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Spreading rate dependence of morphological characteristics in global oceanic transform faults
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Yiming Luo1, 2, 3, 4, 5, 7, , Jian Lin1, 5, 6, , Fan Zhang1, 2, 3, *, Meng Wei7
Acta Oceanologica Sinica | 2021, 40(4) : 39 - 64
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Acta Oceanologica Sinica | 2021, 40(4): 39-64
Marine Geology
Spreading rate dependence of morphological characteristics in global oceanic transform faults
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Yiming Luo1, 2, 3, 4, 5, 7, , Jian Lin1, 5, 6, , Fan Zhang1, 2, 3, *, Meng Wei7
Affiliations
  • 1 Key Laboratory of Ocean and Marginal Sea Geology, South China Sea Institute of Oceanology/Innovation Academy of South China Sea Ecology and Environmental Engineering, Chinese Academy of Sciences, Guangzhou 510301, China
  • 2 Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou), Guangzhou 511458, China
  • 3 China-Pakistan Joint Research Center on Earth Sciences, Chinese Academy of Sciences-Higher Education Commission of Pakistan, Islamabad 45320, Pakistan
  • 4 University of Chinese Academy of Sciences, Beijing 100049, China
  • 5 Department of Ocean Science and Engineering, Southern University of Science and Technology, Shenzhen 518055, China
  • 6 Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA
  • 7 University of Rhode Island, Narragansett, RI 02882, USA
Published: 2021-04-25 doi: 10.1007/s13131-021-1722-5
Outline
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We quantified the systematic variations in global transform fault morphology, revealing a first-order dependence on the spreading rate. (1) The average age offset of both the full transform and transform sub-segments decrease with increasing spreading rate. (2) The average depth of both the transform valley and adjacent ridges are smaller in the fast compared to the slow systems, reflecting possibly density anomalies associated with warmer mantle at the fast systems and rifting at the slow ridges. However, the average depth difference between the transform valley and adjacent ridges is relatively constant from the fast to slow systems. (3) The nodal basin at a ridge-transform intersection is deeper and dominant at the ultraslow and slow systems, possibly reflecting a lower magma supply and stronger viscous resistance to mantle upwelling near a colder transform wall. In contrast, the nodal high, is most prominent in the fast, intermediate, and hotspot-influenced systems, where robust axial volcanic ridges extend toward the ridge-transform intersection. (4) Statistically, the average transform valley is wider at a transform system of larger age offset, reflecting thicker deforming plates flanking the transform fault. (5) The maximum magnitude of the transform earthquakes increases with age offset owing to an increase in the seismogenic area. Individual transform faults also exhibit significant anomalies owing to the complex local tectonic and magmatic processes.

mid-ocean ridge  /  transform fault  /  morphology  /  spreading rate  /  transform earthquakes
Yiming Luo, Jian Lin, Fan Zhang, Meng Wei. Spreading rate dependence of morphological characteristics in global oceanic transform faults[J]. Acta Oceanologica Sinica, 2021 , 40 (4) : 39 -64 . DOI: 10.1007/s13131-021-1722-5
A transform fault is a major plate boundary with predominantly strike-slip motion between two adjacent plates (Wilson, 1965). Oceanic transform faults exhibit significant variability in length and age offset. Globally, the full length of a transform fault ranges from as small as 26 km (Herron transform fault) to as large as 1 099 km (Chile transform fault), and the full transform age offset is in the range of 0.69 Ma (Yaquina transform fault) to 105.8 Ma (Andrew Bain transform fault) (Boettcher and Jordan, 2004; Wolfson-Schwehr, 2015).
High-resolution bathymetry data of the last four decades have revealed the morphological complexity of oceanic transform systems. Transform faults are commonly composed of multiple sub-segments, separated by fault steps, intra-transform extension basins, or intra-transform spreading centers (e.g., Searle, 1983; Fornari et al., 1989; Ligi et al., 2002; Gregg et al., 2006). This complex transform morphology might be caused by a range of tectonic and magmatic processes in the ridge-transform system (e.g., Royden et al., 1982; Lin et al., 1990; Lin and Morgan, 1992; Sempéré et al., 1993; Perfit et al., 1996; Behn et al., 2002; Gregg et al., 2006, 2007; Wolfson-Schwehr, 2015; Wei, 2019; Wolfson-Schwehr and Boettcher, 2019).
