ライフサイエンスコーパス: neon

1 the National Ecological Observatory Network (NEON).

2 US National Ecological Observatory Network (NEON).

3 the National Ecological Observatory Network (NEON).

4 ata and individual-level traits collected by NEON.

5 thin a nebula composed of carbon, oxygen and neon.

6 ally-cooled 22-pole ion trap and tagged with neon.

7 The neon abundance compared with that of hydrogen is about a

8 The neon abundance in the Sun is quite poorly determined.

9 nd real world scenarios, we demonstrate that Neon achieves state-of-the-art performance while requiri

10 Helium, neon and argon isotopes measured in olivine samples of t

11 cal spectrum of the pyrene cation C16H10+ in neon and argon matrices.

12 e measured along with the retention times of neon and the total volume of the chromatographic column

13 lumes, which have the most primitive helium, neon and tungsten isotopic compositions(11-16).

14 owing to the sudden capture of electrons by neon and/or magnesium nuclei.

15 flux, any such flux must be dominated by the neon (and helium) isotopic signature of late accreting m

16 hydrogen upon condensation in excess argon, neon, and deuterium to produce the metal dihydride molec

17 The abundances of methane, water, argon, neon, and hydrogen sulfide were measured; krypton and xe

18 silver, and gold with H(2) in excess argon, neon, and pure hydrogen during condensation at 3.5 K giv

19 giant planets should not have contained much neon, argon and nitrogen, because the temperatures were

20 rotein is more unfolded for the heavy gases (neon, argon, and nitrogen) but not the case for helium.

21 erprints for 10 test gases, that is, helium, neon, argon, hydrogen, nitrogen, carbon dioxide, methane

22 the National Ecological Observatory Network (NEON) as an example, the EDRWG recommends actions, appli

23 n of the Kalpha transition in singly ionized neon at 1.46 nanometres (corresponding to a photon energ

24 via UV photolysis of 2-iodopyridine in solid neon at 4.4 K and reacts with molecular hydrogen - but n

25 tion of infections among children beyond the neon atal period, with high reported prevalence of non-s

26 scale 'blisters' created in the top layer by neon atom intercalates.

27 r equation for ionization of helium atom and neon atom.

28 One or two neon atoms are added to each droplet prior to the additi

29 te the tip-induced subsurface translation of neon atoms.

30 ion reaction of hydroquinone with metastable neon atoms.

31 the NDC process, we show that high-pressure neon can also be trapped in NDCs and that type 2 glassy

32 red functional MRI signals corresponding to "neon color spreading": an illusory transparent surface w

33 underlying genetics of a fluorescent green "Neon" color morph, we show that allelic differences in a

34 Fixating a neon-color spreading configuration led not only to negat

35 including the subjective contour effect and neon-color spreading effect, with circuit-level precisio

36 rgy supernovae is the collapse of the oxygen-neon core of a star of 7-9 solar masses.

37 losion of an accreting, hybrid carbon-oxygen-neon core.

38 undances, implying that they are bare oxygen-neon cores and that they may have descended from the mos

39 ence times of the gas phase, indicating that neon did not dissolve in the liquid phase and could thus

40 ed as the ratio of carbon monoxide uptake to neon dilution, and lungs were fixed for histologic asses

41 gates the rovibrational energy levels of the Neon dimer using the Lippmann-Schwinger equation in both

42 nding energies and spatial properties of the Neon dimer.

43 ((13)CH(4), CD(4), and CH(2)D(2)) in excess neon during condensation at 5 K forms CH(2)=ZrH(2), the

44 the National Ecological Observatory Network (NEON) for 17 lakes and streams in the contiguous United

45 the National Ecological Observatory Network (NEON) from four ecologically variable sites in the South

46 This makes it possible to use neon gas as the nonlinear medium to coherently convert l

47 lated x-ray Raman scattering (SXRS) in dense neon gas, where the most intense inner part of the beam

48 H(2) molecules during condensation in excess neon give the WH, WH(2), WH(3), WH(4), and WH(6) hydride

49 ut the larval phase of a coral reef fish-the neon goby, Elacatinus lori.

50 the first observations of the ionisation of neon in a metastable atomic state utilising a strong-fie

51 lts that indicated a solar-nebula origin for neon in mantle plume material, which is thought to be sa

52 by subsequent recycling of seawater-derived neon in plate tectonic processes.

53 hondrites, requiring the presence of nebular neon in the deep mantle.

54 This is in contrast with the origin of neon in the mantle, which exhibits an isotopic dichotomy

55 Whereas the light noble gases (helium and neon) in the Earth's mantle preserve a solar-like isotop

56 We investigated whether NEON Intervention access benefited adults experiencing n

57 We conclude that the NEON Intervention is an effective and cost-effective new

58 developed the Narrative Experiences Online (NEON) Intervention, a web application providing self-gui

59 The instrument uses both helium and neon ion beams generated by a gas field ion source to ir

60 drogen, helium, carbon, nitrogen, oxygen and neon ions with 0.25-256 MeV/u energy.

