ライフサイエンスコーパス: convective

1 by increasing both viscous pressure drop and convective acceleration pressure drop.

2 nced evapotranspiration, precipitable water, convective activity and rainfall, indicative of amplifie

3 During the Holocene epoch, convective activity appears to track changes in spring a

4 al-eastern Pacific Ocean is mainly driven by convective activity related to ENSO and that the barotro

5 Convective activity, as inferred from oxygen isotopes, r

6 nd circulation exerts a positive feedback on convective aggregation and favors the maintenance of str

7 The extent of denaturation of WPI in convective air drying (65 and 80 degrees C) and isothera

8 enaturation of whey protein isolate (WPI) in convective air drying environments was measured and anal

9 r 600s and compared with those obtained from convective air drying.

10 g and cooling induced by a tungsten lamp and convective air source, respectively.

11 ng of the air surrounding the pileus creates convective airflows capable of carrying spores at speeds

12 n sequence star that emerges is nearly fully convective and chemically homogeneous.

13 ields of these planets originate from a thin convective and conducting shell of material around a sta

14 apply visualization and modeling methods for convective and diffusive flows to public school mathemat

15 lity and cell viability; characterization of convective and diffusive mass transfer of small and larg

16 ractions) and the tissue and systemic scale (convective and diffusive transport of NPs) are analyzed

17 sited on the surface depends on the rates of convective and diffusive transport to the surface and bi

18 Respiratory system cooling occurs via convective and evaporative heat loss, so right-to-left s

19 d by the occurrence of possibly two regimes: convective and hydrodynamic chromatography (HDC) regimes

20 as an atmospheric response to the equatorial convective anomalies is seen advecting cold temperatures

21 at as the surface temperature increases, the convective anvil clouds shrink.

22 en insects are migrating in a well-developed convective atmosphere at high altitude, they become much

23 In fine warm weather, the daytime convective atmosphere over land areas is full of small m

24 speeds of 1.7 million insects in the daytime convective atmospheric boundary layer using vertical-loo

25 ation with elevation is caused by increasing convective available potential energy (CAPE) and decreas

26 We also find that days with high convective available potential energy (CAPE) and strong

27 by 3-24 h when vertical wind shear (VWS) and convective available potential energy (CAPE) are moderat

28 le and characterized by larger values of the convective available potential energy (CAPE) due to grea

29 lightning flash rate is proportional to the convective available potential energy (CAPE) times the p

30 e potential for intense thunderstorms is the convective available potential energy (CAPE).

31 In general, we find that the convective behavior of liquid metal differs substantiall

32 ring is commonly observed in the atmospheric convective boundary layer on warm, sunny days.

33 del of weakly-flying insect movements in the convective boundary layer; a model which is consistent w

34 Convective cells can transport spores from gaps that may

35 r plumes of warm, pure ice called diapirs or convective cells in a thick (>10 kilometres) shell is in

36 are flying, as a succession of fair-weather convective cells pass over the recording site in Oklahom

37 ome from studying the Sun: about two million convective cells with typical sizes of around 2,000 kilo

38 sands of times larger than those on the Sun) convective cells, owing to low surface gravity.

39 information about the physical origin of the convective cells.

40 re similar to self-organized Rayleigh-Benard convective cells.

41 Seismicity localization should occur where convective changes in vertical normal stress are modulat

42 ast, solutions without CO2 develop elongated convective channels known as wormholes, with low breakth

43 he leading edge of a slowly drifting complex convective cloud close to the highest regions at 17 km

44 vations, the roles of ecosystem Hs and LE on convective cloud formation are explored relative to the

45 eneration of hypotheses about the impacts on convective cloud formation driven by afforestation/defor

46 s (echo tops) suggests that droplets in high convective cloud tops scavenge GOM from above the mixing

47 Deep convective clouds (DCCs) play a crucial role in the gene

48 while the tropics have been nearly devoid of convective clouds and have shown an abundance of wind-ca

49 ive forcing is reduced, or "masked," by deep-convective clouds and high humidity; in subsiding region

50 sical and microphysical properties of summer convective clouds and precipitation in the tropics and m

51 ger because the atmosphere is drier and deep-convective clouds are infrequent.

