ライフサイエンスコーパス: solar

1 We conceptually present blackbody-cavity solar absorber designs with nearly ideal spectrally sele

2 siderable interest in the exploration of new solar absorbers that are environmentally stable, absorb

3 S(3) thin films are excellent candidates for solar absorbers.

4 bertian limit for a 10-mum thick silicon for solar absorption over the 300-1,200 nm band.

5 lar cell architectures relies essentially on solar absorption well beyond the Lambertian light trappi

6 architecture has exhibited above-Lambertian solar absorption, integrated over the broad solar spectr

7 rays which are themselves directly linked to solar activity and the earth magnetic field.

8 messaging is twice as effective in inducing solar adoption both during and after the intervention.

9 on focuses on leveraging two motivations for solar adoption: self-interest and prosocial.

10 The co-occurrence of solar and chondritic noble gases in the deep mantle is t

11 y from both the external environment such as solar and radiofrequency, and the human body itself such

12 interest in chemical storage of intermittent solar and wind energy(1,2).

13 but also opens the door for nanoengineered, solar-based methods to remediate recalcitrant micropollu

14 e absence of illumination-a process we call "solar battery swimming"-lasting half an hour and possibl

15 ast, persistent phosphors for higher-energy, solar-blind ultraviolet-C wavelengths (200-280 nm) are l

16 A major challenge for organic solar cell (OSC) research is how to minimize the tradeof

17 Up to now, no solar cell architecture has exhibited above-Lambertian s

18 efficiency in thin film crystalline silicon solar cell architectures relies essentially on solar abs

19 ture of a commercial polycrystalline silicon solar cell by 17 degrees C under one sun condition and e

20 and in delivering insights in, for example, solar cell degradation mechanisms via phase separation,

21 ction and recombination processes that limit solar cell efficiencies.

22 Shockley-Queisser limit for single-junction solar cell efficiency through the production of two elec

23 As a result, the solar cell efficiency was increased to 23.25 % from 21.0

24 The perovskite solar cell modified with a metal-organic framework could

25 contact, however, results in extremely poor solar cell performance.

26 cations involving light-emitting devices and solar cell technology.

27 We developed a stable perovskite solar cell with a bandgap of ~1.7 electron volts that re

28 s leads to a cesium-based ternary perovskite solar cell with stabilized power output of 21.32% at max

29 The photoactive layer of bulk heterojunction solar cell, whose performance is strongly correlated to

30 ntensity that reaches the active part of the solar cell.

31 ly improved CsPbI(3) PQD synthetic yield and solar-cell performance through surface ligand management

32 develop the optimal bulk heterojunction for solar-cell, photodetector, and photocatalytic applicatio

33 Organic solar cells (OSCs) based on D18:Y6 have recently exhibit

34 vice fabrication, the performance of organic solar cells (OSCs) has improved markedly in recent years

35 rphology tuning of the blend film in organic solar cells (OSCs) is a key approach to improve device e

36 ed, non-fullerene-based, and ternary organic solar cells (OSCs) over a wide range of interlayer thick

37 rformance of NiO-based p-type dye-sensitized solar cells (p-DSCs), the function of the surface states

38 the current-voltage hysteresis in perovskite solar cells (PSCs) and, in turn, to impact the interfaci

39 Metal-halide perovskite solar cells (PSCs) are one of the most promising photovo

40 tate-of-the-art, high-performance perovskite solar cells (PSCs) contain a large amount of iodine to r

41 Environmental stability of perovskite solar cells (PSCs) has been improved by trial-and-error

42 The operational instability of perovskite solar cells (PSCs) is known to mainly originate from the

43 Surface passivation of perovskite solar cells (PSCs) using a low-cost industrial organic p

44 istine TiO(2) -based devices, the perovskite solar cells (PSCs) with acid-treated TiO(2) ETL exhibit

45 Currently, blade-coated perovskite solar cells (PSCs) with high power conversion efficienci

46 were synthesized and employed in perovskite solar cells (PSCs).

