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1 he twins in each pair had different CRF (>=1 watt).
2 essive energy efficiency of up to 15.7 GCUPS/Watt.
3 y up to 88.51 tera-operations per second per watt.
4 ielding a power efficiency of 1.7 Gflops per Watt.
5 m with a natural solar light capacity of 257 watts.
6 g a significant power output of the order of Watts.
7 ork (median, range, % change) increased 17.5 watts (-13 to +44 watts, 46%, p < 0.05), maximal oxygen
8 r men and women in Harlem, 4.11 and 3.38; in Watts, 2.92 and 2.60; in central Detroit, 2.79 and 2.58;
9 (0.58 +/- 0.30 versus 0.76 +/- 0.32 L/min), Watts (45 +/- 48 versus 71 +/- 59), V E/MVV (88 +/- 33 v
10 , % change) increased 17.5 watts (-13 to +44 watts, 46%, p < 0.05), maximal oxygen consumption increa
11 energy metric of frames per second (FPS) per watt, a 5 times higher space metric of FPS per transisto
14 wedge pressure, left ventricular dimensions, watts achieved during exercise, heart rate, maximum syst
16 s determined by van't Hoff as well as D'Arcy/Watt analyses of the isotherms at 5, 15, and/or 25 degre
19 g system with a maximum cooling power of 260 watts and a maximum temperature span of 22.5 kelvin.
20 ic capacity and muscle strength (measured in watts and newtons per kilogram of body weight, respectiv
21 uce customer acquisition costs by 15% ($0.07/Watt) and identify new market opportunities for solar co
22 trated adequate efficiencies (1 to 15 lumens/watt) and lifetimes (>5000 hours) for practical use; how
24 and 275 mW (effectively >6,000 frames/s per Watt), and (iii) can be specified and trained using back
25 approximately 0.80 watt at 80 kelvin to 0.2 watt at 200 kelvin has been demonstrated in a superlatti
26 peak powers ranging from approximately 0.80 watt at 80 kelvin to 0.2 watt at 200 kelvin has been dem
27 piratory (TI) and expiratory (TE) times, and watts at rest and during maximal exercise, before and 3
31 ; 0.5 MHz; estimated peak tissue energy 2.26 Watt/cm(2); 10% duty cycle) to engage a target in the AL
33 put of 143.6 kilowatts per cubic meter, a 24-watt commercial lamp can be directly lighted by a contin
35 later using either a surgical blade or a 150-Watt continuous-wave CO2 laser deflected by an x-y galva
36 with photoresponsivity above 0.1 ampere per watt (corresponding to an external quantum efficiency of
37 l pleural surface using 1 min of exposure (5 watts, defocused to 70 W/cm2 power density for both lase
39 association was stronger in pairs with >=60-watt difference in CRF (HR = 0.65, 95% CI: 0.59, 0.71).
40 e risks were similar in twin pairs with >=60-watt difference in CRF (HR = 0.96, 95% CI: 0.57, 1.64).
42 ewidth (0.2 +/- 0.1 angstrom), high-power (3 watts) emission that could be varied in different device
44 tantly, the criticism of our study design by Watts et al. and the designs and analysis of their recen
47 rive from fossil fuels (approximately 10(13) watts), even with improvements in energy efficiency.
54 the same trend reported by Millner-White and Watts for the effectiveness of various monovalent anions
55 um are analyzed with the Kohlrausch-Williams-Watts formalism, the exponent beta decreases with increa
57 chieved a best-in-class energy density of 41 watt hour per kilogram with a negative-to-positive (n/p)
58 tance of 200 F/g, a specific energy of 30-47 Watt-hour/kilogram (Wh/kg), a specific power of 200,000
59 per kilogram and specific energy up to 631.1 watt hours per kilogram at the micrometre-sized cathode
60 citors and can store a specific energy of 41 watt-hours per kilogram (19.5 watt-hours per liter).
61 ivering a high specific energy exceeding 410 watt-hours per kilogram of electrode plus electrolyte.
62 -ion full cell with an energy density of 460 watt-hours per kilogram of total composite electrode and
65 scillation with a threshold of tens of micro-watts in an integrated thin-film lithium niobate photoni
68 4 beats per minute), W(peak) (1.6 versus 2.7 watts/kg), AT (11.1 versus 18.0 ml O(2)/kg/minute) and W
69 ml O(2)/kg/minute) and W(AT) (0.6 versus 1.4 watts/kg), compared to controls (P <or= 0.05 for each).
