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1 entional electron ionization) by collisional cooling.
2 ature T(c) before writing, followed by rapid cooling.
3 o no more than a 12% increase in heating and cooling.
4 HI intensities due to high rural evaporative cooling.
5 hich opens stomatal pores to facilitate leaf cooling.
6 mperatures and modeled using Newton's law of cooling.
7 arge enough to support sustained collisional cooling.
8 rmula: see text] MHz when using only Doppler cooling.
9  radiation since the Eocene/Oligocene global cooling.
10 sensitivity by nanofabrication and cryogenic cooling.
11 ity of sucrose is strongly reduced by modest cooling.
12  the late Neogene, a time of amplified polar cooling.
13 , thereby eliminating the need for cryogenic cooling.
14 T by blocking leaf hyponasty and evaporative cooling.
15 ing their vegetative body plan to facilitate cooling.
16 cts which evolve due to thermal stress under cooling.
17 anthanide ions, and their influence on laser cooling.
18 evolved in response to late Neogene northern cooling.
19  between the delta(13)C excursion and global cooling.
20 chemical vapor deposition process with rapid cooling.
21 d the colorless thiolate adduct favored upon cooling.
22 , 20 newborn piglets were randomized to: (i) Cooling 1-13 h (HT; n = 6); (ii) HT+ 2.5% ethanol vehicl
23 n electronic structure appropriate for laser cooling(6), thus paving the way for its use in high-prec
24 d to achieve the effect of daytime radiative cooling(6-8,10-15).
25                              Winter Eurasian cooling after the mid-1990s has been verified by numerou
26 lex structures unveil the molecular basis of cooling agonist sensing by TRPM8 and the allosteric role
27  uncovered unforeseen binding sites for both cooling agonists and membrane lipid phosphatidylinositol
28           Furthermore, sectional heating and cooling allow for the cage to traverse multiple phase bo
29 nsory neurons (MSNs) are activated by slight cooling, although sugar neurons are insensitive to the s
30 on in ice motion coincident with atmospheric cooling and a ~15% reduction in mean surface melt produc
31 dded to the sample, require cryogenic sample cooling and are not selective for the interface between
32 ling materials, which allow energy-efficient cooling and are paving the way toward technologies that
33 m selective pressures during Cenozoic global cooling and eventual ice conditions beginning in the Ple
34                                         Core cooling and heating protocols were repeated after 16 +/-
35 nge by generating better heat pumps for both cooling and heating.
36                                         Both cooling and image acquisition times were optimized and t
37  spring-index dependencies of twist-enhanced cooling and its origin in a phase transformation for pol
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                        The creation process (cooling and shear rate) can tune its properties.
41                                    Dialysate cooling and sodium modelling may prevent haemodynamic in
42 nd water-binding capacity all along heating, cooling and storage processes.
43 ales is a major strength of the technique of cooling and trapping atomic gases, in which low momentum
44 ical models, to quantify the contribution of cooling and water supply to the yield benefits due to ir
45 uces surface winds and decreases evaporative cooling and wind-driven upper ocean mixing.
46 ering the overall requirements for power and cooling, and reducing acoustic noise.
47  +/- 0.6 in patients receiving -10 degrees C cooling anesthesia (P = 0.8).
48     A total of 44 eyes were treated, 22 with cooling anesthesia and 22 with SOC.
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  IVT and 4 hours after IVT in eyes receiving cooling anesthesia were compared with eyes receiving SOC
52      No dose-related toxicity was found with cooling anesthesia.
53 -based anesthesia and the other eye received cooling-anesthesia at 1 of 5 different temperatures and
54 ing and refrigeration as well as electronics cooling applications.
55 generator device for waste heat recovery and 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 impaired rosette evapotranspiration and leaf cooling at high temperatures.
59 w a surprising region of considerable future cooling at midlatitudes, referred to as the North Atlant
60 ity polyethylene membrane to provide radiant cooling at temperatures below the dew point.
61 esearch has focused mainly on the effects of cooling at temperatures between 28 degrees C and 35 degr
62  which included heating the sample, and then cooling back.
