ライフサイエンスコーパス: convective

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

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

3 sphere, which appears to have sensitized MJO convective activity to QBO-induced changes in static sta

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

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

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

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

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

9 y limitations to exercise are minimized, the convective and diffusive determinants of VMO2peak , at t

10 ll running in rats due, in part, to impaired convective and diffusive O(2) delivery, and thus V O(2)

11 es (PO(2) is; phosphorescence quenching) and convective and diffusive O(2) transport ( Q O(2) and DO(

12 , the hypothesis was tested that both muscle convective and diffusive oxygen (O(2) ) transport, and t

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

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

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

16 s 1979-2017, and we decompose MAPE into both convective and nonconvective components.

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

18 Our satellite analyses reveal that the convective anvil cloud, reaching 16-18 km above sea leve

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

20 During maximal KE, both convective arterial oxygen delivery to the skeletal musc

21 lution, and high throughput, the interfacial convective assembly opens remarkable opportunities for p

22 sembly-based printing technique, interfacial convective assembly, is reported, which utilizes a subst

23 orders of magnitude faster than conventional convective assembly.

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

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

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

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

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

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 compared to those prevailing in the daytime convective boundary layer, but we found that Lagrangian

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

35 hydrated by different methods: freeze- (FD), convective- (CD) and vacuum- (VD) drying.

36 The thermal analysis of these convective cells at steady-state further yield local equ

37 Convective cells can transport spores from gaps that may

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

39 esults correlate the spatial ordering of the convective cells with the evolution of the system's temp

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

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

42 information about the physical origin of the convective cells.

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

44 re convergence (BLMC) to the east of the MJO convective center.

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

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

47 n state with changes in both large-scale and convective circulations, and they suggest that extratrop

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

49 Following the flank collapse, a deep convective cloud column formed over the volcano and acte

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

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

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

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

54 Aerosol effects on convective clouds and associated precipitation constitut

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

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

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

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

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

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

61 nal data, we show that the aerosol effect on convective clouds shifts from invigoration to suppressio

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

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

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

65 ation pattern, due to the energy released by convective condensation over the region which influences

66 varying carbon black concentrations using a convective condition and a gold microelectrode.

67 ver much longer distances than are likely in convective conditions, and is particularly significant f

68 test the predictions of theories, like e.g. convective constraint release.

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

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

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

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

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

74 tellite imagery over the Sahel, we find that convective cores within MCSs are favored on the downstre

75 ils accounting for an additional one in five convective cores.

76 surfaces over very short time periods under convective current.

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

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

79 refore, the combination of magnetic enhanced convective diffusion and the cadherin binding peptide fo

80 e cases, e.g., unsteady diffusion and steady convective diffusion.

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

82 nsport of particles in the CSF via a coupled convective-diffusive transport process.

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

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

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

86 Delamination and convective downwelling are two widely recognized process

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

88 rstitial space, could be utilized to enhance convective drug delivery from the CSF to the parenchyma.

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

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

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

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

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

94 Intermittent microwave convective drying (IMCD) is an advanced drying method wh

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

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

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

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

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

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

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

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

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

104 Thanks to the spinning PDMS and its induced convective effects, we can mold the heat flow robustly w

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

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

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

108 f strong tidal interactions with the stellar convective envelope.

109 achocline between the radiative core and the convective envelope.

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

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

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

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

114 rognostic indicator of the intensity of deep convective events appears to be the convection depth of

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

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

117 oved from the brain's extracellular space by convective exchange between interstitial fluid (ISF) and

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

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

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

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

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

123 LNs), which are likely acidic because of low convective flow and high glucose metabolism.

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

125 samples spun for a short duration induces a convective flow in the drying droplet, thereby leading t

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

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

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

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

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

131 substrate-heating-induced solutal Marangoni convective flow to drive particles toward patterned subs

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

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

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

135 ias to the side electrodes could induce fast convective flow, which facilitates the transport of the

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

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

138 n the absence of strong magnetic fields, the convective flows of the core are expected to be in a reg

139 Dissolution induces these natural convective flows that, in turn, enhance dissolution rate

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

141 cal rotating spinners whose activity creates convective flows.

142 ification which in turn creates a barrier to convective fluid transport and may play a role in tumor

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

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

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

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

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

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

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

150 sue-embedded coating owing to a disparity in convective forces.

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

152 tness previously thought unattainable in the convective format.

153 modular, reconfigurable, and self-sufficient convective heat exchanger for regulation of temperature

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

155 lts indicate that significant changes in the convective heat transfer coefficient are possible, based

156 The convective heat transfer coefficient of the heater is h

157 s multifunctional device also has a superior convective heat transfer coefficient than do other heate

158 ule inclination on system-level flow and the convective heat transfer coefficient.

