Orders@OceanOptics.com(Questions about orders)
TechSupport@OceanOptics.com (Technical support)
Ocean Optics offers the most comprehensive, innovative and high-quality line of modular
spectroscopy tools in the world. We have partnered with ARCoptix (
www.arcoptix.com) to offer
their ARCoptix ANIR FTS spectrometer to work with our SpectraSuite Spectrometer Operating
Software. We invite you to contact us at Ocean Optics, Inc. (see front cover for contact information)
or ARCoptix S.A. with any technical questions, comments, or applications inquiries. ARCoptix can
be contacted at the following location:
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 ARCoptix.
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, re-sold, hired out
or otherwise circulated without the prior consent of ARCoptix and Ocean Optics 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
Every effort has been made to make 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. ARCoptix and Ocean Optics 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 .............................................................................................................iii
Document Purpose and Intended Audience..............................................................................iii
Index ...................................................................................................29
ii ARC-000000-000-02-0310
About This Manual
Document Purpose and Intended Audience
This document provides the user of ARCoptix ANIR Series FTS Spectrometers with instructions for
setting up, and performing experiments with their spectrometer.
Document Summary
ChapterDescription
Contains descriptive information about the ARCoptix Spectrometer
Chapter 1: Introduction
and how sampling works. It also provides a list of system
requirements, interface options, and shipment components.
Chapter 2: Installing the
Spectrometer
Chapter 3: Using the
Spectrometer
Chapter 4:Troubleshooting
Appendix A: How the
ARCoptix ANIR Works
Appendix B: Specifications
Provides hardware and software installation instructions.
Describes how to use operate the spectrometer with SpectraSuite
software.
Contains recommended steps to isolate and correct common
problems.
Discusses Arcspectro ANIR technology.
Contains technical specifications for the ARCoptix ANIR Series
Spectrometer.
Product-Related Documentation
You can access documentation for Ocean Optics products by visiting our website at
http://www.oceanoptics.com. Select Technical → Operating Instructions, then choose the
appropriate document from the available drop-down lists. Or, use the Search by Model Number field
at the bottom of the web page.
Detailed instructions for SpectraSuite Spectrometer Operating Software is located at:
Occasionally, you may find that you need to make a change or an upgrade to your system. To
facilitate these changes, you must first contact Customer Support to obtain a Return Merchandise
Authorization. Please contact Ocean Optics for specific instructions when returning a product.
Warranty
This product is covered by a limited 1-year warranty that starts 30 days after purchasing hteh
spectrometer. Using the equipment in a manner not specified by this manual may impair the
protection provided by the equipment. Information in this document is subject to change without
notice and does not represent a commitment on the part of ARCoptix S.A. or Ocean Optics, Inc. No
responsibility is assumed by ARCoptix S.A. for the use of this software, hardware or other rights of
third parties resulting from its use. The software described in this document is furnished under a
license agreement and may be used or copied only in accordance with the terms of the agreement. The
user may make a single copy of the software for archival purposes.
ARCoptix S.A. and Ocean Optics, Inc. (or Seller) warrants that its products will be free from defects
in materials and workmanship under normal use and service in general process conditions for the
effective period set out below. This warranty and its remedies are in lieu of all other warranties
expressed or implied, oral or written, either in fact or by operation of law, statutory or otherwise,
including warranties of merchantability and fitness for a particular purpose, which Seller specifically
disclaims. Seller shall have no liability for incidental or consequential damages of any kind arising out
of the sale, installation, or use of its products. Seller’s obligation under this warranty shall not arise
until Buyer notifies Seller of the defect. Seller’s sole responsibility under this warranty is, at its
option, to replace or repair any defective component part of the product within the warranty period.
Except in the case of an authorized distributor or seller, authorized in writing by Seller to extend this
warranty to the distributor’s customers, the warranty herein applies only to Buyer as the original
purchaser from Seller and may not be assigned, sold, or otherwise transferred to a third party. No
warranty is made with respect to used, reconstructed, refurbished, or previously owned Products,
which will be so marked on the sales order and will be sold “As Is”.
