ALOHA Cabled Observatory

 

 

Home

ACO Update

Experimenters Guide

Observatory Engineering Documents

Project Timetable

Publications & Reports

Contact

Links

Site Map

About ESF

User Power

Low Voltage Circuit Breakers:

There are six low voltage user ports on the Observatory for local experiments located a few meters away from the Observatory.  The Circuit Breaker boards control the maximum amount of current supplied to each user port. The board is constructed around a Vicor® 48V-48V, DC-DC converter.  The Observatory operator has the ability to monitor and set the current trip level of each Circuit Breaker.  A Rabbit® RCM3000 control module monitors the current draw from each of six low voltage user ports via a Hall Effect current sensor mounted on each Circuit Breaker board. 

The Vicor® 48V-48V, DC-DC converters: The Vicor® converters have a shutdown pin which is used to switch the user power port on. Unlike a hard switch, the Vicor® converter  provides a smooth turn-on which minimizes transients on the system bus. A separate  converter for each user also provides complete floating isolation between users and individually regulated power.

 
Rabbit® RCM3000 Low Voltage Circuit Breaker Module
  Three of six low voltage circuit breakers in the Observatory.

 

 

 

High Voltage Circuit Breakers:

There are two high voltage user ports on the Observatory for remote experiments and moorings.  Power is supplied by two Pico® 48V-200V DC-DC converters.  The outputs are connected in series to supply the user with 400V at the user port.  This high potential is designed to overcome the resistive losses of long cable runs, thus providing sufficient voltage at the remote experiment or mooring site.  The High Voltage Circuit Breakers also use the Rabbit RCM3000 to monitor and control trip levels.

The Pico® 48v-200v, DC-DC Converters:

 

 

Back    Next

 

Page Last Modified 08/10/2007

 

This site maintained by Bill Doi
Copyright © 2004  [SOEST/ESF]. All rights reserved.

The ALOHA Cabled Observatory is funded by the National Science Foundation

Revised: September 19, 2008