ライフサイエンスコーパス: turbulent

1 and non-motile species when conditions turn turbulent.

2 t higher speeds that the entire flow becomes turbulent.

3 recent claims that these scales are strongly turbulent.

4 Experiments and numerical simulations of turbulent (4)He and (3)He-B have established that, at hy

5 es at two sites connected via a time-varying turbulent air path.

6 s and frequencies, such as aircraft wings in turbulent air.

7 ts that this stable state is often born from turbulent and conflicting origins, and that the apparent

8 ents of the three-dimensional flow fields of turbulent and laminar jets covering the Re range 10-10(4

9 ydrodynamic profile within the device is not turbulent and provides an analytical platform for the in

10 tances such as: calcium, copper and iron, 7. turbulent and rapid blood or CSF flow 8. air-containing

11 al periodic pattern and its evolution into a turbulent array of topological defects, and (iv) birefri

12 of compressive fluctuations are observed in turbulent astrophysical plasmas (most vividly, in the so

13 the boundary layers themselves become fully turbulent at very high values of the Rayleigh number [Fo

14 arge-scale polygonal jet forms in the highly turbulent atmosphere of Saturn is lacking.

15 promising new method relying on overlapping turbulent back-trajectories of pathogen-laden parcels of

16 ponding blood damage index (BDI) in stenotic turbulent blood flow.

17 the direct comparison of a freely expanding turbulent Bose-Einstein condensate and a propagating opt

18 commonality between wave chaos, polymers and turbulent Bose-Einstein condensates.

19 scovery, in the inner layer of the developed turbulent boundary layer, of what we call turbulent-turb

20 row and merge downstream to become the fully turbulent boundary layer.

21 Here we observe the emergence of a turbulent cascade in a weakly interacting homogeneous Bo

22 nvariant fluxes are the defining property of turbulent cascades, but their direct measurement is a ch

23 Our measurements, from a multiphase, turbulent cloud chamber, show a clear transition from a

24 tigated in a laboratory chamber that enables turbulent cloud formation through moist convection.

25 The measurements reveal that turbulent clouds are inhomogeneous, with sharp transitio

26 Here, we propose that turbulent coherent structures, long-lasting flow pattern

27 Turbulent conditions (high Reynolds number) in these mia

28 ion polarization is minimized by encouraging turbulent conditions and by reducing the amount of water

29 e particle TD prediction in both laminar and turbulent conditions.

30 We compare turbulent convection in air at Pr=0.7 and in liquid merc

31 We find that turbulent convection in the magnetostrophic regime is, i

32 of Earth and other planets are generated by turbulent convection in the vast oceans of liquid metal

33 The global transport of heat and momentum in turbulent convection is constrained by thin thermal and

34 Turbulent convection is often present in liquids with a

35 y liquid (hydrofluoroether) to a water-based turbulent convection system, a remarkably efficient biph

36 hich quantifies the influence of rotation on turbulent convection.

37 pheric boundary layer by numerical models of turbulent convective flow and combine them with model-fr

38 The fields originate in the turbulent convective layers of stars and have a complex

39 he Earth's core conditions, we find that the turbulent convective length scale in the absence of magn

40 ases very rapidly at smaller scales, so this turbulent convective length scale is a lower limit for t

41 ores remains out of reach, the fact that the turbulent convective length scale is independent of the

42 However, the inhomogeneous turbulent corona strongly affects the propagation of the

43 tive study of the mechanisms that create the turbulent coronal medium through which the emitted radia

44 that motile species may actively respond to turbulent cues to avoid layers of strong turbulence.

45 Turbulent curtains of smoke rise initially as flat plume

46 ted condition, the streamwise and transverse turbulent diffusion coefficients are of the same order o

47 A critical mixing state, in which turbulent diffusion is gradually replaced by double-diff

48 flow employs a statistically-stable model of turbulent diffusion that has been extant since the 1960s

49 pecifically, in contrast to predictions from turbulent diffusion theory, self-sharpened velocity and

50 In contrast, the transverse turbulent diffusion was enhanced, despite the reduction

51 his contributed to a reduction in streamwise turbulent diffusion, relative to the unobstructed condit

52 contaminants and source apportionment using turbulent diffusion.