47 on transport materials (ETMs) for perovskite solar cells (PSCs); however, experimental evidence is la

48 All-inorganic perovskite solar cells (PVSCs) have drawn increasing attention beca

49 for various optoelectronic devices including solar cells and light-emitting diodes for improved stabi

50 of perovskites for more efficient and stable solar cells and other optoelectronic devices.

51 arious optoelectronic applications including solar cells and photodetectors.

52 uences for our current understanding of both solar cells and photodiodes - in the latter case definin

53 erformance of single-junction narrow-bandgap solar cells and, potentially, to give a highly efficient

54 cate high efficiency and low-cost perovskite solar cells at speed.

55 hich has resulted in the highest performance solar cells based on mixtures of Cs, methylammonium, and

56 while it is found challenging in perovskite solar cells because of the difficulty in doping perovski

57 d to impact next generation high performance solar cells because of their extraordinary charge transp

58 ility of hybrid organic-inorganic perovskite solar cells by using different organic agents as additiv

59 property variations in colloidal quantum dot solar cells due to film defects, physical damage, and co

60 ammonium (MA)/formaminidium (FA)) perovskite solar cells from ~19.2% (reference) to 20.8% (using 1 vo

61 State-of-the-art halide perovskite solar cells have bandgaps larger than 1.45 eV, which res

62 Perovskite solar cells have developed into a promising branch of re

63 Specifically, non-fullerene small-molecule solar cells have recently shown a high power conversion

64 ive a highly efficient alternative to bottom solar cells in tandem devices.

65 e doping of semiconductors in heterojunction solar cells shows tremendous success in enhancing the pe

66 Tandem solar cells that pair silicon with a metal halide perovs

67 rgy-harvesting/storage devices, ranging from solar cells to rechargeable batteries.

68 terfacial charge recombination in perovskite solar cells which is in complimentary to broadly applied

69 2D perovskite solar cells with high stability and high efficiency have

70 rection for achieving low-bandgap perovskite solar cells with high stability.

71 help advancing our understanding and lead to solar cells with higher efficiency.

72 e-of-the-art CdS in Cu(In,Ga)Se(2) thin-film solar cells, alternatives rarely exceed reference device

73 mes, in addition to photovoltaic devices and solar cells, among a vast multitude of other usages.

74 Perovskite solar cells, as an emerging high-efficiency and low-cost

75 In metal halide perovskite solar cells, electron transport layers (ETLs) such as Ti

76 s recombination and hysteresis in perovskite solar cells, is revealed.

77 for applications such as solution-processed solar cells, light-emitting diodes, detectors and lasers

78 nt of other optoelectronic devices including solar cells, photodetectors, and light-emitting diodes.

79 icularly challenging in the present best CQD solar cells, since these employ a p-type hole-transport

80 After applying PT-TPA into perovskite solar cells, the doping-induced band bending in perovski

81 the tremendous interest in halide perovskite solar cells, the structural reasons that cause the all-i

82 For next generation organic solar cells, this involves intermolecular charge-transfe

83 ons, including ultrathin flexible materials, solar cells, touch-screen panels, nanotextured surfaces

84 performance perovskite-based photodetectors, solar cells, transistors, scintillators, etc.

85 erence to their target applications, namely: solar cells, transparent film heaters, sensors, and disp

86 e efficiency is by fabricating multijunction solar cells, which can split the solar spectrum, reducin

87 g the performance of many types of inorganic solar cells, while it is found challenging in perovskite

88 ls were embedded, limiting the efficiency of solar cells.

89 iency of 25.7% for perovskite-silicon tandem solar cells.

90 ency approaching 15% for CsPbI(3) -PQD-based solar cells.

91 dustry-relevant textured crystalline silicon solar cells.

92 skite single-crystalline and polycrystalline solar cells.

93 ternary, flexible, and OSC/perovskite hybrid solar cells.

94 energy-density batteries and high-efficiency solar cells.

95 the long-debated ideality factor in organic solar cells.

