All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, by any means, electronic,
mechanical, photocopying, recording, or otherwise, without written permission from Ocean Optics, Inc.
This manual is sold as part of an order and subject to the condition that it shall not, by way of trade or otherwise, be lent, resold, hired out or
otherwise circulated without the prior consent of Ocean Optics, Inc. in any form of binding or cover other than that in which it is published.
Trademarks
All products and services herein are the trademarks, service marks, registered trademarks or registered service marks of their respective owners.
Limit of Liability
Ocean Optics has made every effort to ensure that this manual as complete and as accurate as possible, but no warranty or fitness is implied. The
information provided is on an “as is” basis. Ocean Optics, Inc. shall have neither liability nor responsibility to any person or entity with respect to
any loss or damages arising from the information contained in this manual.
Table of Contents
About This Manual......................................................................................................... v
Document Purpose and Intended Audience..............................................................................v
Index ...................................................................................................47
000-20000-400-01-201108iii
Table of Contents
iv000-20000-400-01-201108
About This Manual
Document Purpose and Intended Audience
This document provides you with installation and operation instructions for your Overture software.
Document Summary
ChapterDescription
Chapter 1: Introduction to Spectroscopy
Chapter 2: Overture Software
Chapter 3: Overture Software Icons and
Menus
Chapter 4: Experiments
Chapter 5: Applications
Appendix A: Sample Experiments
Appendix B: Maintenance
Provides an overview of spectroscopy and spectrometers.
Lists installation procedures for Overture software.
Contains a list of the icons and menu items and their
functions in Overture software.
Provides a variety of experiments to perform using Ocean
Optics spectrometers and Overture software.
Contains applications for Overture software.
Contains some possible experiments for Ocean Optics
spectrometers and Overture software.
Provides suggested maintenance and a table of possible
problems and suggested solutions.
Product-Related Documentation
You can access documentation for Ocean Optics products by visiting our website at
http://www.oceanoptics.com
document from the available drop-down lists. Or, use the
of the web page.
000-20000-400-01-201108v
. Select Technical → Operating Instructions, then choose the appropriate
Search by Model Number field at the bottom
About This Manual
You can also access operating instructions for Ocean Optics products on the Software and Technical
Resources
CD included with the system.
Engineering-level documentation is located on our website at
Technical → Engineering Docs.
Upgrades
Occasionally, you may find that you need Ocean Optics to make a change or an upgrade to your system.
To facilitate these changes, you must first contact Customer Support and obtain a Return Merchandise
Authorization (RMA) number. Please contact Ocean Optics for specific instructions when returning a
product.
vi000-20000-400-01-201108
Chapter 1
Introduction to Spectroscopy
Spectroscopy in a nutshell
A spectrometer is a device that breaks up light into different colors by spreading out, or dispersing
different wavelengths. Rain does this by refraction
through yellow and then red.
of light, creating a rainbow that goes from violet
This spread of colors is called the visible spectrum. Humans can see light between 380nm (violet) and
780nm (deep red). Other creatures can see different ranges.
You can get the same effect by reflecting light with a CD. The very fine markings on a CD are so small
that they are getting close to the wavelength of light and cause the diffraction of light into a spectrum. The
CD surface is acting as a diffraction grating
000-20000-400-01-2011081
. In fact it is a reflecting diffraction grating.
Chapter 1: Introduction to Spectroscopy
If you want to find out how a motorcycle works, the best thing to do is take it apart to its individual pieces
and see what it’s made of. The same applies to light. If we can break it up using refraction or diffraction,
we can see what is going on at each wavelength.
Note
Try searching on the web for the words in blue.
Spectroscope views
Below are three spectra as seen through a traditional spectroscope.
This spectrum is of a tungsten filament lamp:
This is spectrum of sunlight. It is a similar continuous spectrum but it contains fine dark lines caused by
absorption of certain wavelengths in the sun and earth atmospheres. These are called Fraunhofer lines
This is an emission spectrum from a hydrogen gas discharge tube. It shows that the hydrogen gas only
emits light at certain wavelengths. Excited hydrogen atoms emit a specific series of narrow spectral lines
called the Balmer series.
.
2000-20000-400-01-201108
Chapter 1: Introduction to Spectroscopy
The CCD array spectrometer
Looking at sunlight through the spectrometer will tell us a lot about how it works. If you have a pocket
spectroscope you can compare the traditional spectroscope view with the Overture software display.
Sunlight enters the spectrometer through a 50 micron-wide slit. That is very narrow; 5/100ths of a
millimeter.
In a conventional spectroscope you will see a spectrum and any absorbance lines will show as dark lines.
These lines correspond to sharp dips in the Overture spectrum graph.
The light passes through an optical geometry of focusing mirrors and a reflection grating. The spectrum
falls on a linear CCD array
array corresponds to one wavelength.
with 250 tiny sensors in a row so that each sensor (often called a pixel) in the
The number of photons
on the graph. The x-axis is scaled to the pixel number, which indicates wavelength.
hitting each pixel is converted to a voltage which is converted into a y-axis value
Optical Limitations
The Ocean Optics Spectrometers for Education can display peaks separated by less than 2nm, depending
on the model. This is the limit of its resolution.
