ライフサイエンスコーパス: sun

1 ihelia, about 24 million kilometres from the Sun.

2 olarized light cue possibly representing the sun.

3 small as 0.3 astronomical units(2-5) to the Sun.

4 nergy conversion efficiency of 91.5% under 1 Sun.

5 he sky, which depends on the position of the sun.

6 olarized light spot, likely representing the sun.

7 t redistributes the incident energy from the Sun.

8 final distribution of their mass around the Sun.

9 y offset as the Earth rotates and orbits the Sun.

10 tions, which are frequently ejected from the Sun.

11 n enhanced particle flux of the early active sun.

12 hydrodynamic structures within 0.3 AU of the Sun.

13 gered activity at greater distances from the Sun.

14 onizes with the east-west progression of the sun.

15 errestrial events until they are seen on the Sun.

16 sands of times brighter than that of today's sun.

17 at compositionally most closely resemble the Sun.

18 and a possible self-locked state for unbound SUN.

19 capacity, wings can overheat rapidly in the sun.

20 ly experienced an orbital excursion near the Sun.

21 rbivore abundance than those growing in full-sun.

22 by selectively planting their crops in full sun.

23 H <= 4.5) for photon fluxes between 1 and 10 suns.

24 e-light illumination intensities of up to 37 Suns.

25 erature of 880 [Formula: see text]C under 10 suns.

26 temperature (at the GOC) as measured under 1 SUN 1.5 AM condition.

27 rs achieve a high evaporation rate under one sun (1 kW m(-2) ) at 3.2 kg m(-2) h(-1) out of wastewate

28 h radii less than 60 per cent of that of the Sun(1,2).

29 mass that is less than 30 times that of the Sun(1-4).

30 ssive black hole with a mass of four million Suns(1) within an environment that differs markedly from

31 efficiency of 10.6 +/- 0.3% under AM 1.5G 1 sun (100 mW/cm(2)) simulated illumination with V(OC) = 0

32 oximately 0.3 to 0.4 per cent of that of the Sun(4-6).

33 oretically predicted dust-free zone near the Sun(9-11).

34 res across are present on the surface of the Sun-a phenomenon known as granulation.

35 tellar convection has come from studying the Sun: about two million convective cells with typical siz

36 ities of up to one million times that of the Sun, all classical novae are recurrent, on timescales of

37 minosities up to a million times that of the Sun and a high-velocity mass ejection that produces a re

38 ts iron abundance is about 1/800 that of the Sun and about one-third that of the most iron-poor GCs p

39 have never been substantially heated by the Sun and are therefore well preserved since their formati

40 Sun and colleagues (2017) find that individual Grp+ spin

41 e B (1) is a schinortriterpenoid isolated by Sun and colleagues, which possesses a tetrasubstituted b

42 t in the region just above the corona of the Sun and directly explore the physics of particle acceler

43 was nested within the population-based QSkin Sun and Health Study in Queensland, Australia.

44 s geopotential, gravitational effects of the sun and moon, and solar radiation pressure) to reduce th

45 uctures that are common in the corona of the sun and presumably all stars.

46 180 degrees -rotated azimuth of the setting sun and released after translocation during the same nig

47 nephora, but no difference was found between sun and shade for C. arabica.

48 e years (2016 to 2019) from trees growing in sun and shade habitats.

49 We used a common garden experiment with sun and shade treatments to test for variation in plasti

50 f species, and upper- and lower-canopy (i.e. sun and shade) growth environments.

51 ssed under different agricultural practices (sun and shade).

52 hat the bulk of the material that formed the Sun and Solar System accreted within the CAI-forming epo

53 While the core interactions between SUN and the C-terminal residues of the KASH peptide are

54 Two of these are the position of the sun and the pattern of polarized skylight.

55 ster directional information provided by the sun and the wind and can use them in a weighted manner.

56 These include the sun and, in insects, the polarization pattern of the sky

57 erved interactions between Sad-1 and UNC-84 (SUN) and Klarsicht, ANC-1, SYNE homology (KASH) domain p

58 lsive events driven by acceleration near the Sun, and an event related to a coronal mass ejection.