96 the performance and stability of perovskite solar cells.

97 lue of 1.46 eV, suitable for single junction solar cells.

98 ty and voltage issues inherent in perovskite solar cells.

99 ich is promising for incorporation of GeH in solar cells.

100 issue that leads to a loss of efficiency in solar cells.

101 extraction layers in metal-halide perovskite solar cells.

102 igh power conversion efficiencies in organic solar cells.

103 al for the successful application of organic solar cells.

104 e high-performance bulk heterojunction (BHJ) solar cells.

105 atforms for artificial reduction of CO(2) to solar chemicals and fuels.

106 could potentially enable increased efficient solar collection in extreme operating conditions such as

107 (NC)-polymer composite thin-film luminescent solar concentrators (LSCs) featuring high absolute photo

108 n clocks, the pace of which is linked to the solar cycle.

109 circadian oscillators and resonance with the solar day is largely enabled by a neural pacemaker, whic

110 icular interest owing to their potential for solar-driven chemistry and biomedical applications.

111 These insights are extended to solar-driven hydrogen production using MoS(3), MoP, or R

112 and Gd-IHEP-8 show excellent activity toward solar-driven nitrogen fixation, with ammonia production

113 The solar-driven photocatalytic reduction of CO(2) (CO(2) RR

114 tion fundamentally restricts practicality of solar-driven wastewater treatment.

115 Solar-driven water evaporation rate of 2.63 kg m(-2) h(-

116 Solar-driven water evaporation represents an environment

117 a multitude of cues, such as wind speed and solar elevation, and the process is complicated by forec

118 Photosystem II (PS II) captures solar energy and directs charge separation (CS) across t

119 vskites have high potential as materials for solar energy applications, but their microscopic propert

120 uels to generate electrical power, utilizing solar energy as a green and sustainable energy source is

121 The ability to predict wind and solar energy availability in the upcoming season can hel

122 e, and cost-effective strategy of harvesting solar energy by solar heating during the daytime and har

123 erfaces, which is an exploitable behavior in solar energy conversion and other applications that util

124 from water with an overall quantum yield for solar energy conversion to hydrogen gas of ~4.0% (with a

125 ion in energy generation lies the science of solar energy conversion using new or improved photovolta

126 al chemistry, biology, electrochemistry, and solar energy conversion.

127 ontinue to rise, raising their prospects for solar energy conversion.

128 e as electron or hole transport channels for solar energy harvesting and conversion, but their insuff

129 ectrical storage is a worthwhile approach to solar energy harvesting.

130 The storage of solar energy in chemical bonds will depend on pH-univers

131 s been a barrier to realizing utilization of solar energy in photochemical processes on a global scal

132 ocatalysts for the conversion and storage of solar energy into chemical bonds are rare, inefficient a

133 two fundamental processes: the conversion of solar energy into chemical energy, or the diffusion of C

134 rochemical (PEC) water reduction, converting solar energy into environmentally friendly hydrogen fuel

135 The utilization of solar energy is restricted by the intermittent nature of

136 nd gap (0.7 eV) limits its applications as a solar energy material, therefore tuning its electronic p

137 Making use of the intrinsic solar energy storage ability of PHI, we establish the co

138 and double energy conversion efficiency from solar energy to biomass.

139 ectrochemical cells for direct conversion of solar energy to electricity (or hydrogen) are one of the

140 W/m(2) of heating power density (over 93% of solar energy utilized) because of the suppression of the

141 detergents, and heavy metal components using solar energy with long-term durability and stability.

