ライフサイエンスコーパス: magnetize

1 vided by the fact that the Earth is strongly magnetized.

2 low iron content and cannot become strongly magnetized.

3 and cosmic plasmas are thereby ubiquitously magnetized.

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

5 n iron-oxide nanoparticle laden hydrogel and magnetized 3D printer to enable the controlled lifting,

6 white dwarf remnant is expected to be highly magnetized(5,6) because of the strong magnetic dynamo th

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

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

9 avors complete field-free switching of CoFeB magnetized along the in-plane charge current direction.

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

11 Stents were magnetized and implanted in porcine coronary and femoral

12 t the atmosphere of Venus, despite being non-magnetized and less conductive due to lower ultraviolet

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

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

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

16 ale after optical pumping in perpendicularly magnetized asymmetric multilayers.

17 Therefore, the Earth must have been magnetized at a very early epoch, either preimpact or as

18 By exposing mature cerebral organoids to magnetized AuNPs, we were able to cultivate them in less

19 he subsequent 2 weeks under the influence of magnetized AuNPs.

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

21 Magnetizing: Bacteria are often classified into gram-pos

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

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

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

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

26 Rock fragments from the impactites were once magnetized by a geomagnetic field.

27 Magnetic labels magnetized by a homogeneous applied magnetic field weake

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

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

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

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

32 is record can only be explained if EC002 was magnetized by the field prevalent in the solar nebula.

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

34 as demonstrated in the past with magnetic or magnetized catalysts.

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

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

37 ulate spin-wave transport in perpendicularly magnetized channels of Bi-doped yttrium iron garnet.

38 we report Landau-phonon polaritons (LPPs) in magnetized charge-neutral graphene encapsulated in hexag

39 agnetic circular dichroic effects present in magnetized chiral crystal structures, we probe the inter

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

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

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

43 Additionally, a movable magnetized CoFe micro-strip is placed at different posit

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

45 ore broadly, it may be useful for describing magnetized collisionless winds from G-type stars.

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

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

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

49 ater magnetic stability than their uniformly magnetized counterparts.

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

51 a major disk substructure, possibly due to a magnetized disk wind.

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

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

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

55 f Jupiter and in laboratory experiments with magnetized electron plasmas in axisymmetric geometries.

56 ort a diverse range of evidence for a highly magnetized environment in the spider system PSR B1744 -

57 Polarized FRBs originate in highly magnetized environments.

58 Our results show that uniformly magnetized equidimensional iron particles do not provide

59 ry, we show that Fe:MoS(2) monolayers remain magnetized even at ambient conditions, manifesting ferro

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

61 121102 support an origin in a young, highly magnetized, extragalactic neutron star.

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

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

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

65 magnetic and paramagnetic particles within a magnetized ferrofluid.

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

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

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

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

70 sion(7,8), and a multitude of radio-emitting magnetized filaments(9), the origin of which has not bee

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

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

73 Spirulina (Sp) algae was first magnetized, followed by surface modification with dopami

74 he singlet-polarized reaction product into a magnetized form by the application of a radiofrequency p

75 etized out-of-the film plane and an in-plane magnetized free and reference magnetic layer separated b

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

77 shock's exposure, and leaves the individual magnetized grains in random orientations, significantly

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

79 er, the paths might be an artefact caused by magnetized haematite-bearing rocks in cold subducting sl

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

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

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

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

84 nce for a complicated, dynamically evolving, magnetized immediate environment within about an astrono

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

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

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

88 rromagnetic mineral assemblages are strongly magnetized in two nearly antipodal directions.

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

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

91 mediate case where both the unmagnetized and magnetized ion behaviors could be observed because of th

92 heavy metal, we show that in perpendicularly-magnetized iron garnets, rare-earth orbital magnetism gi

93 Magnetars are strongly magnetized, isolated neutron stars(1-3) with magnetic fi

94 The HH 211 jet is a highly collimated, magnetized jet associated with a rotating disk around a

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

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

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

98 istic, however, switching of perpendicularly magnetized materials by SOT requires a mechanism for in-

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

100 ematical model of unsteady thin film flow of magnetized Maxwell fluid with thermo-diffusion effects a

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

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

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

104 -Bohm physical system; free electrons pass a magnetized nanorod and far-field electron diffraction is

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

106 tural magnetic minerals are typically weakly magnetized, necessitating mechanisms to enhance their ma

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

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

109 that FRB 20200120E originates from a highly magnetized neutron star formed either through the accret

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

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

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

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

114 Proposed models include highly magnetized neutron stars(6), white-dwarf pulsars(7) and

115 FRB emission characteristics favour highly magnetized neutron stars, or magnetars, as the sources(1

116 Magnetars are highly magnetized neutron stars, the formation mechanism of whi

117 were formed by magnetolithography (ML) with magnetized nickel masks of column and stripe arrays.

118 Stripe arrays of magnetized nickel were designed to generate cylindrical

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

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

121 s consist of a spin-polarizing layer that is magnetized out-of-the film plane and an in-plane magneti

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

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

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

125 A magnetized path was demonstrated for successful transpor

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

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

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

129 While the potential impact of magnetized phages is high, the current methods of immobi

130 y to the generation of chorus waves in other magnetized planetary magnetospheres.

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

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

133 drifting emission features observed at other magnetized planets like Saturn and Jupiter.

134 etic emissions in the Earth's magnetosphere, magnetized planets, and laboratory plasmas, play an impo

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

136 to the Sun or magnetospheric process akin to magnetized planets.

