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Active Star Coupler

Authors: Hayato Yuuki; Takeharu Ito; Seiji Kawamura;

Active Star Coupler

Abstract

<div class="htmlview paragraph">APF (All Plastic Fiber) has high transmission loss and it is a disadvantage in the optical communication. If it has been used in an optical network with distributed signals, like star type, optical signals are reduced at the star coupler due to scattering loss and insertion loss caused by ray distribution. Therefore, we can use a passive star coupler only in a small area.</div> <div class="htmlview paragraph">One possible solution is light amplification at the optical star coupler using a feed back method. The feed back amplifier is composed of a pair of E/O (Erectrical/Optical), O/E (Optical/Electrical) converters using one channel in the passive star coupler. It has a performance that is able to increase the output level about 3dB at each output port. So, it enables communication between nodes with certainty. We named ACTIVE STAR COUPLER.</div>

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
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