ライフサイエンスコーパス: grain size

1 ather than changes in surface faceting or Au grain size.

2 electric and ferroelectric properties on the grain size.

3 cles of the same total mass but of different grain size.

4 ), 400 keV) is inversely proportional to the grain size.

5 l surface roughness, as well as controllable grain size.

6 tive obstacle spacing is proportional to the grain size.

7 Te-Sb(2)Te(3) nanocomposites with controlled grain size.

8 e nanometre scale is limited by their finite grain size.

9 vily deformed materials with a submicrometre grain size.

10 e, both being proportional to the reciprocal grain size.

11 heir concentration decreases with decreasing grain size.

12 channels through its control on bed surface grain size.

13 boundaries on conductivity as a function of grain size.

14 lents, in part owing to a large reduction in grain size.

15 factants for controlling the deposited metal grain size.

16 ant polarization Pr increase with increasing grain size.

17 hase while showing significant difference in grain size.

18 nine crystalline thin films with macroscopic grain sizes.

19 perties of CVD-graphene films with different grain sizes.

20 ructure (anatase, rutile, mixed phases), and grain size (20-50 nm) were developed along with composit

21 on fluence and energy, a microstructure with grain size 25-30 nm is constructed on the FeN foil sampl

22 range of thicknesses (80-400 nanometers) and grain sizes (50-220 nanometers).

23 nsition temperature which increases with the grain size, a lower thermal shock fatigue resistance, a

24 Sediment grain-sizes affected shorebird community spatial pattern

25 However, grain size alone cannot explain many observed twinning c

26 ailoring of mechanical properties apart from grain size alone.

27 nical properties of a new class of submicron grain-sized alumina ceramics relative to the current sta

28 translucency, the newly developed submicron grain-sized alumina may be considered a suitable materia

29 The strength of these submicron grain-sized aluminas was significantly higher than that

30 n observation, scanning electron microscope, grain size analysis, mineral composition analysis, and p

31 results testified a slightly increase of the grain size and (112) crystal orientation in the Na-incor

32 the grain boundary shows an increase in the grain size and a considerable decrease in the energy bar

33 omic force microscopy reveals an increase in grain size and a decrease in filament number of the muta

34 nd to be an effective method to increase the grain size and carrier diffusion lengths of trihalide pe

35 uch that damage can be inhibited by altering grain size and cation valence variability.

36 structure, including phase content, texture, grain size and chemical homogeneity, are reviewed.

37 -grown at room temperature, which have small grain size and consist of a mixture of body centered tet

38 of polycrystalline graphene by varying both grain size and distribution.

39 ere made at three scales defined by sampling grain size and ecological extent.

40 associated with transgressive variation for grain size and grain weight in this population and featu

41 of VRS1 and VRS5 leads to increased lateral grain size and greater grain uniformity.The VRS genes of

42 -processed CIS and CZTS films featured large grain size and high phase purity, confirming the prospec

43 , nanostructured MAPbI3 film with micrometer grain size and high surface coverage that enables photov

44 columnar structural FePt films with smaller grain size and improved isolation.

45 increasing Q had a major effect on reducing grain size and increasing grain number density.

46 resent an analysis of fan geometry, sediment grain size and lithology in the Ganga Basin.

47 s a cumulative effect of decrease in ferrite grain size and nanoscale cementite.

48 The results indicate that grain size and optimized Cs stoichiometry control cation

49 (n = 45) was pooled to evaluate TRWP metals, grain size and organic carbon correlations by principal

50 rance, Fusarium and brown blotch resistance, grain size and photoperiod sensitivity.

51 fferent initial film qualities (for example, grain size and pinholes) to high-quality MAPbI3-xBrx thi

52 We study the combined effects of grain size and texture on the strength of nanocrystallin

53 t predicts strength as a function of crystal/grain size and the dislocation density.

54 Evaluation of the grain size and the energy barrier height at the grain bo

55 nc-silicene is found to be dependent on the grain size and their orientations.

56 particulate deposition (primarily TRWP with grain size and TOC).

57 on how orthographic transparency constrains grain size and visual strategies underlying letter-strin

58 ence that pericarp cell length affects final grain size and weight in polyploid wheat.

59 h grains of olivine or basalt with different grain sizes and compositions were used to explore the id

60 ate the heating by cosmic rays for different grain sizes and cosmic ray components.

61 characteristic of other metals with similar grain sizes and crystalline packing.

62 ional theory calculations suggest that small grain sizes and polycrystallinity stabilize the 1T ' pha

63 line silicene (nc-silicene) sheet of varying grain sizes and pre-existing cracks at room temperature.

