ライフサイエンスコーパス: haze

1 ensed-ice or dust particles may explain this haze.

2 cal features such as vasculitis and vitreous haze.

3 33)S ratios are sensitive to the presence of haze.

4 eas were clear at 20 years; 3 eyes had trace haze.

5 and the development of fibrosis and corneal haze.

6 al biopsy in 1 affected patient with corneal haze.

7 el role for desmin overexpression in corneal haze.

8 ted with an increased incidence of interface haze.

9 ng effect on the radiative properties of the haze.

10 ent to the cornea and development of corneal haze.

11 al thickness, stromal thickness, and corneal haze.

12 orneal stroma and the development of corneal haze.

13 rophil activation and development of corneal haze.

14 Vitritis was graded by the degree of vitreal haze.

15 rbons, nitrile compounds, and Titan's orange haze.

16 of glaucoma filtration surgery, and corneal haze.

17 n-induced increases in stromal thickness and haze.

18 ly scattered light that corresponds to 0-30% haze.

19 P = .003) compared with absence of vitreous haze.

20 beta3 expression with a reduction in corneal haze.

21 kest features are associated with clouds and hazes.

22 y higher in uveitic eyes with known vitreous haze (0.150) than in uveitic eyes without haze or in hea

23 T-EDI (vasculitis, 0.45 [P < .001]; vitreous haze, 0.59 [P < .001]).

24 hteen patients showed a reduction in corneal haze 1 month after CXL.

25 a significant (P < 0.01) decrease in corneal haze (1.3 +/- 0.3) compared with the no-decorin-delivere

26 riggered resulting in the formation of heavy haze: (1) the dispersal of water vapour is constrained b

27 mon clinical signs reported include vitreous haze (523 of 1153 [45.4%]), retinal vasculitis (374 of 8

28 cally from exhibiting low haze (<1%) to high haze (~56%) without compromising the total forward trans

29 ce level of 7.7sigma), a strongly scattering haze (7.4sigma) and sodium (3.4sigma), and confirms the

30 Postoperative complications included trace haze (8%), epithelial dryness on day 1 (5%), interface i

31 often observed in regions impacted by acidic haze aerosol such as Beijing and other megacities around

32 N-containing molecules, which form the dense haze aerosols that completely cover the moon of Saturn.

33 el of haze extinction to explore how Titan's haze affects its transit spectrum.

34 Previous studies suggest that corneal haze after injury involves changes in the light-scatteri

35 for a link between cellular transparency and haze after injury that is possibly related to loss of pr

36 ASIK and could be used to examine changes in haze after lamellar keratoplasty.

37 fective in inhibiting development of corneal haze after PTK in rabbits.

38 No eyes developed haze all throughout the study.

39 sured in this study (vasculitis and vitreous haze) also showed a significant Spearman rank correlatio

40 ccompanied by continued reduction in corneal haze and aberrations, suggesting ongoing remodeling of t

41 ur at three altitude levels within the upper haze and clouds.

42 Black carbon (BC) in haze and deposited on snow and ice can have strong effec

43 It also decreased corneal haze and fine-grained irregularities in ocular wavefront

44 The study confirmed corneal subepithelial haze and interface haze as important factors limiting vi

45 regraft (133 days), who demonstrated central haze and irregular astigmatism from anterior stromal sca

46 n that MMC is highly effective at preventing haze and is well tolerated, with few reported complicati

47 Compared to the untreated puree, Purple Haze and Nutri Red processed at 303 kJ/kg completely inc

48 ckscattering of light, a function of corneal haze and opacification, was determined regionally using

49 expanded potential patient profiles, reduced haze and pain postoperatively, and increased quality of

50 Post-operative haze and particles can affect the interface quality and,

51 almic pathology in patients includes corneal haze and progressive retinal and optic nerve atrophy.

52 misphere cooling due to infrared emission by haze and trace gases; our results therefore imply that t

53 nts the experimental characterization of low-haze and ultra-transparent electrodes based on silver na

54 eric anthocyanins, color properties (CIELch, haze), and pigments composition before and after spray d

55 des a high-resolution measurement of corneal haze, and Amco Clear provides a means of standardizing t

56 o the corneal stroma, development of corneal haze, and chemokine production were measured.