Transform faults exhibit systematic variations in morphology that contain important information regarding the dynamics of the transforms and adjacent ridges. Almost all transform faults are associated with transform-parallel median valleys, some of which are composed of multiple topographical lows (e.g., Macdonald, 1982; Searle, 1983; Fox and Gallo, 1984; Tucholke and Schouten, 1988; Bonatti et al., 1994; Tucholke and Lin, 1994; Maia, 2019). Transform-parallel topographical highs have been observed in some transform systems either inside the transform valley (forming a median ridge) or flanking the transform fault (forming a transverse range) (Pockalny et al., 1988; 1997; Embley and Wilson, 1992; Maia, 2019). In many transform systems, the greatest depth is located near the ridge-transform intersection, forming noticeable nodal basins (e.g., Karson and Dick, 1983; Fox and Gallo, 1984; Pockalny et al., 1988). On the other hand, distinctive axial volcanic ridges are often observed at the adjacent spreading center axis and at the ridge-transform intersection (i.e., nodal highs). Nodal highs are especially well-developed in systems that have a relatively robust magma supply, such as fast- and intermediate-spreading or hotspot-influenced systems (e.g., Macdonald, 1982; Morgan and Parmentier, 1984).
The majority of studies to date have focused on investigating the morphology of individual transform faults, while quantitative analysis of the global variability in transform faults and the analysis of the dependence on the spreading rate remain limited. This lack of quantitative analyses hinders our understanding of ridge-transform dynamics.
In the present study, we quantified the global variability in transform fault morphology and investigated their dependence on the spreading rate. The investigated transform faults included examples from the ultraslow (full spreading rate<20 mm/a), slow (20–50 mm/a), intermediate (50–80 mm/a), and fast (>80 mm/a) systems (Macdonald, 1982; Dick et al., 2003) (Figs 1 and A1). The investigated systems included those at the East Pacific Rise (EPR), Pacific-Antarctic Ridge (PAR), Juan de Fuca Ridge (JDF), Southeast Indian Ridge (SEIR), Chile Rise (CR), Aden Ridge (ADEN), Central Indian Ridge (CIR), Mid-Atlantic Ridge (MAR), American-Antarctic Ridge (AAR), and Southwest Indian Ridge (SWIR) (Figs 1 and A1). We first quantified the systematic variations in the key morphological parameters and free-air gravity anomaly (FAA) of the global transform systems, including the length, age offset, depth of transform faults and adjacent ridges, depth of ridge-transform intersection, and transform width. We then analyzed the dependence of the morphological variability on the spreading rate and examined the relationship between transform morphology and earthquake magnitude. Finally, we identified anomalous transform features that deviated from the global systematics and investigated the tectonic and magmatic factors controlling the local variability.
We investigated morphological parameters of transform faults through analysis of seafloor bathymetry and gravity data. We used the latest global bathymetry database with grid spacing of 15′′ (Tozer et al., 2019; SRTM15_PLUS Version 2; http://topex.ucsd.edu/WWW_html/mar_topo.html), which combined the available multibeam bathymetry, shipboard soundings, and satellite altimetry-derived seafloor depth. FAA data at 1′ grid spacing were extracted from a global dataset (Sandwell et al. 2014; V26.1; http://topex.ucsd.edu/marine_grav/mar_grav.html).
A total of 137 full transform faults were analyzed for transform length and age offset, based on the dataset of Wolfson-Schwehr (2015) (Fig. 2a1, Table A1). Among the transform faults analyzed, a single transform fault may consist of 1–7 sub-segments according to its morphological structure (Table A1), yielding a total of 201 analyzed transform sub-segments. The transform sub-segment length (LS) was calculated by measuring the distance between its two endpoints following a small circle (Wolfson-Schwehr, 2015). The full transform length (LF) was then obtained by the sum of LS for a given transform fault.