59 cause they receive the least energy from the sun, and this extreme light climate varies on many diffe

60 Humans have several SUN- and KASH-containing proteins, yet what governs thei

61 the animal and the direction of a simulated sun are represented in a compass-like fashion in the cen

62 with masses around 10,000 times that of the Sun-are ideal seed candidates(3-6).

63 ibility of storing energy collected from the sun as heat by sensible, latent, or thermochemical means

64 hese animals use celestial cues, such as the sun, as an orientation reference.

65 2051 B-the sixth-nearest white dwarf to the Sun-as 0.675 +/- 0.051 solar masses.

66 tudied the facial complexity of group-housed sun bears, a typically solitary species, with special fo

67 Traditionally, the tuber is exposed to the sun before consumption, in order to reduce its bitternes

68 sses that transport energy outwards from the Sun before depositing it in the wind.

69 ions in the Khoa Reef near the Island of the Sun, Bolivia.

70 sion forces the corona to co-rotate with the Sun, but any residual rotation far from the Sun reported

71 res of the daytime sky, all generated by the sun, can be exploited for navigation.

72 ; monoculture plantings (Iris ensata 'Rising Sun', Canna xgeneralis 'Firebird', Agrostis alba, Carex

73 irds of 265 species between 1999 and 2010 in sun coffee plantations, riparian corridors, secondary fo

74 n (e.g. Mercury, Jupiter's moon Europa, near-Sun comets), as well as terrestrial applications.

75 D) and shade combined with sun-exposure (SHA-SUN) compared to recently harvested tubers (INIT).

76 well with the previously demonstrated direct sun compass based on unpolarized light stimulation.

77 silicon solar cell by 17 degrees C under one sun condition and enhances its efficiency from 14.5% to

78 % with stability over 10 h under simulated 1 sun conditions employing a broad range of solar fluxes.

79 In an aqueous electrolyte, under 1 sun conditions, a water-soluble AQ salt is employed with

80 ersion efficiencies of over 23% under AM 1.5 sun conditions.

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

82 Using the SUN criteria, our study confirmed that elevated IOP and

83 Standardization of Uveitis Nomenclature (SUN) criteria were used to better assess different types

84 ormal skin can be used to measure cumulative sun damage and risk of skin cancer.

85 techniques to quantify mutational burden in sun-damaged skin and its reduction by various therapies.

86 control of melanomas arising in chronically sun-damaged skin on the head and neck has favorable recu

87 lving white dwarfs within 100 parsecs of the Sun, determined using photometry and parallax data from

88 g various KASH domain proteins with the same SUN domain protein.

89 ion with nuclear inner membrane Sad1/UNC-84 (SUN) domain proteins SUN1 and SUN2.

90 cifically to levels and PTMs of Sad1/UNC-84 (SUN) domain-containing protein 2 (SUN2).

91 teraction vectors, we predict a link between SUN-domain proteins and protein glycosylation in the end

92 Using a SUN dominant-negative strategy, we demonstrate that LINC

93 A must from sun-dried Pedro Ximenez grapes was employed.

94 In artificial photosynthesis, the sun drives water splitting into H(2) and O(2) or convert

95 , 45 and 50 degrees C), tray drying (TD) and sun drying (SD) on the quality of Arabica coffee was eva

96 FD), hot-air drying (HD) at 50 degrees C and sun drying (SD).

97 Sun drying reduces the loss of anthocyanins and gamma-or

98 by two types of small-scale drying (oven or sun drying), over two years of production.

99 ree drying methods (Oven-drying, Air-drying, Sun-drying), as well as the Oven-drying temperature usin

100 ionized regions of the disk surrounding the Sun during its formation may have triggered the formatio

101 itational deflection of starlight around the Sun during the 1919 total solar eclipse provided measure

102 Here we report observations of the near-Sun energetic particle radiation environment over the fi

103 ng unmodified Ru(bpy)(3)Cl(2) photocatalyst, sun energy, atmospheric O(2), and at ambient temperature

104 00 muA/cm(2) and approximately 1 mV under 40 Suns equivalent excitation with 405 nm light.