BUYER’S SOLE AND EXCLUSIVE REMEDY UNDER THIS WARRANTY IS THAT THE
SELLER EITHER AGREES TO REPAIR OR REPLACE, AT SELLER’S SOLE OPTION, ANY
PART OR PARTS OF SUCH PRODUCTS THAT UNDER PROPER AND NORMAL
CONDITIONS OF USE, PROVE(S) TO BE DEFECTIVE WITHIN THE APPLICABLE
WARRANTY PERIOD. ALTERNATELY, SELLER MAY AT ANY TIME, IN ITS SOLE
DISCRETION, ELECT TO DISCHARGE ITS WARRANTY OBLIGATION HEREUNDER BY
ACCEPTING THE RETURN OF ANY DEFECTIVE PRODUCT PURSUANT TO THE TERMS
SET FORTH HEREIN AND REFUNDING THE PURCHASE PRICE PAID BY BUYER.
iv ARC-000000-000-02-0310
About This Manual
Place of Service
Seller shall use its best efforts to assist buyer to resolve all warranty related issues through Ocean
Optics technical support as soon as reasonably practicable after notification by the Buyer of a possible
defect. However, the Seller reserves the right to require the Buyer return the Product to Seller’s
production facility, transportation charges prepaid, when necessary, to provide proper warranty
service.
Effective Date
The effective date of this warranty shall begin on the date of shipment/date of invoice, whichever is
later. Products are warranted to be free from defects in materials and workmanship for parts and labor
for 1 year with the exceptions indicated below:
Limitations
Products are warranted to be free from defects in materials and workmanship for parts and labor for 1
year with the following exceptions:
Any components of the system that are in direct contact with corrosive materials are
warranted to be free from defects in materials and workmanship at time of delivery but cannot
be further warranted due to the unknown nature of the use of the product.
Consumable items such as lamps, cuvettes and optical filters are excluded from this warranty.
If a lamp undergoes a catastrophic failure (e.g., no light at all) within 90 days of shipment
from the factory, it will be replaced at no charge.
Loss, damage, or defects resulting from transportation to the Buyer’s facility, improper or
inadequate maintenance by Buyer, software or interfaces supplied by the buyer, unauthorized
modification or operation outside the environmental specifications for the instrument, use by
unauthorized or untrained personnel or improper site maintenance or preparation.
The sole and exclusive warranty applicable to software and firmware products provided by
Seller for use with a processor internal or external to the Product will be as follows: Seller
warrants that such software and firmware will conform to Seller’s program manuals or other
publicly available documentation made available by Seller current at the time of shipment to
Buyer when properly installed on that processor, provided however that Seller does not
warrant the operation of the processor or software or firmware will be uninterrupted or error
free.
Products that have been altered or repaired by individuals other than Ocean Optics personnel
or its duly authorized representatives, unless the alteration or repair has been performed by an
authorized factory trained service technician in accordance with written procedures supplied
by Ocean Optics.
Products that have been subject to misuse, neglect, accident, or improper installation.
The warranty herein applies only to Products within the country of original delivery. Products
transferred outside the country of original delivery, either by the Seller at the direction of the Buyer or
by Buyer’s actions subsequent to delivery, may be subject to additional charges prior to warranty
repair or replacement of such Products based on the actual location of such Products and Seller’s
warranty and/or service surcharges for such location(s).
ARC-00000-000-02-0310 v
About This Manual
vi ARC-000000-000-02-0310
Chapter 1
Introduction
Overview
The heart of an ARCoptix ANIR FTS Spectrometer is an interferometer module that contains a
micromechanical device, actuation and driving electronics. Additionally there is a laser based feedback system to control the motion of the micromechanical device. Dedicated optical components bring
the light onto the surface of the interferometer mirrors, as well as fibers for in-coupling and outcoupling of light.
The interferometer module is packaged in a friendly cover including the detection board, all necessary
electronics with the A/D converter and the USB data transfer. The instrument is USB powered.
Figure 1-1
In Figure 1 – 1, the Fourier transform is based on the lamellar grating concept. One distinguishes the
input for the optical fiber for bringing the light to the spectrometer. The whole spectrometer is low
consumption. Data transfer to the computer and powered supply are done by the USB plug.
Benefits of the ARCoptix ANIR Spectrometer
The concept of lamellar grating interference (LGI) leads to a drastic simplification of the assembly and
alignment tolerances. Because of the use of the LGI, a different type of actuation could be used,
making the whole device extremely compact. In fact, there is no need of placing a beamsplitter in the
light path. To assure highest precision, a low power laser is used to control of the position of the
scanning system.
ARC-00000-000-02-0310 1
1: Introduction
Thanks to micromechanics technology and to the LGI concept, this instrument could have been made
compact enough to be portable and, because of the principle, easily upgradeable to any much larger
wavelength ranges. The limitation in wavelength range is not due to the concept, but due to the
photodetector that is used. In the standard model the detection of the interferogram is carried with one
single InGaAs photodiode. A single photodiode instead of a CCD line leads to lower noise and costeffective detection solutions, particularly in the near-IR. In addition, the choice of available detectors
is much larger than CCD and it is therefore easier to dedicate a detector to specific needs. There is no
risk of defective pixels as it is generally the case for conventional NIR spectrometers using arrays of
photodiodes.
