ライフサイエンスコーパス: cooling rate

1 n garnet for the purpose of constraining the cooling rate.

2 rder against crystal order near the critical cooling rate.

3 a planar-layered organisation at the slower cooling rate.

4 esponding length scales as a function of the cooling rate.

5 ting above the PIT decreased with increasing cooling rate.

6 embly process may be optimized by tuning the cooling rate.

7 ndence of cation ordering on temperature and cooling rate.

8 alues will tend to underestimate the average cooling rate.

9 ergy of the ions and reduces the collisional cooling rate.

10 om fewer immobile particles formed at higher cooling rates.

11 lline fractions largely fluctuate along with cooling rates.

12 measured magnetic field characteristics and cooling rates.

13 ofter when vitrifying the melts under higher cooling rates.

14 ells in diverse sample matrices at different cooling rates.

15 lipid composition (stearin versus olein) and cooling rate (1 versus 10 degrees C min(-1)) had an infl

16 than 33 degrees C was 10.4 minutes (average cooling rate, 14 degrees C/hr).

17 The high cooling rate, a consequence of a strong interaction pote

18 Cooling rate also affected emulsion thermo-reversibility

19 h can rationalize the effect of composition, cooling rate and annealing on room-temperature plasticit

20 The effect of cooling rate and annealing step on the solid-state forma

21 fraction of the fine eutectic decreased with cooling rate and completely ceased to exist at cooling r

22 this study was to determine the influence of cooling rate and contraction mismatch on the flexural fa

23 ), form preferentially depending on reaction cooling rate and isolation temperature.

24 The influence of cooling rate and pH on structure formation of HM pectin

25 ction enables a reasonable estimation of the cooling rate and phase transformation rate, and the diff

26 age of garnet can be used to calculate both cooling rate and TC if the temperature and age at the pe

27 belief has been that this requires both the cooling rate and the concentration of glass-inducing sol

28 The interactive influence of cooling rate and the sign and magnitude of thermal contr

29 antify freezing response of cells to various cooling rates and solution compositions.

30 ients as functions of emulsion droplet size, cooling rate, and emulsifier type were investigated usin

31 Particle size, cooling rate, and types of emulsifier all had an influen

32 files were recorded at different heating and cooling rates, and at different peptide concentrations.

33 rangement or structural relaxation at a high cooling rate; and (ii) competition of icosahedral order

34 The ultrahigh cooling rate, approaching the highest liquid-quenching r

35 The resulting cooling rates are fit to an evaporative cooling model ba

36 Slow cooling rates are necessary to sufficiently separate mix

37 Experimental heating and cooling rates are usually much faster than rates of unfo

38 ticles, whose population is sensitive to the cooling rate, are found to make the dominant contributio

39 However, at cooling rates below 0.003 degrees C/s (i.e. cooling 10 d

40 to 6 hrs of onset has been hampered by slow cooling rates, but is feasible.

41 The ensemble is exposed to a set of finite cooling rates covering roughly three orders of magnitude

42 The asymmetry between critical heating and cooling rates disappears for small MG nanorods.

43 mperature sensing is mainly dependent on the cooling rate, dT/dt, whereas the absolute temperature T

44 ay's heat flow may be unusually low, secular cooling rates estimated from present-day values will ten

45 Here we report cooling rates for group IVA iron meteorites that range f

46 With an infusion rate of 120 mL/min, cooling rates for the saline and slurry groups were -11.

47 Cooling rates for various groups of iron meteorites sugg

48 D melting curves recorded at several heating/cooling rates from 0.047 to 1.34 K/min show hysteresis a

49 With increasing cooling rates from 0.5 to 1.0 K/min the initial structur

50 oling rate and completely ceased to exist at cooling rates greater than [Formula: see text].

51 of metal alloys that form glasses at modest cooling rates has stimulated broad scientific and techno

52 With heating and cooling rates higher than 10 degrees C/min to 1 degrees

53 formed by slow, large-scale lifting or small cooling rates, including subvisual cirrus.

54 error bars, and new data from an independent cooling rate indicator show that the conventional interp

55 However, a standard cooling rate induced the formation of mannitol hemihydra

56 r, the underlying mechanisms leading to this cooling-rate-induced softening of amorphous solids have

57 Again, the cooling rate is of less consequence.

58 rified into a glassy state provided that the cooling rate is sufficiently high.

