ライフサイエンスコーパス: tectonic

1 n self-sustained subduction and global plate tectonics.

2 st subduction zone without the help of plate tectonics.

3 akness, which are both consequences of plate tectonics.

4 amental to understanding the origin of plate tectonics.

5 udes while in turn being influenced by plate tectonics.

6 he asthenosphere, is a requirement for plate tectonics.

7 er time led to an abrupt transition to plate tectonics.

8 tion of our planet before the onset of plate tectonics.

9 eat-pipe volcanism after initiation of plate tectonics.

10 ago, requiring an early initiation of plate tectonics.

11 nked to the onset of subduction-driven plate tectonics.

12 heric evolution, and the initiation of plate tectonics.

13 rking the onset of the Wilson cycle of plate tectonics.

14 he weaker mantle and is fundamental in plate tectonics.

15 vel changes and Miocene regional extensional tectonics.

16 d ultimately the temporal character of plate tectonics.

17 , where it can significantly influence plate tectonics.

18 processes, crustal heterogeneity and active tectonics.

19 Ma and potentially since the onset of plate tectonics.

20 understanding of mantle convection and plate tectonics.

21 the context of changing weather, climate and tectonics.

22 beneath this boundary is essential for plate tectonics, a consensus on its origin remains elusive.

23 s to the onset of renewed intensification of tectonic activity and mountain building, the development

24 Together, the renewed tectonic activity and oceanographic changes facilitated

25 es and follows a global temperature peak and tectonic activity in the Andes.

26 ape brought about by previously unrecognized tectonic activity in the East African rift system.

27 Himalayan tectonic activity is triggered by downward penetration o

28 Plate tectonics affect geography, but also atmosphere composit

29 ients required deep lamellar keratoplasty (2 tectonic and 1 optical), and 2 underwent cornea gluing a

30 formed in 21 of 36 eyes (58%), 9 therapeutic/tectonic and 12 for visual rehabilitation.

31 nflict with proposed young surface uplift by tectonic and climatic forcing but consistent with the Si

32 oint localities, which occur within the rich tectonic and depositional history of the Awash Valley.

33 ux of dissolved iron to seawater than active-tectonic and dysoxic continental margins.

34 t mantle heterogeneity and its links to past tectonic and geodynamic processes.

35 h this broad region has a relatively uniform tectonic and geologic history, the thermal regimes of it

36 s of 10(4)-10(7) years and is independent of tectonic and geomorphic setting.

37 ion, it can also reveal insights into former tectonic and geomorphological processes.

38 Upon evaluating the overlap between tectonic and Milankovitch periodicities across spreading

39 hese results highlight the crucial impact of tectonic and oceanographic processes on mangrove OC sequ

40 ion, and can be integrated into larger-scale tectonic and palaeoenvironmental studies.

41 r tectonic indications and risk factors for (tectonic and physiologic) graft failure.

42 pore water iron isotope data from a passive-tectonic and semi-arid ocean margin (South Africa), whic

43 ancient material have eluded destruction by tectonic and surface processes operating over billions o

44 early Earth are currently explained by plate tectonic and vertical tectonic models, but these do not

45 As continental rift zones mature the tectonic and volcanic processes associated with crustal

46 ral Asian Orogeny Belt (CAOB) due to varying tectonic and weathering controls.

47 of isolating the respective contributions of tectonics and climate to erosion.

48 h's surface archives the combined history of tectonics and erosion, which tend to roughen landscapes,

49 Pluto's large moon Charon displays tectonics and evidence for a heterogeneous crustal compo

50 alysing mantle convection, lubricating plate tectonics and feeding arc volcanism.

51 Geologic process, including tectonics and global climate change, profoundly impact t

52 Harrison et al. proposed that plate tectonics and granites existed 4.5 billion years ago (Ga

53 This drives surface tectonics and pre-conditions the margins for further def

54 e adiabatic value and is suggestive of plate tectonics and/or advective magmatic heat transport.