64 parameters that results in films with large grain sizes and small-angle boundaries.

65 s thin films is challenging due to submicron grain sizes and the presence of numerous structural defe

66 ese observations show that adjacent sediment grain-size and how recently a pond was excavated influen

67 trable link between changes in Chinese loess grain-size and NH ice-sheet extent, we use loess grain-s

68 The thickness, sediment grain size, and delta(13)C values of the deposited sedim

69 in lithology, percent total organic matter, grain size, and magnetic susceptibility.

70 e TRIP HEA exhibited a substantially smaller grain size, and optimized fractions of face-centered cub

71 The uniformity in thickness, large grain sizes, and excellent electrical performance signif

72 on fraction (strongly correlated to sediment grain size) appeared as a more important controlling fac

73 ed in growing thin films with single-crystal grain sizes approaching 0.1 millimetre (a factor of 20-1

74 periclase occurs as aggregates of crystals (grain size approximately equal to 3 nm) that are prefere

75 g the film thickness and with large in-plane grain size (approximately 1 micrometer).

76 Detrital mineral content and grain size are positively correlated with porosity, pore

77 plitude of the pressure perturbation and the grain size are scaled to those expected in the Earth, th

78 This suggests that larger grain sizes are indicative of better performance by lead

79 for well-sintered nanograined diamonds, the grain sizes are technically limited to 10-30 nm, with de

80 Grain size as well as electrical and optical properties

81 nt supply through adjustments in bed surface grain size, as also shown through numerical modeling.

82 related mechanical behaviour with decreasing grain size, as well as its dependence on the stacking-fa

83 the grains and/or shrinking the sample, the grain size becomes comparable to one or more characteris

84 These particles can refine the grain size by a factor of three and thereby greatly enha

85 al conductivity resulting from the decreased grain size by ball milling and hot pressing, improved bo

86 nge in emissivity due to mineralogy and snow grain size can cause a 1.8-2.0 W m(-2) difference in the

87 ch as control over phase purity, uniformity, grain size, composition, etc., associated with the solut

88 ld, is controlled by the intralayer spacing (grain size, d), and not the intralayer biphase spacing (

89 of attrition (secondary fragmentation) from grain size data.

90 ance of ice-rafted debris, and sortable silt grain size data.

91 For 20 vol. % ZrO(2) doping into TiN, the grain size decreased dramatically from 11.2 nm to 6.4 nm

92 ed explanation for the grain size effect: as grain size decreases the applied stress needed for furth

93 trolled by partial dislocation activity when grain size decreases to tens of nanometers, and they hav

94 lations, we propose a two-dimensional stress-grain size deformation-mechanism map for the mechanical

95 Loop density trends with grain size demonstrated an increase in the nanocrystalli

96 lity, could be responsible for the different grain size dependence observed in the dielectric and pie

97 , and elucidate the nanoscale origins of the grain-size dependence of its strength and toughness.

98 ange in the deformation mode arises from the grain size-dependent competition between the deformation

99 Understanding the grain size-dependent failure behavior of polycrystalline

100 The key ingredient of the theory is a grain-size-dependent nonlocal rheology--inspired by effo

101 Our results reinforce the idea that grain-size disposition in subsurface sandy sediments dri

102 Our results indicate grain size distribution is a good predictor of biogeoche

103 ouge surface areas approach 80 m2 g(-1), and grain size distribution is non-fractal.

104 al treatment of Cu that results in a bimodal grain size distribution, with micrometre-sized grains em

105 gical activity in the Columbia River HZ, the grain size distributions for sediment samples were chara

106 We utilize total grain size distributions from a suite of natural and exp

107 hese measured U concentrations and published grain size distributions, gravel and cobbles were estima

108 ully ultrafine microstructures having a mean grain size down to 0.35 microns can be obtained without

109 t the synthesis of silver nanoparticles with grain sizes down to electron Fermi wavelength.

110 ediment parameters (magnetic susceptibility, grain size, dry bulk density, mineralogy, and organic ca

111 he distributions of stresses on the scale of grain size during or after mechanical or electrical fati

112 The results show that the grain size effect on the dielectric permittivity is near

113 wfound orientation-based explanation for the grain size effect: as grain size decreases the applied s

114 n, and dissociation are currently limited by grain size effects and molecular orientation.

115 d33 and remnant polarization Pr show diverse grain size effects depending on the particle size of the

116 be neglected when analyzing and engineering grain size effects for increasing nanomaterial strength.