105 SEE SUN ET AL DOI101093/AWW306 FOR A SCIENTIFIC COMMENTARY O

106 In this issue of Molecular Cell,Sun et al.

107 In this issue of Cancer Cell, Sun et al. describe context-dependent oncogenic and tumo

108 Sun et al. discover that neuronal firing rates of hippoc

109 A recently published article (Sun et al.) describes the potential mechanism underlying

110 en et al., 2020; Matsumoto et al., 2020, and Sun et al., 2020) demonstrate an equitable homeostatic a

111 human patients, samples were collected from sun-exposed and sun-protected areas, which were then sub

112 aracterized by hyperpigmented patchy skin in sun-exposed areas, especially the face.

113 p between UV-induced mutations in habitually sun-exposed human skin and subsequent development of act

114 Sun-exposed leaves of 50 species at seven sites were mea

115 hielded melanocytes had fewer mutations than sun-exposed melanocytes.

116 he low RTD on the hand and high RTDs on less sun-exposed sites suggest a complex association between

117 burden than melanocytes from intermittently sun-exposed skin (for example, the back).

118 However, melanocytes from chronically sun-exposed skin (for example, the face) had a lower mut

119 Cancers from sun-exposed skin accumulate "driver" mutations, causally

120 Normal sun-exposed skin contains numerous epidermal patches tha

121 We found that sun-exposed skin, esophagus, and lung have a higher muta

122 a de facto endogenous UVA photosensitiser in sun-exposed skin.

123 substantially increased mutational loads in sun-exposed versus sun-protected areas were observed, su

124 CI: 0.92, 1.05), skin reaction to prolonged sun exposure (for painful burn with blisters vs. practic

125 es that the users can be alerted to moderate sun exposure and may prevent skin damage.

126 sites suggest a complex association between sun exposure and occurrence of BCC.

127 stogen users had lower levels of residential sun exposure and were more likely to report sunscreen us

128 ning ability, and skin reaction to prolonged sun exposure as surrogate measures of pigmentation among

129 onic patch whose original color changes upon sun exposure due to its UV-responsive capabilities that

130 Results showed that sun exposure for prolonged times (9 days) resulted in in

131 d eye color; skin cancer family history; and sun exposure history, such as tanning ability and number

132 trient intake from food and supplements (and sun exposure in the case of vitamin D outcomes).

133 ated with decreased uveitis activity, as was sun exposure in those with vitamin D deficiency.

134 Sun exposure is a major environmental risk factor for sk

135 to report sunscreen use, suggesting specific sun exposure profiles in users.

136 ) cells in blood and skin lesions induced by sun exposure that are infiltrated with EBV-infected lymp

137 FICZ is a light-dependent hormone that links sun exposure to regulation of biological pathways in per

138 nalysis of vitamin D-deficient participants, sun exposure was associated significantly with uveitis i

139 d with decreased risk of TNBC, and increased sun exposure was associated with reduced risk of ER+, ER

140 (VDD) may be high in countries with abundant sun exposure year-round, but nationally representative d

141 rting symptoms before vs after 10 minutes of sun exposure, 2233 vs 1524 microg/dL; P </= .001), and i

142 This can have effects on health because sun exposure, although beneficial, when prolonged and re

143 As patients with melanoma commonly avoid sun exposure, and consequent vitamin D deficiency might

144 esses across its subtypes, some unrelated to sun exposure, and extends potential involvement of the n

145 ess of the adverse consequences of excessive sun exposure, modifying sun-seeking behavior is challeng

146 stment for age, sex, percentage of body fat, sun exposure, physical activity, and dietary vitamin D i

147 not show evidence of a confounding effect of sun exposure, progestogen users had lower levels of resi

148 ion of several environmental factors such as sun exposure, temperature, relative humidity, air pollut

149 e the main component of skin aging caused by sun exposure.

150 all exposed body sites 22 to 24 hours after sun exposure.

151 r, this finding is most likely confounded by sun exposure.

152 apeutic drugs, environmental pollutants, and sun exposure.

153 ange material channel in contact with direct sun exposure.

154 d may help improve people's attitudes toward sun exposure.

155 refrigeration (COLD) and shade combined with sun-exposure (SHA-SUN) compared to recently harvested tu

156 bjected to different postharvest treatments: sun-exposure (SUN), shade (SHA), refrigeration (COLD) an

157 However, parasitic light absorption in the sun-facing front molecular layer, through which sun ligh

158 across this ant-plant clade show that a full-sun farming strategy has existed for millions of years,

159 cted from various seeds such as mustard oil, sun flower oil, sesame oil, ground nut oil, coconut oil,

160 r amounts of shaded foliage relative to full-sun foliage.

