ライフサイエンスコーパス: cool

1 y heavier nuclei as the material expands and cools.

2 eclined through the Eocene as global climate cooled.

3 between the delta(13)C excursion and global cooling.

4 chemical vapor deposition process with rapid cooling.

5 d the colorless thiolate adduct favored upon cooling.

6 entional electron ionization) by collisional cooling.

7 ature T(c) before writing, followed by rapid cooling.

8 o no more than a 12% increase in heating and cooling.

9 hich opens stomatal pores to facilitate leaf cooling.

10 HI intensities due to high rural evaporative cooling.

11 mperatures and modeled using Newton's law of cooling.

12 arge enough to support sustained collisional cooling.

13 rmula: see text] MHz when using only Doppler cooling.

14 cts which evolve due to thermal stress under cooling.

15 anthanide ions, and their influence on laser cooling.

16 evolved in response to late Neogene northern cooling.

17 , 20 newborn piglets were randomized to: (i) Cooling 1-13 h (HT; n = 6); (ii) HT+ 2.5% ethanol vehicl

18 on an average by ~60 and 90% when washed in cool (20 degrees C) and warm (50 degrees C) water, respe

19 n electronic structure appropriate for laser cooling(6), thus paving the way for its use in high-prec

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

21 owth is slow and pathogen pressure from this cool-adapted fungus is high.

22 ondensation; and 2) cold surfaces will still cool adjacent air via convection, limiting overall radia

23 Winter Eurasian cooling after the mid-1990s has been verified by numerou

24 lex structures unveil the molecular basis of cooling agonist sensing by TRPM8 and the allosteric role

25 uncovered unforeseen binding sites for both cooling agonists and membrane lipid phosphatidylinositol

26 Furthermore, sectional heating and cooling allow for the cage to traverse multiple phase bo

27 nsory neurons (MSNs) are activated by slight cooling, although sugar neurons are insensitive to the s

28 ct to the optical cavity allowed us to laser-cool an optically trapped nanoparticle into its quantum

29 We found that hosts from cool and warm climates experienced increased disease ris

30 nd dust into Earth's upper atmosphere, which cooled and darkened the planet-a scenario known as an im

31 re receivers can outperform state-of-the-art cooled and room-temperature THz receivers based on low-n

32 different conformer distributions under jet-cooled and thermal conditions.

33 on in ice motion coincident with atmospheric cooling and a ~15% reduction in mean surface melt produc

34 dded to the sample, require cryogenic sample cooling and are not selective for the interface between

35 ling materials, which allow energy-efficient cooling and are paving the way toward technologies that

36 nge by generating better heat pumps for both cooling and heating.

37 Both cooling and image acquisition times were optimized and t

38 acclimation-induced reduction in evaporative cooling and resultant increase in sensible heat flux.

39 but this could be restored to ~95% by simply cooling and rewarming the device.

40 Dialysate cooling and sodium modelling may prevent haemodynamic in

41 nd water-binding capacity all along heating, cooling and storage processes.

42 ales is a major strength of the technique of cooling and trapping atomic gases, in which low momentum

43 ical models, to quantify the contribution of cooling and water supply to the yield benefits due to ir

44 uces surface winds and decreases evaporative cooling and wind-driven upper ocean mixing.

45 Here we find that submarine iceberg melting cools and freshens the fjord by up to ~5 degrees C and 0

46 rmined from total time receiving cooling (TT(cool) ) and cumulative button presses.

47 om about 1.35 Ma, as the Northern Hemisphere cooled, and permanent after about 0.4 Ma.

48 ering the overall requirements for power and cooling, and reducing acoustic noise.

49 124 +/- 5 seconds for patients treated with cooling anesthesia versus 395 +/- 40 seconds for SOC (P

50 ere recorded in 32% of patients treated with cooling anesthesia versus 44% of patients receiving SOC.

51 No dose-related toxicity was found with cooling anesthesia.

52 -based anesthesia and the other eye received cooling-anesthesia at 1 of 5 different temperatures and

53 todetachment spectroscopies of cryogenically-cooled anions.

