... Commons Attribution License ( https://creativecommons.org/licenses/by/4.0/ ), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. Abstract Measuring the magnetic field of the Milky Way reveals the structure and evolution...

... of pulsars with periodic amplitude modulation and subpulse drifting, which will contribute to the future studies on the statistical properties of subpulse drifting as well as its radiation mechanisms. stars: magnetic fields stars: neutron pulsars: individual: PSR J1824−0132 First Study of Subpulse Drifting...

... of systems, possibly compatible with the prediction of 40–70percnt of magnetic cataclysmic variables to be period bouncers. white dwarfs accretion, accretion discs binaries:general novae, cataclysmic variables stars: magnetic fields O RIG IN AL UN ED ITED M A N USCRIPT Discovery of two new polars evolved...

... slightly less well in the umbra, this is likely explained by magnetic field suppression and reduced contrast. Differences in velocities introduced by DeepVel did not affect Lagrangian analysis; consequently, we demonstrate for the first time that the DeepVel-recovered velocities accurately reflected...

... pertinent et donc essaient, autant que possible, de se montrer sympathiques ou de passer inaperçus, en évitant toute interaction, surtout avec le CAE, dans la mesure du possible. armed conflict agency capital fields control Myanmar Rakhine Bourdieu conflicto armado agencia capital campos control...

... fields that are structured on scales greater than the CR Larmor radius. We solve the Vlasov–Fokker–Planck equation for various mixes of mirroring and small-angle scattering and show that relatively small deviations from a uniform magnetic field can induce mirroring and inhibit CR transport to levels...

... of the Creative Commons Attribution License ( https://creativecommons.org/licenses/by/4.0/ ), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. Abstract Magnetic fields are often invoked as playing a primary role in star formation...

... of the Creative Commons Attribution License ( https://creativecommons.org/licenses/by/4.0/ ), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. ABSTRACT We investigate the effects of magnetic field geometry on energy injection...

... of the Creative Commons Attribution License ( https://creativecommons.org/licenses/by/4.0/ ), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. ABSTRACT Magnetic fields are an important component of the interstellar medium (ISM...

... Attribution License ( https://creativecommons.org/licenses/by/4.0/ ), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. Abstract Magnetic fields play an important role in the evolution of galaxies and in shaping the dynamics...

... are strongly magnetized, the significance of magnetic fields in Bok globules has largely been limited to individual case studies, lacking a broader statistical understanding. In this work, we introduce a comprehensive optical polarimetric survey of 21 Bok globules. Using Gaia and near-infrared (IR...

... of CME as magnetic reconnection commences at the current sheet, and its subsequent evolution and propagation to around 0.1 au. A twisted magnetic flux rope (MFR), as the main body of the CME, is created by the continuous reconnection during the eruption. By interacting with the ambient field, the MFR...

... period. We develop a camera capture system using 2 robotic arms combined with a turntable, controlled by a re-deployable and flexible image capture framework. We trained each plant instance using two recent view synthesis models: 3D Gaussian splatting (3DGS) and neural radiance fields (NeRF). Our results...

... between the surface/subsurface poleward/equatorward angular momentum transport and the Joy’s law. There is a suggestion of the strength of the Joy’s law depends on the strength of the poleward angular momentum transport. Sun: activity Sun: magnetic fields Sun: rotation (Sun): sunspots SN 10.13039...

...: corresponding optical depth distributions with values of 1.21e-4 (left) and 3.97e-5 (right) at 850 m. Figure 2. Map of the continuum intensity at 3.6 cm of K3-35 obtained with the VLA (adapted from M+01 ) superimposed with the possible distribution of the magnetic field segments from this work. Figure 1...

... < 0.001. Nonverbal IQ of children was screened with different assessment tools; therefore, a direct between-group comparison was not provided. NA, not available. ND, no data. Table 2 Amplitude and latency of auditory event-related fields in children with and without ASD, M ± SD. Neural...

... other permissions can be obtained through our RightsLink service via the Permissions link on the article page on our site—for further information please contact [email protected]. Abstract Purpose Tumor Treating Fields (TTFields) are alternating electric fields approved for the treatment...

... magnetoacoustic waves in the coronal loops are dispersive. The dispersiveness of these waves can provide a useful tool for the diagnosis of physical conditions inside the coronal loops along which these waves travel. waves Sun: atmosphere Sun: corona Sun: magnetic fields NASA 10.13039/100000104...

... Carlo (MC) and Multilevel Monte Carlo (MLMC) methods applied to partial differential equations with random coefficients. These arise, for example, in groundwater flow modelling, where a commonly used model for the unknown parameter is a random field. We use the circulant embedding procedure for sampling...

... in the Solar system, which contains ultra-relativistic protons (  GeV), electrons (  MeV), and heavier ions like (  MeV) etc. Based on the energies and locations of the charged particles and the strength of local magnetic field, they either get lost or remain trapped in the Jupiter’s magnetosphere...