Princeton Webcam 4411 0143 User Manual

so lane  
Manual  
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Copyright 2012-2013  
Princeton Instruments, a division of Roper Scientific, Inc.  
3660 Quakerbridge Rd  
Trenton, NJ 08619  
TEL: 800-874-9789 / 609-587-9797  
FAX: 609-587-1970  
All rights reserved. No part of this publication may be reproduced by any means without the  
written permission of Princeton Instruments, a division of Roper Scientific, Inc. (“Princeton  
Instruments”).  
Printed in the United States of America.  
IntelliCal and SpectraSense are trademarks, and IsoPlane and LightField are registered  
trademarks of Roper Scientific, Inc.  
Windows and Windows Vista are registered trademarks of Microsoft Corporation in the United  
States and/or other countries.  
The information in this publication is believed to be accurate as of the publication release date.  
However, Princeton Instruments does not assume any responsibility for any consequences including  
any damages resulting from the use thereof. The information contained herein is subject to change  
without notice. Revision of this publication may be issued to incorporate such change.  
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Table of Contents  
Chapter 1 IsoPlane® SCT 320 Description ............................................7  
iii  
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IsoPlane® SCT 320 Manual  
Version 1.B  
Figures  
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Table of Contents  
v
Tables  
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IsoPlane® SCT 320 Manual  
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Chapter 1 IsoPlane® SCT 320 Description  
1.1 Introduction  
This manual is intended to help you set up and operate your new IsoPlane SCT 320  
spectrograph. Even if you are an experienced user of spectroscopic equipment, we suggest that  
you follow the manual (at least initially) to insure proper setup and operation. If you have any  
questions about the information contained in this manual, please feel free to contact the  
Princeton Instruments customer service department at [email protected] or  
800-874-9789 / 609-587-9797.  
1.2 IsoPlane SCT 320 Description  
The IsoPlane SCT 320 (IsoPlane) is a 320 mm focal length spectrograph. Its advanced optical  
design reduces astigmatism to zero, increasing spatial and spectral resolution dramatically over  
traditional spectrographs. Large-diameter optics and interchangeable triple-grating turrets permit  
operation from the UV to NIR with extremely low light levels at high, low or intermediate  
spectral resolution. IsoPlane includes 32-bit microprocessor controlled scanning, built-in USB  
and RS-232 interfaces, and a micrometer-controlled entrance slit. In addition, it has a direct  
digital grating scan mechanism with full wavelength and grating control capabilities. The  
IsoPlane works seamlessly with Princeton Instruments’ industry-leading CCD, EMCCD, ICCD  
and InGaAs array detectors and Princeton Instruments’ LightField® with IntelliCaland  
WinSpec data acquisition software packages.  
Figure 1-1. Light Path within the IsoPlane SCT 320  
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Chapter 2 IsoPlane Setup  
2.1 Unpacking and Inspecting  
Carefully unpack and examine the IsoPlane and any purchased accessories.  
Notes:  
1. Report any damage immediately to the carrier and to Princeton Instruments.  
2. Save all packing material.  
2.2 Initial Setup Procedure  
1. Position the IsoPlane where it will be used.  
2. Connect the power supply shipped with the IsoPlane to the POWER connector  
on the side of the IsoPlane. This power supply provides +5 volts DC for the  
control logic and +24 volts DC for the motor drives.  
3. With the power supply switch in the off position, connect the line cord provided with the  
IsoPlane to the power supply and the AC line. The power supply will operate with line  
voltages between 100 and 240 volts AC, 50/60 Hz.  
4. The IsoPlane is designed to be controlled primarily through Princeton Instruments  
LightField or WinSpec data acquisition and control software when operated with a  
Princeton Instruments detector. Connect the USB port of the IsoPlane to the USB port on  
the control computer using the USB cable provided. RS-2332 may also be used if a USB  
port is not available.  
5. Install the grating turret that is shipped in the same shipping box with the IsoPlane but is  
packaged outside the IsoPlane housing to protect the gratings during shipment. See  
Section 2.7 Turret Installation (starting on page 12) for detailed installation instructions.  
6. Turn on the power switch on the IsoPlane power supply and the IsoPlane should initialize  
to zero wavelength. See the instructions in Chapter 3 for operation with Princeton  
Instruments software.  
2.2.1 Optional Software Packages  
The following software packages are some of the other software packages available for purchase  
from Princeton Instruments.  
2.2.1.1 LightField®  
The IsoPlane is supported by LightField® 4.2, a 64-bit data acquisition platform for spectroscopy  
and imaging. Light Field combines complete control over Princeton Instruments’ spectrographs  
and detectors with easy-to-use tools for experiment setup, data acquisition, and post-processing.  