142 e advantage of the heat and light content of solar energy, it would be advantageous to make indium ox

143 e Janus microswimmers that can be charged by solar energy, thus enabling persistent light-induced pro

144 These include solar energy-to-fuel conversion, solid oxide fuel and el

145 ng traditional rare-metal-based emitters for solar-energy conversion and photoluminescence applicatio

146 As a result, the hydrogel-based solar evaporator can extract water from a variety of con

147 n designing highly efficient cellulose-based solar evaporators, including utilizing extracted cellulo

148 mbination (LRST) are known to increase berry solar exposure affecting berry composition and consequen

149 Water temperature and the solar exposure history of CDOM had a major influence on

150 Using light conditions in full solar exposure, light filtered by oxygenic phototrophs,

151 tored magnetic energy is enough to power the solar flare, including the associated eruption, particle

152 1 sun conditions employing a broad range of solar fluxes.

153 he NAO throughout the Common Era, likely via solar forcing.

154 ission-relevant changes, including growth of solar from ~1 to ~20% of generation in California, and >

155 for organic semiconductor photocathodes for solar fuel production and advances the understanding of

156 energy storage, biological applications, and solar fuels production.

157 ctrocatalyst presents a promising avenue for solar fuels synthesis from carbon dioxide (CO(2)) fixati

158 ectors, thermally super-insulating aerogels, solar gain regulators, and low-emissivity coatings, with

159 To evaluate impacts of solar geoengineering and greenhouse gas-driven climate c

160 ing heterogeneity in the economic impacts of solar geoengineering is a fundamental step towards under

161 However, solar geoengineering may not be fail-safe to prevent glo

162 east in this extreme and idealized scenario, solar geoengineering may not suffice to counter greenhou

163 iscussions of the distribution of impacts of solar geoengineering, a topic of concern in geoengineeri

164 This effect is not mitigated by solar geoengineering.

165 e inequality between countries is lower with solar geoengineering.

166 We focus on the strategic implications of solar geoengineering.

167 ctive strategy of harvesting solar energy by solar heating during the daytime and harnessing the cold

168 te the biota's exposure to sunlight, surface solar heating, and dissolved organic matter dynamics.

169 longer lasting, devolatilization history by solar heating.

170 ceptor bulk heterojunction photocathodes for solar hydrogen production and significantly advance thei

171 effect produces a direct current (DC) under solar illumination owing to the directional separation o

172 Effective use of solar-induced chlorophyll fluorescence (SIF) to estimate

173 d-observed GPP, net primary productivity and solar-induced fluorescence was better or equally well ca

174 erse models from gross primary production or solar-induced fluorescence.

175 is restricted by the intermittent nature of solar influx.

176 Solar insolation and electricity pricing structures were

177 It is found that the solar insolation effect also exists in the Southern Hemi

178 ith the increase of boreal summer integrated solar insolation, and during this stage three millennial

179 was offset by a nearly opposite gradient in solar insolation, such that large-scale spatial patterns

180 overed that the aurora is also controlled by solar insolation.

181 gesting that it is an effect associated with solar insolation.

182 lding) below the ambient temperature under a solar intensity of 744 W m(-2) (850 W m(-2) ), yielding

183 photosynthetic organisms, the conversion of solar into chemical energy occurs in thylakoid membranes

184 and waste stabilization ponds by integrating solar irradiance and aquatic photochemistry models under

185 and environmental data such as temperature, solar irradiance and barometric pressure.

186 h T (mean air-T of 30-d before measurement), solar irradiance and vapour pressure deficit, with growt

187 The remaining 80% of solar irradiance is converted into heat, and thus improv

188 Solar irradiance provides energy to desorb water vapor a

189 range and possible operation at non-coherent solar irradiance.

190 erefore, here, we investigate the effects of solar irradiation on an asphalt binder.

191 R-MS peak intensities with chlorophyll a and solar irradiation were used to define 9 reactivity class

192 sols are on the order of hours under typical solar irradiation, while the absorption and ON lifetimes

193 This study clarified the solar irradiation-triggered self-oxidation process in so

194 the individual and interacting components of solar light and therefore photodamage mechanisms and pho

195 eved, along with outstanding stability under solar light.

196 Exposure to high doses of solar long wavelength ultraviolet radiation (UVA) damage

197 etinal phototoxicity resulting from laser or solar maculopathy (5 eyes); and macular telangiectasia t

198 stem 2MASS J05215658+4359220 has a mass of 1 solar mass (M ( )), then its unseen companion could be a

199 about 1:20 and contains about three million solar masses of gas.

