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1 ave yielded a 100-year average annual global cooling of 0.00088 C.
2        The model output showed a mean annual cooling of 0.25 degrees C associated with a 0.09 albedo
3 with the counterfactual, leading to a global cooling of - 0.1 milli degrees C in 2030.
4 lly [90% CI: (-1.2 million,2.7 million)] for cooling of 1 degrees C from 2.5 degrees C above preindus
5 estimated that fires generate an annual mean cooling of -1.77 +/- 1.35 W/m(2) from albedo under histo
6 r decade), which corresponds to an estimated cooling of -1.8 degrees C to -3.2 degrees C since the in
7 omena and led to Northern Hemisphere climate cooling of ~1 degrees C.
8 t signal of relatively rapid, high-magnitude cooling of ~120 to 200 degrees C interpreted as erosiona
9 2.10 mW m(-2) at the top of atmosphere and a cooling of -2.96 mW m(-2) at the surface.
10                 Importantly, the hot-carrier cooling of (4AMP)PbI(4) can be extended by manipulating
11  the device prototype for a single heat spot cooling of 5 G chip is fabricated utilizing this electro
12 uct provides a constraint on global mean LGM cooling of -6.1 degrees Celsius (95 per cent confidence
13 middle and upper troposphere, with a glacial cooling of -7.35 degrees +/- 1.1 degrees C (66% CI).
14 nt results in an average surface temperature cooling of -77 mK (20 mK to -278 mK) in 2050, which incr
15                      The SRHP demonstrates a cooling of 8.8 kelvin below ambient temperature in 30 se
16                  We demonstrate direct laser cooling of a gas of rubidium-87 ((87)Rb) atoms to quantu
17 uch that the overestimation of the radiative cooling of a given quantity of emitted dust has likely c
18 uses GCMs to also overestimate the radiative cooling of a given quantity of emitted dust.
19 typically formed by melt-quenching, that is, cooling of a liquid on a timescale fast enough to avoid
20 vices by using the self-adaptive evaporative cooling of a lithium- and bromine-enriched polyacrylamid
21 ng the spin-star model paves the way for the cooling of a many-qubit system by means of a collisional
22 th a high-density spin ensemble, enables the cooling of a mechanical resonator from room temperature
23 der standard conditions, is obtained by fast cooling of a melt of stoichiometric composition.
24 llikelvin, the lowest yet achieved by direct cooling of a molecule.
25                                        Laser cooling of a neutral plasma is a challenging task becaus
26            An in-house built setup, allowing cooling of a segment of the column down to temperatures
27                          We also demonstrate cooling of a single Ar(13+) ion by a single Be(+) ion-th
28 and enrichment of olivine through multistage cooling of a thick magma body.
29  describe a very different approach, passive cooling of a whole micromechanical system down to 500 uK
30 e (delta(18)O) record and defines an overall cooling of about 12 degrees C in the deep oceans with fo
31 sitive temperature proxy, indicate an abrupt cooling of about three degrees Celsius at the onset of H
32                         To calculate the net cooling of aerosols in a spherical framework, one must c
33 ter pulses which subsequently trigger abrupt coolings of air temperature in NW Iberia consistent with
34                 Here we demonstrate sideband cooling of an approximately 10-MHz micromechanical oscil
35 sts, the presented model simulates the rapid cooling of an effervescent silicate melt fragment upon a
36 t sink and radiator are used with forced air cooling of an electrophoresis capillary.
37 h solvents, the translational and rotational cooling of an energetic CN radical can be observed direc
38 rpus pollen and wood to infer >/=5 degrees C cooling of Andean forests during Quaternary glacial peri
39 low across the Tasmanian Gateway resulted in cooling of Antarctic surface waters and coasts, which wa
40  by high endemism related to the progressive cooling of Antarctic waters and their isolation by the A
41                    Here we demonstrate laser cooling of antihydrogen(9), the antimatter atom consisti
42 ollowed by a coastal sea surface temperature cooling of approximately 2.5 degrees C, a stepwise expan
43                          Our data indicate a cooling of approximately 5 degrees C in cold-month (wint
44  a consistent forest presence and an ice-age cooling of approximately 5 degrees to 9 degrees C.