2.2.1.2 WinSpec  
WinSpec is a 32-bit data acquisition platform that has been optimized specifically for digital  
spectroscopy. WinSpec provides complete control over the IsoPlane and all other Acton Series  
spectrometers. This software control extends to all instrument options, such as multiple gratings,  
multiple entrance and exit ports, and motorized slits.  
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2.2.1.3 SpectraSense™  
SpectraSense is a comprehensive spectral acquisition and data treatment package. It is designed  
to work exclusively with Princeton Instruments products and accessories including the  
SpectraHub Detector Interface. SpectraSense software will control and acquire data from both  
single channel detection systems, which require scanning of a monochromator, and CCD-based  
detection systems that may or may not require repositioning of a spectrograph.  
2.2.2 Controlling the IsoPlane at the Command Level  
Although it requires more programming on the user’s part, the IsoPlane can also be controlled  
with direct commands through its USB port or RS-232 port. This operation is described in  
2.3 Computer Interface Connectors: USB and RS-232  
Figure 2-1. Details of the RS-232, USB, and Power Connections on the IsoPlane  
2.3.1 Cables and Connections for IsoPlane  
The following computer cables are supplied with the IsoPlane:  
3650-USB-06 USB Cable Type A to Type B.  
CC-499-2 IBM AT or compatible 9-pin female (DB9S) connector to 9-pin male connector  
(DB9P).  
If neither of these cables is compatible with your system, consult Princeton Instruments for a  
custom cable. If you have facilities for constructing a custom cable, use the RS-232 pin  
Pin#  
Description  
1
Open  
2
3
4
5
6
7
8
9
RD data from IsoPlane to computer  
TD data from computer to IsoPlane  
open  
Ground  
Open  
RTS  
CTS  
open  
Table 2-1. RS-232 Computer Interface Pin Arrangement  
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2.3.2 Terminal or RS-232 Port Settings  
A terminal or RS-232 computer port must be set up as follows: 9600 baud, 8 data bits, no parity,  
1 start bit, 1 stop bit.  
2.4 Power Supply with Input Cable  
Figure 2-2. Power Supply  
Pin#  
Description  
1
+5V  
2
3
4
GND  
GND  
+24  
Table 2-2. IsoPlane Power Connector Pin Arrangement  
2.5 Internal Shutter  
The IsoPlane has an optional internal shutter. If the shutter is installed, it  
is located in the Turret Compartment and is mounted to the  
spectrograph wall. Its shutter cable plugs into a keyed 2-pin shutter  
connector in the floor of the IsoPlane. The external connector is  
below the detector mounting plate and can be connected via a shutter  
cable to a detector with a SHUTTER connector. If a detector does  
not have a SHUTTER connector (PI-MAX detectors, for example),  
the Princeton Instruments SHC-EXT Shutter Control Box can be  
used to control the opening and closing of the internal shutter. If the control box is not available,  
the internal shutter can be removed. Instructions for installing and removing the internal shutter  
assembly are provided in Sections 2.13.1 and 2.13.2, respectively.  
2.6 Mounting Accessories to an IsoPlane Slit Assembly  
All Princeton Instruments spectroscopy accessories come with their own set of instructions for  
proper mounting and operation. The instructions below are only general information. Please refer  
to the individual instructions for detailed information.  
Accessories: The full range of spectrograph accessories mount directly to the IsoPlane  
entrance slit assembly (manual or motorized). To assist you in mounting accessories, a drawing  
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IsoPlane® SCT 320 Manual  
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of the manual slit assembly has been provided in Appendix F. The general procedure for  
mounting an accessory to the slit is as follows:  
1. Place the accessory directly against the face of the slit body.  
2. Using four (4) 8-32 screws normally provided with the accessory, secure the accessory to  
the slit body.  
Light sources fitted with light collection/focusing optics are normally factory-aligned to the  
standard slit.  
Note: In some instances with light sources, there is limited access to the bottom two screw holes. In this  
case, Princeton Instruments provides special slotted holes in the light source housing to facilitate  
mounting the source to the slit.  
2.7 Turret Installation  
If you have just received an IsoPlane spectrograph, you will need to install the grating turret. The  
grating turret has been shipped in the same shipping box with the IsoPlane but is packaged in a  
plastic container outside the IsoPlane housing to protect the gratings during shipment.  
CAUTION  
1. The optical surfaces in the spectrograph are extremely delicate and can be permanently damaged by  
contact with solid objects as well as with most liquids and aerosols.  
2. DO NOT TOUCH optical surfaces with anything. Wear thin protective powderless gloves to  
minimize damage from body oils if you accidentally touch any optical surface, especially the grating.  
3. Avoid talking or sneezing near optical surfaces. Do not breathe directly on them.  
The following procedure is for the initial installation of a  
grating turret. Observe proper optical handling procedures.  
Note: See Section 2.15 Turret Interchange (starting on page 25) for  
instructions on changing from one turret assembly to another.  