55 ort bed sediment, independently of climatic, tectonic, and bedrock controls.

56 d China and an assessment of the geomorphic, tectonic, and lithologic controls on quake-induced lands

57 opographic rings, dominate the stratigraphy, tectonics, and crustal structure of the Moon.

58 ents-is incompatible with modern-style plate tectonics, and favours instead the formation of TTGs nea

59 on, the generation of thinner crust by plate tectonics, and mantle overturn following solidification

60 ediment supply in feedbacks between climate, tectonics, and mountain landscape evolution.

61 and quantifiable part in shaping topography, tectonics, and seismic hazard within intraplate settings

62 mbbell shapes and are prepared by a parallel tectonic approach under ambient conditions.

63 ction (about 4 billion years ago) and global tectonics (approximately 3 billion years ago) suggests t

64 ly processes in real time to build arbitrary tectonic architectures.

65 together with crust recycling through plate tectonics, are the primary processes that drive the chem

66 rocks, suggesting the onset of global plate tectonics at ~3.0 billion years ago.

67 his gateway, together with subsiding volcano-tectonic barriers would have played a key role in Late C

68 y different before the onset of global plate tectonics because most present-day subduction initiation

69 entific theories of how subduction and plate tectonics began on Earth--and what the tectonic structur

70 ies to the center, squeezed up by more rigid tectonic blocks in the north and south.

71 The volcanoes that lie along the Earth's tectonic boundaries are fed by melt generated in the man

72 odology, to pinpoint interaction between the tectonic building blocks that construct the metal-organi

73 es quantitatively as a result of climatic or tectonic changes.

74 t, corresponding to independently determined tectonic changes.

75 us landscapes is a complex interplay between tectonics, climate and denudation.

76 While tectonics, climate, and rock-type influence silicate wea

77 on of depositional systems that may preserve tectonic, climatic and anthropogenic signals.

78 orogen with a well-documented late Cenozoic tectonic, climatic and glacial history.

79 ted damage and weak zones, promote increased tectonic complexity, such as oblique subduction, strike-

80 The relative influences of tectonics, continental weathering and seafloor weatherin

81 rong influence of climate in addition to the tectonic control, and we propose that the post Miocene C

82 y assumed to accurately record climatic- and tectonic-controlled mountain denudation and play an impo

83 across vast gulfs of time (dubbed the Wilson tectonic cycle), accompanied by inversion of extensional

84 as volatiles and phase assemblages) and how tectonic cycles drive its secular evolution are still de

85 hort-term fluctuations associated with plate tectonic cyclicity.

86 Seismic rupture produced spectacular tectonic deformation above a 400-kilometer strip of the

87 d rock uplift is important for understanding tectonic deformation in this region.

88 he Appalachian Structural Front, a proxy for tectonic deformation), distance to gas wells was highly

89 Our findings reveal the basin-scale tectonic, depositional and palaeoenvironmental history o

90 ence only subduction zones survive and plate tectonics does not spread, which corresponds to observat

91 ncreased organic burial and that alternative tectonic drivers (erosion, outgassing) provide testable

92 , including the North Sea, implying a common tectonic driving force.

93 tern that is contrary to that expected for a tectonic earthquake and which is dominated by an implosi

94 osion and other mining cavity collapses, and tectonic earthquakes are compared, and the separation of

95 age adjustment or other local (for example, tectonic) effects.

96 cs, as it gives insight into the geohistory, tectonic environment, geohazard mitigation, etc.

97 and imaged an interface that correlates with tectonic environment, varying from 95 +/- 4 kilometers b

98 l for nonvolcanic tremor exist in a range of tectonic environments.

99 lcanism only became widespread after a major tectonic episode of continental stabilization at the beg

100 , responsible for orocline formation and the tectonic escape of the back arc region, is imaged here f

101 ystem develops, as well as the mechanism for tectonic escape of the back-arc region.

