Low-Cost IC Emission Reverse Engineering
summary
Demonstrates that visually correlating 1100nm infrared emissions to logic is practical with low-cost gear: a back-illuminated CMOS or cooled CCD with the IR cut filter removed, 1060/1200nm LEDs, and image processing like dark-frame subtraction and histogram equalization. Experiments show ESD diodes, a two-input NAND and a 4-bit counter switching; night-vision goggles capture live frames. Backside thinning by hand to ~25–30 µm is possible but yields ~18× attenuation versus frontside; CMOS logic remains challenging due to low switching current.
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chapters (21)
- 0:00Intro
- 1:24Infrared (IR) emissions
- 2:40Selecting an 1100 nm camera
- 7:25Lighting preparation
- 9:02Microscope optimization
- 10:32Locating ESD diodes (CD4050)
- 11:17Improving contrast
- 13:48hardwear.io Mystery logic
- 14:37Mystery logic: black box
- 15:18Mystery: output driver
- 17:05Mystery: input buffering
- 18:09hardwear.io Mystery: input diodes
- 18:33Mystery: logic states (O to Rdiv)
- 24:15CD4050 dynamic logic
- 26:51Backthinning: metrology
- 27:50L7805CV (5V regulator)
- 28:46Backthinning: sanding
- 32:12Backthinning: chemical
- 33:06Alternative sensor: PDA400 InGaAs photodiode
- 33:56Alternative sensor: IR scope
- 37:16Summary
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