ライフサイエンスコーパス: radiative

1 xhibited in the band structure of bound (non-radiative) acoustic surface modes supported on a honeyco

2 offset, the blend system is found to exhibit radiative and non-radiative recombination losses that ar

3 nt density functional theory calculations of radiative and nonradiative decay properties and lifetime

4 tution affects the electronic structures and radiative and nonradiative decay rates.

5 resolved fluorescence spectroscopy furnishes radiative and nonradiative fluorescence decay rates in v

6 ns and are lost to ground state through both radiative and nonradiative pathways via the S(1) and non

7 A detailed understanding of radiative and nonradiative processes in peptides contain

8 open circuit voltage by minimizing both non-radiative and radiative components of the diode dark cur

9 PNFs' spectral reflectance to suit different radiative and thermal environments, yields PNFs which ex

10 Examination of the surface energy balance (radiative and turbulent fluxes) reveals that surplus ene

11 rrestrial hydrological cycle through climate-radiative and vegetation-physiological forcings.

12 is molecular ion, in particular the rates of radiative association and dissociative recombination.

13 ond in the helium hydride ion HeH(+) through radiative association with protons.

14 strating that excitons gaining energy in non-radiative Auger processes can be recovered and recombine

15 o the stratosphere could also perturb global radiative balance by affecting high altitude cloud forma

16 form secondary aerosols that affect Earth's radiative balance by scattering solar radiation and serv

17 The radiative balance in the Arctic region is sensitive to i

18 snow and ice can have strong effects on the radiative balance of the Arctic.

19 Cirrus clouds determine the radiative balance of the upper troposphere and the trans

20 ffect cloud properties and therefore Earth's radiative balance(1-3).

21 d properties, altering precipitation and the radiative balance, ultimately regulating Earth's climate

22 ter formation and their impact on the global radiative balance, while changes in cloud coverage, albe

23 have important consequences for the Earth's radiative balance.

24 ar radiation and, thereby, alter the earth's radiative balance.

25 e may have strong impacts on Earth's surface radiative budget and climate, especially at high latitud

26 -surface temperature pattern, stability, and radiative budget are also found in observations on inter

27 feedbacks of forest fire on Earth's surface radiative budget remain uncertain at the global scale.

28 ), increases in albedo dominated the surface radiative budget resulting in a net cooling effect.

29 Radiative communication using electro-magnetic (EM) fiel

30 voltage by minimizing both non-radiative and radiative components of the diode dark current.

31 ly single sided contact, we measure enhanced radiative conduction up to 16 times higher than the blac

32 uto's thermal structure is expected to be in radiative-conductive equilibrium, the required water vap

33 Subambient daytime radiative cooling (SDRC) provides a promising electricit

34 re into the Arctic, which temporarily reduce radiative cooling and henceforth ice growth.

35 he saturation water vapor pressure and hence radiative cooling by water vapor in clear-sky regions.

36 It is argued that radiative cooling by water vapor plays an important role

37 ains three-fourths of the variability in the radiative cooling effect of clouds, mainly through affec

38 ase CH(4) emissions and hence reduce the net radiative cooling effect of estuarine mangrove forests.

39 The unique feature of radiative cooling lies in the high emissivity in the atm

40 However, most of the radiative cooling materials reported possess broad-band

41 Daytime passive radiative cooling materials shed heat from the ground to

42 the recent advancement of daytime subambient radiative cooling materials, which allow energy-efficien

43 towards large-scale applications of all-day radiative cooling materials.

44 MP thin film makes it a practically scalable radiative cooling method.

45 t reflection and therefore excellent all-day radiative cooling performance.

46 the ambient temperature and a corresponding radiative cooling power of 193 W/m2 during a one-day cyc

47 r coating, the metamaterial shows a noontime radiative cooling power of 93 watts per square meter und

48 0 W/m(2) corresponding to a 7x difference in radiative cooling power.

49 d droplet number concentration and modifying radiative cooling relative to current estimates assuming

50 esses create a heterogeneous distribution of radiative cooling that selectively reduces the temperatu

51 sing the coldness of the outer space through radiative cooling to produce electricity at night using

52 duces cloud cover by modulating the longwave radiative cooling within the atmosphere.

