M-sequence of magnetic polarity. The numeric ages of most of these boundaries are inadequately known and some have been determined largely by intuition. An examination of relevant data suggests that 114 Ma, 136 Ma and 146 Ma are optimum estimates for the ages of the Aptian/Barremian, Cretaceous/Jurassic and Kimmeridgian/Oxfordian stage boundaries, respectively. Each of these boundaries has a good correlation to the M-sequence of magnetic reversals. The magnetostratigraphic tie-level ages are linearly related to the spreading distance and have been used to calculate a new magnetic polarity time scale for the Early Cretaceous and Late Jurassic. All stage boundaries in this time interval were correlated by magnetic stratigraphy to the proposed new time scale which was then used to estimate their numeric ages. depend on the accuracy of the tie-level ages.
“…If the later calpionellid zonation scheme of Remane [35] is used, the Valanginian/Berriasian boundary would fall in or just younger than M15. This revision is consistent with the results from the Berriasian stratotype section [20], where the boundary was in a covered interval above a negative magnetozone which may correspond to M15. In view of these observations we place this boundary just younger than M15 which gives it an estimated age of 131 Ma.…”
Section: Stage Boundary Age Estimates From Magnetostratigraphic Corresupporting
confidence: 90%
“…Although this correlation may be associated with a hiatus it agrees favourably with a correlation near M22 found in the magnetostratigraphy of DSDP site 534 [19]. Comparison with the magnetic polarity time scale suggests an age of 143 Ma for this boundary, reasonably close to the 141 Ma age proposed by Van Hinte [30] on the assumption of equal biozone durations.…”
Section: Stage Boundary Age Estimates From Magnetostratigraphic Corresupporting
confidence: 86%
“…However, a different correlation of the boundary close to M18 was found in limestones from the southern Alps [17] and in DSDP sediments from the northern Atlantic [18]. Investigations of the magnetic polarity sequence in the Berriasian type section in southern France [19,20] imply a Cretaceous/Jurassic boundary location older than that found in Umbria, but the stratotype section does not extend completely to the boundary. Discrepancies in the boundary correlation result in part from the use of different biostratigraphic schemes [21,22] and the lack of paleontological unity of the definition of the boundary.…”
Section: Magnetostratigraphic Correlation Of M-sequence Tie-levelsmentioning
The ages of polarity chrons in previous M-sequence magnetic polarity time scales were interpolated using basal sediment ages in suitably drilled DSDP holes. This method is subject to several sources of error, including often large paleontological age ranges. Magnetostratigraphic results have now tied the Early Cretaceous and Late Jurassic paleontological stage boundaries to the M-sequence of magnetic polarity. The numeric ages of most of these boundaries are inadequately known and some have been determined largely by intuition. An examination of relevant data suggests that 114 Ma, 136 Ma and 146 Ma are optimum estimates for the ages of the Aptian/Barremian, Cretaceous/Jurassic and Kimmeridgian/Oxfordian stage boundaries, respectively. Each of these boundaries has a good correlation to the M-sequence of magnetic reversals. The magnetostratigraphic tie-level ages are linearly related to the spreading distance and have been used to calculate a new magnetic polarity time scale for the Early Cretaceous and Late Jurassic. All stage boundaries in this time interval were correlated by magnetic stratigraphy to the proposed new time scale which was then used to estimate their numeric ages. depend on the accuracy of the tie-level ages.
“…Palynocysts in bed 148 at Berrias (grandis subzone) are the same as those in the Hard Cockle beds of Durlston Bay, assigned there to magnetochron M19n (Figure 4). Other species immediately beneath the lowest 'normal' chron recorded at Berrias (Galbrun et al, 1986), putatively M18 and in the grandis subzone, correlate with the Cypris freestones of Dorset (lower M19n). Palynocysts in bed 149 (subalpina subzone) at Berrias (no magnetochron assigned) correlate with the same in the Scallop bed at Durlston in M16n.…”
Section: Magnetostratigraphy and Palynology Combinedmentioning
confidence: 95%
“…M18n was formerly the only 'normal' magnetozone identified in calpionellid zone B, then providing an approximation to a jacobi/grandis zone (Ogg et al, 1991: Channell & Grandesso, 1987. Initially numbering of chrons relied somewhat on Galbrun's original numbering at Berrias (Galbrun et al, 1986); as already mentioned a problematic section (and type area) to have as a standard. Given the nature of the sediments and apparent breaks in the grandis, subalpina and privasensis intervals there, it is perhaps not surprising that it is difficult to match its magnetostratigraphy conclusively with that in thicker and presumed more complete sequences, such as at Durlston or Bosso.…”
The Jurassic-Cretaceous boundary interval has been problematic since the start of stratigraphic study. This is reflected in different stage names being employed in Boreal and Tethyan realms below and above the putative boundary. Despite attempts at homogenisation where stage terminology is concerned, correlative precision over long distances at or close to a boundary has not yet been achieved. But the new Berriasian/ J-K boundary working-group of the Cretaceous Subcommission is now attempting to remedy this situation.
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