53 re exposed; (3) nearshore turbulence is low (turbulent diffusivities approximately 10(-3) m(2) s(-1))

54 g experiment in the Southern Ocean found the turbulent diffusivity inferred from the vertical spreadi

55 ional losses; (2) incorporate the effects of turbulent dispersion; (3) simulate the locations of the

56 Turbulent dissipation in long-lived slots helps maintain

57 Turbulent dissipation makes testable predictions for the

58 kthroughs have come from models invoking the turbulent dissipation of Alfven waves.

59 ive statistical control strategy for complex turbulent dynamical systems based on a recent statistica

60 Turbulent dynamical systems characterized by both a high

61 This result applies to general inhomogeneous turbulent dynamical systems including the above applicat

62 In such inhomogeneous turbulent dynamical systems there is a large dimensional

63 s associated with high-dimensional nonlinear turbulent dynamical systems with conditional Gaussian st

64 In complex turbulent dynamical systems, it is impossible to track a

65 the prediction of extreme events in complex turbulent dynamical systems.

66 esponse to changing aerosols are impacted by turbulent dynamics of the cloudy atmosphere, but integra

67 forcing regimes with various types of fully turbulent dynamics with nearly one-half of the phase spa

68 growth and sustainment through an efficient turbulent dynamo instability are possible in such plasma

69 10(-6) (W kg(-1)), above which the smallest turbulent eddies limit aggregate size.

70 ts in the ocean, which spontaneously develop turbulent eddies through the baroclinic instability.

71 this study is to investigate the anatomy and turbulent effects on polydisperse particle transport and

72 y measure the transfer of energy between the turbulent electromagnetic field and electrons in the Ear

73 ical and aerodynamic surface properties, and turbulent energy fluxes of a lowland boreal forest regio

74 How turbulent energy is dissipated in weakly collisional spa

75 ent spots are generated locally in the fully turbulent environment, and they are persistent with a sy

76 d interactions are probably important in the turbulent environments commonly encountered in natural h

77 locate the source of odor cues in realistic turbulent environments-a common task faced by species th

78 ning to navigate complex, highly fluctuating turbulent environments.

79 quantifying the degree of risk affordable in turbulent environments.

80 hat permit effective control over soaring in turbulent environments.

81 obust interfacial adhesion under dynamic and turbulent environments.

82 for the ability of copepods to reproduce in turbulent environments.

83 Turbulent events in the ocean also exhibit a second char

84 l bidnavirus genes and uncover an unexpected turbulent evolutionary history of these unique viruses.

85 output where the dominant structures in the turbulent field are emphasized.

86 orrect small-scale properties of atmospheric turbulent flow and solar irradiance, and retain consiste

87 thetic drag reducing polymers in large scale turbulent flow applications.

88 mum stationary film thickness) to establish turbulent flow at Reynolds numbers (Re) as high as 9000.

89 drupole-tandem mass spectrometry with online turbulent flow chromatography for sample cleanup and ana

90 comparable drag reduction performance under turbulent flow conditions as aqueous PEO solutions, whil

91 tion of previously unimaginable shock-driven turbulent flow fields that are of significant importance

92 at, in both B. subtilis and P. aeruginosa, a turbulent flow forms in the tube and a zone of clearing

93 rizontal transport properties of the oceanic turbulent flow in which they are embedded.

94 e mixing but less well the manner in which a turbulent flow influences it; but the latter is the more

95 Transition from laminar to turbulent flow occurring over a smooth surface is a part

96 theory assumes that energy transport in a 3D turbulent flow proceeds through a Richardson cascade whe

97 ll-mixed yet simple microfluidic device with turbulent flow profiles in the reaction regions.