45 ed on the nano-coating, enabling heating and cooling of aqueous solutions by ~50 degrees C on a 1-mus
46                                         Mild cooling of area HVC in the Bengalese finch brain-a premo
47 t is likely that the TBJ eruption produced a cooling of around 0.5 degrees C for a few years after th
48                                    We report cooling of as much as 15 degrees C at the targeted regio
49 eir modern distribution indicates a relative cooling of at least 5 degrees C during glacials and pers
50 l statistical physics concept of Evaporative Cooling of atomic gases to perform backward stepwise pri
51 h spontaneous emission, they allow for laser cooling of atomic motion, preparation and manipulation o
52  a general two-step solution to trapping and cooling of atoms.
53 at flux accounts almost entirely for the net cooling of AW along the NwAFC, while oceanic lateral hea
54 stigate the role of air-sea heat flux on the cooling of AW.
55 xception to this rule: efficient vibrational cooling of BaCl(+) by a laser-cooled Ca buffer gas.
56 which are similar to those observed upon the cooling of bacteriorhodopsin.
57                                              Cooling of blood platelets clusters the von Willebrand f
58 tric instability (mechanical lasing) and the cooling of Brownian motion in the fundamental mode throu
59 ling (PDRC) show promise for the sustainable cooling of buildings.
60 s, supports the conclusion of very effective cooling of C(3) to its linear (1)Sigma(g)(+) ground stat
61                                  Collisional cooling of cations in the pressurized Q2 ensures efficie
62 , "in-chip" microstructures for microfluidic cooling of chips, vias, MEMS, photovoltaic applications
63 lecules, thereby opening a path to efficient cooling of chiral molecules and, eventually, optical twe
64 anning calorimetry, we demonstrate that upon cooling of citric acid and sucrose solutions a fast free
65 ymmetric resonator enables a dramatic chiral cooling of clockwise and counterclockwise phonons, while
66        Under aerobic conditions, rapid flash-cooling of crystals prior to deterioration upon illumina
67 tic species ~ 10 Ma, probably related to the cooling of deep water and vertical structuring of the wa
68 ising solution for efficient and sustainable cooling of devices operating at kilowatt levels.
69                      We found that localized cooling of different regions of primary visual cortex ca
70  processing steps (i.e., mixing, baking, and cooling) of dough-based products in light of recent stud
71 sampling biases, effects such as the secular cooling of Earth's mantle and the biologically driven ox
72 lect component of blindness was cancelled by cooling of either the contralateral posterior parietal c
73                                         Deep cooling of electron and nuclear spins is equivalent to a
74 to 300 ps that decouple from the much faster cooling of electronic temperature (about 10 ps).
75                   We demonstrate significant cooling of electrons in a nanostructure below 10 mK by d
76                           Here we report the cooling of electrons in nanoelectronic Coulomb blockade
77 inistration for hypoglycemia; techniques for cooling of exertional hyperthermia and heatstroke; recog
78 een attributed to solar heating and infrared cooling of gaseous constituents only, while the signific
79 re synchronous within age uncertainties with cooling of Greenland, and changes in global monsoon syst
80 us emission data for optoelectrical Sisyphus cooling of H2CO and CH3Cl are discussed.
81 mechanism based on light-induced evaporative cooling of holes in a correlated fermionic system.
82  these conditions is nominal, and therefore, cooling of holoprotein heated to 95 degrees C follows th
83 d halide perovskites (LHPs) is the ultraslow cooling of hot carriers.
84                                      Further cooling of hot polarons occurs on the 10(-10) s timescal
85 y 1 ps) and on structural reorganization and cooling of hot polyyne chains, following internal conver
86  been extensively used for passive radiative cooling of households.
87                                   Unilateral cooling of HVC shows that control of syllables is mostly
88            Heating and subsequent controlled cooling of individual particles with a two-wavelength la
89  exceed the characteristic timescale for the cooling of initially hot photo-generated excitons.