73 -infrared (mid-IR) spectral range, achieving watt-level continuous wave operation in a compact packag
74 spatial-mode lasers with high efficiency and watt-level output in the 97x-nm wavelength range are in
75 metabolic rate and efficiency (O(2) cost per watt), may fall by an average of 10% following 2 h of he
76 lfur has a thermal conductivity of ~19 to 32 Watt meter(-1) Kelvin(-1) from its top to the center, mu
78 y load-insensitive inotropic index, by 0.143 Watts/mL(2).10(4) (P=0.03, a +41% rise; 5-71 CI) and car
79 re well described by the Kohlrausch-Williams-Watts model, from which a characteristic rate constant,
83 als from a few tens of mW to several hundred watts of average power and MW level of peak power, cover
86 during normal walking [generating up to 7.4 watts, or a 300-fold increase over previous shoe devices
87 49% (median increase 17 watts, range 6 to 44 watts, p < 0.05) and maximal minute ventilation (VEmax)
88 A key goal is to achieve operation at sub-watt peak power levels and on sub-picosecond timescales.
90 per square centimeter on NH(3) fuel, and 0.3 watt per square centimeter on CH(4) fuel in fuel cell mo
91 he PCECs achieve a peak power density of 1.6 watt per square centimeter on H(2) fuel, 0.5 watt per sq
92 watt per square centimeter on H(2) fuel, 0.5 watt per square centimeter on NH(3) fuel, and 0.3 watt p
93 e is estimated to be no more than about -0.3 watt per square meter (cooling), compared with +2.45 wat
94 aerosol climate forcings of as much as -0.8 watt per square meter cooling and +0.3 watt per square m
98 of clouds over the TP, with a 1.98 +/- 0.39-watt per square meter reduction in surface net CRE corre
100 rosol changes over this period of about -0.1 watt per square meter, reducing the recent global warmin
102 In 2100, we project median forcings of 5.1 watt per square meters (5th to 95th percentiles of 3.3 t
103 d) century (the probability of exceeding 8.5 watt per square meters increases to about 7% by 2150), a
105 th roughly 0.5% probability of exceeding 8.5 watt per square meters, and a 1% probability of being lo
107 erated peak power densities of less than one watt per square metre, owing to the limitations imposed
108 ray laser, high-intensity radiation (>10(17) watts per cm(2), previously the domain of optical lasers
110 th-run electrochemical muscle generates 1.98 watts per gram of average contractile power-40 times tha
112 an extremely low thermal conductivity of 0.1 watts per kelvin per meter at room temperature along its
113 discharge/regeneration power of 1,061/1,425 watts per kilogram at a 50 per cent state of charge and
116 ernating W and Se layers is as small as 0.05 watts per meter per degree kelvin at room temperature, 3
117 ntally measured thermal conductivity of 1200 watts per meter per kelvin and ambipolar mobility of 160
118 ioxide support is still as high as about 600 watts per meter per kelvin near room temperature, exceed
119 (kappa) of suspended graphene, 3000 to 5000 watts per meter per kelvin, exceeds that of diamond and
122 impact, as expressed by radiative forcing in watts per meter squared, of individual chemical species.
123 sotopes and measured kappa greater than 1600 watts per meter-kelvin at room temperature in samples wi
127 gigahertz and output power densities of 4.6 watts per millimeter at 2 gigahertz and 4.1 watts per mi
128 watts per millimeter at 2 gigahertz and 4.1 watts per millimeter at 6 gigahertz-among the highest fo
129 ed extremely high power densities of about 2 watts per square centimeter at 650 degrees C along with
130 tailored intense laser fields (about 10(13) watts per square centimeter) can dynamically Stark shift
132 for example, at 900 degrees C they deliver 2 watts per square centimetre of power in humidified hydro
133 intense (with intensities approaching 10(20) watts per square centimetre), hard (with photon energies
135 ase in S from 1983 to 2001 at a rate of 0.16 watts per square meter (0.10%) per year; this change is
136 square meter (cooling), compared with +2.45 watts per square meter (warming) due to anthropogenic gr
137 ivities should not exceed 2.5 (range: 1.7-4) watts per square meter (Wm(-2)) of the Earth's surface.
