For a perfect ferrimagnetic material the magnetization should be parallel to the applied field, and the intensity of lines 2 and 5 is therefore expected to vanish as discussed in Section 3.6, but in the spectra
the membrane solution is decanted into a casting dish, which is horizontally placed with a heater in the upright water-cooled magnet well to evaporate the solvent, with a 35 tesla field exerted. The membrane cast with the magnetic field is hence...
When an external magnetic field is applied to a paramagnetic material, these magnetic moments tend to align themselves parallel to the applied field to lower their potential energy. This phenomenon intensifies the lines of force passing through the paramagnetic materials, shown in Figure 7.2(b). ...
The second: the solar magnetic field (MFs) from synoptic magnetographs. The third: CI measured at the east limb. And the fourth (bottom) panel: CI at the west limb. The vertical thick dashed lines show the minimum times of the solar cycles. Full size image Cross-correlation analysis is ...
(1–3) and determine the magnitude and the spatial distribution of the initial magnetic field. In the context of our model, these are the only parameters which are directly related to the intrinsic properties of the medium and not to the collision energy or geometry. We consider the cases ...
Lau, Y.-T.: Magnetic nulls and topology in a class of solar flare models. Sol. Phys. 148(2), 301–324 (1993) [Sects. 4.2.1 and 16.3] Google Scholar Lau, Y.-T., Finn, J.M.: Three-dimensional kinematic reconnection in the presence of field nulls and closed field lines. Astr...
The function 𝑓˜(𝑟˜)f˜(r˜) comes from Equation (12), and we use the parameter values listed in Table 1. Figure 2. Lines of poloidal magnetic field at three different scales, along with a color table of the field strength in units of mG. Table 1. Parameter values ...
In this study, we investigate the crystal structure, magnetic, and magnetocaloric effect properties in the intermetallic compounds SmNi3−𝑥3−xFe𝑥x using a phenomenological model based on Landau mean-field theory and Maxwell relation (conventional method). SmNi3−𝑥3−xFe𝑥x compounds...
Lau YT, Finn JM: Three-dimensional kinematic reconnection in the presence of field nulls and closed field lines. Astrophys J 1990, 350: 672–691. 10.1086/168419 Article Google Scholar Li SY, Deng XH, Zhou M, Tang RX, Liu K, Kojima H, Matsumoto H: Statistical study of electrostatic sol...
Primary Class: 360/135 Other Classes: G9B/5.189, G9B/5.293 International Classes: G11B5/82;C09D5/23;C09D7/12;G11B5/55;G11B21/21;G11B5/596;G11B5/60;G11B33/14; (IPC1-7): G11B5/82 Field of Search: 360/135, 360/77.08, 360/77.11, 360/77.05, 360/78.08, 360/46 ...