As a result, this instrument is unrivaled and perfectly suited for detection in transmission like
measurement of gases and liquids. In particular, the absorption signatures of gases are measured with
high accuracy. The instrument is capable of recording 2 spectra per second but needs more time for
processing so that an effective measurement time results that might be larger.
The spectrometer provides a number of important benefits including the following:
Laser controlled interferometer
Choice of resolution
Different amplification levels
Data acquisition in 500 ms with an effective measurement time of 5 s
A minimum power requirement - The spectrometer is driven by a standard USB 2.0 port
of a personal computer.
The performance is unaffected by stray light
The system is compact and lightweight.
The spectrometer is typically employed as a part of a system that includes a source and a sample
holder (a cuvette holder or a reflectance sphere). As an example, the spectrometer can be used with
the Tungsten Halogen Light Source and the Holder for 1-cm cuvettes. The source and cuvette holder
or reflectance sphere are acquired separately. As an alternative, the spectrometer can be directly
connected to the source to obtain the spectrum provided by the source).
The ARCoptix Near-Infrared Spectrometer can be used in a broad range of applications including
Portable Field Measurements
Laboratory Analyses
Industrial Process Control
Product Description
The ARCoptix ANIR spectrometer is a lamellar grating spectrometer that combines the advantages of
Fourier Spectroscopy with micromechanics technology. The first gives exciting optical features while
the second leads to miniaturization and reliable operation. A lamellar grating interferometer is a
grating that operates in the zeroth order. This particular type of apparatus was invented by Strong [J.
Strong, and G. A. Vanasse, “Lamellar grating far-infrared interferometer”, J. Opt. Soc. Am. 50, 113118 (1960). A scheme of the principle is illustrated in the Fig. 1.2 below.
2 ARC-000000-000-02-0310
1: Introduction
Figure 1-2
Figure 1- 2 shows the principle of operation of a LGI. Incoming light is reflected back by a series of
fixed and mobile mirrors acting as a grating and generating a diffraction pattern. To obtain the
interferogram one records the modulation of the zero order in function of the motion of the mobile
mirrors. The path difference (or depth of the grating)
x is an important parameter and given by the
distance between the fixed and the mobile mirrors.
Contrary to the Michelson interferometer that splits wave amplitudes at the beamsplitter, the lamellar
grating interferometer divides the wavefront. At the grating, the wavefront is divided such that one
half of the beam is reflected from the front facets (fixed mirrors in Fig. 1 - 2) and one half from the
back facets (mobile mirrors in Fig. 1 - 2). The distance between the two series of mirrors determines
the optical path difference (OPD)
x between the two parts of the wave. The enormous advantage of
this configuration, compared with a Michelson interferometer, is the absence of a beamsplitter.
Indeed, any additional micro-optical component is a limitation in the particular case of micro-sized
spectrometers. In general, this type of spectrometer is used for wavelengths larger than 100
m;
below, the tolerances are too tight for most machine shops.
The ARCoptix ANIR (Near Infrared) Fiber Optic Fourier Transform Spectrometer connects to a
notebook or desktop PC via a USB 2.0 port. It does not require an external power supply. The
ARCoptix ANIR and the electronics share a single housing.
The ARCoptix ANIR can connect via the USB 2.0 port to any PC that uses a Windows XP/Vista
operating system and has spectrometer operating software installed and configured for use with your
ARCoptix ANIR.
An EEPROM memory chip in each ARCoptix ANIR spectrometer contains calibration coefficients,
coefficients, and the serial number unique to each spectrometer. ARCoptix spectrometer operating
software reads these values from the spectrometer.
The ARCoptix ANIR has two input connectors:
FSMA receptacle that accepts a fiber optic cable with a standard SMA-905 connector
USB port that connects to a USB host via a standard USB cable
ARC-00000-000-02-0310 3
1: Introduction
Models Available
The following ARCoptix ANIR spectrometer models are available form Ocean Optics:
ANIR 0.9-1.7ANIR 0.9-2.6ANIR 2.0-4.5
Spectral Range900-1700 nm900-26002000-4500
Signal to Noise>1:1000>1:1000>1:1000
Detector TypeInGaAsInGaAsMCT
Items Included with Shipment
Important information and documentation accompany your ARCoptix NIR spectrometer shipment.
This includes:
Packing List – The packing list is located inside a plastic bag attached to the outside of the
shipment box (the invoice is mailed separately). The items listed on the packing slip include
all of the components in the order. The packing list also includes important information, such
as the shipping and billing addresses, as well as any components on back order.
Software CD – Each spectrometer order comes with the Software & Technical Resources CD.