Full spreading rates (UF) for individual transform faults (Table A1) were obtained from the Global Strain Rate Map Project (GSRM, V1.2, Kreemer et al., 2000; Wolfson-Schwehr, 2015). The corresponding full transform age offset (AOF) is given by AOF = 2LF/UF. Similarly, the transform sub-segment age offset (AOS) is given by AOS = 2LS/UF.
We further selected 78 transform faults with relatively good bathymetric data to quantitatively analyze their morphological parameters. The cumulated length of the transform faults analyzed for morphological parameters is 16 473 km. A cumulated length of 9 304 km of the adjacent ridges was also analyzed for comparison with the associated transform faults (Fig. A1, Table A2). For a given transform fault, we first carefully traced the mid-points or the deepest points along the transform valley by visual inspection. We then calculated the average depth of the profile and defined it as the transform fault depth (black lines in Fig. A1, Table A2). We also obtained depth profiles along the axis of the adjacent ridges by visual inspection (red lines in Fig. A1, Table A2). The determination of the ridge axes was also aided by examination of the magnetic anomalies. We defined the average depth of the adjacent ridge axes as the ridge depth (Table A2). At a slow-spreading ridge (e.g., the MAR) (Fig. 2b1), we carefully tracked the deepest points of the axial valley or a small central volcanic high. At a fast-spreading ridge (e.g., the EPR) (Fig. 2a1) or a hotspot-influenced ridge, we carefully tracked the axial topographic high or a small central depression.
We carefully examined the 3D topography of a ridge-transform intersection to determine whether it is associated with a local basin (i.e., nodal basin, Fig. A2a1) or a topographical high (i.e., nodal high, Fig. 2a1). For a local basin, we found the deepest point by visual inspection and defined its depth as the nodal basin depth (Table A3). Similarly, for a local topographic high, we located the shallowest point by visual inspection and defined its depth as the nodal high depth.
We calculated the widths of 44 transform faults with relatively simple structure. We first traced the peaks of the two conjugate transform walls. We then calculated the distance between the two conjugate peak points at the mid-point of the transform fault. The measured distance was defined as the width of the transform fault (Fig. 2d, Table 2).
To the first-order, the oceanic plate adjacent to a transform fault can be approximated as a thermal boundary layer that thickens as the square root of the lithospheric age (Turcotte and Schubert, 2014). Thus, the lithospheric plate thickness (hL) at the mid-point of a full transform fault is shown by hL=2.32$ \sqrt{\kappa {\tau }_{1/2}} $, where $ \kappa $=10−6 m2/s is the thermal diffusivity, and τ1/2=LF/UF is lithospheric age at the mid-point of the transform fault.
The maximum earthquake moment magnitudes of global transform faults ($M_{\rm{w}}^{\max } $, Table A1) were obtained by Wolfson-Schwehr (2015) and Wolfson-Schwehr and Boettcher (2019) from the Global Centroid Moment Tensor Project (Dziewonski and Anderson, 1981; Ekström et al., 2012). A 50 km wide rectangular polygon centered on a transform fault was used to define the earthquakes of a given transform fault (Wolfson-Schwehr, 2015).
The seismogenic area (At) of a transform fault was calculated by integrating the cross-sectional area of the transform wall above the 600°C isotherm (Table A1, Boettcher and Jordan, 2004; Wolfson-Schwehr, 2015).
The oceanic transform faults exhibit common topographical characteristics, including a transform valley, high topography on the flanks (Figs 2 and A2), and a nodal high (Fig. 2a1) or nodal basin (Fig. A2b1) at the ridge-transform intersection. The seafloor topography remains relatively constant away from the transform fault. Across-transform topographical variations are relatively small (1–2 km) and narrow (20–50 km) in the fast (e.g., Clipperton, Figs 2a1 and c) and intermediate (e.g., Zeehaen, Figs A2a1 and c) systems, but are larger (up to ~3.5 km) and wider (up to ~100 km) in the slow (e.g., Romanche, Figs 2b1 and d) and ultraslow (e.g., Du Toit, Figs A2b1 and d) systems.