161 stimuli can lead to complex behavior such as sun following, canopy escape, and plant twining.

162 r exposure, the PolyDOTS were exposed to the sun for 12 h and "charged".

163 panel orientation angle with respect to the sun for efficient energy conversion.

164 Magnetically driven eruptions on the Sun, from stellar-scale coronal mass ejections to small-

165 yielded the greatest immediate food rewards, sun-grown crops contained less nitrogen compared to shad

166 However, for individual sun-grown leaves from three species, photosynthesis is a

167 effect of light environment (shaded vs full-sun habitat) on leaf toughness and leaf nutritional qual

168 tals under excitation intensity close to one sun, highlighting the intrinsically long carrier recombi

169 high solar steam efficiency of 85.6% under 1 sun illumination (1 kW m(-2) ), which is among the best

170 Under 0.82-sun illumination (825 W/m(2)), a GO leaf floating on wat

171 asurements of the solar cell under "light" 1 sun illumination (AM1.5 solar irradiance spectrum).

172 ion of metal halide perovskite films under 1-sun illumination and claim to exclude heat-induced latti

173 and by 4% after 600 h under continuous full-sun illumination and maximum power point tracking, respe

174 1), with energy efficiency of >96% under one sun illumination and under high salinity (25 wt% NaCl),

175 photocathode is able to produce H(2) under 1 Sun illumination at a rate of ca. 100 mumol cm(-2) h(-1)

176 of the initial efficiency retained under one sun illumination for 500 h.

177 A high efficiency of 22.0% under 1 sun illumination for blade-coated PSCs is demonstrated w

178 y carrier mobility (mu(h) or mu(e))] under 1 sun illumination for both n- and p-type Si components of

179 t burn-in" efficiency over 3400 h under full sun illumination in ambient conditions.

180 duced phase segregation in films even at 100-sun illumination intensity and less than 4% degradation

181 gh-efficiency solar steam generation under 1 sun illumination is used.

182 In a non-aqueous electrolyte, under 1 sun illumination, an organic-soluble AQ is applied and t

183 brium minority carrier concentration under 1 sun illumination, minority carrier effective lifetime an

184 At pH = 7 with 3 Sun illumination, the n-Si/TiO2/C/CNT/[1+1(O)] electrode

185 and operational stability under continuous 1 sun illumination, with an extrapolated lifetime of 2011

186 d operational stability under continuous one-sun illumination.

187 nuous operation in N(2) atmosphere under one-sun illumination.

188 initial performance after 1000 hours of full-Sun illumination.

189 e not limited by Auger recombination under 1-sun illumination.

190 (-1) under air mass 1.5 global (AM 1.5G) one-sun illumination.

191 producing vitamin D3 in human skin than the sun in less than 1/60(th) the time.

192 s generated in inner and outer layers of the Sun indicate that the solar activity is heading in the n

193 Recent progress in observing sun-induced Chl fluorescence (SIF) provides an unprecede

194 ined with concurrent satellite retrievals of Sun-induced chlorophyll fluorescence (SIF) and atmospher

195 gnificance of a signaling molecule, Pak1, in sun-induced premalignant skin lesions and indicates that

196 efficiency after constant illumination at 1 sun intensity for 1000 h.

197 L of water per day with 8 h of sunlight at 1 Sun intensity.

198 e shows high operational stability under one-sun-intensity illumination, with T(80) and T(70) lifetim

199 GST pull-down indicated that nesprin-1/lamin/SUN interactions were disrupted.

200 ses the H(2) production efficiency under one sun irradiation by more than 30%.

201 e a mechanism for methanol oxidation under 1 sun irradiation on these metal oxide surfaces and discus

202 entrated salt solution (20 wt% NaCl) under 1 sun irradiation, as well as long-term stability (over 10

203 ured efficiency could achieve ~92% under one sun irradiation.

204 During the solar minimum, when the Sun is at its least active, the solar wind(1,2) is obser

205 t cues are difficult to read, i.e., when the sun is close to the zenith.