57 ry, less postoperative pain, reduced stromal haze, and faster epithelial healing than PRK.

58 seline, persistence or incidence of vitreous haze, and incidence of macular thickening.

59 ual acuity, anterior chamber cells, vitreous haze, and posterior eye segment inflammation were assess

60 ationships between HOAs, BCVA, subepithelial haze, and recipient age were determined.

61 vision and signs of macular edema, vitreous haze, and retinal vasculitis were graded; a second gradi

62 y obscured by an optically thick atmospheric haze, and so its nature has been the subject of consider

63 terile infiltrate, herpes keratitis, central haze, and stromal scar).

64 he viscosity of the solutions and form gels, hazes, and precipitates, they are often related to poor

65 ations; however, substrates with low optical haze are not ideal for thin film solar cells, since most

66 High-altitude clouds and hazes are integral to understanding exoplanet observatio

67 ng formation is unlikely and that clouds and hazes are the cause of weaker spectral signatures.

68 med corneal subepithelial haze and interface haze as important factors limiting visual acuity after D

69 able turbidity reduction and prevent protein haze as was demonstrated by the heat stability tests.

70 ned and intensified by solar heating in dark haze (as found over much of the northern Indian Ocean du

71 ld be the result of obscuration by clouds or hazes, as found in some optical spectra.

72 EK may reduce postoperative pain and corneal haze associated with PRK.

73 Corneas were graded for corneal haze at 0, 1.5, 7, 21, 42, and 91 days after PRK.

74 ent significantly (P < 0.05) reduced corneal haze at 2 weeks and was essentially normal by 12 weeks.

75 A detached haze at an altitude of 500 km is 150-200 km higher than

76 tter gain in eyes that had gradable vitreous haze before surgery (95% CI, 9-18 letters; P < 0.001) 3

77 The initiation and spread of subepithelial haze begins shortly after reepithelialization.

78 eases in anterior chamber cells and vitreous haze (both P < .0001), as well as beneficial effects in

79 circulation are summer-hemisphere heating of haze by absorption of solar radiation and winter-hemisph

80 tly, the data demonstrate that high-altitude hazes can severely limit the atmospheric depths probed b

81 Corneal stromal haze cannot be compared in longitudinal studies or acros

82 sorption isotherms) and optical properties (haze, CIELab parameters) of the resulting materials were

83 probable sublimation of water ice, producing haze clouds inside the crater that appear and disappear

84 ignificant increase in stromal thickness and haze compared with untreated control corneas at each tim

85 ) was probably enshrouded by a photochemical haze composed of fractal aggregate hydrocarbon aerosols.

86 ays after transfer, characterized by corneal haze, conjunctival and episcleral injection, corneal inf

87 The average haze contribution to the nighttime surface UHI is 0.7+/-

88 hat the development of postoperative corneal haze could be due to an increase in light scattering fro

89 , Yellow Solar, Nantes, Nutri Red and Purple Haze cultivars against H2O2-induced oxidative damage.

90 BC concentration during haze days versus non-haze days and found significantly lower eBC fractions in

91 ignificantly lower eBC fractions in PM2.5 on haze days compared to those on non-haze days.

92 poral variations of eBC concentration during haze days versus non-haze days and found significantly l

93 th is increasing-particularly in relation to haze days.

94 PM2.5 on haze days compared to those on non-haze days.

95 e that appears to be separated from the main haze deck.

96 HOAs (RMS third to sixth Zernike order) and haze decreased (P < .001).

97 Severe corneal haze developed by day 42 and persisted to day 91.

98 Significant corneal haze developed in the null and aG1 vector-treated groups

99 ng age constraints, we estimate that organic haze developed rapidly, stabilizing within approximately

100 Protein haze development in bottled white wines is attributed to

101 ted a unique state of the Earth system where haze development played a pivotal role in planetary oxid

102 tary hydrogen loss, with a single episode of haze development providing up to 2.6-18 x 10(18) moles o

103 history, we targeted an episode of inferred haze development.