We also examined the FAA that reflects the integrated gravitational effects of the seafloor topography and density anomalies beneath the seafloor (Figs 2a2–b2 and A2a2–b2). Most of the prominent topographical features, including the transform valley and flanking high, are visible in the FAA (Figs 2c–d and A2c–d).
Among the 137 transform faults that we examined for transform length, 23, 64, and 38 are located at the ultraslow, slow, and intermediate systems, respectively, while 12 are at the fast systems (Fig. 3). At the fast systems, the Menard transform fault (208 km) at the PAR has the greatest length (Fig. 4a1). At the intermediate systems, the Tasman transform fault (625 km) at the SEIR has the greatest length (Fig. 4a2), which is composed of 5 sub-segments, with lengths of 90 km, 218 km, 62 km, 173 km, and 82 km, respectively. At the slow systems, the Chile transform fault (1 099 km) at the CR has the greatest length (Fig. 4a3), which consists of 3 sub-segments, with lengths of 493 km, 186 km, and 420 km, respectively. At the ultraslow systems, the Andrew Bain transform fault (706 km) at the SWIR has the greatest length (Fig. 4a4), which consists of 3 sub-segments, with lengths of 87 km, 148 km, and 471 km, respectively (Fig. 4).
Most of the transform faults are within 400 km in full length (Figs 4a1–a4). Ultra-long transform fault systems (full length>400 km) are located at the intermediate, slow, and ultraslow systems (Figs 4a2–a4), including the George V (414 km), Tasman (625 km), Tharp (462 km), Doldrum (726 km), Romanche (878 km), Saint Paul (589 km), Chile (1 099 km), Valdavia (599 km), Andrew Bain (706 km), and Bullard (526 km). Transform sub-segments with lengths over 400 km include the Tharp, Chile A and C, Romanche, Bullard B, and Andrew Bain C (Figs 4b2–b4, Table A1).
The full transform age offset (Figs 5a1–a4) and transform sub-segment age offset (Figs 5b2–b4) increase with decreasing spreading rate. Transform faults with age offset greater than 40 Ma are observed mainly at ultraslow and slow systems, including the Andrew Bain, Bullard, Shackelton, Doldrum, Romanche, Saint Paul, and Chile (Figs 5a3–a4 and 6c). Transform sub-segments with age offsets greater than 40 Ma include the Andrew Bain C, Bullard B, Shackelton, and Romanche (Figs 5b3–b4 and 6d, Table A1). The average full/sub-segment age offset decreases with increasing spreading rate (Figs 6c and d, Table 1). Furthermore, the standard deviation values of the transform length and age offset are in general greater for the ultraslow and slow systems than the intermediate and fast systems (Fig. 6, Table 1).
Along the global ridge-transform system, transform faults are consistently deeper than the adjacent ridges (Figs 7a1–k1). Correspondingly, the FAA is consistently more negative at the transform faults than the adjacent ridges (Figs 7a2–k2 and A3). Regions affected by hotspots are associated with shallower seafloor and more positive FAA, e.g., the Iceland and Azores (Figs 7h1 and h2). When modeled by Gaussian distribution, the mean depth and FAA of the transform faults are consistently greater than that of the adjacent ridges (Figs 8 and A3).
The average depth of transform faults decreases with increasing spreading rate (Fig. 9a, Table 1). The average depth of the adjacent ridges also decreases with increasing spreading rate (Fig. 9b, Table 1). However, the average depth difference between the transform faults and adjacent ridges is relatively constant, and is only slightly greater at the ultraslow system (Fig. 9c).
