The ions have a large radial momentum in both directions but relatively small pφ, which means the ions are either exploding or imploding. Due to their heavier mass, the ions do not response to the fast oscillating components of the laser field. This is consistent with the energy density ...
Variations in Earth's observed field are discussed in Section 5.1. There is little information about the temporal behavior of other planetary magnetic fields due to a lack of magnetic data resolution, both temporally and spatially. No undisputed magnetic secular variation has been observed for ...
The increase of electron density is gradual and not due to the stochastization of the magnetic field. Thermal diffusivity (defined as the ratio of the normalized heat flux to the temperature gradient) is evaluated for ion and electron transport, with a correction due to the slowing-down ...
The magnitude of the magnetization vector is equal to the magnetic moment per unit volume of the substance. The total magnetic field in a substance depends on both the applied (external) field and the magnetization of the substance. Consider a region where there exists a magnetic field, Bo, ...
Compelling evidence exists that magnetic fields modulate living systems. To date, however, rigorous studies have focused on identifying the molecular-level biosensor (e.g., radical ion pairs or membranes) or on the behavior of whole animals leaving a gap
Find the magnetic field (in 10-7 T) due to 2 long wires as shown at (0,0,1) m. у (wire in xy plane) 60° i=2A z
cosmological magnetogenesis scenarios using radio and gamma-ray astronomy and ultra-high-energy cosmic rays. We argue that primordial magnetic fields are observationally testable. They lead to magnetic fields in the intergalactic medium with magnetic field strength and correlation length in a well ...
At the earliest times after a heavy-ion collision, the magnetic field created by the spectator nucleons will generate an extremely strong, albeit rapidly decreasing in time, magnetic field. The impact of this magnetic field may have detectable consequences, and is believed to drive anomalous transp...
as well as beam depolarization due to a randomized magnetic-field distribution in the POS, prevent this type of studies for most extended regions of clusters, i.e., radio halos26,27. Thus, so far, no polarization mapping of magnetic fields in radio halos has been carried out. This is one...
1b, c, exhibit systematic changes in brightness due to the applied field. Strikingly, the circled emitter brightens whereas the boxed emitter dims in response to B at this orientation. The following discussion focuses on the circled defect, which remained stable over several months. Data for the...