53 nvestigated to achieve the effect of daytime radiative cooling(6-8,10-15).

54 Passive radiative cooling, dissipating an object's heat through

55 t the IR atmospheric transparency window for radiative cooling, in cost-effective infrared sensing de

56 icture of optical heating is supplemented by radiative cooling, which typically takes place at an eve

57 how a new optical resonance arising from the radiative coupling between arrayed silicon NWs can be ha

58 ligands for the relativistic enhancement of radiative deactivation rate processes, especially if Bi-

59 iplet excited states of carbon dots from non-radiative deactivation.

60 uted to fast internal conversion relative to radiative decay and intersystem crossing.

61 OTf) produces a red emission (634-659 nm) by radiative decay from beta-LUMO to beta-SOMO, based on de

62 temperature can be consistently explained by radiative decay of free excitons, bound and trapped exci

63 f triplet-triplet annihilation and promoting radiative decay of the resulting singlet exciton.

64 Auger recombination is the main non-radiative decay pathway for multi-carrier states of coll

65 For the first time, suppression of non-radiative decay pathways of a chromophore was tested by

66 ed entangled photon pairs through a cascaded radiative decay process and do not suffer from any funda

67 ters are decreased and become lower than the radiative decay rate constants (k(r) = 10(5) s(-1)).

68 Our calculations show that the radiative decay rates are dominated in all instances by

69 ld of gold nanocone antennas, we enhance the radiative decay rates of monoexcitons and biexcitons by

70 t rectification ever predicted for far-field radiative diode configurations.

71 sses in materials that-when coupled with non-radiative dissipative processes-allow the conversion of

72 phere can lead to incorrect estimates of the radiative effect and fail to identify unintended consequ

73 y challenge in modeling and quantifying BC's radiative effect on climate is predicting enhancements i

74 th forward for improving predictions of BC's radiative effect on climate.

75 ift would lead to an annual average positive radiative effect over the U.S. of approximately +0.075 W

76 cles would yield a globally uniform negative radiative effect, estimated to be -0.013 W/m(2) over a 2

77 ion nuclei (CCN) that influence the indirect radiative effect, this model-measurement discrepancy in

78 tes 28.25% ( 0.02 W m(-2)) of the whole CCLB radiative effect, twice greater than contrail effect.

79 ly when the inter-model differences in cloud radiative effects are considered.

80 the aerosol-induced public health and direct radiative effects of shifting the U.S. fleet from PFI to

81 crophysics, optical properties and shortwave radiative effects to the surface phase are dictated by a

82 y underestimate SSA scattering (hence direct radiative effects) by a factor of 2 to 5, in addition to

83 interplay of material, thermal, magnetic and radiative effects, allowing a steady shock to form at a

84 g in larger open-circuit voltages and higher radiative efficiencies.

85 high temperature, preventing improvements in radiative efficiency and applications such as thermophot

86 solar cell structures suggests that apparent radiative efficiency is suppressed, and the collection e

87 ll InGaN/GaN LEDs by decoupling the inherent radiative efficiency, injection efficiency, carrier tran

88 urface layer therefore recombine with a high radiative efficiency, with the photoluminescence quantum

89 spin configuration with generally forbidden radiative emission.

90 Photo-induced non-radiative energy dissipation is a potential pathway to i

91 g Solar System planetary atmospheres, as its radiative energy equilibrium is controlled primarily by

92 provide an observational diagnostic for the radiative energy input and the dynamics of the interstel

93 issipative processes-allow the conversion of radiative energy into heat.

94 Massive stars inject mechanical and radiative energy into the surrounding environment, which

95 al flow immunoassay (FLFIA) depending on non-radiative energy transfer between graphene oxide and qua

96 Taking advantage of the highly efficient non-radiative energy transfer occurring between photoexcited

97 velengths shorter than 370 nm, the far field radiative enhancements of aluminum nanostructures are si

98 size of the nanoparticle and have far field radiative enhancements of up to three orders of magnitud

99 In an open radiative environment, the hallmark of collective intera

100 globally relative to non-fixing trees by the radiative equivalent of 0.77 Pg C yr(-1) under nitrogen

101 y, neutral exciton recombination is entirely radiative even in the presence of a high native defect d

102 X-ray-selected black holes that reveals that radiative feedback on dusty gas is the main physical mec

103 ravitational potential of the black hole; by radiative feedback; or by the interplay between outflows

104 rfaces and the perovskite surface on the non-radiative fill factor and open-circuit voltage loss.

