scispace - formally typeset
H

Huaichun Wu

Researcher at China University of Geosciences (Beijing)

Publications -  131
Citations -  4963

Huaichun Wu is an academic researcher from China University of Geosciences (Beijing). The author has contributed to research in topics: Geology & Paleomagnetism. The author has an hindex of 32, co-authored 93 publications receiving 3518 citations. Previous affiliations of Huaichun Wu include China University of Geosciences (Wuhan).

Papers
More filters
Journal ArticleDOI

Pre-Rodinia supercontinent Nuna shaping up: A global synthesis with new paleomagnetic results from North China

TL;DR: The existence of a pre-Rodinia Precambrian supercontinent, variously called Nuna or Columbia, has been widely speculated in the past decade, but the precise timing of its existence and its configuration have been uncertain due to the lack of unequivocal paleomagnetic and geological constraints as mentioned in this paper.
Journal ArticleDOI

Late Mesoproterozoic to earliest Neoproterozoic basin record of the Sibao orogenesis in western South China and relationship to the assembly of Rodinia

TL;DR: The Laowushan Formation has a geochemical signature similar to basalts found in modern intracontinental rifts, with a uniform Nd isotopic character (−087 to +084) as mentioned in this paper.
Journal ArticleDOI

Stratigraphy, Sedimentary Structures, and Textures of the Late Neoproterozoic Doushantuo Cap Carbonate in South China

TL;DR: The 3 to 5mthick Doushantuo cap carbonate in south China overlies the glaciogenic Nantuo Formation (ca. 635 Ma) and consists of laterally persistent, thinly laminated and normally graded dolomite and limestone indicative of relatively deep-water deposition, most likely below storm wave base as discussed by the authors.
Journal ArticleDOI

Time-calibrated Milankovitch cycles for the late Permian

TL;DR: Milankovitch cycles from late Permian (Lopingian) strata at Meishan and Shangsi, South China, time calibrated by recent high-precision U–Pb dating are reported, extending empirical knowledge of Earth’s astronomical parameters before 250 million years ago.