117 Grain size effects on the physical properties of polycry

118 s in rice grain increases with a decrease of grain size (ELS: 0.04; LS: 0.10; MS: 0.16; and SB: 0.33

119 rocess dense alpha-Al(2)O(3) with controlled grain sizes, especially for submicrometre materials.

120 oupling between grain-sensitive rheology and grain-size evolution with damage.

121 tions in spatial, environmental and sediment grain size factors (66% of variance explained), but the

122 show that its breaking strength and average grain size follow an inverse pseudo Hall-Petch relation,

123 Our result suggests that the planar grain size for the perovskite thin films should be large

124 required to mobilize the median bed surface grain size ([Formula: see text]).

125 s were assembled using the sediment with its grain size fractions arranged in different spatial confi

126 drite were physically separated into several grain size fractions by ultracentrifugation.

127 The sediment was sieved into 7 grain size fractions that each exhibited different U(VI)

128 to elucidate the transition with decreasing grain size from a dislocation-based to a grain-boundary-

129 ure of grain boundary absorption efficiency, grain size, grain boundary type and misorientation angle

130 e changes in microstructural features (viz., grain size, grain orientations and texture) are fundamen

131 Recrystallization and grain size growth in PFC materials caused by transients

132 yzed in order to study the effect of spatial grain size heterogeneity on physicochemical and microbia

133 ombination at grain boundaries; however, the grain size in organolead trihalide perovskite (OTP) film

134 iltration program, it is possible to control grain sizes in polycrystalline particles (spheres and op

135 Copper-based alloys with both grain sizes in the nanometre range and distinct grain bo

136 spectra depend on the type of mixing and the grain sizes in the rocks and soils but could be 10 to 10

137 of nitrogen show only minor variations with grain size, indicating a different mechanism of incorpor

138 le nature in these metals when their average grain size is 50 nm or less.

139 When grain size is larger, the same metals regain their macro

140 Grain size is one of the most important components of gr

141 Grain size is positively correlated with detrital minera

142 The lone factor for twinning dependent on grain size is the stress necessary to nucleate partial d

143 uniform growth of TMDC monolayers with large grain sizes is still a considerable challenge.

144 se materials with nanometre-scale structure (grain size less than 100 nm), leading many researchers t

145 l properties and are intrinsically free from grain size limitations.

146 polycrystalline alumina ceramics, an average grain size <1 microm coupled with a porosity level <0.7%

147 than 99.5% dense alpha-Al(2)O(3) with final grain sizes < or =500 nm without sintering aids.

148 Dense and homogeneous microstructure with grain size lying between 2-8 mum can be observed from sc

149 both deformation mechanisms active at these grain sizes, namely dislocation-based plasticity and gra

150 ivity is observed in all the ceramics with a grain size near 1 mum and can be attributed to a maximum

151 and compare its predictions with stishovite grain sizes observed in laser-induced damage and meteoro

152 tained UFG-1 steel showed an average ferrite grain size of 430 nm, containing nanoscale spheroidized

153 ultrafine-grained aluminium with an average grain size of 140 nm, as confirmed by extensive post-imp

154 Petch behaviour in nc-silicene at a critical grain size of 17.32 nm.

155 Y2O3 (melting point, 2,439 degrees C) with a grain size of 60 nm can be prepared by a simple two-step

156 in the perovskite precursor can increase the grain size of a perovskite thin film and reduce the cond

157 nanocrystalline nickel films with an average grain size of about 10 nanometers, which show that grain

158 Cu globular microstructures, with an average grain size of approximately 480 mum, at 555 degrees C (7

159 Nanocrystalline metals, with a mean grain size of less than 100 nanometres, have greater roo

160 line materials (that is, polycrystals with a grain size of less than 100 nm) remains controversial.

161 howed that the perovskite films have a large grain size of more than 1 micrometer, and carrier life-t

162 Both of them exhibit a very small grain size of only several nanometers due to the nature

163 pping regularity is thought to determine the grain size of orthographic information extracted whilst

164 to accommodate plastic deformation when the grain size of polycrystalline materials goes small.

165 up to 600 degrees C leads to an increase in grain size of the anatase nanoparticles to 32 nm.

166 It is shown that the grain size of the FSPS material is halved in comparison

167 M) and scanning TEM analysis showed that the grain size of the milled MgH(2)-0.1TiH(2) powder is appr

168 des (PeLEDs) are obtained by controlling the grain size of the perovskite films.

169 t were several times larger than the average grain size of the sediment.