This disc contains Ocean Optics software and manuals for software operation, spectrometers,
and spectroscopic accessories. Documentation is provided in Portable Document Format
(PDF). You need Adobe Acrobat Reader version 6.0 or higher to view these files.
4 ARC-000000-000-02-0310
Chapter 2
Installing the Spectrometer
Overview
You must install the SpectraSuite spectrometer operating software application prior to connecting the
ARCoptix ANIR spectrometer to the PC. The ARCoptix spectrometer operating software installs the
drivers required for Windows to communicate with the ARCoptix ANIR. If you do not install the
software first, the system will not properly recognize the ARCoptix ANIR.
If you have already connected the ANIR Spectrometer to the PC prior to installing the software,
consult Chapter 4:
Follow the steps in this section to interface the ARCoptix ANIR Spectrometer via the USB port to a
desktop or notebook PC.
To connect the ANIR Spectrometer to a PC via the USB port, the PC must be running the XP/Vista
operating system.
package
.
Troubleshooting for information on correcting a corrupt installation.
You also must have administrator privileges in order to run the installation
Installation Overview
Spectrometer installation consists of the following main tasks:
► Procedure
1. Install SpectraSuite spectrometer operating software on the destination computer. See the
SpectraSuite Spectrometer Operating Software Installation and Operation Manual (refer to
Product-Related Documentation) for more information on installing SpectraSuite.
2. Install SpectraSuiteHub.msi on the destination computer. This is a bundled utilities Windows
service that provides access to the spectrometer. See
information.
3. Reboot the system.
4.
After installing all software files, connect the spectrometer to your computer using the USB
cable (USB-CBL-1) that came with the ANIR Spectrometer. See
more information.
Note
Windows XP users may encounter a Hardware Installation warning window regarding
Windows XP driver testing. Click the
an expected warning.
Continue Installation button at this screen, as this is
ARCoptix Software Installation for more
Hardware Installation for
ARC-00000-000-02-0310 5
2: Installing the Spectrometer
ARCoptix Software Installation
The ARCoptix spectrometer can only be controlled via ARCoptix’s proprietary driver. Thus, a
compatibility layer (SpectraSuiteHub.msi) is necessary to allow SpectraSuite communicate with this
driver.
You can install the SpectraSuite-Hub on any 32-bit Windows computer. Typically you will install it
on the same computer on which SpectraSuite was installed, but this is not a requirement. If you
choose to install the SpectraSuite-Hub on a remote computer (any computer other than the one on
which SpectraSuite was installed), you must modify the Windows firewall settings. See
Windows Firewall Settings for more information.
Installing SpectraSuite-Hub Software
The ARCoptix spectrometer requires version 3.0, or later, of the Microsoft .NET framework. On some
systems, it may be necessary to install this version.
.NET Framework 3.0
If your PC does not have the required version of the .NET framework, the SpectraSuite-Hub
installer will detect this and remind you to install the .NET framework before proceeding:
Modifying
To install the required version of the .NET framework, click OK on this prompt or doubleclick on the dotnetfx3setup.exe installer utility in the directory containing the SpectraSuiteHub installer. Follow the on-screen prompts. This file is also available from Microsoft
here.
► Procedure
1. Run the SpectraSuiteHub.msi software installer (located on your Ocean Optics Software &
Technical Resources CD and also available on our website at
http://www.oceanoptics.com/technical/softwaredownloads.asp as SpectraSuite/ARCoptix
Driver Installer).
2. The installer will verify if your system has a version of the .Net Framework already installed.
If so, you will see the first setup wizard screen. Click
the note above.
6 ARC-000000-000-02-0310
Next. If not, follow the instructions in
3. Follow the prompts for the SpectraSuiteHub Setup Wizard.
2: Installing the Spectrometer
4. When requested by the wizard, connect the spectrometer to the computer’s USB port using
the supplied USB cable. See
Hardware Installation for more information.
5. Click Finish on the SpectraSuiteHub Setup Wizard.
6. The ARCspectro ANIR Setup Wizard appears.
Note
If the ARCspectro ANIR Setup Wizard does not appear automatically, go to C:\Program
Files\Ocean Optics\SpectraSuiteHub and double click on the file ARCspectro ANIR 1.5b
Installation Package.exe. Then follow the on-screen instructions.
ARC-00000-000-02-0310 7
2: Installing the Spectrometer
7. The Select Installation Folder screen appears. Choose the installation directory and press
Next.
8. Verify the information and press Next to start the installation.
8 ARC-000000-000-02-0310
9. The installer will install the necessary files for the software.
2: Installing the Spectrometer
ARC-00000-000-02-0310 9
2: Installing the Spectrometer
10. The device drivers installation will then start automatically. Disconnect the spectrometer if is
connected to the computer and press
OK.