90 ls for use in energy applications and in the cooling of integrated circuits.
91                   Here we show how radiative cooling of intergalactic gas and subsequent supernova he
92 millimetre-size dust grains and regulate the cooling of interstellar gas within galaxies(4,5).
93 nce of the cavity can hamper efficient laser cooling of ions because of geometric constraints that th
94 we avoid this obstacle and demonstrate laser cooling of ions in a neutral plasma.
95                                 Observed LGM cooling of just 1.2 degrees C implies a relaxation of tr
96 ply the need for a approximately 3 degrees C cooling of LGM sea surface temperatures in the western P
97  we demonstrate that moderate local cortical cooling of lightly anesthetized or naturally sleeping mi
98 c glasses are commonly produced by the rapid cooling of liquid alloys.
99                                        Rapid cooling of liquids below a certain temperature range can
100 n of the random mode of timing and that mild cooling of LMAN causes an increase in the durations prod
101 erately manufactured by the melting and slow cooling of local alluvial silts.
102         We further demonstrate that upon sub-cooling of long n-alkane fluids and mixtures, a disconti
103 low chambers or volatile-rich magmas and the cooling of magma by country rock may enhance this releas
104  of quantum degeneracy relies on evaporative cooling of magnetically trapped atoms to ultracold tempe
105 ion by this process may have accelerated the cooling of matter as it collapsed to form the first star
106                                     Photonic cooling of matter has enabled both access to unexplored
107  chaotic quivering of microcavities, optical cooling of mechanical modes, actuation of a tapered-fibr
108  between photons and phonons, and backaction cooling of mechanical modes.
109  including sensitive metrology, ground state cooling of mechanical motion and slowing of light.
110                   We demonstrated that rapid cooling of milk enhances the mechanisms of nucleation an
111 he dynamics of the system during warming and cooling of milk in the range 10-40 degrees C.
112                          Because sympathetic cooling of molecular rotational motion is much more effi
113                                   Buffer gas cooling of molecules to cold and ultracold temperatures
114 al for bio-geoengineering to be a summertime cooling of more than 1 degrees C throughout much of cent
115 ess-stable (more-sensitive) climate, as does cooling of more than 2K.
116                                 Here we show cooling of NaLi molecules to micro- and nanokelvin tempe
117                  Slow solvent evaporation or cooling of nanocrystal solutions (over hours or days) is
118            This subambient daytime radiative cooling of nanoprocessed silk was achieved without compr
119 bust linear correlation between pre-rainfall cooling of near-surface air temperature and extreme rain
120                                              Cooling of neocortex or hippocampus reversibly can atten
121                                       First, cooling of neutral atoms into their motional ground stat
122  observation of microwave-forced evaporative cooling of neutral hydroxyl (OH(*)) molecules loaded fro
123                                We report the cooling of nitric oxide using a single collision between
124 proper ro-vibronic transitions enables laser cooling of nonlinear molecules, thereby opening a path t
125 of biomimetic coatings for passive radiative cooling of objects.
126 of this energy demand is wasted on excessive cooling of offices, a practice known as overcooling.
127  of a trapped nanodiamond cluster results in cooling of one degree of freedom to less than 1 K.
128 g alternative is vitrification, or the rapid cooling of organs to a stable, ice-free, glass-like stat
129 bility of using stretched spin states in the cooling of other molecules.
130                                        Focal cooling of pars triangularis/pars opercularis (Broca's r
131 chanisms include injection, acceleration and cooling of particles, with possible intervention of shoc
132 e of the chip allows for efficient localized cooling of parts of the chip to subzero temperatures by
133 ences in the responses of spinal neurones to cooling of peripheral receptive fields in control versus
134 solely in root endodermal cells, during slow cooling of plants from 20 to 0.5 degrees C over 5 min an
135 nsistent with formation via condensation and cooling of polymetallic melts (immiscible Fe-Al-Pu-U; an
136 rate of antihydrogen, enabled by sympathetic cooling of positrons with laser-cooled beryllium ions.
