ライフサイエンスコーパス: strong magnetic field

1 crystallization process in the presence of a strong magnetic field.

2 of exciton is calculated for an arbitrarily strong magnetic field.

3 of a two-dimensional electron layer under a strong magnetic field.

4 tar is a variable of beta Cep-type and has a strong magnetic field.

5 on emission from relativistic electrons in a strong magnetic field.

6 lute metals upon application of sufficiently strong magnetic field.

7 he fluctuations were found to be enhanced in strong magnetic fields.

8 kable transport anomaly commonly observed at strong magnetic fields.

9 egligible stray fields and is insensitive to strong magnetic fields.

10 superconductor in terms of its behaviour in strong magnetic fields.

11 pins can be manipulated only optically or by strong magnetic fields.

12 gle crystals of uranium dioxide subjected to strong magnetic fields along threefold axes in the magne

13 first evidence that this giant planet has a strong magnetic field and a large magnetosphere.

14 magnet was designed to generate the required strong magnetic field and field profile.

15 s, whose X-ray emission is powered by a very strong magnetic field (B approximately 10(15) G).

16 Moreover, strong magnetic fields can alter the average atmospheric

17 In a two-dimensional electron gas under a strong magnetic field, correlations generate emergent ex

18 e unusually small electric polarization, its strong magnetic field dependence, and the negative therm

19 orescence measurements and the presence of a strong magnetic field effect indicate that up to 90% of

20 me fold or sequence, the maquettes exhibit a strong magnetic field effect that rivals those observed

21 ing in two dimensions under the influence of strong magnetic fields effectively lose their kinetic en

22 Strong magnetic-field effects (MFE) were observed for tw

23 confined to two dimensions and exposed to a strong magnetic field, electrons screen the Coulomb inte

24 Sunspots are regions where strong magnetic fields emerge from the solar interior an

25 icate that the ground state of graphene in a strong magnetic field exhibits spontaneous breaking of S

26 This tool uses a magnetic particle and a strong magnetic field gradient to apply defined forces t

27 The use of strong magnetic field gradients and high magnetic fields

28 The inherently strong magnetic-field gradients of single-sided sensors

29 y mitigate artifacts related to evolution in strong magnetic-field gradients, magnetic fields that va

30 imately 5-12 s) neutron stars with extremely strong magnetic fields (>10(14 )G)--at least an order of

31 iant-branch (AGB) star can indeed generate a strong magnetic field, having as its origin a dynamo at

32 atmosphere, and would also need to possess a strong magnetic field in order to prevent its atmosphere

33 We demonstrate that strong magnetic fields in the cores of red giant stars c

34 cent of our sample show mode suppression, by strong magnetic fields in the cores, but this fraction i

35 erved and the magnetopause was threaded by a strong magnetic field, indicating a reconnection rate ~1

36 Strong magnetic fields lead to Zak-type cloning of the t

37 ing between states near the Fermi level in a strong magnetic field limit.

38 nger than about one micrometre, transport in strong magnetic fields occurs through a zero-energy stat

39 equence of partial alignment of SMM 1 in the strong magnetic field of the NMR spectrometer.

40 ion that are believed to be powered by ultra-strong magnetic fields of >10(14) G, according to the 'm

41 ns include accretion onto neutron stars with strong magnetic fields, onto stellar-mass black holes (o

42 zation is difficult to control, and requires strong magnetic fields or nonlinear optical effects, and

43 The robustness against strong magnetic field perturbations combined with the mu

44 ic particle agglutination via application of strong magnetic field pulses, we obtained identical limi

45 erefore the most decisive test of QED in the strong magnetic field regime, we find a 7-sigma discrepa

46 The strong magnetic field requires considerable changes in t

47 Lying supine in a strong magnetic field, such as in magnetic resonance ima

48 Strong magnetic fields, synchrotron emission, and Compto

49 lated cool white dwarf stars more often have strong magnetic fields than young, hotter white dwarfs,

50 tronic system is subjected to a sufficiently strong magnetic field that the cyclotron energy is much

51 re confined in two dimensions and subject to strong magnetic fields, the Coulomb interactions between

52 ountered with standard techniques by using a strong magnetic field to destabilize an otherwise stable

53 e of Io's plasma is captured by the planet's strong magnetic field to form a co-rotating torus at Io'

54 ma of deuterium and tritium is confined by a strong magnetic field to produce helium ions and release

55 urrent models of magnetars require extremely strong magnetic fields to explain their observed quiesce

56 The strong magnetic fields were associated with unusually lo

57 Spectra recorded in strong magnetic fields were typical of diamagnetic syste

58 0.01(2) mms; analysis of spectra obtained in strong magnetic fields yields parameters characteristic