11. When Window’s Device Driver Installation Wizard window appears, press the Next Button.
12. If the installer informs you that the drivers have not passed the Windows logo, please ignore
the message and press
Continue Anyway.
10 ARC-000000-000-02-0310
13. When the drivers are installed, press Finish.
2: Installing the Spectrometer
14. This completes the installation of the Arcspectro ANIR. Press Close to connect the
Instrument.
ARC-00000-000-02-0310 11
2: Installing the Spectrometer
15. Now you need to connect the device to your USB 2.0 port. The following window will appear
automatically. Select “
Install the software automatically (Recommended)” and press the
Next button.
16. If the installer informs you that the drivers have not passed the Windows logo, please ignore
the message and press
Continue Anyway.
12 ARC-000000-000-02-0310
17. The device is now ready to be used. Press Finish.
2: Installing the Spectrometer
Modifying Windows Firewall Settings
If you installed the SpectraSuite-Hub on a remote computer (i.e., any computer other than the one on
which SpectraSuite was installed), Windows Firewall settings must be modified to allow SpectraSuite
to access the SpectraSuite-Hub. Normally the install script will do this automatically. However, if the
script is unable to do this, you must manually add the SpectraSuiteHub program to the list of the
firewall’s exceptions.
► Procedure
To modify firewall setting on a Windows Vista computer,
1. Open the Windows Control Panel.
2. Click on the Windows Firewall icon (classic view) or select Security
OK until the Windows Firewall dialog box(es) are all dismissed.
| Windows Firewall.
Configuring the ANIR Spectrometer
The ARCoptix ANIR spectrometer has to be used with the included software when connected to the
USB port. There is no particular configuration process. The calibration is included in the software and
cannot be changed.
ARC-00000-000-02-0310 13
2: Installing the Spectrometer
Hardware Installation
Before use the spectrometer must be installed in a measurement setup with the other devices. In
addition to the spectrometer (connected to a computer running SpectraSuite) you need the following
components:
The figure below shows a typical transmission set-up. Yours may differ depending on what you are
measuring and the type of measurement being taken.
14 ARC-000000-000-02-0310
Chapter 3
Using the Spectrometer
Overview
Once you have installed the proper software and connected the spectrometer to the desired hardware,
you are ready to take measurements. This chapter provides information on running the SpectraSuiteHub service and starting SpectraSuite when using an ARCoptix ANIR spectrometer. SpectraSuite
functions specific to the ARCoptix ANIR spectrometer are also discussed. However, general
SpectraSuite operation is covered in the main
Installation and Operation Manual
(see Product-Related Documentation).
Starting the SpectraSuite-Hub Service
The SpectraSuite-Hub service must be running before SpectraSuite can access the ARCoptix ANIR
spectrometer. Normally, this service is started automatically when you boot your Windows system.
However, if it is necessary to manually start or stop the SpectraSuite-Hub service, use the
SpectraSuite-Hub Service Controller utility to do this.
SpectraSuite Spectrometer Operating Software
ARC-00000-000-02-0310 15
3: Using the Spectrometer
If you are running on Vista, read the section below on how to start the Controller utility. Otherwise, to
start this utility, double-click on the desktop icon labeled
an item in the Start Menu within the SpectraSuiteHub folder labeled
SpectraSuiteHubLocator.exe
You can click the “Check Status” button to verify that the SpectraSuite-Hub has been installed and is
started.
Hub.
It also displays the IP address and port number currently used by the SpectraSuite-
You will need this IP address and port number later on when you run SpectraSuite.
.
SpectraSuite Hub Controller. There is also
Shortcut to
Use the
Start Service and Stop Service buttons to start and stop the SpectraSuite-Hub service.
Starting the SpectraSuite-Hub Controller Utility on Vista
When starting the SpectraSuite-Hub Controller task, you must run it with Administrator privileges. If
you do not have the required permissions, you will see the following error message:
“
System.InvalidOperationException: Cannot open SpectraSuiteHub service on computer ‘.’ -->
System.ComponentModel.Win32Exception: Access is denied
To run the SpectraSuite-Hub Controller with Administrator privileges, right-click on the shortcut icon
Start Menu item for the Controller and choose Run as administrator. The User Account
or the
Control pop-up window may appear requesting permission to run this task. Respond by clicking
Allow.
”.
Note
If you only wish to check the status of the SpectraSuite-Hub service, you do not need to run
the SpectraSuite-Hub-Controller task with Administrator privileges. Administrator privileges
are only necessary if you intend to start or stop the SpectraSuite-Hub service.