137                                              Cooling of preheated human insulin-poly(ethylene glycol)
138 Great Ordovician Biodiversification Event to cooling of previously very warm tropical oceans.
139 y of using this technique for the continuous cooling of quantum computers.
140 plication of OEB, we demonstrate algorithmic cooling of quantum gases: a sequence of reversible OEB-b
141                                       Active cooling of qubits, applied to quantum information scienc
142 polymer that enables dual-functional passive cooling of radiation and evaporation.
143 90 intermediate is determined by vibrational cooling of retinal.
144 e Labrador Sea Water (LSW), formed by winter cooling of saline North Atlantic water and subsequent co
145 ling (>5 degrees C/s heating, >7 degrees C/s cooling) of samples as they flowed continuously through
146  the atmosphere, indicative of the planetary cooling of Saturn, reveals remarkable seasonal fluctuati
147 urassic ( approximately 174 Ma) mid-latitude cooling of seawater by as much as 10 degrees C in the no
148 y partially by absence of respiratory system cooling of shunted blood.
149 s was not affected by temperature, and rapid cooling of slices loaded with FM1-43 did not increase th
150 conversion process that also occurs in laser cooling of solids (LCS).
151 s of AC chillers for the sensible and latent cooling of space has hindered the thermal-lift reduction
152 howing its controlling influence on seasonal cooling of SST in a critical oceanic regime.
153                                The prominent cooling of SST is observed only in the vicinity of AR up
154 nd transient kinetics (including hot carrier cooling) of strongly-confined perovskite QDs.
155                                         Slow cooling of such a melt or tempering of hP-Na2ZnSn5 (e.g.
156                   In hybrid perovskites, the cooling of such thermal carrier distributions occurs on
157                                  Vibrational cooling of the (3)MLCT state shows up as early-time dyna
158 included the early 20th century warming, the cooling of the 1960s and 1970s, the accelerated warming
159 oupling, we demonstrate microwave backaction cooling of the 4.48 MHz mechanical resonance of a nanobe
160 rt is hindered by (1) the lack of convective cooling of the ablation electrode and (2) the varying pr
161                                    Recently, cooling of the ablation electrode by saline irrigation h
162 mb itself, and which relates to the relative cooling of the affected limb.
163                Here we show that evaporative cooling of the air surrounding the pileus creates convec
164 arming of the Antarctic Peninsula and slight cooling of the Antarctic continental interior in recent
165   Rather than adaptation being driven by the cooling of the Antarctic, our results highlight the role
166                                      Whereas cooling of the antenna for 24 hours caused only a delay
167                                    Selective cooling of the antenna relative to the body resulted in
168  studies; this record of the Neogene reveals cooling of the Arctic that was synchronous with the expa
169 infall primarily by increasing the radiative cooling of the atmosphere.
170 of 950 nm, and achieved strong, simultaneous cooling of the beam in all degrees of freedom.
171              We compared intensive care plus cooling of the body to 33.5 degrees C for 72 hours and i
172 ve (CS) neurons fire at a higher rate during cooling of the body, and when active, may contribute to
173                 New techniques such as local cooling of the brain and the combination of hypothermia
174 is reduced to tens of nanometres-solid-state cooling of the calorimetric device can be accomplished v
175                                        Rapid cooling of the Cd(im)(2) melt yields a monolithic glass
176 critical point of the liquid, and subsequent cooling of the cell to room temperature.
177 e of the SEOP process) in 4 min, and perform cooling of the cell to the temperature at which the hype
178 OT) marked the most dramatic global climatic cooling of the Cenozoic.
179                 We demonstrate that feedback cooling of the centre-of-mass motion of a trapped nanodi
180  from ocean fertilisation to aerosol induced cooling of the climate may provide a basis for solar rad
181  further with shorter extraction times, mild cooling of the column, or lower flow rates.