102 The hiatuses coincide with regional tectonic events and changes in global thermohaline circu

103 features are well correlated with historical tectonic events in this region, such as extension along

104 actors such as climate and oceanographic and tectonic events shape larger-scale patterns regionally a

105 rent mantle provide more constraints on past tectonic events than previously recognized.

106 rs to be largely the result of ancient plate tectonic events that allowed time for convergent phenoty

107 s consistent with the extended timescales of tectonic evolution of the Antarctic margin, involving th

108 New constraints on the tectonic evolution of the Neo-Tethys Ocean indicate that

109 s may force a reexamination of models of the tectonic evolution of western North America over the las

110 and incorporated into mountain chains during tectonic exhumation.

111 uctions may be superimposed on a first-order tectonic fabric, we emphasize the difficulty of decipher

112 Risk factors for tectonic failure (18/362 eyes, 5.0%) were severe lid dis

113 ock friction have elucidated many aspects of tectonic fault zone processes and earthquake phenomena.

114 -resolution studies of elastic properties in tectonic fault zones may aid in the search for reliable

115 From field observations of a major tectonic fault, and using laboratory experiments and num

116 Tectonic faults also fail in slow earthquakes with ruptu

117 Dynamic stressing of tectonic faults may play a similar role in determining t

118 ke is a result of interplay among injection, tectonic faults, and foreshocks.

119 rthquakes and slow-slip events, occurs along tectonic faults.

120 ubglacial Mountains are the least understood tectonic feature on Earth, because they are completely h

121 How did the tectonic features form?

122 rn hemisphere with a distinct arrangement of tectonic features, intense heat flux, and geyser-like pl

123 d gives a unified explanation of the salient tectonic features, the plumes, and the transport of heat

124 eat flow or temperature; many are related to tectonic features.

125 chemical change that reveal shifts in global tectonic forces connecting Earth ocean-climate processes

126 icate weathering that regulates climatic and tectonic forcing through hydrologic processes and impose

127 red rates of vertical displacement caused by tectonic forcing, and their relationships are consistent

128 t of the Sturtian glaciation has suggested a tectonic forcing.

129 s is controlled by the erosional response to tectonic forcing.

130 consequence of the permeability generated by tectonic fracturing.

131 ation and provides a cohesive structural and tectonic framework defining its relationships to adjacen

132 Plate tectonics gives no insight, however, into where and when

133 mangroves are controlled by the interplay of tectonics, global sea level and sedimentation, including

134 r anatomically successful cases with central tectonic grafts, active corneal inflammation and donor s

135 in anatomically successful eyes with central tectonic grafts.

136 the absence of vigorous convection and plate tectonics has limited the scale of compositional mixing

137 diversification, to document how climate and tectonics have driven ecosystem and evolutionary dynamic

138 Such deviations in the continuity of plate tectonics have important consequences for Earth's therma

139 Thus, a mechanism that causes less efficient tectonic heat transport at higher temperatures may be re

140 ked to the variation of regional climate and tectonic history.

141 ognition of this plume force has substantial tectonic implications: the speed-up and slowdown of Indi

142 Subduction tectonics imposes an important role in the evolution of

143 sion central to the interplay of climate and tectonics in landscape evolution.

144 evious arguments for the importance of plate tectonics in the Cambrian radiation, namely the breakup

145 ision with Asia was a major driver of global tectonics in the Cenozoic and, we argue, of atmospheric

146 The operation of plate tectonics, in general, depends intimately on the manner

147 Outcomes of corneal transplantation for tectonic indications and risk factors for (tectonic and

148 Feedbacks between climate, erosion and tectonics influence the rates of chemical weathering rea

149 pine landscapes and, by linking climate with tectonics, influences a broad array of geophysical pheno

150 ution, the ocean-atmosphere system and plate tectonics is a central goal of Earth science.