63                            Compared with pre-cooling baseline, rewarming was associated with signific
64 f desired, the results can then be erased by cooling below room temperature and the material repeated
65 ral behavior, where the supercells appear on cooling but revert to the original subcell below 100 K,
66 on-based cooling schemes such as evaporative cooling, but thermalization and collisional cooling have
67 ersity dropped markedly during Younger Dryas cooling, but while plant diversity recovered in the earl
68 le subjects (27 +/- 11 years) underwent core cooling by 1.0 degrees C and core heating by 1.5 degrees
69  multi-stressor environments is unknown Core cooling by 1.0 degrees C reduced cerebral blood flow (CB
70 per we demonstrate experimentally how cavity cooling can be implemented to improve the localisation o
71 h of making on-skin electronics with passive-cooling capabilities, which can reduce energy consumptio
72    When the buffer concentration was 100 mM, cooling caused a pH decrease of 3.1 and 2.7 units (for B
73 ils to acknowledge that pan-tropical surface cooling caused by large volcanic eruptions may mask El N
74 ophic ozone depletion, extending the surface cooling caused by the eruption.
75 to climatic variability, with Little Ice Age cooling causing an abrupt ecosystem shift and an increas
76 Sunpower cryo-cooler (typically employed for cooling cellular network antennas) to achieve up to ~87%
77 avelengths of light required for ionization, cooling, coherent operations and quantum state preparati
78 he most stable formulation after the heating-cooling cycles, whereas nanomax was the most stable unde
79 tojoule precision, depends on heating versus cooling cycles.
80 ully reversible through multiple heating and cooling cycles.
81                                           MS cooling decreased theta frequency oscillations of place
82 ased on air temperature alone underestimates cooling demand by as much as 10-15% under both present a
83                                              Cooling demand is projected to increase under climate ch
84 is more than four times higher than other EC cooling demonstrations, and the temperature lift is amon
85 he two materials is investigated using field-cooling-dependent magnetometry and polarized neutron ref
86                                          The cooling device output temperature has the potential to b
87                                              Cooling device output temperature is a potential and eas
88                       A significantly higher cooling device output temperature was seen in infants wi
89 ndidates for next-generation all-solid-state cooling devices.
90                                              Cooling did not affect cord physiology (ISP, SCPP), but
91                            Passive radiative cooling, dissipating an object's heat through an atmosph
92 ture and grows by an order of magnitude upon cooling down to 4 K.
93 cidic metallurgical streams, avoiding costly cooling down.
94 nation of abiotic and biotic factors, with a cooling-driven extinction (negative correlation between
95                                              Cooling due to aerosols (-100 to -300 mW m(-2)) is conce
96 elengths, resulting in continuous subambient cooling during both day and night.
97  One temperature reconstruction shows global cooling during the late Holocene.
98 avourable Purcell effect that can modify the cooling dynamics substantially.
99 bedo warming (+2.3 degrees C) and emissivity cooling effect (-0.8 degrees C) associated with surface
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              We further show that the forest cooling effect is most pronounced when land surface temp
104 sible heat fluxes of forests have an average cooling effect of -2.5 degrees C, which offsets the net
105 emissions and hence reduce the net radiative cooling effect of estuarine mangrove forests.
106 e depth of the nest, but may not, due to the cooling effect of nesting deeper.
107 er than grasslands, indicating a substantial cooling effect of reforestation.
108 g CO(2) -C m(-2) year(-1) , indicating a net cooling effect on climate over decadal to centurial time
109 ng is thus relatively small and has a slight cooling effect on the surface climate.
110           In decades to follow however, this cooling effect would gradually vanish as the Indian Ocea
111 e (CH(4)) emissions can offset their climate cooling effect.
112 air via convection, limiting overall radiant-cooling effectiveness.
113                                        These cooling effects are greatest later in twenty-first centu
114 ation, thereby delivering around 6 degrees C cooling effects under a solar intensity of 840 W.m(-2) O
115 aring of nearby coronary arteries because of cooling endoluminal flow.
116                              The heating and cooling energy consumption of buildings accounts for abo
117 he United States, can save 19.2% heating and cooling energy, which is 1.7 times higher than cooling-o
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 promising starting point to perform motional cooling for exploration of quantum effects at mesoscopic
122  system, and study the breakdown of feedback cooling for very large time delays.
123  over 2 h at 1 h after hypoxia-ischemia with cooling from 1-13 h was safe, achieved therapeutic level
124 degrees C) and toluene (4-fold increase upon cooling from 100 to 50 degrees C).
125                 Here, we probe the effect of cooling from 20 degrees C to 0 degrees C on the structur
126 n water-in-milk fat emulsions during in situ cooling from 40 degrees C to 5 degrees C.
127 s in tetrahydrofuran (200-fold increase upon cooling from 50 to 0 degrees C) and toluene (4-fold incr
128 nstrain the magnitude and pattern of glacial cooling from palaeothermometers(1,2), but the uneven dis
129 n applied to the LC molecular director while cooling from the nematic phase produces a frustrated sme
130  multifunctional smart textiles with passive-cooling functionalities.