104 SMA and TNC at the wound margin mirrored the haze distribution, spread, and intensification with time

105 mice develop increased corneal thickness and haze due to neutrophil infiltration to the corneal strom

106 ining agent to prevent browning and decrease haze during must settling because its effect on grape ph

107 or vitreous cellular activity or in vitreous haze each led to significant improvements in visual outc

108 ted complications include keratitis, corneal haze, endothelial cell loss and failure of treatment.

109 The June 2013 haze episode was one of the worst air pollution events i

110 ere elevated (up to 329 mug/m(3)) during the haze episode, compared to those during the nonhaze perio

111 0.2 mum) were collected during the June 2013 haze episode.

112 has experienced severe and persistent winter haze episodes in recent years due to intensification of

113 ed atmospheric methane concentrations during haze episodes would have expedited planetary hydrogen lo

114 Our study of the 2012-13 winter haze events in Beijing shows that atmospheric water vapo

115 Trans-boundary haze events in Southeast Asia are associated with large

116 In recent years, severe haze events often occurred in China, causing serious env

117 We expect major haze events to be increasingly frequent because of ongoi

118 The results show that these severe haze events were equally affected ( approximately 30%) b

119 plays a critical role in enhancing the heavy haze events.

120 We use a simple model of haze extinction to explore how Titan's haze affects its

121 o disentangle effects of gas absorption from haze extinction.

122 at transmittance of approximately 89% with a haze factor <3%).

123 a, that the Indonesian fires behind the 2013 haze followed a two-month dry spell in a wetter-than-ave

124 rocess because residual phenols cause severe haze formation affecting juice quality and impairing cus

125 , the sustained methane fluxes necessary for haze formation can only be reconciled with a biological

126 We demonstrate that indeed tholin-like haze formation could occur on condensed aerosols through

127 Fss is a key growth factor promoting stromal haze formation in corneas after PRK and suggests that li

128 To examine the role of haze formation in Earth's history, we targeted an episod

129 anterior corneal ultrastructural changes and haze formation in Fuchs' dystrophy, and should not be ig

130 sed to remove grape proteins responsible for haze formation in white wines.

131 al stability of wine proteins and thus delay haze formation in wine during storage.

132 mprove the current model of light-scattering haze formation in wounded corneas, which will improve th

133 Haze formation is a significant problem for the wine ind

134 parameter space in which high-altitude cloud/haze formation is not expected to be significant for hyd

135 mechanism responsible for white wine protein haze formation is not fully characterized.

136 esent models assume that Titan's tholin-like haze formation occurs high in atmosphere through gas-pha

137 A daily image time course of haze formation was generated using macrophotography.

138 s critical to corneal wound healing, stromal haze formation, and scarring.

139 The mechanisms responsible for the haze formation, however, are still not well understood,

140 y, previously problematic for regression and haze formation, is gaining new prominence as early exper

141 in C 0.02% was used after the PRK to prevent haze formation.

142 procedure that carries an increased risk for haze formation.

143 a viable tool in the management of scar and haze formation.

144 like proteins and chitinases are involved in haze formation.

145 in small amounts in wine, but contribute to haze formation.

146 , as measured by inability to grade vitreous haze, gained an additional 42 letters (95% CI, 34-56 let

147 Agreement in vitreous haze grade between each pair of specialists was evaluate

148 erior chamber cell grade, change in vitreous haze grade, and change in best corrected visual acuity)

149 sions, anterior chamber cell grade, vitreous haze grade, and visual acuity.

150 y, anterior chamber cell grade, and vitreous haze grade.

151 (BCVA), IVCM (subepithelial haze, interface haze, graft thickness) and AS-OCT (graft thickness).

152 e 1 involvement occurred in 55% and vitreous haze >/=grade 2+ occurred in 25%.