151 ution of the planetary interior during plate tectonics is controlled by slow convection within the ma

152 narios for the onset of subduction and plate tectonics is hampered by the fact that subduction initia

153 Plate tectonics is regulated by driving and resisting forces c

154 A primary consequence of plate tectonics is that basaltic oceanic crust subducts with l

155 One of the most powerful features of plate tectonics is that the known plate motions give insight i

156 'RNA tectonics' is the design of modular RNA units, called te

157 heric plates and basaltic magmatism of plate tectonics, is a key unknown in the evolutionary history

158 confirm that lobate scarps are the dominant tectonic landform and record global contraction associat

159 scarps and associated meter-scale secondary tectonic landforms that include narrow extensional troug

160 Tectonic landforms, contractional wrinkle ridges and ext

161 The megathrust north of the Median Tectonic Line is interseismically locked, has a history

162 ents the offshore continuation of the Median Tectonic Line, which onshore juxtaposes geological terra

163 continental interiors, indicates that either tectonic loading rates or fault properties vary over a f

164 osed feedbacks among topography, climate and tectonics may occur.

165 er and Behn proposed that intermittent plate tectonics may resolve a long-standing paradox in Earth's

166 from clustered-Fe domains and 1,412+/-56 Ma (tectonic metamorphism) from planar and subgrain boundary

167 Most tectonic models have assumed that the subducting oceanic

168 tly explained by plate tectonic and vertical tectonic models, but these do not offer a global synthes

169 on spicules with skeletonlike morphology, 3D tectonic motifs, and reduced symmetries.

170 At plate margins, tectonic motions quickly reload earthquake ruptures, mak

171 ce might be ice warmed, melted or crushed by tectonic motions.

172 of the lithosphere as well as to present-day tectonic motions.

173 ism are typical surface expressions of plate tectonic movement on top of narrow plumes of hot materia

174 We argue that tectonic movements were the primary control on the clima

175 de a solution to a puzzling mystery of plate tectonics, namely why the oldest continents, in contrast

176 Tectonic 'non-volcanic' tremor, a recently discovered se

177 agnetic field, convective mantle, mobile lid tectonics, oceans of liquid water, dynamic climate and a

178 d to explain the complex oceanic-continental tectonics of these subduction zones.

179 The initiation of plate tectonics on Earth is a critical event in our planet's h

180 creation of short-wavelength relief by plate tectonics on Earth.

181 n the Southern Ocean that was enabled by the tectonic opening of key oceanic gateways during the brea

182 from greenhouse to icehouse climates to the tectonic opening of Southern Ocean gateways, more recent

183 rement interval complicates efforts to infer tectonic or climatic forcing from changes in rates of ri

184 les, while local, basin-scale changes (e.g., tectonic or hydrographic) and biotic interactions ruled

185 ies as a function of strain accommodation by tectonic or magmatic processes.

186 thern Sierra Nevada previously attributed to tectonic or mantle-derived forces is partly a consequenc

187 Ideas leading to the hypothesis of plate tectonics originated largely with an oceanic focus, wher

188 been common since the onset of modern plate tectonics, our findings suggest that similar processes m

189 eveal scant atmosphere, no evidence of plate tectonics, past evidence for abundant water, and a protr

190 The tectonic patterns and stress history of Europa are excee

191 lineaments, suggesting that many of Europa's tectonic patterns may also be related to true polar wand

192 on-deformation relationship is influenced by tectonic, petrological and volcanic factors.

193 rofiles across the asthenosphere for various tectonic plate ages.

194 Earthquakes far from tectonic plate boundaries generally exploit ancient faul

195 urface that show no obvious association with tectonic plate boundaries.

196 The direction of tectonic plate motion at the Earth's surface and the flo

197 us convection within the mantle is linked to tectonic plate motions and deforms Earth's surface acros

198 in which the lithosphere comprised a single tectonic plate, with only the warmer, lower crust involv

199 Tectonic plates are a key feature of Earth's structure,

200 The stretching and break-up of tectonic plates by rifting control the evolution of cont

201 te boundaries and eventually to fully formed tectonic plates driven by subduction alone.