The spreading rate dependence of the transform and ridge depth could be associated with a combination of factors including thermal structure and dynamic topography. First, at a given distance from the ridge axis, the mantle temperature is higher and thus the density is lower at a faster ridge (Turcotte and Schubert, 2014). The overall higher mantle temperature also leads to a greater degree of partial melting at a faster ridge. Both the thermal and partial melting density anomalies contribute to shallower seafloor (Magde and Detrick, 1995). Second, slow-spreading ridges are often associated with an axial rift valley that could be caused by hydraulic head loss in the upwelling mantle (Sleep, 1969; Sleep and Biehler, 1970), tectonic faulting (Shaw and Lin, 1996), and lithospheric necking (e.g., Tapponnier and Francheteau, 1978; Lin and Parmentier, 1989; Chen and Morgan, 1990).
The average depth of the global nodal basins (Fig. 10a) is 0.38–1.25 km deeper than those of the nodal highs (Fig. 10b, Table A3). The nodal high is dominant at the fast (Fig. 10c) and intermediate (Fig. 10d) systems. In contrast, nodal basin is prevalent at the slow (Fig. 10e) and ultraslow (Fig. 10f) systems.
The average depths of nodal highs are relatively constant (3.25–3.27 km) for the slow and ultraslow systems, but slightly smaller (2.75–3.01 km) for fast and intermediate systems (Fig. 10a, Table 1). The average depths of nodal basins decrease with increasing spreading rate (Fig. 10b, Table 1).
The commonly observed nodal basins at slow and ultraslow systems might reflect a decrease in ridge-axis magma supply (Fox and Gallo, 1984) and viscous resistance to mantle upwelling by the cold transform wall (Sleep, 1969; Sleep and Biehler, 1970). In contrast, nodal highs might appear at ridge systems where robust axial volcanic ridges extend toward ridge-transform intersections (Fig. 2, Table A3).
In general, the transform width (w) decreases with increasing spreading rate for the ultraslow (29–45 km), slow (17–50 km), intermediate (10–36 km), and fast (12–25 km) systems (Fig. 11a). Ultra-wide transform systems with widths greater than 40 km include the Romanche (w of 50 km, age offset of 62.1 Ma) of the MAR, Atlantis II (45 km, 33.4 Ma) of the SWIR, and Bullard B (40 km, 78.3 Ma) of the AAR (Table 2). In general, the transform width is systematically greater for systems of larger age offset (Fig. 11a). In a special case when a transform valley is bounded by two inward-dipping normal faults, the transform width (w) is expected to depend on the plate thickness (hL) (Fig. 11b inset). However, other factors might also control the transform fault width, including multiple transform faults and extension episodes.
While the investigated transform parameters show first-order dependence on spreading rate, the variation within each spreading rate group is large, especially for the slow and ultraslow systems (Figs 6, 9 and 10, Table 1). Furthermore, for each of the investigated parameters, multiple examples of major exceptions were observed. In particular, several transform systems have anomalies in more than one parameter (Table 3). These major anomalies reveal unusually complex local tectonic and magma variability.
The Romanche transform fault (Fig. 2b1) is one of the longest (878 km) and deepest (7.9 km) transform systems on Earth (Bonatti et al., 1994; Wolfson-Schwehr, 2015). It is associated with unusually large values in length (Figs 6a and b), age offset (Figs 6c and d), transform depth (Fig. 9a), and transform width (Fig. 11a). The active transform boundary, previously located in the northern valley, had migrated southward to its present location a few million years ago and formed ridges inside the transform domain. The morphological complexity of the Romanche transform was probably caused by alternating across-transform transtension and transpression induced by plate motion changes (Bonatti et al., 1994; Searle et al., 1994; Ligi et al., 2002).
For the Andrew Bain transform at the SWIR, Sclater et al. (2005) similarly proposed that its morphological complexity was a response to transtension across the transform system, causing multiple transform sub-segments (Fig. A4a). Geodynamic modeling illustrated the possibility of alternating activation of multiple sub-parallel strike-slip faults within a wide transform domain, such as those observed in the Romanche and Andrew Bain systems (Ligi et al., 2002).