Using SpectraSuite
Once you have installed the SpectraSuite-Hub service, ensured it is in the “started” state, and plugged
in the ARCoptix ANIR spectrometer to the computer running SpectraSuite, you can control the
spectrometer and view spectra using the SpectraSuite application.
► Procedure
1. Start SpectraSuite.
2. From the menu, select
3. Click on the
16 ARC-000000-000-02-0310
ARCoptix spectrometer radio button. The following window appears:
Spectrometer | Network Spectrometer.
4: Troubleshooting
4. Enter the IP address and port number of the ARCoptix ANIR spectrometer.
You can determine the IP address and port number by running the SpectraSuite-Hub
Controller utility on the computer attached to the ARCoptix ANIR spectrometer. See
the SpectraSuite-Hub Controller Utility on Vista for information on how to obtain these
numbers. When finished, click
Next.
Starting
ARC-00000-000-02-0310 17
3: Using the Spectrometer
5. Highlight the serial number of the spectrometer you wish to view. Then, click Next.
6. Click
7. Right-click on the ARCoptix ANIR icon and choose
Finish. The icon for the ARCoptix ANIR spectrometer now appears in the Data
Sources
pane.
Spectrum Graph.
Note
The ARCoptix ANIR spectrometer requires several seconds to acquire each spectrum.
Gain Setting
The ARCoptix ANIR spectrometer does not use an integration time setting to control its operation.
However, the spectrometer does have a unique setting called Gain you can use to accomplish a similar
purpose. Scans-to-average and boxcar averaging are supported by the ANIR.
You can set the gain to one of four values: low, medium, high, and extreme.
► Procedure
To set the gain on your ARCoptix ANIR spectrometer:
1. Right-click on the ARCoptix ANIR icon and choose
2. Click on the
Gain tab.
Spectrometer Features.
3. After selecting the desired gain setting, be sure to click
Update Now.
Shutting Down
When you shut down SpectraSuite, it is not necessary to shut down the SpectraSuite-Hub service.
The service will remain idle in the background waiting for SpectraSuite to restart.
18 ARC-000000-000-02-0310
Chapter 4
Troubleshooting
Overview
The ARCoptix ANIR Spectrometer is an instrument that is designed for use in a laboratory or field
application with a minimum amount of maintenance. Since it is normally used with a source and
cuvette holder, we describe the maintenance and troubleshooting with respect to the entire system.
The user should refer to the documentation provided with the integrating sphere or source and sample
holder, as it is very possible that the problem is in one of these components, rather than the
spectrometer.
Maintenance
The ARCoptix ANIR requires a minimum amount of maintenance. If necessary, the unit can be wiped
clean with a damp cloth. The lamp in the source should be replaced on a periodic basis as described in
the documentation provided with the source. Typically, the lamp life is 1000-2000 hours, but this time
is dependent on the lamp and the degree of noise that can be tolerated in the spectrum.
Caution
There are no user-replaceable parts inside the spectrometer. Do not take it apart.
Troubleshooting Tips
Since the ARCoptix ANIR spectrometer is employed in a system that includes a source and a sample
holder or integrating sphere, all troubleshooting activities should include all components of the
system. Troubleshooting can be simplified with following guidelines:
In almost all cases, there is a single cause for the problem. As an example, a noisy spectrum can be
due to one or more of the following causes:
The lamp is weak.
The fiber optic cable does not make good contact with the spectrometer or the sample holder.
There is an internal defect in the spectrometer.
A fundamental knowledge of the role of each component in the system is extremely useful in
diagnosing the problem. It is also helpful to have spare components on hand to substitute for those in
the system.
If any aspect of the analytical conditions is to be changed, run a “before and after” test to
verify that the effect of the change is well understood. Do not consider any change as trivial.
ARC-00000-000-02-0310 19
4: Troubleshooting
As an example, if you change the supplier of a solvent, verify that the change has no effect on
the analysis.
Run a standard (or a series of standards) on a periodic basis to verify that the system is
performing properly. When abnormal data is obtained, collect the spectrum of a standard and
compare the spectrum to one that was previously obtained.
If an error message is presented, press the Continue button indicated on the Error Message
dialog box. If this does not remedy the problem, turn off the spectrometer, disconnect the
USB cable and then reinstall the cable.
The following SpectraSuite error message can be caused by the Windows firewall, which
blocks applications from communicating over the Internet. If this is the cause, follow the steps
given in the
you have entered the wrong IP address or port number (see
Service).