202 thenospheric layer underlying Earth's mobile tectonic plates is fundamental to our understanding of m

203 Because the inertia of tectonic plates is negligible, plate velocities result f

204 The majority are believed to form as Earth's tectonic plates move over long-lived mantle plumes: buoy

205 Tectonic plates that fragment ancestral ranges (vicarian

206 lling due to viscous drag from the diverging tectonic plates, but have been challenged by geophysical

207 sliding of rock masses at a boundary between tectonic plates.

208 rrestrial systems, we demonstrate that plate tectonics played a major role in driving tropical marine

209 w subduction zones initiate is a fundamental tectonic problem, yet there are few well-constrained geo

210 it is the result of the large compressional tectonic process.

211 discoveries allow us to understand regional tectonic processes and highlight the importance of satel

212 ks between tropical reef availability, plate tectonic processes and marine biodiversity distribution

213 Normal plate tectonic processes are responsible both for plate bounda

214 tan plateau provides direct insight into the tectonic processes associated with continent-continent c

215 eformation within mountain ranges relates to tectonic processes at depth is not well understood.

216 We hypothesize that active tectonic processes in the south polar terrain of Encelad

217 time of global climatic changes and ongoing tectonic processes that formed the East African Rift.

218 The degree to which short-term non-tectonic processes, either natural and anthropogenic, in

219 deformation and flow patterns resulting from tectonic processes, large-scale observations have been l

220 ing the presence of shear related to current tectonic processes, whereas in the lithosphere (80-200 k

221 cured or destroyed by surface weathering and tectonic processes.

222 butions and is associated with deeply rooted tectonic processes.

223 that are not directly associated with plate tectonic processes.

224 e morphology may be used to infer changes in tectonic rates.

225 crustal perspective must balance slow (plate tectonic) rates of melt generation and segregation in th

226 ls crustal features at depth that aid in the tectonic reconstruction of southern California, such as

227 Here we infer from a tectonic reconstruction of the Andes constructed in a ma

228 ls embedded with the latest geological paleo-tectonic reconstructions and ground-truthed with new Hf-

229 and quadrupole moments of plate motions from tectonic reconstructions extended back to the early Meso

230 The timing is consistent with recent tectonic reconstructions of a relatively narrow Central

231 e global length of subduction zones in plate tectonic reconstructions, and by sea-level inversion.

232 progressive accumulation of new crust or the tectonic recycling of old crust.

233 ng to show that this can be explained by the tectonic recycling of previously accumulated sedimentary

234 rogeneity is continually introduced by plate tectonic recycling, and redistributed by viscous stretch

235 nates from partial melt extraction and plate tectonic recycling, whereas stirring during mantle conve

236 Here, however, we show that the contrast in tectonic regime between primarily strike-slip faulting i

237 ial of early Martian crust in a stagnant-lid tectonic regime, in which the lithosphere comprised a si

238 he range of expected temperatures in various tectonic regions.

239 Valentine and Moores hypothesized that plate tectonics regulates global biodiversity by changing the

240 ountain belts, emphasizing the importance of tectonic regulation of global climate over geologic time

241 provide new insight into strike-slip volcano-tectonic relations by analysing Bouguer gravity data fro

242 iring definitive field evidence of an active tectonic response to global climate cooling has been elu

243 Its causes remain unresolved, with tectonic restrictions to the Atlantic Ocean or glacio-eu

244 nderstood more than 40 years after the plate tectonic revolution.

245 a combination of multiple forcings, such as tectonics, sea-level fall and long-term decline in green

246 pedition divided the Gakkel ridge into three tectonic segments, composed of robust western and easter

247 mental controls on magma metal fertility are tectonic setting, the nature of source rocks, and magma

248 -constrained geologic tests that address the tectonic settings and dynamics of the process.

249 ence the occurrence of earthquakes in active tectonic settings or 'stable' plate interiors, remains a

250 centrations of magmas formed in a variety of tectonic settings using in situ trace-element measuremen

251 artial melting is predicted to occur in many tectonic settings, and in both the crust and the mantle,

252 that eleven terrestrial samples from diverse tectonic settings, including five early Archean samples

253 In both tectonic settings, our results indicate that fractional

254 ent continental lithosphere in certain plate tectonic settings.

