ライフサイエンスコーパス: magnetic field strength

1 gnetic activity that increases with inferred magnetic field strength.

2 nsible for the observed antipodal decline in magnetic field strength.

3 e by exploiting the MRI signal phase at high magnetic field strength.

4 asurements of the local electron density and magnetic field strength.

5 tance distribution which is dependent on the magnetic field strength.

6 t density (Jc) drops rapidly with increasing magnetic field strength.

7 ive contrast on T(1)-weighted images at high magnetic field strengths.

8 d Ca(2+)-loaded states of the protein at two magnetic field strengths.

9 ts of T1, T1rho, and steady-state NOE at two magnetic field strengths.

10 T(1)(rho), and the steady-state NOE at three magnetic field strengths.

11 ferent origins, and repeated at a variety of magnetic field strengths.

12 ance in dehydrated zeolite HY, by using high magnetic-field strengths.

13 working electrode size (10 microm-3 mm), and magnetic field strengths (0-1.77 T) generated with elect

14 Purpose To determine the impact of different magnetic field strengths (1, 1.5, 3, and 7 T) and the ef

15 dicular) ) diffusivity were measured at high magnetic field strength (11.7T) and analyzed relative to

16 o temperatures (29 and 34 degrees C) and two magnetic field strengths (11.7 and 14.1 T).

17 15N relaxation data at two magnetic field strengths, 11.74 T and 14.10 T, were used

18 the backbone amide group at three different magnetic field strengths (18.8, 14.1, and 8.5 T) and fou

19 lowing quantitative diffusometry even at low magnetic field strengths (30 MHz).

20 4H] (4+) species when employed under modest magnetic field strength (3T) and a data acquisition dura

21 The high magnetic field strength (4.9 T) employed in these 139.5

22 lts show that the 207Pb T1 is independent of magnetic field strength and inversely proportional to th

23 The magnetic field strength and not the magnet type is impor

24 ma flows in the heliosheath to determine the magnetic field strength and orientation in the interstel

25 o the appropriate experimental conditions of magnetic field strength and rotational speed of the capi

26 actor 2 reduction in near-Earth heliospheric magnetic field strength and solar wind speed, and up to

27 ets align progressively well with increasing magnetic field strength and that the alignment is effect

28 Additionally, the influence of magnetic field strength and the presence of a breathable

29 There is a stark boundary as a function of magnetic field strength and toggle frequency distinguish

30 Higher magnetic field strengths and improved signal detectors h

31 R(2) approximately 1 mM(-1)s(-1)) at typical magnetic field strengths and so requires high levels of

32 nge of relaxation data measured at different magnetic field strengths and temperatures.

33 neither head movement nor dynamic change in magnetic field strength) and directional (sensitive to m

34 ce, sequence parameters, spatial resolution, magnetic field strength, and image post-processing, emph

35 especially in larger phantoms and at a high magnetic field strength, are not necessarily applicable

36 An estimate of the compression ratio of the magnetic field strength B (+/- standard error of the mea

37 The magnetic field strength B increased across this boundary

38 specific conditions of pH, temperature, and magnetic field strength, because changes in conditions c

39 ively, are observed for Gly residues at high magnetic field strengths, but even at much lower fields

40 s could be obtained in minutes at a moderate magnetic field strength by using dynamic nuclear polariz

41 ample volumes to be investigated at moderate magnetic field strengths, compared with conventional NMR

42 al spin labels are reported as a function of magnetic field strength corresponding to proton Larmor f

43 enine residues, the 1H T2 values exhibited a magnetic field strength dependence for all adenosine H8

44 It is generally accepted that Earth's magnetic field strength drops to low levels during polar

45 itable planet, little is known about Earth's magnetic field strength during that time.

46 stant, 1/T(1), was measured as a function of magnetic field strength for several dilute protein solut

47 We infer a surface magnetic field strength for the white dwarf in MV Lyrae

48 ntly strong to explain the observed range of magnetic field strengths for isolated, high-field magnet

49 75 cm and 20 cm respectively in the range of magnetic field strengths from 0 to 200 mT.

50 ded (94+/-8%, N = 4, where B(r) = 0.41 T and magnetic field strength is 0.20 T) magnets, were similar

51 d (210+/-14%, N = 4, where B(r) = 1.23 T and magnetic field strength is 0.55 T) and bonded (94+/-8%,

52 MR spectroscopy and the availability of high magnetic field strengths now offer the possibility to re

53 determine the risks associated with MRI at a magnetic field strength of 1.5 tesla for patients who ha

54 mized study to assess the safety of MRI at a magnetic field strength of 1.5 Tesla in 1509 patients wh

55 mperature range of 290-320 K and at a static magnetic field strength of 14.1 T.

56 hem; for one source, we have inferred a high magnetic field strength of 5 x 10(13) G.

57 Oe) recorded on all three aporepressors at a magnetic field strength of 600 MHz ((1)H Larmor frequenc

58 ils are compatible with MR imaging at static magnetic field strengths of 1.5 T or less.

59 axation data acquired at 310 K and at static magnetic field strengths of 11.7, 14.1 and 18.8 T are an

60 fect is demonstrated in glycogen phantoms at magnetic field strengths of 4.7 and 9.4 T, showing impro

61 correlated spin relaxation rates at multiple magnetic field strengths on the C-terminal domain of the

62 nce method and diffusion measurements at two magnetic field strengths on water and NAA phantoms in vi

63 ons of bovine serum albumin as a function of magnetic field strength, oxygen concentration, and solve

64 lar ballooning, NASH diagnosis, fibrosis, or magnetic field strength (P = .65).

65 easurements performed over 310-140 K and two magnetic field strengths provide insights into conformat

66 singly rapid carbonyl relaxation at the high magnetic field strengths required by TROSY techniques re

67 s static (continuous, proportional to static magnetic field strength, requiring neither head movement

68 Small pockets of low magnetic field strength, small radius of curvature, and

69 cation year, functional MR imaging paradigm, magnetic field strength, statistical threshold, and anal

70 on analysis, (b) avoid the need for multiple magnetic field strengths to extract dynamic parameters,

71 s of chemical shift anisotropy (CSA) at high magnetic field strengths varies.

72 We found that magnetic field strength was nearly constant throughout t

73 on spin relaxation rate over a wide range of magnetic field strengths, we determine the populations o

74 s and structural parameters obtained at each magnetic field strength were compared in corresponding s

75 derable residue-by-residue variations in the magnetic field strengths where TROSY line narrowing is m

76 range of available spectrometers of varying magnetic field strengths with a standard 5 mm probe setu

77 greement with experiment for three different magnetic field strengths without adjusting any parameter

78 vement is equivalent to doubling the applied magnetic field strength, without loss in signal-to-noise

79 Tesla, K(NAA) in the absence of any applied magnetic field strength would be 32.