## The B(3) Field in Vacuo and in Material Matter

In a message dated 30/07/2013 23:19:32 GMT Daylight Time, :

With these formulas the situation looks quite different. for a frequency of

omega = 2 pi * 1 MHz

one obtains

These B(3) fields are quite strong and should give huge effects.
Horst

Am 30.07.2013 18:28, schrieb EMyrone

Thanks for this, the correct formula to use for B(3) is given in eq. (6.3.44) of the book by Crowell and myself on the Omnia Opera:

B(3) = (e mu0 c/ h bar) I / omega squared = 5.723 ten power 17 I / omega squared

in free space. However teh important formula is eq. (1.10.103) of the book by Crowell and myself, writeen in 2001. At autoresonance:

omega sub res = 1.532 ten power 25 I / omega squared

I Am not sure what formula you have used for B(3).

In a message dated 30/07/2013 16:16:22 GMT Daylight Time, horsteck writes:

Currently we discuss RFR in our Munich group. we made a table by the formulas given in paper 84. Assuming a resonance frequency of 100 MHz we obtain (for several power densities I) a range of input frequencies of circularly polarized light beginning at 200 MHz. We are concerned that the B(3) field strength, given by B(0), is very small. Have you any experience on a minimum B(0) value above which any effect is observable? Maybe a value below the magnetic field of the earth will only be detected as noise.

Horst