54 generator device for waste heat recovery and cooling applications.

55 ing and refrigeration as well as electronics cooling applications.

56 over the last 15 million years (Myr) during cooling associated with global expansion of temperate ha

57 face properties because of the high rates of cooling associated with it.

58 esearch has focused mainly on the effects of cooling at temperatures between 28 degrees C and 35 degr

59 arm ionized(5,6) (10(4) to 10(5) kelvin) and cool atomic(7,8) (10(3) to 10(4) kelvin) gas.

60 In previous work with laser-cooled atoms and ions, and solid-state defects, spin rea

61 which included heating the sample, and then cooling back.

62 f desired, the results can then be erased by cooling below room temperature and the material repeated

63 nd viscous boundary layers at the heated and cooled boundaries of the system.

64 ral behavior, where the supercells appear on cooling but revert to the original subcell below 100 K,

65 on-based cooling schemes such as evaporative cooling, but thermalization and collisional cooling have

66 ersity dropped markedly during Younger Dryas cooling, but while plant diversity recovered in the earl

67 Sediments were then cooled by 10-40 degrees C, mimicking the cooling in subs

68 h global temperatures are stabilized or over-cooled by blocking solar radiation.

69 le subjects (27 +/- 11 years) underwent core cooling by 1.0 degrees C and core heating by 1.5 degrees

70 multi-stressor environments is unknown Core cooling by 1.0 degrees C reduced cerebral blood flow (CB

71 per we demonstrate experimentally how cavity cooling can be implemented to improve the localisation o

72 h of making on-skin electronics with passive-cooling capabilities, which can reduce energy consumptio

73 o fast localization to a lower energy state (cool carriers) with electrons occupying Cu center and ho

74 The cool carriers, which have super long lifetime (>17 ns),

75 When the buffer concentration was 100 mM, cooling caused a pH decrease of 3.1 and 2.7 units (for B

76 ils to acknowledge that pan-tropical surface cooling caused by large volcanic eruptions may mask El N

77 ophic ozone depletion, extending the surface cooling caused by the eruption.

78 to climatic variability, with Little Ice Age cooling causing an abrupt ecosystem shift and an increas

79 d a contact imaging portable device based on cooled CCD, and measured the light signal resulting from

80 Sunpower cryo-cooler (typically employed for cooling cellular network antennas) to achieve up to ~87%

81 Our system utilizes water cooled chromium doped zinc selenide (Cr(2+):ZnSe) as the

82 ally providing information for winemaking in cool climate regions.

83 avelengths of light required for ionization, cooling, coherent operations and quantum state preparati

84 n inert gas stream before they condense in a cooled collector.

85 tojoule precision, depends on heating versus cooling cycles.

86 ully reversible through multiple heating and cooling cycles.

87 MS cooling decreased theta frequency oscillations of place

88 Cooling demand is projected to increase under climate ch

89 The cooling device output temperature has the potential to b

90 Cooling device output temperature is a potential and eas

91 A significantly higher cooling device output temperature was seen in infants wi

92 ndidates for next-generation all-solid-state cooling devices.

93 Passive radiative cooling, dissipating an object's heat through an atmosph

94 T) was performed, followed by a 5-min active cool down.

95 ture and grows by an order of magnitude upon cooling down to 4 K.

96 Cooling due to aerosols (-100 to -300 mW m(-2)) is conce

97 cover large swaths of subtropical oceans and cool Earth by reflecting incident sunlight, their loss w

98 ide emissions produced sulfate aerosols that cooled Earth's climate with a range of impacts on societ

99 uences such as stress, training both hot and cool EF skills, and adding a reflective, metacognitive c

100 rctic glaciation, highlighting the important cooling effect exerted by ice albedo under high levels o

101 fires burning in the current era (2016) the cooling effect from long-term postfire albedo will be re

102 The irrigation cooling effect is also observed on air temperature (-0.3

103 emissions and hence reduce the net radiative cooling effect of estuarine mangrove forests.

104 e depth of the nest, but may not, due to the cooling effect of nesting deeper.

105 er than grasslands, indicating a substantial cooling effect of reforestation.