131 rameters, in particular pressure of the N(2) cooling gas in the ion source, delay between the two las
132 bations over geological time, such as global cooling, global warming, and changes in ocean chemistry.
133                Our results suggest long-term cooling had a disproportionate effect on non-tropical di
134  For atoms and small molecules, direct laser cooling has proven to be a powerful tool for quantum sci
135  cooling, but thermalization and collisional cooling have not yet been realized for ultracold molecul
136       These seasonal patterns of warming and cooling have significant implications for heat mitigatio
137 lium during the gHDX process for collisional cooling helps mitigate such variations in exchange kinet
138                                  For 2100, a cooling impact from the Master Plan leading to market sa
139         As a result, we observe ~3 degrees C cooling improvement of this selective thermal emitter as
140                        We also find that the cooling in autumn is stronger than that in winter.
141               We demonstrate that the autumn cooling in Eurasia is likely influenced by the Pacific D
142 ains approximately 54% and 18% of the autumn cooling in Eurasia, respectively.
143  1) The low temperature required for radiant cooling in humid environments will form condensation; an
144 ngs highlight the powerful influence of core cooling in reducing CDO(2) .
145  saturated in plagioclase after stalling and cooling in shallow-level chambers.
146 hen cooled by 10-40 degrees C, mimicking the cooling in subsurface oil reservoirs subjected to seawat
147 e effects of reforestation on warming and/or cooling in temperate zones are less certain.
148 ement of heated meteoric waters during their cooling in the crust.
149 thane deposits may not result from adiabatic cooling in upwardly moving air like on our planet, but f
150 tmospheric transparency window for radiative cooling, in cost-effective infrared sensing devices, and
151                  We use this laser for laser-cooling, in-situ isotope purifcation, and probing barium
152 ypothermia synchronises the circadian clock: cooling induces nuclear accumulation of transcripts that
153  crystals, form I, melt and crystallize upon cooling into a polymorph, form II, which is much faster
154                          Electrocaloric (EC) cooling is an emerging technology that has broad potenti
155                                  Because the cooling is not uniform at different spatial and temporal
156  be performed at either 4 degrees C (in situ cooling [ISC]) or 33-36 degrees C (normothermic regional
157  polymer coating is also expected to resolve cooling issues for old buildings with no air conditionin
158 rcularly polarized light on 1T-TiSe(2) while cooling it below the critical temperature leads to the p
159            However, the feasibility of laser-cooling larger, nonlinear polyatomic molecules has remai
160              The unique feature of radiative cooling lies in the high emissivity in the atmospheric t
161 ly characterizing the climate sensitivity of cooling load, and that near-surface humidity plays an eq
162 olatiles exsolved through crystallization of cooling magma stalled beneath the crust.
163 may more commonly be indicative of stagnant, cooling magma.
164  provide significant improvements at reduced cooling mass flow rates.
165               However, most of the radiative cooling materials reported possess broad-band absorption
166                    Daytime passive radiative cooling materials shed heat from the ground to the cold
167  advancement of daytime subambient radiative cooling materials, which allow energy-efficient cooling
168 arge-scale applications of all-day radiative cooling materials.
169 ng evolution mosquito heat seeking relied on cooling-mediated repulsion.
170 e show that both a global warming mode and a cooling mode emerge when performing a spatio-temporal an
171                                The simulated cooling mode is determined by changes in the seasonal cy
172 e dominates in the mid-Holocene, whereas the cooling mode takes over in the late Holocene.
173 d confirm that major Asian aridification and cooling occurred at Oi-1.
174                             With the gradual cooling occurrence in winter, more accumulation of antho
175 with the counterfactual, leading to a global cooling of - 0.1 milli degrees C in 2030.
176 estimated that fires generate an annual mean cooling of -1.77 +/- 1.35 W/m(2) from albedo under histo
177 uct provides a constraint on global mean LGM cooling of -6.1 degrees Celsius (95 per cent confidence
178 vices by using the self-adaptive evaporative cooling of a lithium- and bromine-enriched polyacrylamid
179                                        Laser cooling of a neutral plasma is a challenging task becaus
180 t is likely that the TBJ eruption produced a cooling of around 0.5 degrees C for a few years after th
181 lecules, thereby opening a path to efficient cooling of chiral molecules and, eventually, optical twe
182 sampling biases, effects such as the secular cooling of Earth's mantle and the biologically driven ox
183 inistration for hypoglycemia; techniques for cooling of exertional hyperthermia and heatstroke; recog
184 nce of the cavity can hamper efficient laser cooling of ions because of geometric constraints that th
185  including sensitive metrology, ground state cooling of mechanical motion and slowing of light.
