ライフサイエンスコーパス: haze

1 beta3 expression with a reduction in corneal haze.

2 e showed normal appearing corneas, devoid of haze.

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

4 cal features such as vasculitis and vitreous haze.

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

6 ottled beverages leading to the formation of haze.

7 and the development of fibrosis and corneal haze.

8 al biopsy in 1 affected patient with corneal haze.

9 el role for desmin overexpression in corneal haze.

10 ted with an increased incidence of interface haze.

11 ng effect on the radiative properties of the haze.

12 nvolvement of oxidized tannins in reversible haze.

13 s risk to developing post refractive corneal haze.

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

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

16 kest features are associated with clouds and hazes.

17 gional and global environmental impacts from hazes.

18 s a coyote approached a human to necessitate hazing.

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

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

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

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

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

24 jects were grouped into those that developed haze 12 months post surgery (n = 6 eyes; haze predispose

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

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

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

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

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

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

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

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

33 No eyes developed haze all throughout the study.

34 thogenesis-related proteins are able to form haze alone when thermally denatured.

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

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

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

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

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

40 lated (PR) proteins in white wine can induce haze and hinder the sale of the product.

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

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

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

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

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

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

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

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

49 In bottled wines, haze and turbidity are phenomena to be avoided.

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

51 e posterior uveitis manifestations (vitreous haze and vasculitis) were more common in the older age g

52 an adult or child can alter the outcomes of hazing and must be considered in determining the efficac

53 coyotes learn to avoid behaviors warranting hazing and that this could be used as a non-lethal manag

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

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

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

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

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

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

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

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

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

65 particulate air pollution in Beijing (winter haze) are associated with high relative humidity (RH) an

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

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

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

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

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

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

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

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

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

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

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

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

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

79 Fog and cloud readily form under winter haze conditions, leading to high liquid water contents w

80 tion for sulfate formation under some winter haze conditions.

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

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

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

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

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

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

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

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

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

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

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

92 QMOM) to simulate the abrupt-rise process of haze development and to calibrate the contribution of th

93 Protein haze development in bottled white wines is attributed to

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

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

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

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

98 d fluorescence images are often corrupted by haze due to out-of-focus light, i.e., to cross-talk betw

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

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

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

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

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

104 0.2 mum) were collected during the June 2013 haze episode.

105 evere haze episodes in Xi'an and four severe haze episodes in Beijing, which were characterized by tw

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

107 of about one month, we monitored five severe haze episodes in Xi'an and four severe haze episodes in

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

109 to the missing sulfate source during severe haze episodes.

110 e show evidence from field observations of a haze event that rapid oxidation of SO(2) by nitrogen dio

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

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

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

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

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

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

117 with children had no impact on the number of hazing events.

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

119 o disentangle effects of gas absorption from haze extinction.

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

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

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

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

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

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

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

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

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

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

130 Haze formation is a significant problem for the wine ind

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

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

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

134 been shown to remove PR proteins and reduce haze formation on a lab scale, however the effect on win

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

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

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

138 tially lower doses of GSP (5 g/L) to prevent haze formation.

139 like proteins and chitinases are involved in haze formation.

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

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

142 ochemical facilities, contributing to severe haze formation.

143 procedure that carries an increased risk for haze formation.

144 only oxidized procyanidins were involved in haze formation.

145 the mechanisms by which they are involved in haze formation.

146 ent of intramolecular coupling in reversible haze formation.

147 SAB, respectively, and reduced the amount of haze formed in a heat test by up to 75% and 80%, respect

148 The haze formed in a model solution was partially reversible

149 rying different surface properties to remove haze-forming proteins from Semillon and Sauvignon Blanc

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

151 study, we showed the presence of proteins in haze gathered from apple juices.

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

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

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

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

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

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

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

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

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

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

162 Hazing, i.e., scaring wildlife, is frequently promoted a

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

164 predisposed) and those that did not develop haze in a similar follow up duration (n = 11 eyes; contr

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

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

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

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

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

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

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

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

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

174 Haze in the rabbit cornea was produced with photorefract

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

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

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

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

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

180 rape pathogenesis-related proteins can cause haze in wine that is undesirable for consumers.

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

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

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

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

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

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

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

188 endothelial cell density, corneal thickness, haze, intraocular pressure, and visual function before a

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

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

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

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

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

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

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

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

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

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

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

200 e predisposed subjects and those with active haze(n = 3), indicating their pro-fibrotic role.

201 Haze occupied the central cornea, accompanied by corneal

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

203 98.69% at high transmittance of ~77% during haze occurrence.

204 athogenesis-related proteins (PRPs) from the haze of a commercial apple juice.

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

206 ies (an average transmittance of ~ 80% and a haze of ~ 93%), good UV-blocking ability, and low therma

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

208 oyote interactions and subsequent effects of hazing on coyote behavior.

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

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

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

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

213 reoperative apical scarring led to worsening haze (P = .0001), more astigmatism (P = .002), more cent

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

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

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

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

218 Thick haze plagued northeastern China in January 2013, strongl

219 fur dioxide (SO(2)) to sulfate during severe haze pollution events, indicating that our understanding

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

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

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

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

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

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

226 ular factors altered in corneas that develop haze post refractive surgery have been described, but pr

227 egulated and 1780 downregulated genes in the haze predisposed group revealed alterations in pathways

228 DN were found to be significantly altered in haze predisposed subjects and those with active haze(n =

229 PREX1 was significantly upregulated in haze predisposed subjects.

230 ped haze 12 months post surgery (n = 6 eyes; haze predisposed) and those that did not develop haze in

231 gh doses (25-32 g/L) for protein removal and haze prevention and this induced changes to wine composi

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

233 be considered in determining the efficacy of hazing programs.

234 new technology for the selective removal of haze proteins from white wines.

235 = 0.59; P<0.001; n = 27), with subepithelial haze (r = 0.41; P = 0.01; n = 25), and with recipient ag

236 .46, P = 0.003), postoperative subepithelial haze (r = 0.43, P = 0.004 and r = 0.39, P = 0.001) were

237 < 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

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

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

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

241 Haze reduction via preserved epithelial flaps, smoother

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

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

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

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

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

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

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

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

250 =+0.5, n = 45) had a probability of vitreous haze score improvement (2-step decrease or change from +

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

268 ys based on the accumulative number of times hazed, suggesting coyotes learn to avoid behaviors warra

269 hand fed by adults had to be more frequently hazed than coyotes with other or no past experiences wit

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

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

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

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

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

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

276 patients with >=2-step reduction in vitreous haze (VH) on the Miami scale or with a reduction of syst

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

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

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

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

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

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 Corneal haze was quantified with corneal densitometry (Pentacam)

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

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

289 Corneal haze was the most frequently reported crosslinking-relat

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

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

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

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

294 Patients with stromal haze were excluded.

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

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

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

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

299 China has experienced severe hazes with high concentrations of particulate matter in

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