106 g CO(2) -C m(-2) year(-1) , indicating a net cooling effect on climate over decadal to centurial time

107 ng is thus relatively small and has a slight cooling effect on the surface climate.

108 In decades to follow however, this cooling effect would gradually vanish as the Indian Ocea

109 e (CH(4)) emissions can offset their climate cooling effect.

110 air via convection, limiting overall radiant-cooling effectiveness.

111 These cooling effects are greatest later in twenty-first centu

112 aring of nearby coronary arteries because of cooling endoluminal flow.

113 The heating and cooling energy consumption of buildings accounts for abo

114 he United States, can save 19.2% heating and cooling energy, which is 1.7 times higher than cooling-o

115 slowly compress the sample, while keeping it cool enough to stay below the melt curve.

116 he survival and development of ant larvae in cool environments.

117 ese data therefore suggest that regionalised cool episodes punctuated the background warmth of the ea

118 warming potential of current refrigerants in cooling equipment based on the vapor-compression cycle h

119 Upon cooling, ER-derived LICVs phase-partition into microscop

120 Eocene-Oligocene transition (EOT): the EOT-1 cooling event at ~34.1-33.9 Ma and the Oi-1 glaciation e

121 assing through an inductively coupled plasma cool from ~5000 to 1000 K within milliseconds and form n

122 degrees C) and toluene (4-fold increase upon cooling from 100 to 50 degrees C).

123 n water-in-milk fat emulsions during in situ cooling from 40 degrees C to 5 degrees C.

124 s in tetrahydrofuran (200-fold increase upon cooling from 50 to 0 degrees C) and toluene (4-fold incr

125 nstrain the magnitude and pattern of glacial cooling from palaeothermometers(1,2), but the uneven dis

126 rameters, in particular pressure of the N(2) cooling gas in the ion source, delay between the two las

127 nd S((1)D) atoms formed by photolysis of jet-cooled H(2)S molecules at many wavelengths in the range

128 Our results suggest long-term cooling had a disproportionate effect on non-tropical di

129 cooling, but thermalization and collisional cooling have not yet been realized for ultracold molecul

130 These seasonal patterns of warming and cooling have significant implications for heat mitigatio

131 nal on-skin electronics, which can passively cool human bodies without needing any energy consumption

132 For 2100, a cooling impact from the Master Plan leading to market sa

133 As a result, we observe ~3 degrees C cooling improvement of this selective thermal emitter as

134 We also find that the cooling in autumn is stronger than that in winter.

135 ains approximately 54% and 18% of the autumn cooling in Eurasia, respectively.

136 1) The low temperature required for radiant cooling in humid environments will form condensation; an

137 ngs highlight the powerful influence of core cooling in reducing CDO(2) .

138 saturated in plagioclase after stalling and cooling in shallow-level chambers.

139 hen cooled by 10-40 degrees C, mimicking the cooling in subsurface oil reservoirs subjected to seawat

140 e effects of reforestation on warming and/or cooling in temperate zones are less certain.

141 ement of heated meteoric waters during their cooling in the crust.

142 thane deposits may not result from adiabatic cooling in upwardly moving air like on our planet, but f

143 tmospheric transparency window for radiative cooling, in cost-effective infrared sensing devices, and

144 We use this laser for laser-cooling, in-situ isotope purifcation, and probing barium

145 is expressed and required in bitter GRNs for cool-induced suppression of sugar appeal.

146 ypothermia synchronises the circadian clock: cooling induces nuclear accumulation of transcripts that

147 crystals, form I, melt and crystallize upon cooling into a polymorph, form II, which is much faster

148 mperature of the probed medium, we introduce cooled IR optoacoustic spectroscopy (CIROAS) to mute wat

149 Electrocaloric (EC) cooling is an emerging technology that has broad potenti

150 Because the cooling is not uniform at different spatial and temporal

151 be performed at either 4 degrees C (in situ cooling [ISC]) or 33-36 degrees C (normothermic regional

152 rcularly polarized light on 1T-TiSe(2) while cooling it below the critical temperature leads to the p

153 However, the feasibility of laser-cooling larger, nonlinear polyatomic molecules has remai

154 The unique feature of radiative cooling lies in the high emissivity in the atmospheric t

155 ly characterizing the climate sensitivity of cooling load, and that near-surface humidity plays an eq

156 olatiles exsolved through crystallization of cooling magma stalled beneath the crust.