105 ve caused an extraordinary downward longwave radiative flux to the ice surface, which may then amplif

106 even today, the direct measurement of global radiative fluxes is difficult, such that most assessment

107 f precipitation, rain-snow partitioning, and radiative fluxes.

108 The optical radiative force on the mechanical structure is also cons

109 ate and land use change decreases the direct radiative forcing (-0.38 W m(-2)) by 6.3% and the indire

110 ing (-0.38 W m(-2)) by 6.3% and the indirect radiative forcing (-1.68 W m(-2)) by 3.5% due to the siz

111 nalytical model is developed to estimate the radiative forcing (RF) using a novel model form and an i

112 Converted to radiative forcing (RF), we estimated that fires generate

113 and may play an important role in planetary radiative forcing and climate.

114 ore likely to have larger impacts on aerosol radiative forcing and could serve as biomass burning tra

115 iodine emissions have implications for ozone radiative forcing and possibly new particle formation ne

116 ion of clouds and their properties including radiative forcing and precipitation, yet the sources and

117 tion in pristine atmospheres, altering cloud radiative forcing and precipitation.

118 s of emissions scenarios, not just the total radiative forcing and resultant warming level, must be c

119 orous particles like dust could impact cloud radiative forcing and, thus, the climate via ice cloud f

120 Overall, the total radiative forcing associated with anthropogenic aerosols

121 sum of the total aerosol direct and indirect radiative forcing by 12.5%.

122 ther proposals suggest masking the increased radiative forcing by an increase in particles and/or clo

123 les should be measured or controlled and (2) radiative forcing by BrC aerosols could be overestimated

124 overestimation of BC loadings and BC Direct Radiative Forcing by current models over North Pacific,

125 at mangrove F(CH4) could offset the negative radiative forcing caused by CO(2) uptake by 52% and 24%

126 a systematic shift, being comparable to the radiative forcing change from preindustrial to present,

127 ls to show that in a CO(2)-enriched climate, radiative forcing changes drive annual precipitation inc

128 equatorial Pacific than expected from simple radiative forcing considerations.

129 The corresponding negative radiative forcing due to aerosol cloud interactions (RF[

130 ncentrations of PM(2.5) and ozone and direct radiative forcing due to aerosols and ozone.

131 -eq yr(-1) ), producing an overall positive radiative forcing effect of 2.4 +/- 0.3 kt CO2 -eq yr(-1

132 change to estimate GHG fluxes and associated radiative forcing effects for the whole wetland, and sep

133 Pbio factors using a forest growth model and radiative forcing effects with a time horizon of 100 yea

134 ts to Arctic warming represents about 10% of radiative forcing effects.

135 (roughly 3/4) of the total aerosol indirect radiative forcing estimate.

136 the largest source of uncertainty in global radiative forcing estimates, hampering our understanding

137 The negative radiative forcing expected from this CO2 uptake is up to

138 a major (35-53%) contributor of atmospheric radiative forcing from the estuary, while N2O contribute

139 is up to 231 times greater than the positive radiative forcing from the methane emissions.

140 Earth system modeling suggests that radiative forcing from this massive, high-latitude erupt

141 he past two decades, with enhanced post-fire radiative forcing in 2018 causing earlier melt and snow

142 implications for aerosol hygroscopicity and radiative forcing in areas with wildfire influence owing

143 their potential impacts in human health and radiative forcing in the air.

144 ios, with stronger drying as the strength of radiative forcing increases.

145 We argue that the latter, even if the radiative forcing is negligible, should more appropriate

146 ensitivity of this region to slow changes in radiative forcing is thus strongly mediated by internal

147 ities < 0.2 m/s, and causes a direct aerosol radiative forcing of +0.15 W/m(2).