170 toring, patients strategically regulated the grain size of their memory reporting and proved able to

171 The crystalline fraction and grain size of these films determines electronic and opti

172 -fine grained (UFG) 304 L SS with an average grain size of ~100 nm, can withstand Fe ion irradiation

173 mation in nanocrystalline aluminum with mean grain sizes of 10, 20, and 30 nm.

174 nanocrystalline aluminum and gold films with grain sizes of 65 nanometers and 50 nanometers, respecti

175 Nanocrystalline metals--with grain sizes of less than 100 nm--have strengths exceedin

176 Nanocrystalline metals with average grain sizes of only a few nanometers have recently been

177 its more Li during the first cycle, with the grain sizes of the Li deposits being significantly large

178 explicit effects of heat on grain number and grain size often switched projected yield impacts from p

179 ecent studies have focused on the effects of grain size on deformation twinning in nanocrystalline fc

180 nanocrystalline aluminum and gold films with grain sizes on the order of 50 nm are partially recovera

181 olivine separate (47.8 wt % MgO) of similar grain size, only 5 wt % of the initial MgO content react

182 f different sets of 'splotches' of different grain size (or spatial frequency) on the skin, the fish

183 reatly reduce the melt viscosity or increase grain size, or both, thereby facilitating melt transport

184 However, irrespective of grain size, plastic deformation is considered irrecovera

185 Our results suggest that the impacts from grain size, porosity, and internal strain etc. can be su

186 cates that the quality factor depends on the grain size, porosity, internal strain, structure, phase

187 ink" with accurate control of metal loading, grain size/porosity, composition, and micro/nanomorpholo

188 hand, sudden transition from coarse-to-fine grain sizes promoted a hot-spot of organic matter degrad

189 oratory measurements indicates that the dust grain size ranges from 1 to 12 micrometers, assuming a t

190 response of Al microstructures comprising of grain sizes ranging from 50 nm to 3.20 microm and corres

191 pted signal processing of the BDP-98 average grain-size record, but in constructing their age model t

192 n-size and NH ice-sheet extent, we use loess grain-size records to confirm that northern ice-sheets w

193 However, the influence of ultrasonics on grain size reduces with increasing addition of the maste

194 gth of the BCC matrix above that provided by grain size reduction alone.

195 Grain size reduction and gouge formation are found to be

196 Nanosize particle formation and grain size reduction are also utilized.

197 the enhancements in strength that accompany grain size reductions.

198 ypothesis that defect density decreases with grain size refinement due to the increase in grain bound

199 ent defect absorption in the nanocrystalline grain size regime, but loop coalescence in the ultra-fin

200 gime, but loop coalescence in the ultra-fine grain size regime.

201 ultaneously, columnar structure with smaller grain size retained.

202 model to analyse the experimentally measured grain sizes revealed that the results of this study and

203 demonstrated by investigating the effect of grain size, shock pulse and system size on the shock res

204 Yet, grain-size specific magnetic properties associated with

205 correlated with detrital mineral content and grain size standard deviation while negatively related t

206 ed Barium concentration and reduced sediment grain size suggest persistence of disturbance for three

207 oduces highly ordered films with macroscopic grain sizes suitable for optical studies.

208 ism results in a maximum yield strength at a grain size (the 'strongest size') that depends strongly

209 th depend on the grain size: the smaller the grain size, the smaller the critical twin-boundary spaci

210 For larger grain sizes, the grain growth usually takes place at hig

211 opper and the maximum strength depend on the grain size: the smaller the grain size, the smaller the

212 rain-refinement treatment, which refines the grain size to 4 mum.

213 Inversely modeled storm conditions from grain size trends show that a more compact yet more inte

214 InP thin-films on Mo foils with ultra-large grain size up to 100 mum, which is ~100 times larger tha

215 rface coverage, small surface roughness, and grain size up to microscale.

216 bly appear pervasive and can be discerned at grain sizes up to four orders of magnitude larger than t

217 an additional mechanism for the reduction of grain size, via liquation assisted transgranular crackin

218 better isolated from each other and the FePt grain size was reduced.

219 emoval of particles in sand of two different grain sizes were examined.

220 Dense BaTiO3 ceramics with different grain sizes were fabricated by either conventional sinte

221 function of both sample-size dependence and grain size, when the operative obstacle spacing is propo

222 fine matrix of pyroclastic rocks with finer grain size, which are more degraded.

223 d grain numbers per unit area and individual grain size, while heat stress during grain filling mainl

224 rthermore, the type of OC is also related to grain size with the clay containing mostly (immature) pl

225 eresis loops that are strongly influenced by grain size, with the energy dissipated being significant