The DDO work led to the 1963 measurement of the absolute flux density of Cassiopeia A at 320 MHz, a radiometric standard.
42.
Where p is the momentum of the positron, e is the charge of the positron and B is the magnetic flux density.
43.
Therefore, the specific radiative intenstity is unsuitable for the description of a collimated beam, while spectral flux density is suitable for that purpose.
44.
This is a derivation of the magnetic flux density around a solenoid that is long enough so that fringe effects can be ignored.
45.
The magnetic flux density is increased by 30 % in the coil rolling direction, although its magnetic saturation is decreased by 5 %.
46.
We can, under suitable conditions, derive these new variables by locally defining the gradients and flux densities of the basic locally defined macroscopic quantities.
47.
Most published flux values for the inner and outer belts may not show the maximum probable flux densities that are possible in the belts.
48.
Abrikosov vortices form a lattice, usually triangular, with the average vortex density ( flux density ) approximately equal to the externally applied magnetic field.
49.
This is closely related to energy flux density, which is the rate of energy transfer per unit area ( measured in W / m?).
50.
The heat flux density is the amount of energy that flows through soil per unit area per unit time and has both magnitude and direction.
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