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

160 osphere-only model with a specified positive convective heating anomaly in the eastern Indian/western

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

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

163 Rolston et al suggest through a convective heating scheme that the mechanism of light-in

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

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

166 of Earth's history, partially shielded from convective homogenization.

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

168 ses in the fraction of precipitation that is convective in all seasons.

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

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

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

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

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

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

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

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

177 gned to explore this regime to show that the convective length scale becomes independent of the visco

178 core conditions, we find that the turbulent convective length scale in the absence of magnetic field

179 rapidly at smaller scales, so this turbulent convective length scale is a lower limit for the energy-

180 ns out of reach, the fact that the turbulent convective length scale is independent of the viscosity

181 We interpret that these gradients are due to convective magma transport in a propagating dyke to the

182 /(36)Ar values relative to estimates for the convective mantle provided by mid-ocean-ridge basalts(11

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

184 alues substantially greater than that of the convective mantle, resembling surface components(12-15),

185 tios are indistinguishable from those of the convective mantle.

186 atmospheres indicate that nonconvective and convective MAPE both increase with increasing mean surfa

187 EKE and extratropical cyclone activity, but convective MAPE increased, implying an increase in the e

188 meridional surface temperature gradient, but convective MAPE is relatively more sensitive to the incr

189 bridge electrolyte into the sample is small, convective mass transport of sample into the nanoporous

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

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

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

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

194 ar and in the membrane (i.e. diffusional and convective mass transport) is essential.

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

196 the IEF stage, the gel functions as an anti-convective medium and not as a molecular sieving matrix.

197 that this loss of snow is undermining winter convective mixing and causing stratification of the uppe

198 heavy materials in metallic hydrogen and on convective mixing as the planet evolves(11,12).

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

200 The effect of convective mixing on the rate of magnetophoresis is also

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

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

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

204 omoted Legionella growth in pipes subject to convective mixing.

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

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

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

208 rapid ventilation of deep-ocean heat through convective mixing.

209 ssfully capture Chl-a variability related to convective mixing.

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

211 Convective morphologies (supercells, disorganized, and Q

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

213 ghly context-dependent, in certain settings, convective motion could provide a previously unrecognize

214 Convective motion in the deep metallic hydrogen region o

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

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

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

218 Both muscle convective O(2) delivery (0.44 +/- 0.06 vs.

219 rried out in hypoxia ( FIO2 = 0.12), whereas convective O(2) delivery was maintained at normal levels

220 uscle preparation during hypoxia (but normal convective O(2) delivery) with nitrite infusion.

221 ic conditions, but in the presence of normal convective O(2) delivery, an elevated plasma nitrite con

222 In conclusion, in the absence of changes in convective O(2) delivery, muscle force, muscle contracti

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

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

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

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

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

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

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

230 e data show good concurrent validity between convective oxygen delivery and DCS-derived blood flow in

231 icrovascular perfusion can be uncoupled from convective oxygen delivery, and that tissue saturation s

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

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

234 We have developed a stand-alone convective PCR (cPCR) device linked to a smartphone for

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

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

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

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

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

240 ral Pacific paired with an eastward shift of convective precipitation that brings more rainfall to th

241 e Asia because of a combination of increased convective precipitation, mixture of air masses, and wid

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

243 bridging the scales of global transport and convective precipitation.

244 nformation on rainfall amount and stratiform/convective proportions provide a valuable tool for rainf

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

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

247 within climate models in their depiction of convective rainfall.

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

249 d from a persistently dry state to an active convective regime at 9000 yr BP and has remained strong

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

251 ve intense NPF at high altitudes in tropical convective regions over both Pacific and Atlantic oceans

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

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

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

255 therapeutic ultrasound is thought to rely on convective shear.

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

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

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

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

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

261 possible due to the coexistence of multiple convective states.

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

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

264 calm July 4, 2003, hours after a fast-moving convective storm had crossed the lake.

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

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

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

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

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

270 of thermal fluctuations when stable complex convective structures emerge.

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

272 Similar convective surface renewal may also occur on other dwarf

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

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

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

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

277 rain comes from remotely triggered mesoscale convective systems (MCSs).

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

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

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

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

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

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

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

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

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

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

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

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

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

291 s; however, biofilms' small pore size limits convective transport, thus, reducing pH stress in these

292 ction in cytokines passage through SNM under convective transport.

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

294 onless parameter that describes the vigor of convective turbulence.

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

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

297 intracellular fluid motion, we quantify the convective velocities that could result from the tempera

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

299 western basin in the absence of intense deep convective winters until 2018.

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