153 The presence of vitreous haze had a statistically significant association (HR, 1.

154 egression analysis, the presence of vitreous haze had an adjusted HR of 2.98 (95% CI, 1.50-5.94; P =

155 If anything similar to Titan's haze has ever existed on our planet, it is reasonable to

156 nditions-featuring a methane-derived organic-haze-have recently been suggested, yet their occurrence,

157 The distribution of haze imaged in the macrophotographs and density of alpha

158 stroma, and increased corneal thickness and haze in C57BL/6 mice.

159 l stroma and increased corneal thickness and haze in control C57BL/6 mice but not in TLR2(-/-) or MyD

160 used intraoperatively as prophylaxis against haze in higher myopic ablations.

161 LPS-induced haze in mice corneas was decreased by 2-fold upon EP tre

162 s nanomaterials were used to prevent protein haze in Muscat Ottonel and Pedro Ximenez wines.

163 ant component of fine particulate matter and haze in national parks and wilderness areas where visibi

164 of potentially hazy worlds, the slope set by haze in our spectra is not flat, and creates a variation

165 human cornea in vitro and markedly decreases haze in rabbit cornea in vivo.

166 Prolonged stromal haze in the cornea is associated with abnormal regenerat

167 This method can detect subtle decreases in haze in the corneal flap 3 years after LASIK and could b

168 Haze in the rabbit cornea was produced with photorefract

169 Density of haze in the rabbit eye was graded with slit lamp biomicr

170 eitis specialists clinically graded vitreous haze in the same eyes, one after the other using the sam

171 ced alpha-smooth muscle actin expression and haze in the stromal ablation zone.

172 ratory can serve as analogs for the observed haze in Titan's atmosphere.

173 PRK induced significant haze in vehicle-treated corneas that peaked at 2 weeks a

174 to -9 D PRK significantly decreased corneal haze in vivo.

175 of these polysaccharides is able to prevent haze in wine.

176 ne, which is coincident with frequent severe hazes in South Korea.

177 rregular and less transparent, with a higher haze index.

178 n-induced increases in stromal thickness and haze, indicating an essential role for these cells.

179 ignificant increase in corneal thickness and haze, indicative of disruption of corneal clarity; howev

180 crease of both anterior chamber and vitreous haze inflammation levels, and by the size reduction in c

181 y world, Titan, to clarify how high-altitude hazes influence transit spectra.

182 all corneas also had some central islands of haze initiation.

183 ed visual acuity (BCVA), IVCM (subepithelial haze, interface haze, graft thickness) and AS-OCT (graft

184 Severe haze is a major public health concern in China and India

185 Recurring biomass burning-induced smoke haze is a serious regional air pollution problem in Sout

186 rnea, the incidence of post-surface ablation haze is decreased.

187 It has been suggested that a similar haze layer may have formed on the early Earth.

188 ents are presented, and implications for the haze layer properties are discussed.

189 st captivating features is the thick organic haze layer surrounding the moon, believed to be formed f

190 results from the presence of a high-altitude haze layer that is absorbing at solar wavelengths but tr

191 If the haze layer were removed, the antigreenhouse effect would

192 extended, with trace hydrocarbons, a global haze layer, and a surface pressure near 10 microbars.

193 n that observed by Voyager, and more tenuous haze layers are also resolved.

194 hemical evolution of Titan's orange-brownish haze layers is also discussed.

195 red as important constituents of the visible haze layers on Titan.

196 -injected Lum(-/-) mice had elevated corneal haze levels compared with that of Kera(-/-) and wild-typ

197 longwave emissivity resulting from elevated haze levels.

198 periments that demonstrate the properties of haze likely to form through photochemistry on Titan and

199 o case in the AMT group demonstrated corneal haze, limbal stem cell deficiency, symblepharon, ankylob

200 xible glass dramatically from exhibiting low haze (<1%) to high haze (~56%) without compromising the

201 surface irregularities and anterior corneal haze may be the most important limiting factors in visua

202 Haze may be treated or prevented using numerous remedies

203 er-order aberrations, and surgical interface haze may contribute to poor visual outcomes after big-bu

204 Earth suggest a significant optical depth of haze may have dominated the early Earth's atmosphere.

205 ectra that inherently include the effects of haze multiple scattering, refraction, and gas absorption

206 Among eyes in the MT group, corneal haze occurred in 44% (11/25; P = 0.001), corneal vascula

207 98.69% at high transmittance of ~77% during haze occurrence.