52 orecast model reveal that the increased deep convective clouds are reproduced when accounting for the

53 be first-order controls on the formation of convective clouds in the atmospheric boundary layer.

54 gh-altitude cirrus clouds and anvils of high convective clouds in the tropics and midlatitudes, humid

55 nd that TMLCs are formed by detrainment from convective clouds near the zero-degree isotherm.

56 by a ring of high clouds (the eye wall), and convective clouds outside the eye.

57 We show here a trend of increasing deep convective clouds over the Pacific Ocean in winter from

58 erosol formation can readily occur in highly convective clouds, which are widespread in the tropics a

59 eric clouds such as stratus, cirrus and deep convective clouds.

60 ave cold collars and are not associated with convective clouds.

61 % and up to 50% of rainfall evaporating near convective clouds.

62 SSWCA follows primarily the variation of the convective component of the Nernst-Plank equation for fl

63 This mechanism adds a convective component to interstitial transfer of biologi

64 by 0.7 mL/min because of the transcapillary convective component.

65 verned primarily by changes in diffusive and convective contributions to solute flux and not by press

66 imes may be used to deduce the efficiency of convective cooling and ultimately the temporal character

67 Convective cooling of the fine-sized fuel particles in w

68 and 27% of the total variance of the IWC in convective cores and anvil, respectively, during the dec

69 l dynamos were very common in the previously convective cores of these stars.

70 These stars do have convective cores that might produce internal magnetic fi

71 nd venules were similar, the contribution of convective coupling differs as a result of the higher hy

72 surfaces over very short time periods under convective current.

73 he drying multiphase drops exhibit different convective currents, drop morphologies, and deposition p

74 ehydration ratio, microstructure changes) of convective dehydrated carrots has been assessed.

75 ling of the jet hydrodynamics and associated convective-diffusion equation, coupled to a first-order

76 A transport model, based on the convective-diffusive flux of reactants, is developed tha

77 se electrodes, and accurately described by a convective-diffusive transport model, provided a means t

78 alance between molecular adhesive forces and convective dispersive forces.

79 cell-autonomous (active) displacements from convective displacements caused by large-scale (bulk) mo

80 ring injection at US storage sites, but that convective dissolution is unlikely to trap all injected

81 om diffusion and provides field evidence for convective dissolution with a rate of 0.1 g/(m(2)y).

82 t equilibrium and on the aspect ratio of the convective domain.

83 layer during precipitation events by strong convective downdrafts and weaker downward motions in the

84 Delamination and convective downwelling are two widely recognized process

85 ressure zone is equivalent to the suction of convective downwellings.

86 e of interstitial fluid transport, lymphatic-convective drain, and vascularization in the regional sp

87 t (Crataegus spp.) were investigated using a convective dryer at air temperatures 50, 60 and 70 degre

88 t of freeze-drying (FD), vacuum drying (VD), convective drying (CD), microwave-vacuum drying (MVD) an

89 e effect of different dying methods, such as convective drying (CD: 50, 60, 70 degrees C), vacuum-mic

90 black garlic obtainment and the inclusion of convective drying (CDP) and ohmic heating (OHP) were ass

91 study was to evaluate the effect of hot air convective drying (HACD), microwave vacuum drying (MWVD)

92 ng at -50 degrees C and 30Pa, FD sample; and convective drying at 60 degrees C and 2m/s, CD sample) o

93 he results showed that at the end of 600s of convective drying at 65 degrees C the denaturation of WP

94 on of WPI was found to be more stable in the convective drying conditions than beta-lactoglobulin and

95 uroylmethyl amino acids, 2-FM-AA) during the convective drying of strawberries has been carried out f

96 samples, pointed out the suitability of the convective drying system to obtain dried strawberries of

97 ed in the laboratory by freeze-drying and by convective drying were used as control samples.