206 Dynamics Observatory, to show that when the Sun is observed as a star, the variation of coronal comp

207 Here, the authors show that if the Sun is observed as a star, then the variation of coronal

208 composition in full-disk observations of the Sun is related to the evolution of coronal magnetic fiel

209 tostability of photovoltaic devices up to 10-Suns is observed, which is a direct result of the superi

210 y gravitational forces from the Moon and the Sun-is sensitive to the density of the two Large Low She

211 rotein binding for NE enrichment, and direct SUN-KASH binding are conserved between plant species.

212 luminal KASH domain, and the function of the SUN-KASH complex.

213 ve distinct differences between the examined SUN-KASH complexes.

214 may have an important role in regulating the SUN-KASH network.

215 -facing front molecular layer, through which sun light must propagate before reaching the perovskite

216 pheric loss than their counterparts orbiting Sun-like stars(3-6).

217 with a mass just eight per cent that of the Sun, located 12 parsecs away.

218 ave masses less than 60 per cent that of the Sun, make up 75 per cent of the population of the stars

219 Here we use full-Sun observations from the Solar Dynamics Observatory, to

220 nd group of organic photovoltaic cells to 20 Suns of ultraviolet illumination (centred at 365 nanomet

221 raviolet B (UVB) radiation (whether from the sun or from an artificial source).

222 n informed by a hierarchical reliance on the sun, overhead polarization patterns, and idiothetic (int

223 e flow velocity of the solar wind around the Sun, peaking at 35 to 50 kilometres per second-considera

224 Previous studies farther from the Sun (performed mostly at a distance of 1 astronomical un

225 ynergistic effect, while Iris ensata 'Rising Sun' performed poorly (fixed less N) within the complete

226 the power block is possible even during off-sun periods, providing CSP plants with a remarkable disp

227 es coated with a MoS(3):MoP composite gave 1 Sun photocurrent density up to 8.7 mA cm(-2) at 0 V vs R

228 sing molecular networks to harvest diffusive sun photons on large areas and funnel them onto much sma

229 er in shade plantations of C. canephora than sun plantations.

230 nce can be used to approximate the change in sun position over time, allowing the compass to remain f

231 d the sky polarization pattern of particular sun positions.

232 d 241 women) aged 57-91 y recruited from the SUN Project (Spain, 1999-2018).

233 n of the Seguimiento Universidad de Navarra (SUN) Project.

234 eased mutational loads in sun-exposed versus sun-protected areas were observed, suggesting that genom

235 ack OTRs, 6 of 9 lesions (66.7%) occurred in sun-protected areas, specifically the genitals.

236 samples were collected from sun-exposed and sun-protected areas, which were then subjected to high-d

237 reduction in the number of epidermal LCs in sun-protected skin with age.

238 the BsmI SNP may emphasize the importance of sun protection and facilitate skin cancer prevention and

239 g bed avoidance, it is critical to emphasize sun protection and skin cancer screening in individuals

240 Furthermore, in vitro sun protection factor (SPF) of berry waxes depicted good

241 a, and the other using only sunscreen with a sun protection factor of 100.

242 o educate the public that combining multiple sun protection measures may be needed to achieve optimal

243 Sun protection should continue to be emphasized in white

244 about sun safety behavior, which would make sun protective behavior more likely, could be promoted a

245 Sun-protective behavior affects skin cancer prevention.

246 localization, dependence of KASH proteins on SUN protein binding for NE enrichment, and direct SUN-KA

247 DC tsMSQ, we demonstrate the ability of the SUN protein SUN2 and the Klarsicht/ANC-1/SYNE homology p

248 For example, in Caenorhabditis elegans, SUN protein UNC-84 binds to two KASH proteins UNC-83 and

249 We find that the Sad1-UNC-84 (SUN) protein Mps3 forms a ring-like structure around the

250 directly with the SUN (Sad1/Unc84) domain of Sun proteins [5-7], a family of transmembrane proteins o

251 s traversing the outer nuclear membrane, and SUN proteins crossing the inner nuclear membrane.

252 arsicht/ANC-1/SYNE homology and Sad1/UNC-84 (SUN) proteins, in the NE of living cells.

