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radial component sentence in Hindi

"radial component" meaning in Hindiradial component in a sentence
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  • Electric current ( proportional to the radial component of velocity ) will decrease with increasing magnetic field and hence the resistance of the device will increase.
  • For example, this kind of differential equation appears in Quantum Mechanics while solving the radial component of the Schr�dinger's Equation with hypothetical cylindrical infinite potential barrier.
  • As the radar only sees the radial component and has a certain elevation from ground, the radial velocities are contaminated by some fraction of the falling speed.
  • The operation of these systems is based on the fact that the Doppler frequency shift in the target echo is proportional to the radial component of target velocity.
  • The radial component of this velocity in the direction of the Sun is  " 13.9 km / s, while the transverse velocity is 9.9 km / s.
  • Two have already been discussed above, in the cases that either the radial components or the angular components are zero, and the non-zero component of motion describes uniform acceleration.
  • If the boundary is a sphere in three space dimensions, the angular components of the eigenfunctions are spherical harmonics, and the radial components are Bessel functions of half-integer order.
  • Later Newton identified another resolution of the perturbing acceleration LM + MS = LS, into orthogonal components : a transverse component parallel to LE, and a radial component, effectively ES.
  • A radial motion produces no change in the direction of the particle relative to the origin, so, for the purpose of finding the angular velocity, the radial component can be ignored.
  • The inner surface corresponds to an event horizon similar to that observed in the Schwarzschild metric; this occurs where the purely radial component " g rr " of the metric goes to infinity.
  • If initially is nonzero but 0 } }, while and are arbitrary, then the initial velocity of the particle has no radial component, is constant, so the motion will be in a perfect helix.
  • The radial component of the velocity will be zero; this must be true if we are to use the annular ring approach; to assume otherwise would suggest interference between annular rings at some point downstream.
  • To derive this, Moore and Saffman solved the linearised Navier-Stokes Equation along in cylindrical coordinates, where some of the vertical and radial components of the viscous term are taken to be small relative to the Coriolis term:
  • If " B " is a circle, then these eigenfunctions have an angular component that is a trigonometric function of the polar angle ?, multiplied by a Bessel function ( of integer order ) of the radial component.
  • Where particles are assumed to have mass " m " and charge " q ", " r " is radial distance from the trap axis and " E r " is the radial component of the electric field.
  • It may change the magnitude and / or direction of the angular momentum vector, depending on the angle between the velocity vector and the non-radial component of the force vector, as viewed in the pivot's frame of reference.
  • It shows the radial component of the incident electric field, which causes the charged particles at the scattering point to exhibit a radial component of acceleration ( i . e, a component tangent to the plane of observation ).
  • It shows the radial component of the incident electric field, which causes the charged particles at the scattering point to exhibit a radial component of acceleration ( i . e, a component tangent to the plane of observation ).
  • It ignores the fact that Faraday's law is defined by the total, not partial, derivative of magnetic flux and also the fact that EMF is not necessarily confined to a closed path but may also have radial components as discussed below.
  • The electric current in the heliospheric current sheet has a radial component ( directed inward ) as well as an azimuthal component, the radial circuit being closed by outward currents aligned with the Sun's magnetic field in the solar polar regions.
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