Earth-Science Reviews最新文献

Effective selection of climate predictors is a fundamental aspect of climate modeling research. Predictor Screening (PS) plays a crucial role in identifying regional climate drivers, reducing noise, expediting convergence, and minimizing time consumption, ultimately leading to the development of robust models. This review delves into the complex landscape of PS techniques within the context of Numerical Climate Modeling (NCM), with a specific focus on their applicability across various Köppen climate classifications and PS model structures. The analysis revealed substantial variations in the performance of PS methods, shedding light on their ability to capture –and prioritize predictors related to precipitation and temperature within distinct climate contexts. Furthermore, the provided methods have been categorized into two subsections: Feature Selection (FS) and Feature Extraction (FE), with FS encompassing filter, wrapper, embedded, and ensemble/hybrid techniques, and FE covering Linear Feature Extraction (LFE), Time-Domain Analysis (TDA), deep learning, and clustering methods. The initial compilation of papers, acquired through a keyword search on Scopus, consisted of 3650 documents. Following a meticulous evaluation process, 206 papers were identified as fitting for inclusion in the literature review, covering the time frame from 1974 to November 3, 2023. In conclusion, the results provide a detailed understanding of the strengths and limitations of each approach, establishing a hierarchy of effectiveness contingent upon the specific climate context. Additionally, insights into promising avenues for future research in this field are offered. This review follows the PRISMA (Preferred Reporting Items for Systematic Reviews and Meta-Analyses) standard as its foundation.

The general configuration of the main continental blocks in the Gondwana supercontinent and the Ediacaran–early Paleozoic tectonic evolution of its northern margin are widely accepted. However, reconstruction of the original positions and the question of potential separation of the Gondwana-derived crustal segments that are now included in the Variscan and Alpine orogenic belts remain controversial. The Western Carpathians, part of the Alpine–Carpathian belt, represents an important crustal segment broken-off from northern Gondwana and later incorporated into both the Variscan and Alpine collisional orogens. The earliest tectonic evolution and paleogeography of the pre-Variscan basement of the Western Carpathians remains poorly known, due to insufficient age data and intense polyphase tectonometamorphic overprints, both Variscan and Alpine. This paper provides new results of U–Pb dating and Hf isotopic analysis of detrital zircons as well as a whole-rock geochemical study from metavolcanic-sedimentary basement units of the Western Carpathians. The obtained age spectra suggest that the sedimentary succession was supplied dominantly by Ediacaran (c. 600 Ma) zircons, with a relatively minor role for Stenian–Tonian (c. 1.2–0.9 Ga) and Paleoproterozoic cratonic (c. 2.2–1.8 Ga) zircons. The mixed Hf isotopic signature (ε_Hf(t) values ranging from −20 to +12) of the Ediacaran zircons indicates substantial mixing of mantle-derived magmas with mature crustal material, typical of continental magmatic arcs. In contrast, the mostly negative ε_Hf(t) values (−15 to +4) of the cratonic zircons suggest recycling of an older continental crust. The presumably youngest part of the sequence is also characterised by high proportion of early Paleozoic zircons with generally negative ε_Hf(t) values (−10 to −2). The zircon U–Pb age spectra, Hf isotopic patterns and whole-rock geochemical signatures of the studied Western Carpathians sequences are interpreted as reflecting deposition at a progressively developing Cambrian–Silurian passive margin setting. The West Carpathian data have been correlated with a comprehensive detrital zircon U–Pb age and Hf isotope data set compiled from possible source areas and other Gondwana-derived units to test the possibility of their primary linkages. These correlations indicate strong similarity in both zircon U–Pb age spectra and Hf isotopic compositions to other parts of the Ediacaran (Cadomian) continental magmatic arc. Older, cratonic sources are linked to the Saharan or East African parts of northern Gondwana, whereas the early Paleozoic detritus must represent a local volcanic source. Taken together, our new data from the Western Carpathians provide constraints for a new paleogeographic model of the northern African part of the Gondwana passive margin.