253 NC-1/Syne-1 Homology (KASH) and Sad1/UNC-84 (SUN) proteins.

254 The closet exoplanets to the Sun provide opportunities for detailed characterization

255 ts benefited from cultivating plants in full sun, receiving 7.5-fold more floral food rewards compare

256 for an ST-OPV with a PCE = 8.0 +/- 0.2% at 1 sun, reference AM1.5G spectrum.

257 Sun, but any residual rotation far from the Sun reported until now has been much smaller than the am

258 entrated in the thin Galactic disk where the Sun resides.

259 The sun rises at an earlier clock time in the eastern region

260 Mammalian NOP2/Sun RNA Methyltransferase Family Member 2 (NSUN2) has be

261 ct measurements of the magnetic field in the Sun's corona are difficult to obtain.

262 omposition of solar-like stellar coronae.The Sun's elemental composition is a vital part of understan

263 organisms such as cyanobacteria utilize the sun's energy to convert atmospheric carbon dioxide into

264 The existence of the Sun's hot atmosphere and the solar wind acceleration con

265 ely, that a "solar tsunami" occurring in the Sun's interior shear-fluid layer can trigger new cycle's

266 ow that magnetic circular dichroism (MCD) of sun's ultraviolet C light by oxygen in Archaean earth's

267 ay that requires its oligomerization and the SUN (Sad1 and UNc-84)-domain protein, Mps3.

268 This domain interacts directly with the SUN (Sad1/Unc84) domain of Sun proteins [5-7], a family

269 keletal and cardiac muscle and together with SUN (Sad1p/UNC84)-domain containing proteins and lamin A

270 Positive attitudes and beliefs about sun safety behavior, which would make sun protective beh

271 Overall, sun safety practices were not common among schools.

272 Prevalence of sun safety practices.

273 y associated with the adoption of any of the sun safety school practices studied (eg, metropolitan st

274 d with having adopted practices that promote sun safety.

275 from 2,500 United Kingdom twins, we observed sun seeking to be significantly heritable (h2 >= 58%).

276 In a GWAS meta-analysis of sun-seeking behavior in 261,915 subjects of European anc

277 quences of excessive sun exposure, modifying sun-seeking behavior is challenging because it appears t

278 Cases and controls were selected from the SUN (Seguimiento Universidad de Navarra) cohort using ri

279 e of back nevi, presence of many freckles, a sun-sensitive phenotypic index, and prior amelanotic mel

280 uld otherwise arise from clouds/aerosols and sun-sensor geometry).

281 s of forest SIF are not strongly affected by sun-sensor geometry, which was attributed as creating a

282 ferent postharvest treatments: sun-exposure (SUN), shade (SHA), refrigeration (COLD) and shade combin

283 As expected, sun-shielded melanocytes had fewer mutations than sun-ex

284 Pollen total nitrogen content was lower in sun than shade plantations of C. canephora, but no diffe

285 example, when plants self-orient to face the sun throughout the day.

286 bility to efficiently convert light from the sun to form chemical bonds.

287 plunged through the inner heliosphere of the Sun to its perihelia, about 24 million kilometres from t

288 own toward the time-averaged position of the sun, to maximize solar harvesting.

289 age, 1744 vs 1567 microg/dL; P = .02), less sun tolerance (median ePPIX levels for those reporting s

290 Under nonsteady-state conditions of shade to sun transition, stomatal conductance was the major limit

291 Induction during shade to sun transitions of 14 accessions representing five subpo

292 Our results reflect that the sun treatment activates defense systems and osmoprotecti

293 Consequently, moderate sun/UV exposure is strongly recommended.

294 However, the increasing incidence of sun/UV exposure-related illness, such as skin cancer, is

295 d outdoor activities to avoid times when the sun was at peak intensity (15.0%; 95% CI, 11.4%-19.6%),

296 d outdoor activities to avoid times when the sun was at peak intensity.

297 We propose that CAIs formed while the Sun was in transition from the protostellar to pre-main

298 ir investigative work.-Liu, C.-H., Wang, Z., Sun, Y., Chen, J.

299 s from the training set of 227 patients from Sun Yat-sen University (Guangzhou, Guangdong, China) wit

300 Fight for Sight, the Sun Yat-Sen University 5010 Project Fund, Moorfields Eye