208 yphal-specific dispersal of the Golgi into a haze of finely dispersed vesicles with a sedimentation d

209 age fiber length decreases, the transmission haze of TOWF-coated flexible glass illustrates a decreas

210 Vitreous haze often was present (46.1% of eyes).

211 f a Golgi enzyme marker in the mitotic Golgi haze or in Golgi vesicles generated by ilimaquinone.

212 us haze (0.150) than in uveitic eyes without haze or in healthy controls (0.0767, P = 0.0001).

213 No case showed clinical haze or scarring by month 3.

214 ogenic emissions are the main factor causing haze over eastern China, we conclude that natural emissi

215 eading to formation of nanoparticles of blue haze over forested areas are highly complex and not full

216 r the detached haze, such as a transition in haze particle growth from monomers to fractal structures

217 We find that haze particles have substantially larger solar heating a

218 The number density of haze particles increases by a factor of just a few from

219 nergy equilibrium is controlled primarily by haze particles instead of gas molecules.

220 ocyanin pathway through the R2R3-MYBs PURPLE HAZE (PHZ) and DEEP PURPLE, with predominantly petunidin

221 Thick haze plagued northeastern China in January 2013, strongl

222 he biogeochemical effect of urban aerosol or haze pollution is also a contributor to the UHI.

223 s China is the urban-rural difference in the haze pollution level.

224 Mitigation of haze pollution therefore provides a co-benefit of reduci

225 Air pollution, especially haze pollution, is creating health issues for both human

226 od, hindering the forecast and mitigation of haze pollution.

227 des a unique example of animals' response to haze pollution; future studies are needed to identify pr

228 ictated the feedback cycle involving organic haze production and global cooling.

229 ined as being due to the co-location of peak haze production and the limit of dynamical transport by

230 = 0.59; P<0.001; n = 27), with subepithelial haze (r = 0.41; P = 0.01; n = 25), and with recipient ag

231 .46, P = 0.003), postoperative subepithelial haze (r = 0.43, P = 0.004 and r = 0.39, P = 0.001) were

232 < 0.001 and r = 0.46, P = 0.002), interface haze (r = 0.51, P < 0.001 and r = 0.46, P = 0.003), post

233 between BCVA and preoperative subepithelial haze (r = 0.61, P < 0.001 and r = 0.46, P = 0.002), inte

234 Here we report that atmospheric hazes, rather than gases, can explain Pluto's temperatur

235 ittle hydrogen), opaque clouds or scattering hazes, reducing our ability to observe the composition o

236 Haze reduction via preserved epithelial flaps, smoother

237 Despite this, haze remains severe in China, indicating the importance

238 The Regional Haze Rule set the goal of returning visibility in CIAs o

239 orneal findings on clinical examination were haze, scarring, vascularization, stromal edema, pigment

240 Eyes with baseline vitritis (vitreous haze score >/=+0.5, n = 45) had a probability of vitreou

241 gnificant positive correlation with vitreous haze score (r = 0.535, P < .001) that remained significa

242 Vitreous haze score at month 2 was chosen as primary endpoint.

243 eyes (105 patients) with different vitreous haze score grades according to standardized protocols an

244 also observed between the different vitreous haze score groups (P < .001).

245 =+0.5, n = 45) had a probability of vitreous haze score improvement (2-step decrease or change from +

246 Time to visual acuity and vitreous haze score improvement as per the Standardization of Uve

247 lescents, 6 to 17 years old, with a vitreous haze score of >/=1.5+ or cystoid macular edema (CME) of

248 the percentage of eyes achieving a vitreous haze score of 0 increased from 41% to 88% (P = .006).

249 the percentage of eyes achieving a vitreous haze score of 0 increased from 58% to 83% (P = 0.03).

250 rovides favorable visual acuity and vitreous haze score outcomes but requires repeated injections, an

251 , overall and respectively for each vitreous haze score subgroup.