Modifying Windows Firewall Settings section. This error may also occur because
Starting the SpectraSuite-Hub
Spectrum is Noisy
Possible CauseCommentSuggested Solution
Lamp is weakThe lamp has a finite
lifetime
The absorbance is weak or
% T is very high (noisy
spectrum)
The absorbance is too
strong
Cable is looseCheck all cables for good contact
Fiber optic cable is
defective
Transient internal
spectrometer fault
Defect in SpectrometerContact Ocean Optics
The sample is too dilute or
too thin
The sample is too
concentrated or thick
Replace the lamp
Prepare a more concentrated
sample
Use Spectrum Averaging to reduce
noise
Dilute the sample or reduce its
thickness
Replace fiber optic cable
Remove USB cable and re-insert
20 ARC-000000-000-02-0310
No Signal
Possible CauseCommentSuggested Solution
USB cable is looseCheck cables for good contact
Light not onCheck light
Sample not appropriateUse a different sample
4: Troubleshooting
Transient internal
spectrometer fault
Defect in SpectrometerContact Ocean Optics
Remove USB cable and re-insert
Signal Intensity is Not Constant
Possible CauseCommentSuggested Solution
Fiber optic cable has shifted
in position
Lamp is not stableDefective lampReplace the lamp
Sample is not
homogeneous (cuvette)
Sample is not
homogeneous (integrating
sphere)
Sample is decomposingReplace sample
Cuvette is scratchedAlways place cuvette in
sample holder with same
plane facing the source
Tape fiber optic cable to bench
Mix sample and filter if necessary to
remove particulate matter
Move integrating sphere to a
different region of the sample
Replace cuvette
Defect in SpectrometerContact Ocean Optics
Peak Wavelength Has Shifted
CauseCommentSolution
The background spectrum
is not valid
Sample is not
homogeneous
Defect in SpectrometerContact Ocean Optics
ARC-00000-000-02-0310 21
Run a new background spectrum
Find another region of the sample
4: Troubleshooting
22 ARC-000000-000-02-0310
Appendix A
How the ARCoptix ANIR Works
Overview
The ARCoptix ANIR is a miniaturized Fourier Transform Spectrometer (FTS). It is based on the
principle named “Lamellar Grating Interferometer” (LGI). The active part of the LGI is driven by a
micrommechanical System. A Fourier Transform Spectrometer (FTS) has distinct advantages
compared to grating spectrometer in terms of throughput and Signal-to-Noise Ratio (SNR).
The principle of the LGI was invented by Strong [J. Strong, and G. A. Vanasse, “Lamellar grating farinfrared interferometer”, J. Opt. Soc. Am. 50, 113-118 (1960). The implementation of the LGI using
the emerging technology of micro-machining is unique.
Principle of Operation
An FTS splits the in-coming light in two beams, which are then recombined after having been shifted
in phase. The output modulation of the light is recorded as a function of time and called
interferogram. The interferogram contains all information about the spectra but contrary to grating
spectrometers the information is encoded via a Fourier transform. To obtain the spectra the recorded
data have to be Fourier transformed.
The particularity of the instrument developed by ARCoptix consists in using the so-called Lamellar
Grating Interferometer (LGI) configuration to produce the interferogram. Instead of using the
conventional Michelson interferometer (more precisely, the Twyman-Green interferometer) where
two mirrors and a beam splitter are used, the LGI consists of a series of mirrors that from a grating as
shown in Fig. A - 1.
Figure A- 1. The principle of operation of an LGI
ARC-00000-000-02-0310 23
A: How the ARCoptix ANIR Works
Figure A-1 shows incoming light is reflected back by a series of fixed and mobile mirrors acting as a
grating and generating a diffraction pattern. To obtain the interferogram one records the modulation of
the zero order in function of the motion of the mobile mirrors. The path difference (or depth of the
grating)
x is an important parameter and given by the distance between the fixed and the mobile
mirrors.
While in the Michelson interferometer one mirror changes its position, in the lamellar grating
interferometer a series of mirrors move. The configuration does not need a beam splitter. The LGI
splits the wavefront at the mirrors, contrary to the Michelson interferometer that splits the wave
amplitude at the beamsplitter. The whole arrangement of mirrors performs like a grating having a
variable depth. The interferogram is recorded by measuring the modulation of the zero order, reflected
back by the grating, as a function of the depth of the grating. Note that there is no dispersion in the
zero order. Exactly like in a conventional Michelson interferometer, the important notion, here, is the
phase delay generating at the grating, which is the double of the distance between the fixed series of
mirrors and the mobile ones. Figure A - 2 shows the resultant diffraction patterns for selected
positions of the movable mirror grating.
Figure A - 2.
The depth of the grating x determines the resulting efficiencies in the different diffraction orders. For
x = 0 the grating acts like a simple mirror while for x = /4 no light is found in the zero order. The
effect is wavelengths depended. For each wavelengths this conditions is realized for a different
The zero order intensity A for a single wavelength
2
cosxAA
00
24 ARC-000000-000-02-0310
0
0can be written as a function of x and becomes:
Eq. A - 1
x.
