AbstractFew astronomically calibrated high-resolution (≤5 kyr) climate records exist that span the Oligocene–Miocene time interval. Notably, available proxy records show responses varying in amplitude at frequencies related to astronomical forcing, and the main pacemakers of global change on astronomical time-scales remain debated. Here we present newly generated X-ray fluorescence core scanning and benthic foraminiferal stable oxygen and carbon isotope records from Ocean Drilling Program Site 1264 (Walvis Ridge, southeastern Atlantic Ocean). Complemented by data from nearby Site 1265, the Site 1264 benthic stable isotope records span a continuous ∼13-Myr interval of the Oligo-Miocene (30.1–17.1 Ma) at high resolution (∼3.0 kyr). Spectral a...
Orbital‐scale climate variability during the latest Miocene‐early Pliocene is poorly understood due ...
To assess the influence of orbital-scale variations on late Oligocene to early Miocene climate and o...
Accurate age control of the late Tortonian to early Messinian (8.3–6.0 Ma) is essential to ascertain...
Few astronomically calibrated high-resolution (?5 kyr) climate records exist that span the Oligocene...
Few astronomically calibrated high-resolution (≤5 kyr) climate records exist that span the Oligocene...
AbstractFew astronomically calibrated high-resolution (≤5 kyr) climate records exist that span the O...
Few astronomically calibrated high-resolution (<=5 kyr) climate records exist that span the Oligocen...
In this thesis newly generated high-resolution Oligo-Miocene climate proxy records from Walvis Ridge...
Astronomical tuning of sediment sequences requires both unambiguous cycle pattern recognition in cli...
The evolution of the Cenozoic cryosphere from unipolar to bipolar over the past 30 million years (My...
This is the author accepted manuscript. The final version is available from Elsevier via the DOI in ...
A 13-million-year continuous record of Oligocene climate from the equatorial Pacific reveals a prono...
Stable isotope records of benthic foraminifera from ODP Site 1264 in the southeastern Atlantic Ocean...
Astronomical tuning of sediment sequences requires both unambiguous cycle-pattern recognition in cli...
The late Oligocene to early Miocene (20-26Ma) is characterized by a complex climate history that inc...
Orbital‐scale climate variability during the latest Miocene‐early Pliocene is poorly understood due ...
To assess the influence of orbital-scale variations on late Oligocene to early Miocene climate and o...
Accurate age control of the late Tortonian to early Messinian (8.3–6.0 Ma) is essential to ascertain...
Few astronomically calibrated high-resolution (?5 kyr) climate records exist that span the Oligocene...
Few astronomically calibrated high-resolution (≤5 kyr) climate records exist that span the Oligocene...
AbstractFew astronomically calibrated high-resolution (≤5 kyr) climate records exist that span the O...
Few astronomically calibrated high-resolution (<=5 kyr) climate records exist that span the Oligocen...
In this thesis newly generated high-resolution Oligo-Miocene climate proxy records from Walvis Ridge...
Astronomical tuning of sediment sequences requires both unambiguous cycle pattern recognition in cli...
The evolution of the Cenozoic cryosphere from unipolar to bipolar over the past 30 million years (My...
This is the author accepted manuscript. The final version is available from Elsevier via the DOI in ...
A 13-million-year continuous record of Oligocene climate from the equatorial Pacific reveals a prono...
Stable isotope records of benthic foraminifera from ODP Site 1264 in the southeastern Atlantic Ocean...
Astronomical tuning of sediment sequences requires both unambiguous cycle-pattern recognition in cli...
The late Oligocene to early Miocene (20-26Ma) is characterized by a complex climate history that inc...
Orbital‐scale climate variability during the latest Miocene‐early Pliocene is poorly understood due ...
To assess the influence of orbital-scale variations on late Oligocene to early Miocene climate and o...
Accurate age control of the late Tortonian to early Messinian (8.3–6.0 Ma) is essential to ascertain...