148 tration by ~10 % and causes a direct aerosol radiative forcing of -0.10 W/m(2).

149 amely, the ocean carbon buffer capacity, the radiative forcing of carbon dioxide and the carbon inven

150 bon (BrC) is an important contributor to the radiative forcing of climate by organic aerosols.

151 Given assumptions concerning the radiative forcing of greenhouse gases, ice sheets and mi

152 2) yr(-1) is required to offset the positive radiative forcing of increasing CH4 emissions until the

153 Notably, the overall radiative forcing of open-water fluxes (3.5 +/- 0.3 kg C

154 air quality, atmospheric deposition and the radiative forcing of sulfate aerosols.

155 anding for how such aerosols influence solar radiative forcing of the atmosphere.

156 We also estimate that the radiative forcing of tropospheric O(3) since 1850 AD is

157 diation, moisture and wind (e.g. topography, radiative forcing or cold-air pooling).

158 age; and its absorption character may add to radiative forcing processes in the atmosphere.

159 ains, Canada, and evaluate its impact on net radiative forcing relative to potential long-term net ca

160 of the twenty-first century for the steepest radiative forcing scenario is about 15 per cent warmer (

161 In a high radiative forcing scenario, such decreases in economic a

162 tor of approximately two even under the same radiative forcing scenarios.

163 Future modeling of OA radiative forcing should consider the importance of both

164 The palsa site (intact permafrost and low radiative forcing signature) had a phylogenetically clus

165 The bog (thawing permafrost and low radiative forcing signature) had lower alpha diversity a

166 The fen (no underlying permafrost, high radiative forcing signature) had the highest alpha, beta

167 logenetic diversity associated with a higher radiative forcing signature.

168 een 8 cm(-3) and 24 cm(-3) By extension, the radiative forcing since 1850 from aerosol-cloud interact

169 These represent scenarios in which total radiative forcing stabilizes before 2100 (RCP 4.5) or co

170 ula: see text]) is one of the most uncertain radiative forcing terms as reported in the 5th Assessmen

171 reveals a much greater sensitivity of cloud radiative forcing to CCN than previously reported, which

172 rs (an increase of approximately 9 Wm(-2) of radiative forcing) was almost completely negated by a lo

173 contrail age, coverage, optical properties, radiative forcing, and energy forcing (EF) from individu

174 ntury, then the associated large increase in radiative forcing, and how the Earth system would respon

175 o different processes: a rapid adjustment to radiative forcing, followed by a slower response to surf

176 O(2) + HONO) decrease air quality and impact radiative forcing, yet the factors responsible for their

177 tly missing in model calculations of aerosol radiative forcing.

178 vely to understand the contribution of BB to radiative forcing.

179 t has the potential to be a strong source of radiative forcing.

180 ue to reductions in short-lived gases or net radiative forcing.

181 ncy in dry deposition alters modeled CCN and radiative forcing.

182 ncern because of the contribution to climate radiative forcing.

183 m(-2), which is much larger than some of the radiative forcings considered in the Intergovernmental P

184 antiago, and southern Chile; respective mean radiative forcings for the winter months were 2.8, 1.4,

185 ion, and climate's response to anthropogenic radiative forcings.

186 ission increases likely exert a positive net radiative greenhouse gas forcing through the 21st centur

187 sent, experimental techniques to measure the radiative heat flow relied on steady-state systems.

188 reports have experimentally shown near-field radiative heat transfer (NFRHT) exceeding the far-field

189 Super-Planckian near-field radiative heat transfer allows effective heat transfer b

190 experimental studies have demonstrated that radiative heat transfer between macroscopic objects sepa

191 t but also presents a computational study of radiative heat transfer between rectangular dielectric m

192 Here, we show that the radiative heat transfer between two coplanar SiN membran

193 Here we report studies of radiative heat transfer in few A to 5 nm gap sizes, perf

194 7.5 to 14 um are particularly important for radiative heat transfer in the ambient environment, beca

195 the T(4) law limits the ability to regulate radiative heat.

196 tensity can create concurrent sounds through radiative heating of common dielectric materials like ha

197 normal textile, greatly outperforming other radiative heating textiles by more than 3 degrees C.

