|
Basic Concept
The carrier of information in
optical fibre telecommunications is laser light which is
generated by separate highly stabilised laser sources. For each
of the optical channels, such a source must be provided to
deliver a stable wavelength. It is a well known phenomena that
the stabilistaion process is severly disturbed when even very
small fractions of laser light is coupled back to the source.
However, along a fibre optical transmission line many reflecting
surfaces, like conectors or other optical omponents exist.
Therefore, it is a must to protect the laser sources against
back reflected light. This is done by so-called optical
isolators. The most commonly used isolator is still a
combination of a Faraday rotator operated between two polarisers
based on the magneto-optical effect.
Experimental Set-up
The concept of using optical diodes formed by a polarising
beamsplitter and a quarter wave plate will be treated within the
theoretical part of this experiment, since it is not applied to
such an extent as the magneto optical isolators. Therfore, this
experiment focuses on optical isolators with their operation
wavelengths in the 1.30-1.55 um range used widely in optical
fiber communication. The basic of operation, its structures,
mechanisms, and applications will be demonstrated. To understand
this extremely important issue for optical data transmission the
set-up provides a free space Farady isolator in conjunction with
a 1.5 µm diode laser.
The light of the laser diode leaves the fibre telescope (FT-1)
almost parallel. The polariser, as well as the Farady rotator,
are mounted in rotaional holders with a 360° scale. The light
which passes the optical isolator is collimated by the fibre
telescope (FT-2). The task of the experiment is to find the best
settings for maximum suppression and transmission. Especially
for low intensities, it is recommended to modulate the diode
laser and monitor the AC signal using an oscilloscope. |