98 entally friendly technology that accelerates convective drying, allowing the obtainment of dried stra

99 d 68.7% during isothermal heat treatment and convective drying, respectively.

100 A promising way of probing the Jovian convective dynamo is to measure its effect on the extern

101 ase of an inert substrate, where tip-induced convective effects compared to diffusion are greatest.

102 , and isolates diffusive mass transport from convective effects.

103 orona to millions of degrees by transporting convective energy from the photosphere into the diffuse

104 tures becomes very significant and overcomes convective energy transport by majority carriers in the

105 sible solar surface that strongly affect the convective energy transport in their interior and surrou

106 as a possible mechanism to transport magneto-convective energy upwards along the Sun's magnetic field

107 el in which CAPE depends on the influence of convective entrainment on the tropospheric lapse rate, a

108 extremes using a climate model in which the convective entrainment rate is varied.

109 helium isotope 3He, which they mix into the convective envelope on the giant branch and should distr

110 e hydrogen-burning shell and the base of the convective envelope.

111 f strong tidal interactions with the stellar convective envelope.

112 achocline between the radiative core and the convective envelope.

113 n solar-type stars (with radiative cores and convective envelopes like our Sun), the magnetic field p

114 Intermediate-mass stars do not have deep convective envelopes, although 10 per cent exhibit stron

115 t are generated by dynamo processes in their convective envelopes.

116 By analyzing radiative-convective equilibrium simulations, we show that this be

117 ust differences between extreme rainfall and convective events are found in the rainfall characterist

118 e fluxes are sensitive to soil moisture, and convective events are frequent.

119 that a relatively small fraction of extreme convective events produces extreme rainfall rates in any

120 l space, resulting in a striking increase in convective exchange of cerebrospinal fluid with intersti

121 med by paravascular pathways that facilitate convective exchange of water and soluble contents betwee

122 ces to diffusive loading from the source and convective export through the phloem.

123 increase vascular permeability and result in convective extravasation of an 8.5-nm-diameter model dru

124 e obtained perpendicular to the direction of convective flow across the aqueous phase/Fe(III)-oxide m

125 ndary layer by numerical models of turbulent convective flow and combine them with model-free, experi

126 ition on porous substrates is shown to block convective flow at much lower mass loadings than other c

127 Both static magnetic fields and convective flow can induce the initial alignment.

128 We study effects of oscillatory convective flow in extracellular space on the velocity o

129 This orientation change suggests convective flow in the hydrated forearc mantle.

130 The importance of convective flow in the subarachnoid and paravascular spa

131 Chemical reactions and/or convective flow of cytoplasm of plausible magnitude affe

132 on of charge transfer resistance with forced convective flow of electrolytes as a result of better ma

133 It was discovered that forced convective flow of electrolytes greatly enhanced the pho

134 rates the advantages of CED in enhancing the convective flow of interstitial fluid and reducing the d

135 Intriguingly, the outward convective flow triggered by fast solvent evaporation at

136 As these forces produce a convective flow which is the primary mechanism of specie

137 ially varying reagent concentration induce a convective flow, which carries the suspended particles u

138 s where buoyancy forces give rise to focused convective flow.

139 ntibody binding site occupancy transverse to convective flow.

140 lower mantle, and hence severely affect the convective flow.

141 e systematic outflows are a component of the convective flows that provide the upward energy transpor

142 scence recovery that includes the effects of convective flows within a system.

143 By leveraging convective flows, recirculation, and mixing of a process

144 cal rotating spinners whose activity creates convective flows.

145 erular hydraulic pressure and transcapillary convective flux of ultrafiltrate and macromolecules.

146 c cavitation microjets within LTRs induces a convective flux.