98 f thinner yet denser biofilms under high and turbulent flow regimes of drinking water, in comparison

99 Here, we consider bubble pinch-off in a turbulent flow representative of natural conditions in t

100 cts were injected directly into an automated turbulent flow sample clean-up system, coupled to a liqu

101 y Simulation (ILES) is proposed for unsteady turbulent flow simulations involving the three-dimension

102 en qualitatively visualizing the large-scale turbulent flow structures around full-scale turbines do

103 Turbulent flow through vegetation are characterized by a

104 A method utilizing turbulent flow to perform ultrafast separations and scre

105 Upon crossing the laminar-to-turbulent flow transition regime, a significant reductio

106 that are interspersed in a smoother and less turbulent flow with a near-radial magnetic field.

107 olisms for early life in a simple model of a turbulent flow, and find that balancing the turnover tim

108 The turbulent flow, characteristic of active nematics, is in

109 ated by shear stresses in highly fluctuating turbulent flow, has not been feasible.

110 In two-dimensional turbulent flow, the seemingly random swirling motion of

111 ive control strategies for drag reduction in turbulent flow.

112 vides a way to quantify irreversibility in a turbulent flow.

113 Understanding turbulent flows arising from random dispersive waves tha

114 IPS pipe capable of withstanding laminar and turbulent flows for 180 and 90 minutes, respectively.

115 which corresponds to sediment particles and turbulent flows impacting along the riverbed where the r

116 Turbulent flows in nature and technology possess a range

117 es a new scenario that can be common to many turbulent flows in photonic quantum fluids, hydrodynamic

118 Variability of turbulent flows in the atmosphere and oceans exhibits re

119 In the present work, we study three turbulent flows of systematically increasing complexity.

120 he universal statistical properties that all turbulent flows share despite their different large-scal

121 These results were obtained for turbulent flows with Reynolds numbers 10,000 to 32,500.

122 Enstrophy is an intrinsic feature of turbulent flows, and its transport properties are essent

123 the velocity time series of fully-developed turbulent flows, generated by (i) a regular grid; (ii) a

124 of oil-particle aggregates (OPAs) formed in turbulent flows, we elucidated a new mechanism of partic

125 a universal description of extreme events in turbulent flows.

126 s an experimental challenge in particular in turbulent flows.

127 ar self-organization, defines a new class of turbulent flows.

128 tanding of the onset of turbulence and fully turbulent flows.

129 nsive drag reducers in large Reynolds number turbulent flows.

130 ures is fundamental to the energy cascade in turbulent flows.

131 ns where a large-scale ensemble mean and the turbulent fluctuations exchange energy and strongly infl

132 ction (pdf) for its fluctuations whereas the turbulent fluctuations have decreasing energy and correl

133 l models involve a large-scale mean flow and turbulent fluctuations on a variety of spatial scales wi

134 ion of thermals unavoidably generates strong turbulent fluctuations, which constitute an essential el

135 change between the mean flow and the related turbulent fluctuations.

136 Turbulent fluid flows are ubiquitous in nature and techn

137 energy of a small fluid particle moving in a turbulent fluid.

138 nes, vortex lines and magnetic flux tubes in turbulent fluids and plasmas display a great amount of c

139 it consists of two coupled, interpenetrating turbulent fluids: the first is inviscid with quantized v

140 measurements of aerosol solar absorption and turbulent fluxes have not been reported thus far.

141 cted to look at wind patterns, mean flow and turbulent fluxes of momentum and energy.

142 of the surface energy balance (radiative and turbulent fluxes) reveals that surplus energy that can h

143 satlantic flight corridor by creating a more turbulent flying environment for aircraft.

144 approximation for extremely high-dimensional turbulent forecast models.

145 Observational evidence for turbulent fragmentation on scales of more than 1,000 ast

146 em with nonlinear propagation (advection) of turbulent fronts.

147 A protostar is formed in the dense, turbulent gas cloud, and it grows by sporadic mass accre

148 e star systems: large-scale fragmentation of turbulent gas cores and filaments or smaller-scale fragm

149 iolent gravitational instabilities in highly turbulent gas-rich disks.

150 s motility displayed by droplet-encapsulated turbulent gels [12].