186                                 Here we show cooling of NaLi molecules to micro- and nanokelvin tempe
187 proper ro-vibronic transitions enables laser cooling of nonlinear molecules, thereby opening a path t
188 bility of using stretched spin states in the cooling of other molecules.
189 e of the SEOP process) in 4 min, and perform cooling of the cell to the temperature at which the hype
190                                  Ultra-rapid cooling of the eye for anesthesia was well tolerated, wi
191                                              Cooling of the MS reduced both theta frequency and power
192 show that irrigation leads to a considerable cooling on daytime land surface temperature (-1.63 degre
193    In the present study, the effect of rapid cooling on the silicon particle size, distribution, and
194 oling energy, which is 1.7 times higher than cooling-only and 2.2 times higher than heating-only appr
195 tes through enhanced daytime transpirational cooling or by permitting maximal gas exchange when condi
196 e subpolar North Atlantic experienced slight cooling or suppressed warming, relative to the backgroun
197 g light irradiation, pH adjustment, heating, cooling, or chemical addition.
198                           Additional daytime cooling over forests is driven by local feedbacks to inc
199                                              Cooling patients to sub-physiological temperatures is an
200  constructed a demonstrative outdoor radiant-cooling pavilion in Singapore that used an infrared-tran
201 differential privacy and private evaporative cooling (pEC).
202                           With its excellent cooling performance and a scalable process, this hierarc
203                Therefore, for achieving high cooling performance, the design and fabrication of selec
204 on and therefore excellent all-day radiative cooling performance.
205 ce drastically approaches to zero during the cooling period.
206 ion of cellobiose attenuated the pH shift on cooling (pH decrease of ~1.0 unit), and no evidence of e
207 transitions that have made solid-state laser-cooling possible.
208 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
209 duction and convection are limited and a net cooling power greater than 78 W/m(2) at a cost less than
210 at temperatures below 100 millikelvin, where cooling power is extremely limited, and this severely af
211 ty of 744 W m(-2) (850 W m(-2) ), yielding a cooling power of 84.2 W m(-2) .
212 at this transition is consistent with Arctic cooling: Prior to 6 Ma, low-latitude continental carbon
213                                      After a cooling procedure to activate BAT, volunteers underwent
214 terize their thermal behavior on heating and cooling processes, using TG/DTG/DTA, TG-MS, DSC, hot sta
215 sponses to acute cold rather than to natural cooling profiles.
216                                         Fast cooling rate and ultrasonic treatment favored the oil-ge
217 fast quenching back to room temperature at a cooling rate of 10(5) K/s to inhibit sintering.
218                                          The cooling rate of excited carriers is monitored at doping
219 s C and 1100 degrees C, under the super-high cooling rate of ~ 10(6) degrees C/s, in cooperation with
220                                       Faster cooling rate resulted in an earlier onset of crystalliza
221 t are typical of glass formation at a higher cooling rate) lowers its yield stress, which might enabl
222 e indicates crystallization at an increasing cooling rate, such as would occur during magma ascent th
223  lattice contraction which is invariant with cooling rate.
224 h is greater for the beta-Ti phase at slower cooling rates and a change in the relative phase fractio
225 s microstructure, for example, by using high cooling rates and cyclic re-heating(4-10).
226                                 The measured cooling rates are seen to correlate to the level of resi
227                                   The higher cooling rates associated with laser powder bed fusion re
228 peed X-ray diffraction to extract subsurface cooling rates following resolidification from the melt a
229 verse relationship with laser power and bulk cooling rates.
230 eta-Ti phase with increased strain at slower cooling rates.
231 owed the expected reversible heated melt and cooling recrystallization in only a few examples.
232                            Cryogenic (cryo-) cooling reduces the global radiation damage rate and, th
233 number concentration and modifying radiative cooling relative to current estimates assuming a water s
234                                The degree of cooling required to achieve TH may therefore act as a bi
235 s faster and slower by 6-9% with heating and cooling, respectively (both P < 0.01), but central (brai
236 structing neurons downstream of heating- and cooling-responsive VP PNs.
237 vidence of the existence of a suitable laser-cooling scheme for these molecules and represent a key s
238 d atoms can be created using collision-based cooling schemes such as evaporative cooling, but thermal
239                 Subambient daytime radiative cooling (SDRC) provides a promising electricity- and cry
240 ulations and the data collected in a radiant cooling setup together demonstrate the influence of free
241 ar temperature distribution in a homogeneous cooling state.