147 etween the gradients of electromigrative and convective fluxes and (b) ion concentration readjustment

148 conditions are met with high fluid shear and convective fluxes at the membrane-liquid interface, resu

149 To quantify the convective fluxes from the radiographs, we introduced a

150 In turn, convective fluxes of interstitial fluid increased the ra

151 ments at night under the assumption that the convective fluxes were negligible.

152 e microwire and the possible interference of convective force due to the nonrigid nature of the wires

153 This convective forcing provides additional Hg(0) to the surf

154 tness previously thought unattainable in the convective format.

155 Therefore, the tropical convective heat engine can either stabilize or amplify g

156 Our primary diagnostic is the efficiency of convective heat transfer (Nu).

157 Convective heat transfer through jugular venous return a

158 WDM minimizes thermal resistance by convective heat transfer to a constantly moving droplet

159 monstrating equivalence between conventional convective heating and microwave heating, data was gathe

160 ly offset heating by thermal radiation until convective heating by contact with flames and hot gasses

161 Following this approach, it was found that convective heating methods such as oil bath or electrica

162 ts has been examined under both conventional convective heating with an oil bath and heating using mi

163 as observed in the microwave over that using convective heating; this means that the microwave reacti

164 ng (SD), lyophilisation (LD), and ultrasonic convective hot air-drying (HUD).

165 , increasing the occurrence of high-CAPE/low-convective inhibition days.

166 over South America and an increase of local convective inhibition energy in austral winter (June-Aug

167 h CAPE is most concentrated in days with low convective inhibition, increasing the occurrence of high

168 atalytic system extraordinarily sensitive to convective injection into the mid-latitude lower stratos

169 Were the intensity and frequency of convective injection to increase as a result of climate

170 ong evidence for the development of low-mode convective instabilities in core-collapse supernovae.

171 isk, most likely from a centrifugally driven convective instability and an associated plasma outflow

172 ly attributed to the increase in atmospheric convective instability in the TC outer region below the

173 by transient nonnormal amplification due to convective instability or the onset of turbulence.

174 his work Ni species were separated on a weak convective interaction media diethylamine (CIM DEAE) mon

175 es, we find no need for hidden reservoirs or convective isolation of the lower mantle for any length

176 icochemical conditions prevails in the lower convective layer (LCL) of the brine pool at Atlantis II

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

178 Earth, with its core-driven magnetic field, convective mantle, mobile lid tectonics, oceans of liqui

179 f soluble chemicals within the scaffold with convective mass transfer via microfluidic networks embed

180 rate suggests increasing contributions from convective mass transport that are indicative of flow fi

181 These characteristics are mainly due to the convective mass transport which dominates the separation

182 iquity of such interfaces, the importance of convective mass transport within the near-interface regi

183 lms, with its concomitant contributions from convective mass transport within the near-interface regi

184 m the source, and also appear to enhance the convective mass-transfer coefficient itself.

185 We analyzed the convective mixing action with micro particle image veloc

186 Microfluidic fuel cells exploit the lack of convective mixing at low Reynolds number to eliminate th

187 ng within the microdomain is limited because convective mixing cannot be achieved since diffusion dom

188 y of nutrients to biofilm on the pipes under convective mixing conditions.

189 mmetric explosions even with a high level of convective mixing, as well as highly asymmetric bipolar

190 e subduction of oceanic crust and subsequent convective mixing, however, seems to have largely erased

191 Low wintertime insolation limits convective mixing, such that pollutant concentrations ca

192 Following convective mixing, the entire water column returned to a

193 omoted Legionella growth in pipes subject to convective mixing.

194 inties associated with stellar mass-loss and convective mixing.

195 ms favoured by nutrient-enriched waters from convective mixing.

196 quifer at fast advective time-scales through convective mixing.