157 provide significant improvements at reduced cooling mass flow rates.

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

159 advancement of daytime subambient radiative cooling materials, which allow energy-efficient cooling

160 arge-scale applications of all-day radiative cooling materials.

161 ng evolution mosquito heat seeking relied on cooling-mediated repulsion.

162 ity laser light source, a thermoelectrically cooled mercury cadmium telluride balanced detection modu

163 The simulated cooling mode is determined by changes in the seasonal cy

164 e dominates in the mid-Holocene, whereas the cooling mode takes over in the late Holocene.

165 associated with internal waves that advected cool, nutrient-rich water across the reef.

166 With the gradual cooling occurrence in winter, more accumulation of antho

167 a few meters depth, or for the effect of the cool ocean surface skin.

168 with the counterfactual, leading to a global cooling of - 0.1 milli degrees C in 2030.

169 estimated that fires generate an annual mean cooling of -1.77 +/- 1.35 W/m(2) from albedo under histo

170 vices by using the self-adaptive evaporative cooling of a lithium- and bromine-enriched polyacrylamid

171 t is likely that the TBJ eruption produced a cooling of around 0.5 degrees C for a few years after th

172 lecules, thereby opening a path to efficient cooling of chiral molecules and, eventually, optical twe

173 inistration for hypoglycemia; techniques for cooling of exertional hyperthermia and heatstroke; recog

174 including sensitive metrology, ground state cooling of mechanical motion and slowing of light.

175 Here we show cooling of NaLi molecules to micro- and nanokelvin tempe

176 proper ro-vibronic transitions enables laser cooling of nonlinear molecules, thereby opening a path t

177 bility of using stretched spin states in the cooling of other molecules.

178 e of the SEOP process) in 4 min, and perform cooling of the cell to the temperature at which the hype

179 Cooling of the MS reduced both theta frequency and power

180 In the present study, the effect of rapid cooling on the silicon particle size, distribution, and

181 oling energy, which is 1.7 times higher than cooling-only and 2.2 times higher than heating-only appr

182 tes through enhanced daytime transpirational cooling or by permitting maximal gas exchange when condi

183 e subpolar North Atlantic experienced slight cooling or suppressed warming, relative to the backgroun

184 g light irradiation, pH adjustment, heating, cooling, or chemical addition.

185 Additional daytime cooling over forests is driven by local feedbacks to inc

186 Cooling patients to sub-physiological temperatures is an

187 differential privacy and private evaporative cooling (pEC).

188 With its excellent cooling performance and a scalable process, this hierarc

189 Therefore, for achieving high cooling performance, the design and fabrication of selec

190 on and therefore excellent all-day radiative cooling performance.

191 ce drastically approaches to zero during the cooling period.

192 ion of cellobiose attenuated the pH shift on cooling (pH decrease of ~1.0 unit), and no evidence of e

193 transitions that have made solid-state laser-cooling possible.

194 ance, which can achieve up to 71.6 W/m(2) of cooling power density and up to 643.4 W/m(2) of heating

195 duction and convection are limited and a net cooling power greater than 78 W/m(2) at a cost less than

196 at temperatures below 100 millikelvin, where cooling power is extremely limited, and this severely af

197 ty of 744 W m(-2) (850 W m(-2) ), yielding a cooling power of 84.2 W m(-2) .

198 iting increased sensitivity of cryogenically cooled probes.

199 After a cooling procedure to activate BAT, volunteers underwent

200 terize their thermal behavior on heating and cooling processes, using TG/DTG/DTA, TG-MS, DSC, hot sta

201 Fast cooling rate and ultrasonic treatment favored the oil-ge

202 fast quenching back to room temperature at a cooling rate of 10(5) K/s to inhibit sintering.