138 rane achieved a record power density of 85.1 watts per square meter and an osmotic potential of 181.5
139 urement Missions and is found to average 1.8 watts per square meter between 30 degrees S and 30 degre
140 ke instantaneous forcing of climate from -28 watts per square meter in cloud-free conditions to +8 wa
141 cking up to 97% of UV radiation from 5 to 90 watts per square meter in less than 16.9 seconds, demons
142 es that Earth is now absorbing 0.85 +/- 0.15 watts per square meter more energy from the Sun than it
143 ive forcing during the first year (34 +/- 31 Watts per square meter of burned area), but to decrease
144 imum power density using acetate reached 5.6 watts per square meter of cathode surface area, which wa
145 square meter in cloud-free conditions to +8 watts per square meter once the reduction of cloud cover
146 eased atmospheric heating locally by about 3 watts per square meter per decade (similar in magnitude
147 cooling increases at a rate of 0.11 +/- 0.31 watts per square meter per decade (Wm(-2) dec(-1)).
148 centimeter, an average power output of 4.46 watts per square meter per hertz, and an energy conversi
149 ck had a magnitude of 0.54 +/- 0.74 (2sigma) watts per square meter per kelvin, meaning that it is li
151 a global aerosol radiative forcing of +0.14 watts per square meter relative to business-as-usual sce
152 ls that the model underestimates by 25 to 30 watts per square meter the amount of solar energy absorb
155 ged over an 80-year fire cycle (-2.3 +/- 2.2 Watts per square meter) because multidecadal increases i
156 equire local surface heat flux changes (+/-4 watts per square meter) much larger than the basinwide a
157 ve flux at the top of the atmosphere was -15 watts per square meter, comparable to the aerosol indire
158 reflected sunlight decreased by less than 2 watts per square meter, in the tropics over the period 1
160 ly summer from BC in Arctic snow was about 3 watts per square meter, which is eight times the typical
161 alent to a radiative forcing of -0.5 +/- 0.4 watts per square meter, which suggests that reaching low
162 d by Earth to space increased by more than 5 watts per square meter, while reflected sunlight decreas
166 t has increased since 1750 by -0.05 +/- 0.03 watts per square metre (61 per cent), driven by the anth
168 global-mean radiative forcing of around -0.2 watts per square metre for September to October 2014.
169 this leads to an increase of an average 3.4 watts per square metre in the surface longwave fluxes.
171 hen exposed to direct sunlight exceeding 850 watts per square metre on a rooftop, the photonic radiat
172 per square metre), aerosols (+0.03 +/- 0.01 watts per square metre) and stratospheric water vapour (
173 ct cooling effect at present (-0.13 +/- 0.03 watts per square metre) that arises from halogen-mediate
174 nsated by those from methane (+0.09 +/- 0.01 watts per square metre), aerosols (+0.03 +/- 0.01 watts
175 ative perturbations of ozone (-0.24 +/- 0.02 watts per square metre), compensated by those from metha
177 (3) since 1850 AD is probably less than +0.4 watts per square metre, consistent with results from rec
178 hows a noise-equivalent power of 7 x 10(-19) watts per square-root hertz, which corresponds to an ene
182 ncreased a median of 49% (median increase 17 watts, range 6 to 44 watts, p < 0.05) and maximal minute
188 evention Trial (BCPT) Symptom Checklist; the Watts Sexual Functioning Questionnaire (WSFQ); and subsc
190 the reconstructed neutron spectra resembled Watt spectra, which gave confidence that the interrogate
191 pabilities, a neutron image resolution for a Watt spectrum of 9.65 +/- 0.94 degrees in the azimuthal
192 We use three network models, Erdos-Renyi, Watts-Strogatz and structured nodes, to generate network
194 e biologically appealing modification of the Watts-Strogatz model to describe residue networks is pro
195 scale-free, and is best approximated by the Watts-Strogatz model, which generates "small-world" netw
197 considering Erdos-Renyi, Barabasi-Albert and Watts-Strogatz networks whose temporal dynamics follow a
198 legantly explained by mechanisms such as the Watts-Strogatz or the Barabasi-Albert models, among othe
199 chastic network models-small-world networks (Watts-Strogatz), random networks (Erdos-Renyi), and scal
205 tput (direct Fick) were assessed at rest, 20 Watts (W), and peak exercise during both placebo and nit
207 wer at 6 months than at baseline, both at 20 watts workload (mean 32 mm Hg [SD 8] at baseline vs 29 m