Synchrotron radiation assumes relativistic particles. The total power radiated by an accelerated charge is given by the Lienard formula.
[tex]P = \frac{2}{3}\frac{e^2}{c} \gamma^6 \left[ \left( \dot{\boldsymbol{\beta}} \right)^2 - \left( \boldsymbol{\beta} \times \dot{\boldsymbol{\beta}} \right) ^2 \right][/tex]
where
[tex]\boldsymbol{\beta} = \frac{\mathbf{v}}{c}[/tex]
[tex]\gamma = \left[ 1-\left( \boldsymbol{\beta} \right)^2 \right]^{\left(-1/2\right)}[/tex]
As we approach non-relativistic speeds, \beta goes to 0 and \gamma goes to 1. So in the non-relativistic limit we regain the Larmor formula,
[tex]P = \frac{2}{3} \frac{e^2}{c^3} \left( \dot{\mathbf{v}} \right)^2[/tex]
Since the speeds are very low, the acceleration around any bend will also be low compared with c. The acceleration for a circular orbit is v^2/r, r will be on the order of millimeters for most PCB traces given their large width. So really, the total power radiated will be very small given the fact that in comparison to c^3, the charge density, velocities and the inverse of the "radius of orbit" for a common bend in a wire or microstrip line are all small. So for a circuilar orbit,
[tex]P = \frac{2}{3} \frac{e^2v^4}{c^3r^2} = \frac{2}{3} \frac{e^2\beta^4c}{r^2}[/tex]
For synchrotron, assuming a perfect orbit and doing a quick back of the envelope from Lienard, gives
[tex]P = \frac{2}{3} \frac{e^2c}{r^2}\gamma^4\beta^4[/tex]
I'm not sure if the above equation is completely valid because the analysis of the synchrotron radiation is rather complex but we are only considering the total power radiated and the actual radiated power is spatially and frequency dependent which requires much more detailed analysis. Anyway, we can see though in the last equation that the power radiated is much much larger.
EDIT: Making the extra reduction we can see that the relativistic properties cause an increase in the power of \gamma^4. Hey, that sounds familiar now that I think about it, probably derived this before. Anyway, so we can see that relativistic speeds will cause an increase of \gamma^4-fold, which can be pretty significant when you consider that \gamma goes to 0 as we approach c.