198 for the fabrication of ceramic materials by radiative heating under an inert atmosphere.

199 e determined by the compensation between the radiative imbalance and poleward energy transport (mainl

200 estimate the long-term evolution of Earth's radiative imbalance in the past.

201 of atmospheric dynamics and cloud effects to radiative imbalance, the satellite-measured radiative re

202 this quantity must be equal to the planetary radiative imbalance.

203 Representing Sc and their radiative impact is one of the largest challenges for gl

204 hrough a 4-8 times decrease in excited state radiative lifetime compared to a bare organic material i

205 ed attribution of the sub-nanosecond exciton radiative lifetime in nanoprecipitates of CsPbBr3 in mel

206 rrow exciton linewidth (18 mueV) reaches the radiative lifetime limit, which is promising towards gen

207 redictions and are primarily dictated by the radiative lifetime of the atomic quantum state instead o

208 laws of photoluminescence quantum yield and radiative lifetime with respect to the aspect ratio of n

209 states of these complexes, and estimate the radiative lifetimes in the ground states of these "semi-

210 appreciable fraction of their 210-picosecond radiative lifetimes.

211 on timescales between the exciton and trion radiative lifetimes.

212 ssion and absorption results in non-physical radiative limits for the V(OC).

213 tions provide estimates of the excited state radiative line width, which we relate to the entangled t

214 r light manipulation, but also leads to high radiative loss rates and commensurately low Q-factors, g

215 pen-circuit voltage (V(OC) ) losses outweigh radiative losses in materials with n > 2.

216 with reduced mode volumes and negligible non-radiative losses.

217 d materials, as well as weak emitters or non-radiative materials.

218 ng a surface-plasmon-enhanced excitation and radiative mechanism for the amplification.

219 Here we present a joint hydrodynamic and radiative model showing that during the first seconds of

220 However, owing to such radiative nature of the traditional wireless communicati

221 s, competing with vibrational relaxation and radiative or nonradiative processes occurring in upper e

222 e field due to an abundance of competing non-radiative pathways, including phenomena such as aggregat

223 An increasing trend in fire radiative power (FRP) were found for Cambodia (p = 0.005

224 ize, ignition date, time since last fire and radiative power.

225 oop) results from carriers shifting from the radiative process to the non-radiative processes.

226 ISC) rates in combination with effective non-radiative processes in those systems.

227 ifting from the radiative process to the non-radiative processes.

228 ), BC could affect the lifetime, albedo, and radiative properties of clouds containing both supercool

229 ry to gain a better understanding on how the radiative properties of soot are affected by coating wit

230 many efforts have been made to evaluate the radiative properties of soot in flames.

231 are one of the leading contributors to cloud radiative properties relevant to climate.

232 erature regulation; chemical, mechanical, or radiative protection; or energy storage.

233 ommunication regime by achieving single-side radiative quality factors as high as 1.6 x 10(5).

234 e emergence of an emissive transition with a radiative rate constant an order of magnitude higher tha

235 tion of a metallacage also decreases the non-radiative rate constant by inhibiting the intramolecular

236 d delayed fluorescence (TADF) emitter with a radiative rate constant k(r) of ca. 9 x 10(5) s(-1), exc

237 he addition of platinum, which increases the radiative rate constant via the heavy atom effect.

238 es were determined from correlations between radiative rate constants and average emission frequencie

239 The radiative rate constants for the Cu(I) complexes ( k(r)

240 ve, respectively) due mainly to decreases in radiative rate constants.

241 t with indirect Auger) and saturation of the radiative rate.

242 orescence behavior of the nanorings: the low radiative rates that are characteristic of a circular de

243 Radiative recombination ( k(rad)) is calculated through

244 ies is caused by a combination of strong non-radiative recombination (with temperature dependence con

245 icient charge transport, tend also to reduce radiative recombination and lead to solid-state quenchin

246 the carrier transport and behave as the non-radiative recombination centers.

247 le of dislocations which normally act as non-radiative recombination centers.

248 , but not the c-plane case, which act as non-radiative recombination centres.