197 the so-called sluggish lid regime, a unique convective mode not previously definitively observed in

198 ler-scale numerical simulations suggest that convective momentum transport (CMT) from the unresolved

199 Convective morphologies (supercells, disorganized, and Q

200 The amplitude, structure and depth of the convective motion are unknown.

201 Convective motion in the deep metallic hydrogen region o

202 gravitational signature of non-axisymmetric convective motion in the Jovian metallic hydrogen region

203 ost 30% of the Sun's interior by overturning convective motions.

204 ts provide insight into the mechanics of and convective nutrient transport within a cyclically strain

205 well regulated and appropriately distributed convective O(2) supply.

206 n matching cardiac mitochondrial mass to the convective O(2) transport capacity as erythrocyte mass e

207 s for gas and vapor, and the transport mode (convective or diffusive).

208 se Hg concentrations by 50% relative to weak convective or stratiform events of equal precipitation d

209 is work was to study drying of pequi slices (convective or vacuum drying at 40 degrees C and 60 degre

210 IO was observed in both recent deep convective outflow and aged free tropospheric air, sugge

211 ustering of deep convection also reduces the convective outflow and the anvil cloud fraction.

212 osphere; this enhanced stability reduces the convective outflow in the upper troposphere and decrease

213 More importantly, we show numerically that convective overturn in a several-kilometre-thick layer o

214 upwelling in divergence zones and by winter convective overturn of the water column, and the primary

215 (2,max) emphasize its critical dependence on convective oxygen transport to working skeletal muscle,

216 find that the stellar surface has a complex convective pattern with an average intensity contrast of

217 obscured by dust, which partially masks the convective patterns.

218 ions defining (i) the frequency and depth of convective penetration of water into the stratosphere ov

219 by a combination of mass flow and diffusion (convective phloem unloading).

220 originated from the authors' laboratory as a convective platform to support different analytical tech

221 owave-vacuum drying (MVD) and combination of convective pre-drying and microwave finish-drying (CPD-M

222 (VMD: 120, 480, 480-120 W), a combination of convective pre-drying and vacuum-microwave finish drying

223 r the arils were dried by a combined method (convective pre-drying+vacuum microwave finish drying).

224 On eastern AP slopes, summer convective precipitation increases by up to 6 millimeter

225 bridging the scales of global transport and convective precipitation.

226 tion sites, seasonally during summer, and in convective precipitation.

227 tial variations in tidal heating, asymmetric convective processes or asymmetric crystallization of th

228 These observations show that convective pulses at one latitude can trigger short-term

229 Mounting evidence shows that sub-daily convective rainfall extremes are increasing faster than

230 y aspects of the hydrologic cycle, including convective rainfall, which is the focus of the present w

231 n reflects initiation and intensification of convective rainfall.

232 within climate models in their depiction of convective rainfall.

233 and redistributed by viscous stretching and convective refolding.

234 nucleation of the core leads to a different convective regime and potentially different magnetic fie

235 By assessing the contributions of various convective regimes to precipitation, we find that the sp

236 well before reaching the Asian monsoon deep convective region.

237 dakitic magmatism supports the hypothesis of convective removal of thickened Tibetan lithosphere caus

238 s magnitude, likely due to insufficient deep convective scavenging of oxidized Hg from the upper trop

239 f monolayered Polystyrene (PS) followed by a convective self-assembly drop coating protocol onto the

240 therapeutic ultrasound is thought to rely on convective shear.

241 support the proposed glymphatic mechanism of convective solute transport in brain parenchyma.

242 netic dynamo, these results imply that fully convective stars also operate a solar-type dynamo.

243 Fully convective stars do not have a tachocline and their dyna

244 The lack of a tachocline in fully convective stars therefore suggests that this is not a c

245 Here we report observations of four fully convective stars whose X-ray emission correlates with th

246 possible due to the coexistence of multiple convective states.