200 ionized carbon emission of about 72 billion solar masses.

201 e measurements of emerging materials such as solar materials, electrocatalysts, and nanomaterials.

202 f the empirical system was far away from the solar maximum.

203 t containing an outermost layer of primitive solar nebula materials.

204 7-kiloparsec arrangement of dense gas in the solar neighbourhood that contains many of the clouds tho

205 ered by renewable electricity generated from solar or wind sources.

206 ns for replacing power plants with new wind, solar, or natural gas to meet a CO(2) reduction target i

207 We demonstrate unassisted solar overall water splitting by combining the optimised

208 verall power increase of ~5% and decrease of solar panel degradation by +0.3%/year.

209 manufacturing linked to technologies such as solar panels and electric vehicles.

210 diation (GCR) and the possibility of a large solar particle event (SPE).

211 ermine the optimal location for constructing solar photovoltaic (PV) farms.

212 ge-scale initiative to systematically deploy solar photovoltaic (PV) projects to alleviate poverty in

213 associated with onshore wind, hydropower and solar photovoltaic generation, within three important co

214 nductors relevant to improved performance in solar photovoltaics or light-emitting diodes.

215 The costs for solar photovoltaics, wind, and battery storage have drop

216 obust material offering high efficiencies in solar photovoltaics.

217 he horizontal components of these calculated solar positions were topographically encoded in the prot

218 mal absorption characteristics for efficient solar power conversion.

219 While solar power systems have offered a wide variety of elect

220 rea by roll-to-roll printing for lightweight solar power systems.

221 are a versatile and compact route to harness solar power.

222 h selecting a specific site for constructing solar PV farms.

223 normalized difference vegetation index, and solar radiation all significantly predicted likelihood o

224 requires particle-phase humic acid to absorb solar radiation and become photoexcited, then directly o

225 strongly correlated with exposure to higher solar radiation and evaporative demand.

226 me mesic regions (10 degrees -15 degrees S), solar radiation and increased temperature caused increas

227 fect Earth's radiative balance by scattering solar radiation and serving as cloud condensation nuclei

228 he Earth's climate system because it absorbs solar radiation and therefore potentially warms the clim

229 ly-September season to predict wind speed or solar radiation during the subsequent November-January s

230 ive skill is highest for both wind speed and solar radiation during winter, and lowest during summer.

231 s more sensitive to the fluctuations of mean solar radiation in hot arid regions.

232 6 h, corresponding to 3 to 6 days of natural solar radiation in summer at the sampling locations.

233 ure regimes, absolute and relative inputs of solar radiation in ultraviolet and photosynthetically ac

234 d fuzzy_DS methods at 20 points with various solar radiation intensities and the number of dusty days

235 (0.2 mum) samples were exposed to artificial solar radiation of 350 W m(-2) for 48 to 96 h, correspon

236 the wavelength dependence of the effects of solar radiation on biological and ecological processes;

237 avitational effects of the sun and moon, and solar radiation pressure) to reduce their propellant and

238 n the future power supply and long-term mean solar radiation trends is spatially heterogeneous, showi

239 Solar radiation was used as the surrogate variable to de

240 d further analyses suggest that xeric areas, solar radiation, and non-forest plant productivity are a

241 cularly those with nests exposed to incident solar radiation, have darker eggs.

242 Black carbon (BC) absorbs solar radiation, leading to a strong but uncertain warmi

243 osses more than changes in precipitation and solar radiation, leading to strongest impacts in tempera

244 g winter are mitigated by the seasonality of solar radiation.

245 s and a consequent decrease in reflection of solar radiation.

246 n to outer space and simultaneously maximize solar reflectance.

247 A metasurface optical solar reflector is shown to produce infrared emissivity

248 that harvest three times more energy in the solar's spectrum peak for GaInP photovoltaics.