151 Inspired by in vitro work on active turbulent gels of microtubules and kinesin [12, 13], we

152 We have performed a set of turbulent global simulations that exhibit magnetic cycle

153 The increased turbulent heat flux is used to increase air temperature

154 effect of sea ice loss and associated upward turbulent heat fluxes are relatively minor in this event

155 biphasic dynamics is born, which supersedes turbulent heat transport by up to 500%.

156 We find that turbulent heating is sufficient to offset radiative cool

157 lasma via Alfvenic turbulence: Collisionless turbulent heating typically acts to disequilibrate the i

158 e reduction in length-scale, due to enhanced turbulent intensity and the transverse deflection of flo

159 energy is trapped at large scales-nonlinear turbulent interactions transfer energy to larger scales,

160 showed relatively slower flow, IRMAs showed turbulent, intermediate to slow flow, and venous beading

161 Yet, detailed analyses of the turbulent, intermittent structure of water- and air-born

162 e quantum entanglement encoded in OAM over a turbulent intracity link of 3 km.

163 This study presents and analyzes turbulent jets issued into an obstructed cross-flow, wit

164 flux into the North Pacific basin and 55% of turbulent kinetic dissipation rate in the thermocline, s

165 Turbulent kinetic energy (TKE), assessed by 4-dimensiona

166 entropy increases as the square root of the turbulent kinetic energy and is directly related to the

167 nhances aggregate formation up to a critical turbulent kinetic energy dissipation rate of 10(-6) (W k

168 March with no CAP indicates that the average turbulent kinetic energy during the CAP was suppressed b

169 e UAV and surface data reveal a reduction in turbulent kinetic energy in the surface mixed layer at t

170 flow degree, helicity, maximal velocity, and turbulent kinetic energy were evaluated to characterize

171 Our simulations demonstrate that the turbulent Kolmogorov-like cascade is extended both at th

172 . akashiwo to increase the chance of evading turbulent layers by diversifying the direction of migrat

173 from their constituent elements and exhibit turbulent-like and chaotic patterns.

174 s have reached the magnetostrophic regime in turbulent liquid metal convection.

175 designed to be accessible for people facing turbulent lives with multiple problems.

176 nt results from the first, to our knowledge, turbulent, magnetostrophic convection experiments using

177 nting is that clouds themselves are complex, turbulent, microphysical entities and, by their very nat

178 e index of refraction of water or air due to turbulent microstructure can lead to so-called optical t

179 geometry, and in their absence Eg5 powers a turbulent microtubule network inside mitotic cells.

180 eletion, the mitotic microtubule network is "turbulent"; microtubule bundles extend and bend against

181 It is an open question whether turbulent mixing across density surfaces is sufficiently

182 ng vertical and horizontal currents, and the turbulent mixing caused by their breaking, they affect a

183 We show that turbulent mixing during cloud assembly naturally produce

184 presents observational data to quantify the turbulent mixing during two CAP episodes in Utah's Salt

185 f uniformity and stability because the rapid turbulent mixing facilitated a homogeneous distribution

186 Turbulent mixing in the ocean is key to regulate the tra

187 strong vertical and horizontal currents and turbulent mixing in the ocean.

188 by shear forces occurring in flow or during turbulent mixing of polymersome dispersions.

189 We propose that turbulent mixing of the seamount sheath-water stimulates

190 This internal structure may originate from turbulent mixing processes that encouraged outwardly exp

191 vity), point out some fundamental aspects of turbulent mixing that render it difficult to be addresse

192 In particular, we examine turbulent mixing when the substance is a scalar (i.e., c

193 atmospheric clouds are largely determined by turbulent mixing with their environment.

194 s vigorous lateral export, rapid dilution by turbulent mixing, and finally settling of meltwater at d

195 We focus here on turbulent mixing, with more attention paid to the postmi

196 This is the simplest paradigm of turbulent mixing.

197 ake's thermodynamical properties by means of turbulent mixing.

198 w have exceeded the inherent limits posed by turbulent-mixing.