137 he space environments of the Earth and other magnetized planets.

138 econnection-a process rarely observed at non-magnetized planets.

139 energetic electrons near the Earth and other magnetized planets.

140 interactions between the solar wind and non-magnetized planets.

141 ndings demonstrate that turbulent motions of magnetized plasma can power black-hole accretion flow co

142 s ejections (CMEs) are massive expulsions of magnetized plasma from a star and are the largest contri

143 ules are rapidly evolving fine-scale jets of magnetized plasma in the solar chromosphere.

144 Magnetized plasma interactions are ubiquitous in astroph

145 ing the inherent structure and properties of magnetized plasma jets spanning both laboratory and astr

146 uilibrium solutions are used for analyses of magnetized plasma phenomena.

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

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

149 blazars, active galactic nuclei with jets of magnetized plasma that point nearly along the line of si

150 aneously, which opens up the possibility for magnetized plasma tolerating steady-state voltage drops

151 ctures suggest coherent emission from highly magnetized plasma(3,4).

152 waves interacting with vortices in turbulent magnetized plasma, and Tollmien-Schlichting waves amplif

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

154 In a collisionless, magnetized plasma, particles may stream freely along mag

155 nce for passage through additional turbulent magnetized plasma, potentially associated with the host

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

157 vortex beam transmission from an adjustable magnetized plasma-ferrite structure with negative refrac

158 t of Fermi acceleration, in a laser-produced magnetized plasma.

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

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

161 es and topological phase transitions in cold magnetized plasmas is still missing.

162 ron wave (TLCW), a topological excitation in magnetized plasmas recently identified by numerical simu

163 ns in Earth's radiation belts, as well as in magnetized plasmas throughout the solar system.

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

165 Because of the many degrees of freedom in magnetized plasmas, the plasma is largely reconfigured w

166 tablish the bulk-edge correspondence in cold magnetized plasmas.

167 n scales leading to electron energization in magnetized plasmas.

168 d reconnection, are ubiquitous structures in magnetized plasmas.

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

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

171 The magnetizing process was discussed in detail and the phys

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

173 des reveal spin-polarized edge states in the magnetized quantum spin Hall insulator.

174 -matter and report results on aggregation of magnetized quark nuggets (MQNs) after formation from the

175 represents the dense central component of a magnetized radial wind.

176 is how plasma is transported within strongly magnetized, rapidly rotating systems.

177 dized iron-bearing phyllosilicates in highly magnetized regions of the Martian crust supports the hyp

178 ic geodynamo simulations, at least in weakly magnetized regions.

179 rstand instabilities and special dynamics in magnetized relativistic jets.

180 tability onset recalls the Landau damping in magnetized relativistic plasma.

181 elling Janus particles, and unidirectionally-magnetized robotic particles, via this static-state part

182 Magnetized rocks can record the history of the magnetic

183 ubduction geotherms, forming a frame of deep magnetized rocks in the West Pacific region.

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

185 rrobots') for precise and robust handling of magnetized sample droplets and high-fidelity delivery of

186 result from propagation through a turbulent magnetized screen of plasma, located 10(-5) to [Formula:

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

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

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

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

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

192 similar explosions of fast-spinning strongly magnetized stars occurred during the earliest epochs of

193 buted to either the emergence of a uniformly magnetized state or a reversal of the cycloid polarity.

194 ement with long-range magnetic order creates magnetized states and displaces the hysteresis loop.

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

196 While SOT switching of out-of-plane (OOP) magnetized states requires lateral symmetry breaking, in

197 res lateral symmetry breaking, in-plane (IP) magnetized states suffer from low storage density.

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

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

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

201 oscopy confirmed uniform cell capture at the magnetized surface.

202 Magnetized surfaces are prebiotically plausible chiral a

203 he polymerization was carried out upon three magnetized surfaces of silica aerogel, zeolite Y, and MI

204 In magnetized systems, the minimum entanglement characteris

205 r interaction that can be observed in chiral magnetized systems.

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

207 d RuAl layers and ultrathin, perpendicularly magnetized, tetragonal ferrimagnetic Heusler layers.

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

209 asma, we have constructed an experiment that magnetizes the electrons but not the ions.

210 Rather than magnetizing the objects within the hydrogel, the magneti

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

212 If the substrate is magnetized, then the current we measure with conductive

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

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

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

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

217 between windings of azimuthally and radially magnetized tubular objects.

218 mely small intermittent structures formed in magnetized turbulent plasmas, where the turbulence energ

219 ions and electrons in a weakly collisional, magnetized, turbulent plasma?

220 However, this theory breaks down in magnetized, turbulent, weakly collisional plasmas, altho

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

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

223 study elucidates the mechanism through which magnetized water influences these properties.

224 Additionally, magnetized water notably enhances the flexural and compr

225 h systematically investigates the effects of magnetized water on the fundamental grouting properties

226 The results indicate that magnetized water positively impacts the stability of cem

227 exploratory approach using green, economical magnetized water technology to enhance the performance o

228 ch mass is accreted onto a moderately strong magnetized white dwarf from a low-mass companion, have b

229 source could be an old magnetar or an ultra-magnetized white dwarf; however, both interpretations pr

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

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

232 ke magnetic depth profile when the system is magnetized within the film plane.

233 We propose that the magnetized Wolf-Rayet star formed by the merger of two l