247 low-mass pair probe the poorly sampled fully convective stellar domain offering a crucial benchmark f

248 um isotopic composition of MORB requires the convective stirring of recycled uranium throughout the u

249 se in the number of days favorable to severe convective storm formation over the Great Lakes, particu

250 nvective systems (MCSs), the largest type of convective storm, with increased frequency and intensity

251 ble uncertainty in how soil moisture affects convective storms across the world, owing to a lack of o

252 monstrate that, even in regions where severe convective storms are representative extreme weather eve

253 hich hydrometeors and moisture are lifted by convective storms over CEI and the Himalayan foothills a

254 il moisture can influence the development of convective storms through such modifications of low-leve

255 has been linked to the tallest, most intense convective storms.

256 mid-summer and are associated primarily with convective storms.

257 Moreover, the large ants that walk above the convective superheated surface air also showed more net

258 Similar convective surface renewal may also occur on other dwarf

259 perature (CTT) in a well-developed mesoscale convective system (MCS) was studied using both satellite

260 ents were generated by atmospheric mesoscale convective systems (MCSs) propagating from inland to off

261 ral United States are dominated by mesoscale convective systems (MCSs), the largest type of convectiv

262 important group of intense storms-mesoscale convective systems (MCSs)-poses a particular challenge,

263 ical conditions on the lifetime of mesoscale convective systems (MCSs).

264 in disorganized thunderstorms, quasi-linear convective systems (QLCS), extratropical cyclones, light

265 ied under microwave heating and conventional convective (thermal) heating.

266 in locations and seasons with frequent deep convective thunderstorms, but it has never been demonstr

267 Time-lapse studies show how convective tissue displacement patterns, as visualized b

268 Our results reveal the following: (i) Convective tissue motion contributes significantly to to

269 cloud types (congestus, stratiform, and deep convective) together with their differing vertical heati

270 he roots depended similarly on diffusive and convective transport and (2) the axial transport of D2O

271 e PCB record were explained by variabilty in convective transport and postdepositional processes such

272 urthermore, we found that the effects of the convective transport becomes more significant in systems

273 gnal in epithelial systems influenced by the convective transport can propagate almost independently

274 xtracellular spaces at the brain surface and convective transport in perivascular spaces of cerebral

275 hape, density and surface chemistry dominate convective transport in the bloodstream, margination, ce

276 e difference was caused almost completely by convective transport in the outlet tubing with negligibl

277 usion into the cerebrospinal fluid, although convective transport in the perivascular spaces of cereb

278 ons, which may be linked to the promotion of convective transport in the vaginal environment rather t

279 When the convective transport is oriented against the propagating

280 Interstitial flow is the convective transport of fluid through tissue extracellul

281 After ultrasound application, convective transport of the model drug was observed thro

282 We study effects of convective transport on a chemical front wave representi

283 rarchical tree-like structures for efficient convective transport over large distances, combined with

284 aquaporin-4 (AQP4) water channels facilitate convective transport through brain parenchyma.

285 Moreover, the use of convective transport with a pressure differential across

286 rovasculature with complex effects including convective transport, high interstitial pressure and enh

287 d formation rates appeared to be enhanced by convective transport, whereas P-selectin rates were inhi

288 by >10x over a comparable structure without convective transport.

289 ptor binding constant under influence of the convective transport.

290 ction in cytokines passage through SNM under convective transport.

291 manner consistent with diffusive rather than convective transport; (ii) transport of dextrans in the

292 hat no sharp threshold for the transition to convective turbulence exists, a situation similar to wal

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

294 ealistic land conditions improved mass flux, convective updrafts and diabatic heating in the boundary

295 Within the wavenumber band l < 60, convective velocities are 20-100 times weaker than curre

296 systems and study their statistics to bound convective velocity magnitudes in the solar interior, as

297 igand-conjugated nanoparticles highly resist convective washout and enable photothermal stimulation w

298 paration does not appear to directly control convective wavelengths, but rather indirectly affects ho

299 DTS), i.e., a deepening and narrowing of the convective zone, enhanced ascent, increased high clouds,

300 n decreases that occur at the margins of the convective zones, with percent error bars of magnitude s