182                                      Similar cooling of the cortex during light anesthesia rapidly an
183 cks heal either upon further heating or upon cooling of the crystals due to the topochemical polymeri
184                                 We find that cooling of the deep ocean and a small heat gain in the u
185            Phase separation is observed upon cooling of the droplets, leading to the formation of amo
186               Our results imply that secular cooling of the Earth has extended the stability of glauc
187                                          The cooling of the Earth's climate through the effects of an
188 h heating of the tropical Pacific leads to a cooling of the east equatorial Pacific and a La Nina-lik
189 oth cases, climate warming corresponded with cooling of the eastern tropical Pacific despite differen
190                       This suggests that the cooling of the eastern tropical Pacific may be associate
191 rs ago did not interrupt an almost monotonic cooling of the EEP during the Plio-Pleistocene.
192                                       Saline cooling of the electrode during radiofrequency (RF) abla
193 Doran et al. claim that there has been a net cooling of the entire continent between 1966 and 2000, p
194  maximum rated power, and after dilution and cooling of the exhaust gas, there was a bimodal number s
195                                  Ultra-rapid cooling of the eye for anesthesia was well tolerated, wi
196                                   Convective cooling of the fine-sized fuel particles in wildland veg
197  This process is faster than the vibrational cooling of the Franck-Condon excited state, indicative o
198  time, a model was developed to simulate the cooling of the Fukushima Daiichi Nuclear Power Plant rea
199 lling, we infer that these changes reflect a cooling of the Galapagos mantle plume from a potential t
200     Observations reveal that the substantial cooling of the global lower stratosphere over 1979-2003
201        We observe that water accelerates the cooling of the graphene electrons, whereas other polar l
202 e might only form as a metastable phase upon cooling of the H(II) phase.
203 rdial infarct size can be reduced by topical cooling of the heart.
204 ransition of the mixtures, as well as during cooling of the HII phase.
205                                              Cooling of the hot intracluster medium in cluster center
206                It eliminates the undesirable cooling of the hot junction by thermally isolating the a
207 a sudden growth of the Antarctic ice sheets, cooling of the interior ocean, and the establishment of
208                           Vitrification upon cooling of the liquid phase gives rise to the first Fe-m
209 e is an inevitable consequence of conductive cooling of the lithosphere, even when the underlying ast
210 is than is predicted by models of conductive cooling of the lithosphere.
211 e models analyzed underestimate the observed cooling of the lower stratosphere and overestimate the w
212  than thermochemical convection from secular cooling of the lunar interior.
213      We interpret this dispersion to reflect cooling of the magma reservoir margins below approximate
214 f mantle melting resulting from the enhanced cooling of the mantle at ca. 2.1 Ga.
215  regime has developed gradually with secular cooling of the mantle since the Neoarchaean era, 2.5 bil
216  regime plays an important role in the rapid cooling of the mantle, and thickening and strengthening
217  has evolved through time due to the secular cooling of the mantle.
218 al reduction in heat load leading to optical cooling of the mechanics without added damping, an effec
219  membrane structural changes since in silico cooling of the membrane alone, while maintaining the hig
220                                To verify the cooling of the membrane motion to a phonon occupation of
221 ectable by fluorescent labeling, followed by cooling of the membranes below their miscibility phase t
222  quantum dot electron spin qubits where deep cooling of the mesoscopic nuclear spin ensemble is used
223 s that occur during the frequent heating and cooling of the metal oxide.
224                                   Pronounced cooling of the mid- to upper stratosphere, mainly driven
225                           Here we report the cooling of the motion of a radio-frequency nanomechanica
226                                              Cooling of the MS reduced both theta frequency and power
227 iased near a transport resonance, we observe cooling of the nanomechanical mode from 550 mK to 300 mK
228 uitive European warming developed amid rapid cooling of the North Atlantic and North America from 5.8
229  Atlantic Deep Water formation and attendant cooling of the North Atlantic at this time, indicating a
230 model simulations indicating that a relative cooling of the Northern Hemisphere caused a southward sh
231 ponse to this flow, concentrating the entire cooling of the northern North Atlantic by the colder atm
232                         Volcanically induced cooling of the ocean surface penetrated into deeper laye
233                            In contrast, mild cooling of the ocular surface has been reported to incre
234 ised demagnetisation process, we demonstrate cooling of the on-chip electrons from 9 mK to below 5 mK
235 ent standard for liver preservation involves cooling of the organ on ice (0-4 degrees C).
