ライフサイエンスコーパス: magnetize

1 pollo era that the lunar rocks and crust are magnetized.

2 ear a black hole, differential rotation of a magnetized accretion disk is thought to produce an insta

3 e self-sustained turbulence that develops in magnetized accretion disks is suppressed in the weakly i

4 The detection of strongly magnetized ancient crust on Mars is one of the most surp

5 Stents were magnetized and implanted in porcine coronary and femoral

6 the magnetic nanoparticles (MNPs) are first magnetized and then the temporal response is monitored a

7 onvection, leading to dark spots in the most magnetized areas.

8 ial application to Jupiter, Saturn and other magnetized astrophysical objects.

9 , main sequence star is pulled onto a highly magnetized (B>10 MG) white dwarf.

10 Magnetizing: Bacteria are often classified into gram-pos

11 angle that is predicted to remain stable in magnetized baryonic jet models or vary randomly with tim

12 larization properties show that GRBs contain magnetized baryonic jets with large-scale uniform fields

13 ters per kilogram for meter-size homogeneous magnetized boulders.

14 The lunar crust and returned samples are magnetized, but the source of this magnetization could b

15 Magnetic labels magnetized by a homogeneous applied magnetic field weake

16 rate that a simple metal such as gold can be magnetized by a temperature gradient or magnetic resonan

17 ation in the BaFe12O19 film when the film is magnetized by an in-plane magnetic field.

18 Ferromagnets are commonly magnetized by either external magnetic fields or spin po

19 Composite airborne dust particles appear magnetized by freeze-dried maghemite stain or cement tha

20 s, our results suggest that the Pt is likely magnetized by YIG due to the magnetic proximity effect (

21 -dense iron-containing aggregates within the magnetized cells.

22 Current methods for magnetizing cells use artificial MNPs and have disadvant

23 the Galactic disk, driven by rotation of the magnetized circumnuclear gas disk.

24 driven domain-wall motion in perpendicularly magnetized Co/Ni/Co trilayers, we find an internal effec

25 ires formed from ultra-thin, perpendicularly magnetized cobalt layers and cobalt/nickel multilayers d

26 l magnetoresistance (TMR) in perpendicularly magnetized CoFeB/MgO/CoFeB MTJs can be achieved by both

27 Unwanted labeled cells are retained in the magnetized column, permitting high recovery (70%) and pu

28 ical models for the accretion of matter onto magnetized compact objects.

29 s, which we interpret as stars with strongly magnetized cores.

30 ater magnetic stability than their uniformly magnetized counterparts.

31 es a circular Halbach array of diametrically magnetized, cylindrical permanent magnets.

32 agneto-spin alignment" mechanism that causes magnetized disks and jets to align with the BH spin near

33 elf assembly in a system of millimeter-sized magnetized disks floating at a liquid-air interface and

34 Here we describe experiments on magnetized DNA-modified electrodes to explore spin-selec

35 of these structures studied through in-situ magnetizing experiments performed at room temperature, c

36 121102 support an origin in a young, highly magnetized, extragalactic neutron star.

37 inhomogeneous magnetic field, generated by a magnetized Fe-wire, has been applied to an electrochemic

38 mal to the layers, we find a perpendicularly magnetized feature that exhibits non-volatile electrical

39 racterization of a synthetic perpendicularly-magnetized ferrimagnet based on [Mn2.9Ga/Co2MnSi]n super

40 magnetic and paramagnetic particles within a magnetized ferrofluid.

41 the magnetization completely in out-of-plane magnetized ferromagnetic elements, but the switching is

42 the edge of the gap, close to the edge of a magnetized ferromagnetic wedge, or close to a small (<1

43 tical shift register between perpendicularly magnetized ferromagnets of subnanometre thickness, simil

44 orm spontaneously in the absence of external magnetizing fields, and their geometry is determined by

45 lization of chiral spin textures in in-plane magnetized films has remained rare.

46 While in-plane magnetized films have been studied extensively as media

47 ucture of a domain wall in a perpendicularly magnetized GaMnAsP/GaAs ferromagnetic semiconductor and

48 Hence, nonuniformly magnetized grains, which are commonly the main remanence

49 ign, even though these layers are oppositely magnetized, high-tunnelling magnetoresistance is possibl

50 Magnetofection, the process of magnetizing HIV by coupling it to ferrous nanoparticles

51 th emission from a magnetar, but also from a magnetized hot white dwarf, or an accreting isolated neu

52 Here we demonstrate a transgenic approach to magnetize human mesenchymal stem cells (MSCs).

53 chondrules from the Semarkona meteorite were magnetized in a nebular field of 54 +/- 21 microteslas.

54 ld mare basalts demonstrating that they were magnetized in a stable and surprisingly intense dynamo m

55 TPrA(*)] complexes may become magnetized in magnetic field and experience a long magne

56 ld, without the need to assume that Io has a magnetized interior.

57 dly place endothelial cells at the site of a magnetized intravascular stent.

