ライフサイエンスコーパス: neon

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

34 Neon isotope heterogeneity in different mantle sources s

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

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

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

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

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

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

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

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

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

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

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

46 852.5 wave numbers (cm(-1))] than in a solid neon matrix (872.2 and 1047.3 cm(-1)).

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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