A: How the ARCoptix ANIR Works
The intensity is thus modulated and changes with a cosine function of the grating depths x. The
period is given by the wavelengths. If the lamellar grating is illuminated with a source containing
several wavelengths of intensities A
), then the interferogram is the integral over all wavelengths .
(
2
cos)(
The recorded intensity I(
A(
) that can be extracted by using a Fourier transform.
It is useful to define the contrast (or visibility) as follows:
C(
x) = I
max
An important measurement point is the zero path difference (
positions and the grating acts as a simple mirror. At this point, all intensity values A(
since the cosine term is maximum for all wavelengths. At the zero path difference, the contrast is
maximum and equal to unity. If
smaller the contrast. On the other hand, the narrower the spectrum (e.g. monochromatic light source),
the higher the contrast.
x) contains information about the spectral composition of the incoming light
(x) – I
(x) / I
min
dxAxI
(x) + I
max
x is non-zero, then the broader the spectrum of the source, the
Eq. A - 2
(x) Eq. A - 3
min
x = 0) when all mirrors are at the same
) are added
Reference Laser
The ARCoptix NIR contains a reference laser to precisely control the position of the movable parts in
the interferometer. The reference laser operates at about 635 nm and its spectra can be measured
depended on the light level in the measurement channel. To check the operation of the reference laser
choose the
EXTREME detection gain and choose the spectral range in the graphing options.
Resolution
In Fourier spectroscopy, resolution is depending of the maximum optical path difference (i.e., phase
delay) that you can achieve with the interferometer. The longer the scanning range the higher the
resolution. Strictly speaking, the smallest spectral interval that can be discerned is defined as:
1
x
max
Resolution is usually defined as the smallest spectral interval multiplied by the truncation effect of a
boxcar. This corresponds to the full width half maximum of a monochromatic radiation. If no
apodization is used, resolution is about 1.2*
1.7*
.
and if a triangle apodization is used, then resolution is
Eq. A - 4
Detector Nonlinearity
If the detector response does not increase linearly with the illumination intensity the measured
interferogram will be distorted. Every detector (or analogue/digital converter) shows some nonlinearity, especially when approaching the saturation level or the detection limit of the detector.
However, if detectors are used in useful range below saturation very good linearity is obtained and
distortions are negligible. This has to be respected when the gain level is chosen. To high gain will
increase effects of nonlinearity.
ARC-00000-000-02-0310 25
A: How the ARCoptix ANIR Works
Noise
The last aspect treated in this chapter is related to the effect of noise in Fourier transform
spectroscopy. The interferogram signal is always accompanied by statistical errors and we want to
know their effect on the spectrum. Several types of noise and their origins will be presented in this
section.
Signal-to-noise ratio
We define the Signal-to-Noise ratio (SNR) of a set of measurements as the ratio between the mean
value of the signals and their standard deviation.
Types of Noise
In spectroscopy, we usually distinguish between additive noise and multiplicative noise. The first one
is the noise added to the signal; the latter varies with the signal power. Previously, we have mentioned
the multiplex advantage of an interferometer over a dispersive spectrometer (Fellgett advantage). This
advantage occurs only for additive noise.
Additive Noise
Thermal noise (or Johnson noise) arises from thermal fluctuations of the current in the detector and is
independent of the signal level. In the infrared region, photon energies are smaller than these thermal
fluctuations and, therefore, detectors will mainly be limited by thermal noise.
In addition, we mention the dark-current noise, which is an additive noise as well. Photodetection
devices also generate dark-current noise, which is present even in the absence of light and results from
random electron-hole pairs generated thermally or by tunneling.
Multiplicative Noise
Photon noise (or quantum noise, shot noise) is associated to the electromagnetic radiation itself and is
a fundamental quantity. It refers to the fluctuations resulting from the random arrival of photons at the
detector. The standard deviation of these fluctuations is proportional to the square root of the number
of photons arriving. Therefore, the noise power is proportional to the square root of the signal power.
Photon noise is a multiplicative noise. In the near-infrared and visible region, very sensitive detectors
(e.g. photodiodes) are available, which allow to approach photon-noise-limited detection. In this case,
there is no multiplex advantage of the FTS over a dispersive instrument (note that the interferometer
still enjoys the luminosity or Etendue advantage).
26 ARC-000000-000-02-0310
SpecificationValue
Appendix B
Specifications
Resolution:
500nm
1000 nm
1700 nm
2600 nm
Wavelengths accuracy<0.5 nm
A/D converter24 bit
Fiber optical connectorSMA 905
Optical fiber entrance0.6 mm (Fiber core diameter)