58 switching of both out-of-plane and in-plane magnetized layers.

59 m the solar 'surface' (photosphere) into the magnetized low atmosphere of the Sun.

60 emonstrate the effectiveness of out-of-plane magnetized magnetic microdiscs for cancer treatment thro

61 e been predicted to occur in perpendicularly magnetized materials in the absence of damping.

62 in diamond can be coupled to the motion of a magnetized mechanical resonator.

63 ing fluids are manufactured ferrofluids with magnetized nanoparticles embedded in liquid carriers.

64 lmonella enterica spp. and utilized strongly magnetized nanoparticles to enhance the detection signal

65 in walls in atomically thin, perpendicularly magnetized nanowires, which are interfaced with adjacent

66 One possibility is that AXPs are highly magnetized neuron stars or 'magnetars' having surface ma

67 where extra energy is injected by a strongly magnetized neutron star (a magnetar), which has also bee

68 The pulsations result from the rotation of a magnetized neutron star, and the modulation arises from

69 Pulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the e

70 Pulsars are rotating, magnetized neutron stars that are born in supernova expl

71 They are thought to be magnetars: strongly magnetized neutron stars with emissions powered by the d

72 etic fields has been the method of choice to magnetize non-magnetic materials, but they are difficult

73 omagnetic topological insulator thin film is magnetized out-of-plane, conduction ideally occurs throu

74 iously published theories, such nonuniformly magnetized particles provide greater magnetic stability

75 ls in rocks are usually larger, nonuniformly magnetized particles, for which there is no empirically

76 ssume only the existence of small, uniformly magnetized particles, whereas the carriers of paleomagne

77 A magnetized path was demonstrated for successful transpor

78 orbed onto the microspheres, captured with a magnetized permalloy wire, and then directly injected as

79 Media that are magnetized perpendicular to the plane of the film, such

80 hat levitated three-dimensional culture with magnetized phage-based hydrogels more closely recapitula

81 he space environments--or magnetospheres--of magnetized planets emit copious quantities of energetic

82 Aurorae are detected from all the magnetized planets in our Solar System, including Earth.

83 reconnection than that of Earth or the other magnetized planets.

84 ve tearing and thinning into two-dimensional magnetized plasma structures having successively finer s

85 release is a common phenomenon occurring in magnetized plasma systems ranging from laboratories, Ear

86 c Weyl points in a naturally existing medium-magnetized plasma, in which Weyl points arise as crossin

87 numerically investigate an interface between magnetized plasma, using a realistic model for parameter

88 l surface states in a simple natural system- magnetized plasma.

89 occurs in classical and superfluids, and in magnetized plasmas and superconductors.

90 he Sun's output of ultraviolet light, and of magnetized plasmas, cannot be ruled out.

91 ng of the physical processes at work in hot (magnetized) plasmas in stars and their immediate environ

92 the aggregation of millimeter-sized, chiral magnetized plates floating at a liquid-air interface and

93 The magnetizing process was discussed in detail and the phys

94 e magnetic structure and the analysis of the magnetizing process.

95 Magnetized rocks can record the history of the magnetic

96 Pulsars are highly magnetized rotating neutron stars and are well known for

97 lly demonstrate how, in an astutely designed magnetized semiconductor heterostructure, the above limi

98 interactions between magnetic particles and magnetized sensors dramatically impact particle transpor

99 behaviour (in which the nanoparticles can be magnetized similarly to a paramagnet under an external m

100 formation is the evolution of a gaseous and magnetized solar nebula.

101 usible that Io, like Earth and Mercury, is a magnetized solid planet.

102 J, enough to make predictions for the highly magnetized states and the effects of applied pressure on

103 We hypothesized that a magnetized stent would facilitate local retention of sup

104 c new phases of quark matter and of strongly magnetized superconductors.

105 y and uniform cell coverage was noted on the magnetized surface.

106 oscopy confirmed uniform cell capture at the magnetized surface.

107 ere, we report the switching of out-of-plane magnetized Ta/Co(20)Fe(60)B(20)/TaO(x) structures by spi

108 A magnetic dynamo in a convecting fluid core magnetized the crust, and the global field shielded a mo

109 The beads are magnetized, then subjected to a twisting field, with the

110 rrent-induced switching of a perpendicularly magnetized thulium iron garnet film driven by charge cur

111 Mn-Ge termination layers that are oppositely magnetized to the higher moment Mn-Mn layers.

112 nterference device to show that current in a magnetized topological insulator heterostructure (EuS/Bi

113 radient boundary region (called pedestal) of magnetized toroidal plasma in the KSTAR tokamak device.

114 between windings of azimuthally and radially magnetized tubular objects.

115 rt a phase of spin structures in an in-plane magnetized ultrathin film system where out-of-plane spin

116 They are magnetized using a bias field to produce a particle capt

117 The origin of highly magnetized white dwarfs has remained a mystery since the

118 se to the critical transition to much weaker magnetized winds.