The phenomenon is derived from Snell's Law: , where represents the refractive index of the media.
At the critical angle (), the angle of refraction is . Since , the formula simplifies to .
The general formula for the critical angle is:
Step 1: Verify Media Density: Ensure the light is traveling from a medium with a higher refractive index (e.g., glass) to one with a lower refractive index (e.g., air).
Step 2: Calculate the Critical Angle: Use the ratio of refractive indices to find the threshold angle using .
Step 3: Compare Incident Angle: Measure the angle of incidence relative to the normal; if , the ray will reflect internally.
Step 4: Apply Reflection Laws: Once TIR is confirmed, treat the boundary as a perfect mirror where the angle of incidence equals the angle of reflection.
| Feature | Refraction | Total Internal Reflection |
|---|---|---|
| Direction | Bends away from normal | Reflects back into medium |
| Energy | Shared between reflected/refracted rays | reflected energy |
| Condition | ||
| Media Path | Denser to Rarer (or vice versa) | Denser to Rarer ONLY |
Check the Direction: Always verify that the light is moving from a high- to a low- material; if it moves from air to glass, TIR is physically impossible.
The Sine Limit: If your calculation for results in a value greater than , you have likely swapped the refractive indices in the formula.
Normal Line Accuracy: Ensure all angles are measured from the normal (perpendicular to the surface), not the surface itself, which is a frequent source of calculation errors.
Boundary Behavior: Remember that at exactly the critical angle, the light does not reflect back; it travels along the boundary (grazing emergence).