measurement of speed of this beam shielded from magnetic field, measurement of its deviation from straight-forward direction under effect of magnetic field from the moment when beam leaves shielded region, distance from shielding region to anode being known; flux density is found from formula given ...
Extended free energy equality with magnetic flux The amplification is a joint effect of the driving force and the magnetic field. To uncover the mechanism of the amplification, we need to investigate the driving process and evaluate the free energy change. Through using the two-point work measurem...
The structure and dynamics of the solar corona is dominated by the magnetic field. In most areas in the corona magnetic forces are so dominant that all non-magnetic forces like plasma pressure gradient and gravity can be neglected in the lowest order. This model assumption is called the force...
The sun is magnetic, and its magnetic field elements can be classified into 5 groups according to their magnetic flux content. The main categories are magnetic elements of Component-I, II, and III. These three categories account for more than 95% of the total magnetic flux in a solar cycle...
To reduce the calculation errors caused by magnetic flux leakage, the magnetic field strength formula was employed to deduce B, which can be calculated according to Equation (2):(2)B=B0π(tan−1LW2xL2+W2+4x2−tan−1Lw2(x=H)L2+W2+4(x+H)2)where B0 is the magnetic field strength...
The magnetic field (flux density) within the core of the solenoid, B, where B = Φ/A, and A is the cross-sectional area of the solenoid, is measured by increasing the current in the solenoid coil from zero to I. As the current changes, the magnetic flux through the secondary coil ch...
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...
A soft magnetic ribbon that especially in a relatively low magnetic field region of 500 A/m or less, is high in the squareness of magnetic flux density-magnetization curve. There is disclosed a soft magnetic ribbon of 100 μm or less thickness comprising a parent phase structure in which by...
(TEM, JEM-ARM200F, JEOL) with a probe aberration corrector. The magnetic domain structure was observed using a TEM (Talos F200S, FEI) with differential phase contrast (DPC) mode. The elemental distribution was characterized by high-angle annular dark-field detector (HAADF) and energy ...
The design parameters for the hold-off time are: the core material; the cross sectional area; and the number of turns. The hold-off time can be calculated with the formula: ∫V dt=N AeuΔB Where V is the applied voltage, N is the number of turns, B is the magnetic flux density ...