Optical modules emit light at specific wavelengths with bandwidths typically ranging from several GHz to tens of GHz, and their sensitivity is defined by the minimum optical power detectable at a give...
Optical modules use a Transmitter Optical Sub-Assembly (TOSA), usually containing a laser diode (LD) or LED, to convert electrical signals into optical signals. The emission frequency is determined by the modulation rate of the laser and the wavelength of the light source. For high-speed modules, the −3 dB bandwidth of each channel can exceed 20 GHz, allowing data rates up to tens of Gbit/s per channel . Multi-channel modules may have channel wavelength spacing of approximately 1 nm to minimize crosstalk . The emission frequency is also influenced by the modulation technique, such as on-off keying (OOK), M-PAM, or M-QAM, which affects spectral efficiency and signal integrity .
Receiver sensitivity refers to the minimum average optical power that the Receiving Optical Sub-Assembly (ROSA) can detect while maintaining a specified bit error rate (BER), commonly 10^-12 . Sensitivity is measured in dBm, and higher data rates generally require higher received optical power due to increased signal-to-noise ratio demands. If the received optical power falls below the sensitivity threshold, the module may fail to detect signals correctly. Conversely, exceeding the overload optical power can also cause errors due to signal saturation .
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