203 The cooling rate of excited carriers is monitored at doping

204 s C and 1100 degrees C, under the super-high cooling rate of ~ 10(6) degrees C/s, in cooperation with

205 Faster cooling rate resulted in an earlier onset of crystalliza

206 t are typical of glass formation at a higher cooling rate) lowers its yield stress, which might enabl

207 e indicates crystallization at an increasing cooling rate, such as would occur during magma ascent th

208 lattice contraction which is invariant with cooling rate.

209 h is greater for the beta-Ti phase at slower cooling rates and a change in the relative phase fractio

210 s microstructure, for example, by using high cooling rates and cyclic re-heating(4-10).

211 The measured cooling rates are seen to correlate to the level of resi

212 The higher cooling rates associated with laser powder bed fusion re

213 verse relationship with laser power and bulk cooling rates.

214 eta-Ti phase with increased strain at slower cooling rates.

215 owed the expected reversible heated melt and cooling recrystallization in only a few examples.

216 Cryogenic (cryo-) cooling reduces the global radiation damage rate and, th

217 leaves increase water loss to evaporatively cool regardless of carbon uptake; or heat failure, where

218 s faster and slower by 6-9% with heating and cooling, respectively (both P < 0.01), but central (brai

219 structing neurons downstream of heating- and cooling-responsive VP PNs.

220 vidence of the existence of a suitable laser-cooling scheme for these molecules and represent a key s

221 d atoms can be created using collision-based cooling schemes such as evaporative cooling, but thermal

222 Subambient daytime radiative cooling (SDRC) provides a promising electricity- and cry

223 easonal drought are most apparent during the cool season; when soil water availability is projected t

224 nadine inputs were greater during warm- than cool-season conditions but also attenuated faster.

225 sis that elevations in skin wetness augments cool-seeking behaviour during passive heat stress.

226 kin wetness enhances the desire to engage in cool-seeking behaviour during passive heat stress.

227 sed skin wetness amplifies the engagement in cool-seeking behaviour during passive heat stress.

228 dence indicates that skin wetness stimulates cool-seeking behaviour to a greater extent than increase

229 Cool-seeking behaviour was determined from total time re

230 mal discomfort, the precursor to engaging in cool-seeking behaviour.

231 ts in SSA, including cool subhumid Ethiopia, cool semi-arid Rwanda, hot subhumid Ghana and hot semi-a

232 ne of which depends on a rhodopsin (Rh6) for cool sensation.

233 ulations and the data collected in a radiant cooling setup together demonstrate the influence of free

234 Concurrently, Earth's climate has cooled since the Miocene Climatic Optimum, leading to gr

235 ater (up to 30 days) in 1983 and 1996 due to cool spring temperatures.

236 ar temperature distribution in a homogeneous cooling state.

237 /ha) for five environments in SSA, including cool subhumid Ethiopia, cool semi-arid Rwanda, hot subhu

238 vel, Ir21a is essential for the detection of cooling, suggesting that during evolution mosquito heat

239 overed this error in an experimental radiant cooling system with high separation of air to radiant te

240 Traditional cooling systems consume tremendous amounts of energy and

241 patients amounted to 614 825 kWh, dedicated cooling systems to 492 624 kWh, representing 44.5% of th

242 ds Three CT scanners, four MRI scanners, and cooling systems were equipped with kilowatt-hour energy

243 he melting, resolidification, and subsequent cooling take place at much higher rates and with much hi

244 Our cooling technique, in combination with optical trap mani

245 would be achievable only with cryogenically cooled technologies and could represent a significant st

246 of widespread commercial adoption of radiant-cooling technologies is due to two widely held views: 1)

247 bility of sugary food is reduced by slightly cool temperatures through different sets of thermally ac

248 ncreased disease risk at abnormally warm and cool temperatures, respectively, as predicted by the the

249 water demand but also creates an evaporative cooling that mitigates crop heat stress.

250 te a heterogeneous distribution of radiative cooling that selectively reduces the temperature of stru

251 loited to provide a mechanism to efficiently cool the ion.

