Engineering Handbook/Physics/Radiation

ElectroMagnetic Radiation when there exists an Electric Field perpendicular to a Magnetic Field

${\displaystyle C=\lambda f}$

${\displaystyle E=hf=h{\frac {C}{\lambda }}}$

Any unstable nucleus when decay under the sun light exhibit

1. Heat of Energy . ${\displaystyle E=(m_{2}-m_{1})C^{2}}$
2. ElectroMagnetic Radiation . ${\displaystyle E=hf=h{\frac {C}{\lambda }}}$