236 tion but also suggest that rigidification or cooling of the overall structure upon effector binding p
237 uid iron core, which convects in response to cooling of the overlying rocky mantle.
238 tail electron loss is known to predict rapid cooling of the parallel electron temperature [Formula: s
239                                        Rapid cooling of the particles causes rapid strengthening, and
240 We examined the effect of mild passive focal cooling of the perilesional neocortex on the development
241 nd record global contraction associated with cooling of the planet.
242 tes entail a steepening subduction angle and cooling of the plate interface, allowing for subduction
243     Here we experimentally demonstrate laser cooling of the polar molecule strontium monofluoride (Sr
244 exciton-photon detuning suggests evaporative cooling of the polaritons as they are transported into t
245   In 8 rabbit heart atrial-AVN preparations, cooling of the posterior and/or the anterior AVN approac
246   Gravitational condensation, accompanied by cooling of the primordial gas via molecular hydrogen, yi
247 hermal stresses produced by the differential cooling of the province relative to its surroundings, co
248 er scale geothermal development will lead to cooling of the recreational thermal springs or a reducti
249 expect that the method also allows efficient cooling of the rotational motion of the molecules.
250 hemia in comparison to forced brief external cooling of the same duration.
251 r improving neurologic outcome than external cooling of the same duration.
252 lm reduces the inhomogeneous broadening, and cooling of the samples to 77K reduces the homogenous bro
253 s paradox, the heat effects upon heating and cooling of the separate DNA strands have been measured b
254 e, in part, to absence of respiratory system cooling of the shunted blood and that this effect would
255 nteraction processes and observe sympathetic cooling of the single ion by the condensate.
256 nomously" release the enzyme upon subsequent cooling of the solution.
257  time separation between pulses for temporal cooling of the specimen made possible studies of fleetin
258                                     Although cooling of the SPM lowered dark count rates and improved
259                             This showed that cooling of the strands from 100 degrees C to -10 degrees
260      Their primary contributions are through cooling of the stratosphere (caused by ozone) and warmin
261  of watermass changes involved in the recent cooling of the subpolar gyre.
262 e deficit matches that induced by unilateral cooling of the superior colliculus.
263 arming of the initial state--slows radiative cooling of the surface and amplifies continental warming
264 ndary organic aerosol (SOA) production and a cooling of the surface via impacts on cloud radiative pr
265 g-induced deficits resemble those induced by cooling of the topologically equivalent inferotemporal c
266 osols over South America and Africa causes a cooling of the tropical Pacific and Atlantic, respective
267         A subsequent multiyear ensemble mean cooling of the tropical Pacific is simulated through the
268                 We demonstrate that by local cooling of the tumor the melittin is rapidly released fr
269 icant additional warming over the Amazon and cooling of the upper air column and nearby oceans.
270 ring simultaneously with the sudden climatic cooling of the Younger Dryas event.
271 d-infrared observations, indicate a dramatic cooling of Titan's atmosphere inside the winter polar vo
272  demonstration provides an analog to optical cooling of trapped ions and atoms and is generalizable t
273                                  Sympathetic cooling of trapped ions through collisions with neutral
274              We find a remarkable speedup in cooling of twisted bilayer graphene near the magic angle
275 tic glaciation alone, combined with deep-sea cooling of up to 4 degrees C and Antarctic ice that is l
276                                We found that cooling of V4 or V2|3 did not lead to consistent changes
277  we demonstrate subambient daytime radiative cooling of vertical surfaces under peak sunlight using a
278                                       During cooling of vPS cortex, the cats could neither learn the
279 th biogas capture was the open pond used for cooling of wastewater before it enters the biogas recove
280 hese ice packages result from the conductive cooling of water ponded near the Gamburtsev Subglacial M

 
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