249 these neural phenotypes was calculated using SOLAR (Sequential Oligogenic Linkage Analysis Routines).

250 onversion efficiency of 4.33% under AM 1.5 G solar simulated light.

251 al UVR dose, to 85% body surface area, using solar simulated UVR or narrowband UVB (311 nm).

252 dized on artificial seawater by the use of a solar simulator.

253 lead to utilization of a larger part of the solar spectrum and (ii) in NIR stimulated biological app

254 ltijunction solar cells, which can split the solar spectrum, reducing thermalization loss.

255 solar absorption, integrated over the broad solar spectrum.

256 Solar steam generation, which harnesses the abundant sun

257 ractive as supporting substrate materials in solar steam generators are briefly discussed.

258 ability, are highly attractive for realizing solar steam generators.

259 increased radio frequency noise generated by solar storms, suggesting the potential for magnetorecept

260 The solar system (SS) moves through the interstellar medium

261 t with volatile-rich material from the outer Solar System being delivered to Earth during late accret

262 features, unlike those on previously visited Solar System bodies.

263 The gas and ice giants in our solar system can be seen as a natural laboratory for the

264 h differentiation within the first 100 My of solar system formation.

265 star formation and cosmochemical studies of Solar System formation.

266 for evidence of extraterrestrial life in our Solar System is currently guided by our understanding of

267 The outer Solar System object (486958) Arrokoth (provisional desig

268 C-type) asteroids(1) are relics of the early Solar System that have preserved primitive materials sin

269 te meteorites, which originated in the outer Solar System where water was more abundant.

270 bolic and hyperbolic escaping orbits, of the solar system without learning or knowing Newton's laws o

271 discovered thousands of planets outside the Solar System(1), most of which orbit stars that will eve

272 s are the first solids to have formed in the Solar System, defining the epoch of its birth on an abso

273 cretion processes that operated in the early Solar System.

274 well as in magnetized plasmas throughout the solar system.

275 the surface dates from the formation of the Solar System.

276 eologic processes that occurred in the early Solar System.

277 iled characterization of planets outside the Solar System.

278 t of a gentle, low-speed merger in the early Solar System.

279 id of water because they formed in the inner Solar System.

280 neration approaches including photovoltaics, solar thermal power systems, and solar thermoelectric ge

281 tovoltaics, solar thermal power systems, and solar thermoelectric generators, the ability to generate

282 eases the likelihood that adopters recommend solar to their friends and neighbors.

283 ctions induced by plasmons achieve effective solar-to-chemical energy conversion.

284 The tantalizing possibility of 31% solar-to-electric power conversion efficiency in thin fi

285 e split water without any external bias at a solar-to-hydrogen conversion efficiency of 0.51 % at the

286 f 0.55 V vs. RHE and a record high half-cell solar-to-hydrogen conversion efficiency of 4.33% under A

287 thode with a BiVO(4) photoanode, achieving a solar-to-hydrogen efficiency of 1.5% with stability over

288 lytic system allows efficient photocatalytic solar transformations.

289 X-ray emission from young solar-type stars is thousands of times brighter than tha

290 any classes of pulsators, including low-mass solar-type stars(2), red giants(3), high-mass stars(4) a

291 squamous cell carcinoma (cSCC) is caused by solar ultraviolet (SUV) exposure and is the most common

292 The ability of solar ultraviolet (UV) to induce skin cancer and photoag

293 hat provide pigmentation and protection from solar UV radiation to the skin.

294 ssibilities for a deployable, cost-effective solar water purification system with assured water quali

295 This trend is independent of the solar wind driving, suggesting that it is an effect asso

296 lux density at geosynchronous orbit, and the solar wind dynamic pressure and IMF flux density at L1.

297 Solar wind provides an example of a weakly collisional p

298 position that the ripples propagate from the solar wind to the F-region, and that they are a related,

299 ere recently ionized, and "picked up" by the solar wind.

300 tion of the sulfide by energetic ions of the solar wind.