The spectrometer resolution is limited by a number of factors, including:
Slit width
Grating specification (lines per mm) and quality
Number of pixels in the array
Physical size of the system
This causes an apparent spreading of emission and absorption lines in the Overture display so that they
appear as sharp Gaussian peaks, but this is still remarkably high resolution for a compact instrument.
In chemistry applications this is not a problem as the absorption peaks are usually over a hundred
nanometers wide. In fact you will deliberately “smooth” the spectrum by averaging the array output using
Overture software.
For chemistry applications it is the sensitivity or dynamic range that is more important. This allows the
spectrometer to detect small changes in absorption on the y-axis.
000-20000-400-01-2011083
Chapter 1: Introduction to Spectroscopy
Here is what an emission spectrum looks like. This is from a Hydrogen lamp for observing Balmer lines:
Emission lines look like sharp peaks. It is possible to identify elements from their emission peaks. Notice
that some peaks go beyond the visible range.
4000-20000-400-01-201108
Chapter 2
Overture Software
Product Overview
Overture is a spectroscopy operating software platform for 32-bit and 64-bit Windows. The following
operating systems are supported:
Windows XP
Vista
Windows 7
This software can control the following Ocean Optics spectrometers:
Overture can be downloaded from the Ocean Optics Software Downloads site, or retrieved from the CD
that you received with your purchase of an Ocean Optics spectrometer.
Retrieving from a CD
Your Overture software is shipped to you from Ocean Optics on a CD. The software is located either on
the main
separate CD labeled
jacket of the CD containing your SpectraSuite software to complete the installation.
Software and Technical Resources CD, or (in the case of the Windows 64-bit version) on a
Overture Windows 64-bit Version. You will need the password located on the
► Procedure
1.Insert the CD containing your Overture software into your computer.
2.Select the Overture software for your computer’s operating platform via the CD interface. Then
follow the prompts in the installation wizard.
Or,
Browse to the appropriate Overture set-up file for your computer and double-click it to start the
software installation. Set-up files are as follows:
3.Click on the Overture software appropriate for your Windows operating system.
\Program
4.Save the software to the desired location. The default installation directory is
Files\Ocean Optics\Overture
6000-20000-400-01-201108
. The installer wizard guides you through the installation process.
\Program
Chapter 3
Overture Software Icons and
Menus
Overview
The following table provides a quick guide to the Overture Software icons. See the paragraphs following
the table for information on how to use these icons when taking a measurement.
000-20000-400-01-2011087
Chapter 3: Overture Software Icons and Menus
IconFunction
New Graph
Open Spectrum
Save Spectrum
Copy Data to Clipboard
Store Reference Spectrum
Store Dark Spectrum
Intensity
Overture Software Icons
Absorbance
Transmission
Concentration
Snapshot
Wavelength Range
Zoom In
Zoom Out
Print
Reference Lines
Color
8000-20000-400-01-201108
Chapter 2: Overture Software Icons and Menus
Integration Time
Integration time is the exposure time for each pixel in the array. Each of the pixels is “read” in turn and
the time between readings controls the amount of charge in each CCD sensor. The charge decreases with
every photon that hits the sensor, so if there are not many photons around it takes a long time to reduce
the charge. Too many photons will discharge the sensor completely in a short time.
If the time is too long, the sensors will “saturate” and the spectrum line will go off scale. This does not
harm the sensor, but the data you collect will have no value.
For very dim sources a longer integration time is needed, but the penalty is more noise for less signal. The
default integration time is 100 ms.
The integration time is set in the Integration Time filed in the status bar at the bottom of the screen.
Intensity
Intensity is the default mode.
The y-axis reads Intensity, which is a count of how many photons have hit each pixel in the array during
one integration time. It is a relative measurement.
Intensity mode is ideal for most physics-based applications using just the fiber optic input.
Store Dark Spectrum
Before we can move on to any mathematical comparisons between sample spectra we have to tell the
spectrometer where zero is. To do this, block any light entering the fiber and click the
spectrum
You will not see any change, but the Overture software now has a zero or “dark” reading stored for every
wavelength.
icon.
Store dark
Reference spectrum
Next we have to tell the spectrometer about the source we are comparing to. This is the reference source.
Typically this would be a cuvette containing a colorless solvent, but no dissolved sample.
Set up your reference sample so that the highest point on the intensity y-axis is about 85% of full scale.
Click the store
stored.
Be careful. If you change anything about your reference source now, you must store a new reference. You
can click the icon to update the reference as many times as you like. If you change the integration time
you will need to store a new reference reading.
reference spectrum icon. You will see no change, but your reference spectrum is now
Once you have stored dark and reference spectra, the Transmission and Absorbance modes are enabled.
000-20000-400-01-2011089
Loading...
+ 39 hidden pages
You need points to download manuals.
1 point = 1 manual.
You can buy points or you can get point for every manual you upload.