252 f systemic immunosuppression drugs, vitreous haze score, and presence of raised intraocular pressure

253 isual acuity, intraocular pressure, vitreous haze score, central retinal thickness by optical coheren

254 nge in visual acuity, and change in vitreous haze score, showed numeric trends favoring IV dosing.

255 positive correlation with clinical vitreous haze scores (r = 0.566, P = 0.0001).

256 There was an improvement in haze scores between 1 and 20 years (P < 0.02).

257 efined as anterior chamber cell and vitreous haze scores of 0 or 0.5+ in both eyes without corticoste

258 Golgi proteins within mitotic Golgi haze-seen during metaphase-were found to redistribute wi

259 Similarly, at day 13, mean vitreous haze severity scores (SD) for the DEX implant versus the

260 e primary congenital glaucoma group, corneal haze showed a significant relationship with most clinica

261 Quantitative measurement of corneal haze showed that the postnatal cornea was hazy after bir

262 The surface of Saturn's haze-shrouded moon Titan has long been proposed to have

263 the surface thus far imaged by radar of the haze-shrouded Titan is very young, with persistent geolo

264 With time, the haze spread within the ablated zone and intensified.

265 an alternative explanation for the detached haze, such as a transition in haze particle growth from

266 to 500 kilometres, where there is a layer of haze that appears to be separated from the main haze dec

267 er seems to be correlated with the amount of haze that develops after cross-linking.

268 lgi clusters and an extensive, nonresolvable haze that either represents scattered vesicles or a merg

269 d likely feed the production of an extensive haze that encompasses Pluto.

270 he gaseous constituents produces an extended haze that obscures the surface.

271 en-dominated, then it must contain clouds or hazes that are optically thick at the observed wavelengt

272 The haze then spreads from the loci of initiation and become

273 ime (TBUT), conjunctival congestion, corneal haze, vascularization, conjunctivalization, and limbal s

274 mean change in visual acuity (VA), vitreous haze (VH), and central macular thickness (CMT) at month

275 cimer laser and were observed and graded for haze via slit lamp, imaged, and graded by macrophotograp

276 support the interpretation that atmospheric haze was a transient response of the biosphere to increa

277 The Golgi haze was also studied using BODIPY ceramide.

278 The haze was distributed as a ring at the wound margin in al

279 Corneal haze was evaluated before surgery and at 2, 3, and 4 wee

280 In this study, a fractal aggregate haze was found to be optically thick in the ultraviolet

281 In contrast, development of corneal haze was inhibited in the dnG1 vector-treated group when

282 Corneal haze was measured by in vivo confocal microscopy before

283 etinopathy Study protocol, and subepithelial haze was measured from the brightness of confocal images

284 Corneal haze was present in 52 of 56 eyes 1 hour after treatment

285 This 'detached' haze was previously explained as being due to the co-loc

286 At month 2, vitreous haze was reduced from a score of 1.5+ to 0.5+ and 0 and

287 Mild haze was seen in 22.2% of eyes (12 eyes) after diamond b

288 Corneal haze was the most frequently reported crosslinking-relat

289 Corneal haze was the most frequently reported CXL-related advers

290 Corneal backscatter (haze) was measured from the confocal image light intensi

291 The first signs of corneal haze were apparent shortly after reepithelialization.

292 The presence and severity of vitreous haze were classified according to the National Eye Insti

293 Patients with stromal haze were excluded.

294 Corneal thickness and haze were measured by in vivo confocal microscopy, neutr

295 Stromal thickness and haze were measured by in vivo scanning confocal microsco

296 roteins, i.e. those not contributing to wine hazing, were not affected by the treatments and therefor

297 ionship was noted with C/D ratio and corneal haze, whereas for secondary congenital glaucoma only axi

298 into the corneal stroma and elevated corneal haze, which is an indicator of loss of corneal transpare

299 ellow colour that comes from its atmospheric haze, whose formation and dynamics are far from well und

300 average monomer radius of 50 nanometers, the haze would have provided a strong shield against ultravi