61 a new band for the Cs(+) [F3 ](-) complex in neon is reported.

62 Neon is used as a chemically inert, near-hydrostatic pre

63 Neon isotope heterogeneity in different mantle sources s

64 Here we present neon isotope measurements from deep mantle plumes that r

65 Nonterrestrial nitrogen and neon isotope ratios suggest that indigenous organic matt

66 Here we show that neon isotopes in the convecting mantle, resolved in magm

67 Neon isotopes indicate that the melts originate from a d

68 The ratio of the two primordial neon isotopes, (20)Ne/(22)Ne, is significantly different

69 posed to Ganzfeld illumination from a helium-neon laser (543 nm).

70 single dose of 10 mW for 3 min from a helium-neon laser (632 nm).

71 amel samples were photographed with a helium-neon laser beam (lambda = 633 nm).

72 Time-varying helium-neon laser speckle images were acquired from 118 aortic

73 The scanner uses a helium/neon laser to image and measure bead-bound fluorescence

74 a simple optical train composed of a helium-neon laser, a microfluidic channel, and a position senso

75 ompression of single atoms in a non-reactive neon-like environment.

76 ted with the collapse of a lower-mass oxygen-neon-magnesium core as it loses pressure support owing t

77 olysis of 1-azulenyldiazomethane in argon or neon matrices at 3-10 K.

78 been observed under cryogenic conditions in neon matrices at 850 cm(-1) .

79 852.5 wave numbers (cm(-1))] than in a solid neon matrix (872.2 and 1047.3 cm(-1)).

80 ccumulation of some femto- to picomoles in a neon matrix (over a time scale of tens of minutes to sev

81 Excellent agreement between four observed neon matrix and four DFT calculated W-H stretching modes

82 ies and trap weakly-bound polyfluorides in a neon matrix at cryogenic temperatures.

83 the gas phase by electron diffraction, in a neon matrix by IR spectroscopy, in solution by diffusion

84 This observation contrasts a recent neon matrix investigation, which trapped CUO in a linear

85 tion modes (a(1) and e) confirms the present neon matrix preparation of WH(6) and the previous theore

86 rgon matrix and 4,395 +/- 5 angstroms in the neon matrix, both close to the strong 4,430-angstroms DI

87 eric hindrance and electronic effects in the neon matrix.

88 prebiotic isocyanic acid (HNCO) in the solid neon matrix.

89 MetaSystems Mycobacteria Scanner running the NEON Metafer AFB Module.

90 ession, and mapped 26 foliar traits in seven NEON (National Ecological Observatory Network) ecoregion

91 platinum (Pt), the NaCl-B2 phase, and solid neon (Ne) at 300 K and high temperatures up to megabar p

92 of Saturn(1,3), and the depletion of He and neon (Ne) in Jupiter's atmosphere as observed by the Gal

93 In this paper, we introduce Neon (Neural Epistemic Operator Networks), an architectu

94 he effects of different drift gases (helium, neon, nitrogen, and argon) on the transport of multiply

95 ith argon, carbon, helium [alpha particles], neon, nitrogen, and silicon) have been assessed for thei

96 it is also valid for all other gases tested (neon, nitrogen, oxygen, argon, krypton and xenon), excep

97 individuals, ranging from those living in a neon orosensory world to those living in a pastel world.

98 lium burning, and affects subsequent carbon, neon, oxygen, and silicon burning stages.

99 e plot level or ecological-community scales (NEON plots are 400 m(2)).

100 results indicate that the electron-on-solid-neon qubit already performs near the state of the art fo

101 nments of species identities at the scale of NEON sites (mean area ~ 27 km(2)).

102 raits and their uncertainties for eastern US NEON sites are available for download, and are being exp

103 s 9 National Ecological Observatory Network (NEON) sites distributed in the interior West and Great P

104 iments in a matrix consisting of 1% argon in neon suggest that the argon atoms are interacting direct

105 gle electrons trapped on an ultraclean solid neon surface in vacuum(6-13).

106 At this fluence, the neon target inevitably changes during the course of a si

107 e-dependent absorbance changes of an ionized neon target, we show how the frequency chirp can be dire

108 ejecting electrons-to produce fully-stripped neon through absorption of six photons.

109 (1/2)) X-ray lasing in elements ranging from neon to copper, which has been used for nonlinear spectr

110 Here we report neon-to-oxygen ratios measured in a sample of nearby sol

111 h an argon transition at 82 nanometres and a neon transition at 63 nanometres, thus confirming the co

112 Neon was found to be depleted in the cometary ice by mor

113 hepatic ischemia reperfusion injury, whereas neon was only explored in myocardial ischemia reperfusio

114 The measured retention times of neon were consistently equivalent to the calculated resi

115 arising from highly ionized iron, oxygen and neon with a cumulative significance in excess of five st

116 t is, detection of valence-excited states in neon with a near Fourier-limited joint energy-time resol

117 The container gas consists of helium and neon with an extraterrestrial (3)He/(4)He and (20)Ne/(22