199 proved to be a tipping point for an already turbulent mixture, leading to an abrupt and uncontrolled

200 ttency of the small-scale fluctuations where turbulent modes with small variance have relatively freq

201 The term quantum turbulence denotes the turbulent motion of quantum fluids, systems such as supe

202 ar advection of the particle distribution by turbulent motions.

203 o Pr suggest that the modelling strategy for turbulent natural convection of gaseous fluids may not b

204 ot be equally well suited for simulations of turbulent natural convection of liquids with high values

205 s a high degree of coherence in spite of the turbulent nature of the solar convection zone.

206 ], we explore the kinematics of this in vivo turbulent network.

207 nd detection of structured images mixed with turbulent noise.

208 f Laguerre-Gaussian spatial modes mixed with turbulent noise.

209 loyed by flying insects when foraging within turbulent odor plumes.

210 f encoding time at intervals relevant to the turbulent odor world in which many animals live.

211 ns (in the case of diffuse aurora) or by the turbulent or stochastic downward acceleration of electro

212 Here, we (1) suggest that this turbulent period owes to conflict, between a woman's mat

213 of a strong instability leading to a laminar-turbulent phase transition through a self-consistently d

214 io that explains the transformation to fully turbulent pipe flow and describe the front dynamics of t

215 ostrophic state is the natural expression of turbulent planetary dynamo systems.

216 dau damping could play a significant role in turbulent plasma heating, and that the technique is a va

217 collision of two laser-driven high-velocity turbulent plasma jets.

218 ectrons in a weakly collisional, magnetized, turbulent plasma?

219 biological and physical systems, from DNA to turbulent plasmas, as well as in climbing, weaving, sail

220 intermittent structures formed in magnetized turbulent plasmas, where the turbulence energy cascaded

221 Using detailed data from a turbulent plume created in the laboratory, we reconstruc

222 For turbulent plumes and jets, the transition distance scale

223 's diameter, as influenced by the convective turbulent plumes in the rural area.

224 ming algorithm with physical measurements of turbulent plumes, we determine the optimal strategy for

225 transport conditional on flow topologies in turbulent premixed flames has been analysed using a Dire

226 rgy budget of the resolved velocity field in turbulent premixed flames is investigated.

227 s), the competition between self-gravity and turbulent pressure along the dynamically dominant interc

228 Understanding the complexity of anisotropic turbulent processes in engineering and environmental flu

229 Understanding the complexity of anisotropic turbulent processes over a wide range of spatiotemporal

230 Here we use observations of the turbulent properties of the meltwater outflows from bene

231 repeater over a realistic high-loss and even turbulent quantum channel.

232 close analogy existing between an expanding turbulent quantum gas and a traveling optical speckle mi

233 measurement for a direct energy cascade in a turbulent quantum gas.

234 t numerical simulations of three-dimensional turbulent Rayleigh-Benard convection flows in a slender

235 We explore heat transport properties of turbulent Rayleigh-Benard convection in horizontally ext

236 near response drives the system from a fully turbulent regime, featuring a sea of coherent small-scal

237 separation remains in the strongly nonlinear turbulent regime, provided there is sufficient drag at t

238 e for nonlinear blended filtering in various turbulent regimes with at least nine positive Lyapunov e

239 However, there is also evidence of quantum turbulent regimes without Kolmogorov scaling.

240 g this transition, the front dynamics of the turbulent regions and the transformation to full turbule

241 ansitioning and very low Reynolds number but turbulent regions.

242 The CH(+) absorption lines reveal highly turbulent reservoirs of cool (about 100 kelvin), low-den

243 An alternative explanation is that turbulent Richardson advection brings field lines implos

244 than this instability scale are energized by turbulent scale interactions.