Dunes form where winds blow over a bed of mobile sediment grains — conditions that are common in our solar system. On Earth, dunes abound in arid continental interiors and along sandy coastlines. Dune fields have also been recognized on Venus, Mars, Saturn’s moon Titan, and Pluto. In response to the different boundary conditions and other environmental forcings, dunes adopt a rich diversity of shapes, sizes, and behaviors. Thus, people around the globe and over centuries have developed a rich vocabulary to describe dunes and their complexity. As a result, existing dune nomenclature often includes redundant terms with differing definitions across scientific communities. Previous studies have endeavored to link dune shape to environmental forcing, usually by means of correlation. Although instructive, correlation-based classifications can be misleading if not based on underlying mechanics or if dune morphogenetic classes are not uniquely defined. Here, we synthesize existing dune terminology and use the last two decades of research on dune morphodynamics to propose three complementary dune classification schemes based on: (1) descriptive dune geomorphology, (2) morphodynamic processes, and (3) fluid mechanics and physics of sediment transport. The first classification relates dune types to geomorphic setting, the presence or absence of vegetation or obstacles, and dune shape (including planform shape, and cross-sectional symmetry or asymmetry). Dune classes can be further subdivided where the direction of sand transport is known independently. The second classification relates dune types and shapes to bed properties (sand-covered vs partially starved bed) and wind forcing (directional variability or the relative strengths and directions of wind modes) that together influence dune dynamics (growth, migration, elongation) and select the dominant processes by which dunes are shaped and oriented relative to the resultant transport direction. The third classification relates, for different planetary environments, the range of possible dune sizes, from minimum to maximum wavelength, to fluid flow regime (rough or smooth) and the response of sediment flux, which influence the coupling between sand bed topography, fluid flow, and sediment transport. These characteristic lengths are useful scales for comparative geomorphology. The three classification schemes provide complementary information. Together, they form a unified framework for geomorphologists, sedimentologists, geographers, physicists, and others to describe windblown sand dunes on Earth and beyond through their shape, dynamics, and size as a response to winds and boundary conditions.

The closure of the Paleo-Asian Ocean (PAO) is crucial for understanding the late Paleozoic–early Mesozoic paleogeography of Proto-Asia and the tectonic configuration of NE Pangea. However, the timing and mechanism for the PAO closure and final amalgamation of the Central Asian Orogenic Belt (CAOB) remain highly controversial. Available studies argue either for a pre-Carboniferous closure or eastward, scissor-style diachronous closure from late Carboniferous to late Permian. This ambiguity is mainly caused by the different criteria applied to evaluate the final closure of oceanic basins and termination of accretionary orogenesis. Here we summarize new evidence including the youngest mélange-bearing accretionary complex and provenance change of syn-orogenic sediments in order to trace the terminal closure of the PAO from Tianshan in the west, through Beishan and Alxa, to Solonker and Changchun-Yanji in the east, a total distance of ∼5000 km.

The Tianshan marks the demise of the western segment of the PAO where the Tarim Craton collided with the Kazakhstan–Yili–Central Tianshan arc. Several ophiolitic mélanges from the Kyrgyz and Chinese Tianshan show the relicts of Permian–Triassic oceanic lithosphere that amalgamated during the Middle-Late Triassic. In Beishan, three ophiolitic mélanges contain Permian igneous rocks and Permian–Triassic sedimentary matrix, suggesting closure of the ocean between ∼245–222 Ma. In the Engger Us mélange of Alxa, a turbidite matrix overlying Permian ocean plate stratigraphy yields a ∼244 Ma maximum depositional age, constraining the time of emplacement of the accretionary complex. To the east, several ophiolitic mélanges in Inner Mongolia contain Permian–Early Triassic gabbro/basalt and middle-late Permian radiolarians, suggesting subduction-accretion continued into the Early Triassic. Along the Changchun–Yanji suture in NE China, several accretionary complexes yield emplacement ages of ∼246–234 Ma. Therefore, the youngest ophiolitic mélanges and accretionary complexes across the whole southern CAOB were formed during the Middle-Late Triassic. In addition, Middle-Late Triassic provenance changes have been identified in syn-orogenic sediments in Tianshan, Beishan, Alxa, Inner Mongolia and NE China. These data are in agreement with Triassic deformation and high-pressure metamorphism, which together indicate that the western, central, and eastern segments of the PAO were closed almost contemporaneously during the Middle-Late Triassic.

To the south, multidisciplinary data suggest that the amalgamation between South China, Sibumasu, Indochina, Qiangtang, and North China took place between ∼230–225 Ma, which led to the closure of the Paleo-Tethys Ocean. Taken together, the Indosinian orogeny leading to the amalgamation of the East Asian blocks marks the final assembly of Pangea. The joining of East Asia in the Late Triassic maximized the land area of Pangea, which potentially fostered the dramatic climate