255 nd melt inclusions covering a range of plate tectonic settings.

256 esented here may also be applicable in other tectonic settings.

257 evolution of the Earth's crust in a range of tectonic settings.

258 measured uplift is potentially attributed to tectonic shortening, lithospheric delamination and unloa

259 Further quantification of tissue tectonics showed patterns of rotations, contractions and

260 ving northwestward 11 mm a(-1) as part of a tectonic sliver.

261 In analogy to plate tectonics, smooth macroscopic-scale crystalline glide ar

262 he Mesozoic and later, long-lasting relative tectonic stability.

263 se is important for understanding when plate tectonics started and how the supply of nutrients to the

264 When plate tectonics started on Earth has been uncertain, and its r

265 ntial portion of the spreading may be due to tectonic stress building up to a critical level rather t

266 least 35 kilometres of the ridge axis, where tectonic stress had built up to a critical level, trigge

267 The roles of magma pressure and tectonic stress in the development of seafloor spreading

268 ation generates large (approximately 10 MPa) tectonic stress patterns that are compatible with the ob

269 Tarim Basin rather than in the compressional tectonic stress regime as in the periphery of the Tarim

270 , nearby fault that is experiencing regional tectonic stress.

271 rocks, as well as regions where magmatic and tectonic stresses create fractures that increase porosit

272 tions predict these results, suggesting that tectonic stresses interact with topography to influence

273 hy where the ratio of horizontal compressive tectonic stresses to near-surface gravitational stresses

274 plate tectonics began on Earth--and what the tectonic structure of Earth was before this--remain enig

275 The spatial pattern of magmatic-tectonic structures bounding Procellarum is consistent w

276 ravity models are powerful tools for mapping tectonic structures, especially in the deep ocean basins

277 features not previously resolved, including tectonic structures, volcanic landforms, basin rings, cr

278 is a crucial component of the Earth's plate tectonic style of mantle convection.

279 ove organic carbon (OC) was promoted by high tectonic subsidence and fluvial sediment supply.

280 Plate tectonics successfully describes the surface of Earth as

281 s are some of the weakest parts of the plate tectonic system, but previous studies have not favored t

282 sphere is one of the central themes of plate tectonics, the recycling of continental lithosphere appe

283 uch as the separation of continents by plate tectonics, the uplift of mountains or the formation of l

284 challenging, as it requires extending plate tectonic theory to the dynamics of continental deformati

285 For plate tectonics to operate on a terrestrial planet, the surfac

286 s from mantle flow beneath, and allows plate tectonics to work.

287 Our study does not disprove coupling between tectonic uplift and erosion but suggests that this coupl

288 ss balance is also significantly affected by tectonic uplift and erosion via changes to the inorganic

289 ination of a permanent El Nino state or with tectonic uplift are not large enough to contribute signi

290 California, United States, to assess whether tectonic uplift history can be reconstructed using measu

291 than today at 125 ka indicating net maximum tectonic uplift of 19 m with an average rate of 0.015

292 thering, this source is probably enhanced by tectonic uplift, and so may have contributed to the rela

293 eathering that are consistent with increased tectonic uplift, more rapid continental denudation, incr

294 and slow cooling, which gives rise to plate tectonics, volcanoes and mountain building.

295 preserved, these results suggest that plate tectonics was operating as early as Paleoarchean times,

296 ic continental crust is the product of plate tectonics, whereas the Moon acquired its feldspar-rich c

297 nvection provides the mechanism behind plate tectonics, which allows oceanic lithosphere to be subduc

298 e, however, an update of the theory of plate tectonics would be expected with continuing discovery of

299 key role in terrestrial magmatism and plate tectonics, yet despite experimental demonstration of the

300 ght to play an important part in the Earth's tectonics, yet it has been difficult to isolate the effe