In addition to the Romanche and Andrew Bain systems, there are several examples of major morphological anomalies that might have been caused by across-transform transtension and/or transpression. For example, it was proposed that the Atlantis II transform (Fig. A4b) has experienced transtension for 12 million years due to plate rotation of 10° since ~19.5 Ma (Baines et al., 2003); the Bullard transform (Fig. A4c) was subjected to transpression during the early Miocene period (Livermore et al., 1991); and the Heezen and Tharp transforms at the PAR had undergone transtension since 12 Ma, resulting in the formation of extra deep transform valleys (Fig. A4d) (Lonsdale, 1994; Croon et al., 2008).
The Bouvet transform fault at the SWIR is located close to the Bouvet hotspot (Fig. A4e). The average depth of the eastern ridge segment is smaller than that of the conjugate western segment by about 1 km (Fig. 9b). Such a transform-ridge depth difference (–2.7 km) is about 1.6 km greater than the global average value for the corresponding spreading rate (Fig. 9c). Thus, the observed anomalies in the depth difference between ridge and transform fault of the Bouvet system are attributed to excess magma, thicker crust, and shallower seafloor at the ridge axis due to hotspot-ridge interaction (Georgen et al., 2001).
The Jan Mayen transform fault at the northern MAR connects the Jan Mayen Ridge and is located north of Iceland (Figs A1e and A4f). The depths of the Jan Mayen transform fault (Fig. 9a) and the adjacent ridges (Fig. 9b) are exceptionally shallow and are interpreted as the result of the excess magma supply from the Jan Mayen hotspot (Zhang et al., 2020).
The $M_{\rm{w}}^{\max } $ in general increases with increasing transform length (Fig. 12a) for length less than 300 km, as well as with increasing age offset (Fig. 12c) for age offset less than 40 Ma. At systems of greater transform length and age offset, the $M_{\rm{w}}^{\max } $ increases only slightly.
$M_{\rm{w}}^{\max } $ increases with increasing At (Fig. 12d), which is consistent with theoretical consideration. The moment magnitude (Mw) of an earthquake is defined as Mw=2/3×log10 (μ×At×S) – 10.7 (Kanamori, 1977), where μ=3×1010 Pa is the rock rigidity, and S is the average slip during an earthquake. Therefore, $M_{\rm{w}}^{\max } $ should increase with increasing At and S (Fig. 12d). Roland et al. (2010) proposed that the base of the seismogenic area (600°C isotherm) is nearly flat, which differs from the half-space cooling model (Boettcher and Jordan, 2004). Therefore, using the half-space cooling model might underestimate At and MW.
$ M_{\rm{w}}^{\max }$ decreases moderately with increasing spreading rate (Fig. 12b). Bird et al. (2002) also found that the corner magnitude of transform earthquakes decreases with increasing spreading rate. Such spreading rate dependence could be due to multiple factors. First, the age offset is in general smaller for fast systems, leading to smaller At and thus Mw. Second, the lizardite mineral phases might exist only at transforms with slow rates, where serpentinization might be present at transform faults. The presence of lizardite in slow-spreading systems might promote unstable sliding along the transform fault, leading to large transform earthquakes (Bird et al., 2002).
Our quantitative analysis of the morphological parameters of global oceanic transform faults yielded the following key results.
(1) The age offset of transform faults and transform sub-segments decrease with increasing spreading rate.
(2) Both transform faults and adjacent ridges are shallower at the fast-spreading compared to the slow-spreading systems, likely reflecting density anomalies associated with warmer mantle at the fast systems and rifting at the slow ridges. However, the average depth difference between the transform fault and adjacent ridges is relatively constant from the slow- to fast-spreading systems.
(3) Nodal basins are mostly observed at the slow and ultraslow systems; whereas nodal highs are prevalent at the fast and intermediate systems. The nodal basin is possibly related to reduced ridge-axis magma supply and stronger viscous resistance to mantle upwelling by the cold transform wall, whereas a nodal high is formed where the robust ridge-axis volcanic ridges extend toward a transform fault.