59 However, for DMTAP, cooling rates mainly affected size and only slightly mod

60 o near component shape, where a higher local cooling rate may be afforded by for example transient la

61 Under such a high cooling rate, melts of pure refractory body-centred cubi

62 nstance, an order of magnitude change in the cooling rate merely modifies the value of the glass tran

63 Improvements in the cooling rate model, smaller error bars, and new data fro

64 e is incompatible, however, with the diverse cooling rates observed within certain groups, most notab

65 A standard cooling rate of 1 degrees C/min with or without an annea

66 d ramp rate of 2.5 degrees C s(-1) and a low cooling rate of 1.5 degrees C s(-1) for reaching an anne

67 A fast cooling rate of 10 degrees C/min mainly produced delta a

68 y relevant solidification front velocity and cooling rate of 10.3 mm/s and 4500 K/s, respectively.

69 s by use of dilatometry data obtained at the cooling rate of 3 degrees C/min.

70 We measured the cooling rate of 3 M ammonium sulfate droplets undergoing

71 ve thick atmosphere on Mars that reduces the cooling rate of the interior.

72 eutectic volume fractions by controlling the cooling rate of the laser solidification process has bee

73 mo could have arisen through a change in the cooling rate of the mantle, or even a switch in convecti

74 to profound hypothermia of vital organs at a cooling rate of up to 3 degrees C per minute.

75 Heating rates of >15 degrees C s(-1) and cooling rates of >10 degrees C s(-1) allow cycle times o

76 sures of approximately 1000 bar, heating and cooling rates of >10(10) K s(-1); these extraordinary co

77 erential scanning calorimetry at heating and cooling rates of 10 and 1 degrees C/min.

78 ied out on oriented samples with heating and cooling rates of 20 to 0.2 degrees C/min.

79 To test these conclusions, the evaporative cooling rates of a droplet train of liquid water injecte

80 bidopsis roots were found to be sensitive to cooling rates of less than dT/dt = 0.01 degrees C/s.

81 Cooling rates of molten PbTe-CdTe compositions play a de

82 diffraction patterns provide the heating and cooling rates of single nanotubes.

83 that these droplets experience the expected cooling rates of ten to a thousand kelvin per hour.

84 Reducing the cooling rate or probe concentration for DPTAP bilayers r

85 n decompression-phase pressure) and cerebral cooling rate (r = .79; p < .022).

86 glasses (MGs) is quantified by the critical cooling rate (R C).

87 )(r) - T(LH)/, was identical for heating and cooling rates, +/-r, and varied as /r/beta for beta appr

88 Mn NbTi-microalloyed steel solidified in the cooling rate range of 1-50 Cs(-1).

89 Glass transformation in this cooling rate region is determined by atomic structure fl

90 ined results demonstrate that there exists a cooling rate region of 6.3 x 10(11)-16.6 x 10(11) K/s, i

91 This cooling rate requires a large-scale thermal event in the

92 bstantially larger solar heating and thermal cooling rates than gas molecules, dominating the atmosph

93 The lower the cooling rates, the firmer and more elastic were the fina

94 n due to relatively large ratios of electron cooling rate to electron transfer rate.

95 res the sensitivity of instantaneous OLR and cooling rates to changes in far-IR surface emissivity an

96 mes of temperature changes with well-defined cooling rates to intact roots of Arabidopsis thaliana ex

97 (strong) pulses, associated with low (high) cooling rates, to be followed by stronger (weaker) pulse

98 (117,000 degrees C/min) even when the prior cooling rate was as low as 880 degrees C/min.

99 ween phase selection of crystal or glass and cooling rate was investigated using molecular dynamic si

100 robiological culture results showed that the cooling rate was the most critical factor influencing ce

101 as a function of temperature and heating and cooling rate, was employed for their structural analysis

102 ature of bond-orientation order at different cooling rates, we propose two mechanisms of glass format

103 tgoing longwave radiation (OLR) and infrared cooling rates where the column precipitable water vapor

104 )GaMnO(6) has been found to depend on sample cooling rates, with detailed characterization necessary