Ophir Optronics Ltd QSR ユーザーズマニュアル
Chapter 1 – Introduction
Definition of Terms
Some applications include:
Peak-to-peak stability of energy pulses.
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Power drift of CW lasers over time.
Graphical display of dB loss measured in a fiber optic cable.
Logging energy of rapidly pulsing lasers at 1000Hz or more.
Definition of Terms
The USBI, Pulsar or Quasar instrument is referred to in this guide as the device
or the instrument. The connection between the smart head detector, referred to
as a head, the USBI, Pulsar or Quasar device, and the StarLab application
running on your PC, is referred to as a channel. Using the StarLab system, you
can view each channel’s laser power and energy information. You can work with
multiple channels depending on the type of device you have and the number of
free USB or Bluetooth ports you have on your PC.
or the instrument. The connection between the smart head detector, referred to
as a head, the USBI, Pulsar or Quasar device, and the StarLab application
running on your PC, is referred to as a channel. Using the StarLab system, you
can view each channel’s laser power and energy information. You can work with
multiple channels depending on the type of device you have and the number of
free USB or Bluetooth ports you have on your PC.
Software Features
The StarLab software features include:
Easy configuration of measurement parameters (range, laser, etc.).
Data logging.
User adjustable calibration factors.
Real time update of measurement statistics.
Printing of graphs and data.
Interfaces and supports data logging with Ophir’s Nova-II and Vega
(see Uploading Files from the Nova-II and Vega).
(see Uploading Files from the Nova-II and Vega).
StarLab User Guide
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