245 nd droplet size distribution at the smallest turbulent scales, thereby observing their response to en

246 Turbulent SFC provides a separation method for users des

247 Recent laboratory experiments in weakly turbulent shallow water reveal a remarkable transition f

248 Turbulent shear does not boost settlement by itself.

249 and isotropic turbulence in a periodic box, turbulent shear flow between two parallel walls, and the

250 sea is low in energy, it also can be highly turbulent, since the vertical density gradient which sup

251 Analyzing highly-resolved numerical turbulent solutions to Navier-Stokes equations, we find

252 Finally, we see that turbulent spindles can drive both flow of cytoplasmic or

253 We find that turbulent spindles display decreased nematic order and t

254 esin-5 Eg5, and that acute Eg5 inhibition in turbulent spindles recovers spindle geometry and stabili

255 fined herein, we found that the transitional-turbulent spot inception mechanism is analogous to the s

256 hairpin vortex, and subsequently grow into a turbulent spot, which is itself a local concentration of

257 s infected by a nearby existing transitional-turbulent spot.

258 Results provide evidence that turbulent spots exhibit high-Reynolds-number fractal-sca

259 mechanisms for the inception of transitional-turbulent spots found here.

260 ructurally quite similar to the transitional-turbulent spots, these turbulent-turbulent spots are gen

261 rowth and spreading of existing transitional-turbulent spots.

262 laminar regime to a non-desirable disordered turbulent state.

263 t transition arriving at the fully developed turbulent state.

264 cological and biogeochemical consequences of turbulent stirring is the horizontal dilution rate, whic

265 ease with M(2/3) times the bulk speed of the turbulent stream that carries the eddy.

266 Using recent insights from gas exchange in turbulent streams, we found that areal CO(2) evasion flu

267 t a detailed internal space map, searches in turbulent streams.

268 When turbulent stresses are less able to be counteracted by s

269 ts has been assumed as indicative of dilute, turbulent, supercritical flows causing traction-dominate

270 els can account for the unusual behaviour of turbulent superfluid helium.

271 t expansion branch, to reduce the complex 3D turbulent superstructure to a temporal planar network in

272 lar attention is paid to the slowly evolving turbulent superstructures-so called because they are lar

273 e is also useful for multiscale filtering of turbulent systems and a simple application is sketched b

274 features of vastly more complex anisotropic turbulent systems in a qualitative fashion.

275 ture key features of vastly more complicated turbulent systems.

276 ation, and data assimilation for anisotropic turbulent systems.

277 eem to have a better prognosis than the less turbulent temperamental symptoms of the disorder.

278 w field, but after the pinch-off starts, the turbulent time at the neck scale becomes much slower tha

279 Physician reimbursement is in a turbulent time.

280 ently three-dimensional transition from bulk-turbulent to confined-coherent flows occurs concomitantl

281 ence of the scales of fish on the laminar-to-turbulent transition in the boundary layer is investigat

282 s in a motion that is otherwise dominated by turbulent transport allows for the possibility of active

283 elopments would enable continuum modeling of turbulent transport at interfaces to incorporate the rel

284 mate is to properly include the eddy-induced turbulent transport of properties like heat, moisture, a

285 Turbulent transport of SO2 to the leaf boundary layer an

286 re important than large initial velocity and turbulent transport with dilute suspension in promoting

287 These turbulent-turbulent spots are dense concentrations of sm

288 r to the transitional-turbulent spots, these turbulent-turbulent spots are generated locally in the f

289 ed turbulent boundary layer, of what we call turbulent-turbulent spots.

290 of the indentation pockets arising from the turbulent-turbulent spots.

291 te, which we model accurately by superposing turbulent velocity and organism motion.

292 ture, the observed spectra of the superfluid turbulent velocity at sufficiently large length scales a

293 The mean turbulent velocity fields are shown to be self-similar a

294 In contrast, the square sum of the turbulent viscous shear stress (TVSS), which is used for

295 erature-dependent transition from laminar to turbulent vortex motion and the decoupling from the refe

296 t open question concerns what happens in the turbulent waters of the surface ocean.

297 rtically reorient while sinking from surface turbulent waters to a more stable environment (i.e., und

298 retention on the amended site can be low in turbulent waters.

299 mportant connection between highly nonlinear turbulent wave systems, possibly with no discernible dis

300 kely due to regional mixing of pollutants in turbulent weather conditions.