252 large volcanic eruptions: Volcanic eruptions cool the surface, thus masking the relative El Nino warm

253 We laser-cooled the symmetric top molecule calcium monomethoxide

254 ixed layer in the presence of a NIW, thereby cooling the mixed layer at a rate of 244 W m(-2) over th

255 Cooling the sediments induced sulfate reduction, coincid

256 The pH shift was measured upon cooling the solutions from 20 to -25 degrees C.

257 On tidally-locked planets, dust cools the day-side and warms the night-side, significant

258 Once cooled, the actuated shape can be locked.

259 in THF solution, where aggregates form upon cooling, the TADF mechanism takes over around room tempe

260 s that multi-plate tectonics was preceded by cooling through a single-plate lithosphere, but models f

261 Falling atmospheric CO(2) levels led to cooling through the Eocene and the expansion of Antarcti

262 sthesia at 1 of 5 different temperatures and cooling times.

263 lation properties of CsPbBr(3) crystals when cooled to cryogenic temperatures.

264 Stainless steel coupons were cooled to generate a thermal gradient in relation to bio

265 In vivo pancreatic cooling to 25 degrees C reduced the increase in circulat

266 the emission pattern of water after a sudden cooling to 4 K, signifying the conversion of ortho-water

267 us hypothermia, and thus require less active cooling to attain TH.

268 rt for a dynamical response linking volcanic cooling to El Nino remains ambiguous, Robock raises some

269 es with an unfavourable outcome require less cooling to maintain a core temperature between 33 and 34

270 rey matter injury on MRI require less active cooling to maintain target temperature during TH.

271 oldness of the outer space through radiative cooling to produce electricity at night using a commerci

272 -phase is formed from the cubic phase during cooling to room temperature and subsequently deforms in

273 competition with vibrational relaxation and cooling to the relaxed (3) MLCT state.

274 he non-negligible contribution of irrigation cooling to the yield benefits of irrigation, and such an

275 , ice sheets and mineral dust aerosols, this cooling translates to an equilibrium climate sensitivity

276 n Eurasian temperature reveals a significant cooling trend (P < 0.05).

277 ds played a significant role in driving this cooling trend through increasing global weatherability.

278 our was determined from total time receiving cooling (TT(cool) ) and cumulative button presses.

279 elvin in one dimension and state-selectively cooling two nuclear spin isomers.

280 as an exchange bias when the sample is field-cooled under an out-of-plane magnetic field, and an exch

281 veloped photonic materials permit subambient cooling under direct sunshine, and their applications ar

282 ferropericlase followed by decompression and cooling under oxidized conditions, leading to the format

283 mitter at night, and 5 degrees C sub-ambient cooling under sunlight.

284 Short-term (aerosol cooling) volcanism still allows equatorial habitability.

285 his behavior changes close to the heated and cooled walls for high values of Pr (e.g. [Formula: see t

286 o mitigate the 1(st)-order economic risks of cooling water shortage during droughts.

287 investigate the electricity price impacts of cooling water shortages on Britain's power supplies usin

288 The risks of cooling water shortages to thermo-electric power plants

289 regional climate, hydrological droughts and cooling water shortages, coupled with an economic model

290 cantly greater compared with prior years yet cool-water affinity species did not show commensurate de

291 By using cavity cooling we obtain an enhanced ion-cavity coupling of [Fo

292 a) to assess variations in Eurasian seasonal cooling, we examine the causes of these changes.

293 ae provides support for climate models for a cool, wet climate on early Venus and could be an attract

294 ng a gradient of increasing aridity from the cool-wet forest to the hot-dry Sahel, from south to nort

295 idinfrared emissivity can facilitate surface cooling, whereas a low midinfrared emissivity can minimi

296 rigation yield increase is due to irrigation cooling, while the rest (84%) is due to water supply and

297 of the three metal halide species, warm- to cool-white emissions could be generated by controlling t

298 d cover by modulating the longwave radiative cooling within the atmosphere.

299 corded in Antarctic ice cores imply that the cooling would have been more pronounced in the Southern

300 nal SDRC, and also leads to enhanced daytime cooling yet suppressed nighttime overcooling.