(4) The average transform width is greater at a larger age offset, possibly reflecting greater effective elastic thickness of the deforming plates flanking the transform valley.
(5) The average maximum moment magnitude of the transform earthquakes increases with the transform length, age offset, and seismogenic area of the transform faults. The maximum moment magnitude decreases with increasing spreading rate, reflecting relatively small age offset and seismogenic area of fast-spreading systems, as well as the presence of lizardite mineral phases in slow-spreading systems that might promote unstable transform sliding.
This work benefited from constructive discussion with Jason Phipps Morgan, Marcia Maia, Hongfeng Yang, Zhiyuan Zhou, and the Deep Ocean Geodynamics Group of the South China Sea Institute of Oceanology.
  • The foundation of Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou) under contract No. GML2019ZD0205; the National Natural Science Foundation of China under contract Nos 41976064, 41890813, 41976066, 91958211, and 41706056; the scholarship of China Scholarship Council; the foundations of the Chinese Academy of Sciences under contract Nos Y4SL021001, QYZDY-SSW-DQC005, 133244KYSB20180029, and 131551KYSB20200021; the National Key Research and Development Program of China under contract Nos 2018YFC0309800 and 2018YFC0310105; the Foundation of the China Ocean Mineral Resources Research and Development Association under contract No. DY135-S2-1-04; the Guangdong Basic and Applied Basic Research Foundation under contract No. 2021A1515012227.
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Year 2021 volume 40 Issue 4
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doi: 10.1007/s13131-021-1722-5
  • Receive Date:2020-02-28
  • Online Date:2026-02-28
  • Published:2021-04-25
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  • Received:2020-02-28
  • Accepted:2020-06-29
Funding
The foundation of Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou) under contract No. GML2019ZD0205; the National Natural Science Foundation of China under contract Nos 41976064, 41890813, 41976066, 91958211, and 41706056; the scholarship of China Scholarship Council; the foundations of the Chinese Academy of Sciences under contract Nos Y4SL021001, QYZDY-SSW-DQC005, 133244KYSB20180029, and 131551KYSB20200021; the National Key Research and Development Program of China under contract Nos 2018YFC0309800 and 2018YFC0310105; the Foundation of the China Ocean Mineral Resources Research and Development Association under contract No. DY135-S2-1-04; the Guangdong Basic and Applied Basic Research Foundation under contract No. 2021A1515012227.
Affiliations
    1 Key Laboratory of Ocean and Marginal Sea Geology, South China Sea Institute of Oceanology/Innovation Academy of South China Sea Ecology and Environmental Engineering, Chinese Academy of Sciences, Guangzhou 510301, China
    2 Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou), Guangzhou 511458, China
    3 China-Pakistan Joint Research Center on Earth Sciences, Chinese Academy of Sciences-Higher Education Commission of Pakistan, Islamabad 45320, Pakistan
    4 University of Chinese Academy of Sciences, Beijing 100049, China
    5 Department of Ocean Science and Engineering, Southern University of Science and Technology, Shenzhen 518055, China
    6 Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA
    7 University of Rhode Island, Narragansett, RI 02882, USA

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表12种不同金属材料的力学参数

Family
属数
Number of
genus
种数
Number of
species
占总种数比例
Percentage of
total species (%)

Genus
种数
Number of
species
占总种数比例
Percentage of total
species (%)
鹅膏菌科Amanitaceae 2 11 5.26 鹅膏菌属 Amanita 10 4.78
小菇科 Mycenaceae 2 12 5.74 丝盖伞属 Inocybe 5 2.39
多孔菌科 Polyporaceae 8 14 6.70 蜡蘑属 Laccaria 5 2.39
红菇科 Russulaceae 3 23 11.00 小皮伞属 Marasmius 6 2.87
小菇属 Mycena 11 5.26
光柄菇属 Pluteus 5 2.39
红菇属 Russula 17 8.13
栓菌属 Trametes 5 2.39
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