242 werful electronic devices requires effective cooling strategies to efficiently remove ever-greater he
243 vel, Ir21a is essential for the detection of cooling, suggesting that during evolution mosquito heat
244 itiation mechanism of Earth's plate tectonic cooling system remains uncertain.
245              We present results of a radiant cooling system that made the hot and humid tropical clim
246 overed this error in an experimental radiant cooling system with high separation of air to radiant te
247                                  Traditional cooling systems consume tremendous amounts of energy and
248 lysis of the EIA and EPA data indicated that cooling systems operated on average 13% more than their
249  patients amounted to 614 825 kWh, dedicated cooling systems to 492 624 kWh, representing 44.5% of th
250 ds Three CT scanners, four MRI scanners, and cooling systems were equipped with kilowatt-hour energy
251 he melting, resolidification, and subsequent cooling take place at much higher rates and with much hi
252                                          Our cooling technique, in combination with optical trap mani
253 of widespread commercial adoption of radiant-cooling technologies is due to two widely held views: 1)
254 mosquitoes feeding in the evening experience cooling temperatures during the night, whereas mosquitoe
255 water demand but also creates an evaporative cooling that mitigates crop heat stress.
256 d periods of burial, heating, exhumation and cooling that reflect the tectonic environments in which
257 te a heterogeneous distribution of radiative cooling that selectively reduces the temperature of stru
258 ixed layer in the presence of a NIW, thereby cooling the mixed layer at a rate of 244 W m(-2) over th
259                                              Cooling the sediments induced sulfate reduction, coincid
260               The pH shift was measured upon cooling the solutions from 20 to -25 degrees C.
261 n surface westerly winds south of Greenland, cooling the subpolar North Atlantic.
262  in THF solution, where aggregates form upon cooling, the TADF mechanism takes over around room tempe
263  for gender, trial randomisation allocation (cooling therapy versus usual care) and estimated blood l
264 s that multi-plate tectonics was preceded by cooling through a single-plate lithosphere, but models f
265      Falling atmospheric CO(2) levels led to cooling through the Eocene and the expansion of Antarcti
266 sthesia at 1 of 5 different temperatures and cooling times.
267                           In vivo pancreatic cooling to 25 degrees C reduced the increase in circulat
268 the emission pattern of water after a sudden cooling to 4 K, signifying the conversion of ortho-water
269 vice was developed to provide anesthesia via cooling to a focal area on the surface of the eye before
270 us hypothermia, and thus require less active cooling to attain TH.
271 rt for a dynamical response linking volcanic cooling to El Nino remains ambiguous, Robock raises some
272 es with an unfavourable outcome require less cooling to maintain a core temperature between 33 and 34
273 rey matter injury on MRI require less active cooling to maintain target temperature during TH.
274 oldness of the outer space through radiative cooling to produce electricity at night using a commerci
275 -phase is formed from the cubic phase during cooling to room temperature and subsequently deforms in
276  competition with vibrational relaxation and cooling to the relaxed (3) MLCT state.
277 he non-negligible contribution of irrigation cooling to the yield benefits of irrigation, and such an
278 , ice sheets and mineral dust aerosols, this cooling translates to an equilibrium climate sensitivity
279 n Eurasian temperature reveals a significant cooling trend (P < 0.05).
280 ds played a significant role in driving this cooling trend through increasing global weatherability.
281 our was determined from total time receiving cooling (TT(cool) ) and cumulative button presses.
282 elvin in one dimension and state-selectively cooling two nuclear spin isomers.
283 veloped photonic materials permit subambient cooling under direct sunshine, and their applications ar
284 ferropericlase followed by decompression and cooling under oxidized conditions, leading to the format
285 mitter at night, and 5 degrees C sub-ambient cooling under sunlight.
286                          Short-term (aerosol cooling) volcanism still allows equatorial habitability.
287 o mitigate the 1(st)-order economic risks of cooling water shortage during droughts.
288 investigate the electricity price impacts of cooling water shortages on Britain's power supplies usin
289                                 The risks of cooling water shortages to thermo-electric power plants
290  regional climate, hydrological droughts and cooling water shortages, coupled with an economic model
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 rotein solutions during thermal gelation and cooling were evaluated.
294                   Subjects were able to seek cooling when their neck was thermally uncomfortable by p
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 d cover by modulating the longwave radiative cooling within the atmosphere.
298 corded in Antarctic ice cores imply that the cooling would have been more pronounced in the Southern
299 nal SDRC, and also leads to enhanced daytime cooling yet suppressed nighttime overcooling.
300  trap leads to efficient dipolar evaporative cooling, yielding a rapid increase in phase-space densit

 
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