249 confinement approaches substantially enhance radiative recombination in MHPs, but an increased surfac

250 lm and thus significantly suppresses the non-radiative recombination in the derived PVSC by passivati

251 improve charge generation at the cost of non-radiative recombination loss.

252 s due to poor interfaces and also due to non-radiative recombination losses arising from inferior per

253 ith near-infrared absorption lead to low non-radiative recombination losses in the resulting organic

254 system is found to exhibit radiative and non-radiative recombination losses that are among the lower

255 t formation, which otherwise would cause non-radiative recombination losses).

256 rs due to a combination of resistive and non-radiative recombination losses.

257 al-based light-emitting diodes relies on the radiative recombination of electrically generated excito

258 gration-immune surface in addition to a fast radiative recombination owing to its spatially and poten

259 ein, we explore cross-relaxation (CR), a non-radiative recombination pathway typically perceived as d

260 rge perovskite grain sizes, which lowers the radiative recombination probability and results in grain

261 ectrons and holes, often used to explain the radiative recombination process in [Formula: see text]-p

262 and-to-band recombination is the most likely radiative recombination process.

263 tion is further increased by suppressing the radiative recombination rate with the introduction of an

264 oblem; combining a tuneable energy gap, fast radiative recombination rates and luminescence quantum e

265 ring the effective carrier lifetime, the non-radiative recombination velocity due to edge defects is

266 ency of 14.0% and a great suppression of non-radiative recombination within the inorganic perovskite,

267 er charge transfer state energy and less non-radiative recombination, resulting in larger open-circui

268 imiting the specific detectivity (D*) is non-radiative recombination, which is also known to be the m

269 suppressed hot carrier cooling and enhanced radiative recombination.

270 charge carriers inside grains for efficient radiative recombination.

271 ace, leading to significantly suppressed non-radiative recombination.

272 charge separation and achieve suppressed non-radiative recombination.

273 n annihilation, with typical reduction in PL radiative relaxation times from 270 ps to 190 ps upon in

274 iconductors that can couple to light through radiative relaxation.

275 prevent excessive Arctic warming against the radiative response of 0.11 W m(-2) K(-1) as measured fro

276 radiative imbalance, the satellite-measured radiative response will be a crucial indicator of future

277 Considerable inter-model spreads in the radiative responses suggest that future Arctic warming m

278 observed and modeled top-of-atmosphere (TOA) radiative responses to surface air-temperature changes o

279 bed: (i) at an ablation front, (ii) behind a radiative shock, and (iii) due to material strength.

280 ipoles to harvest nonradiative triplets into radiative singlets in exciplex light-emitting diodes are

281 Our findings have implications for how the radiative, surface, and aerodynamic properties, and the

282 Devices fabricated from films formed via radiative thermal annealing have equivalent efficiencies

283 Here we present the application of radiative thermal annealing, an easily scalable processi

284 dielectric offers a promising way to reduce radiative thermal losses at high temperatures.

285 c cells must utilize the broad spectrum of a radiative thermal source.

286 ce gases and the relatively long atmospheric radiative time constant.

287 et this, we propose a distance-dependent non-radiative transfer model of excitation electrons and sup

288 Using a combination of mapping, and radiative transfer modelling utilising in situ measureme

289 we performed coupled chemical transport and radiative transfer simulations to estimate the aerosol-i

290 flectance for minimizing thermal losses from radiative transfer.

291 The few current radiative-transfer and chemical-transport models that in

292 c-physics phenomena-firstly, an interspecies radiative transition; and, secondly, the breaking down o

293 superdense plasma mixtures, both interatomic radiative transitions and dipole-forbidden transitions c

294 eaking down of the dipole-selection rule for radiative transitions in isolated atoms.

295 ensity borrowing effect commonly invoked for radiative transitions, enhance as well the nonradiative

296 orophyll f is best supported as a low-energy radiative trap, the physical location should be close to

297 and emissive excitons that enable small non-radiative voltage loss, and (ii) delocalization of elect

298 be explained by greenhouse-gas-induced (GHG) radiative warming alone.

299 delivery of electrical power by exciting non-radiative waves over metal surfaces to multiple loads.

300 A decade ago, non-radiative wireless power transmission re-emerged as a pr