1. Locate the storage container with the grating turret to be  
installed.  
2. Become familiar with the components as labeled on  
Turret  
Compartment  
3. Using the 9/64” hex wrench, remove the four Turret  
Compartment cover screws and remove the cover. Become  
familiar with the grating turret and its components.  
4. Before removing the grating turret from the shipping  
container, use a 3/32” hex wrench to loosen the three set  
screws on the bottom of the container (about 1 turn).  
5. Then remove the cover from the shipping  
Figure 2-3. Turret Compartment  
container, grasp the Center Torque Screw and turn  
it counter-clockwise until the turret can be lifted straight up.  
6. Locate the hole near the edge between gratings on the grating turret assembly (see Figure 2-5).  
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SCT 320 Operation  
13  
7. Locate the vertical post on the Grating Spindle Assembly (see Figure 2-6).  
8. Position the grating turret on the grating spindle so the hole in the turret assembly aligns with  
the post in the turret assembly as shown in Figure 2-8.  
9. Make sure the turret is properly seated.  
10. Tighten the Center Torque Screw until it clicks. This sets the torque on the spindle correctly.  
Note: You cannot overtighten this screw. It is designed to slip once the correct torque is attained.  
11. Place the Turret Cover on the spectrograph. Replace and tighten all of the cover screws.  
12. Replace the plastic cover on the storage container and store it in a safe location.  
13. Plug the power supply into an outlet and connect the supply to the IsoPlane. Turn on the  
IsoPlane to allow for auto-identification of the grating turret. Note that if the power supply is  
on while a turret is being installed, the IsoPlane should always be re-started afterwards.  
Center Torque Screw  
Figure 2-4. Center Torque Screw  
Hole  
Figure 2-5. Location of Hole on Turret Grating Assembly  
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Post  
Figure 2-6. Location of Post on Grating Spindle Assembly  
Figure 2-7. Lower Turret into the Turret Compartment  
Aligned  
Hole and Post  
Figure 2-8. Turret Installed (Hole and Post Aligned)  
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Chapter 3  
SCT 320 Operation  
15  
2.8 Array Detector Mounting Instructions  
2.8.1 Introduction  
The standard mounting plate for CCDs, FPAs, and diode arrays accommodates detectors with a  
slotted flange or mounting holes aligned on a 3.60” bolt circle pattern. There are six (6) equally  
spaced #10-32 tapped holes on a 3.60” bolt circle designed to accept #10-32 hex head screws.  
Figure 2-9. Mounting Plate  
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2.8.2 Mounting an Array Detector to the IsoPlane  
The array detector mounting plate is mounted to the entrance port of the IsoPlane.  
1. Remove the shipping cover from the mounting plate.  
2. If the detector has a three-slotted flange (3.60” bolt circle):  
a. If the detector has a three-slotted flange, screw three  
#10-321/2 hex head bolts into the plate and leave 1/4" of  
thread exposed.  
b. Mount the detector to the plate and position the detector so the  
text on the back of the detector is right-reading (i.e., not upside-  
down). The exception to this orientation is the PI-MAX2:  
1024x256 which should be mounted with the text upside-down.  
c. Tighten down the bolts with a 5/16” open end wrench.  
3. If the detector is a PyLoN or SPEC-10 LN detector without shutter, you will need to  
remove the shroud at the front of the detector, mount the  
shroud to the plate, and then resecure the shroud to the  
detector. It may be easier to remove the mounting plate  
from the IsoPlane for this operation.  
a. Using a 3/32” ball head hex wrench, remove the 4  
socket head screws that secure the shroud to the nose of the  
detector.  
b. Carefully slide the shroud off.  
c. Remove the mounting plate from the IsoPlane.  
d. Place the front of the shroud against the front of the plate and orient the nose until the  
appropriate hole pattern matches the mounting holes on the plate.  
e. From the inside of the shroud screw three 10-32 x 1/4”, flat head stainless steel  
screws through the shroud and into the mounting plate.  
f. Carefully mount the shroud and plate assembly onto the front of the detector and  
resecure the shroud with the previously removed 4 socket head screws.  
g. Re-mount the plate to the IsoPlane. The detector should be upright.  
Note: Refer to the detector’s system manual for specific instructions on how to mount the array  
detector to the mounting plate. These instructions vary with the detector nose design.  
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SCT 320 Operation  
17  
2.8.3 Rotational Alignment  
This general procedure assumes that you have already mounted the array detector to the exit port  
of the spectrograph and that there is a light source at the entrance port. The basic actions are  
listed below. Refer to Chapter 3 of this manual for detailed LightField and WinSpec instructions  
for performing this function. For other application software, refer to that software’s manual or  
help file.  
1. Make sure the computer interface cables (for the spectrograph and detector) are  
connected.  
2. Verify that the power supplies are plugged into an AC source and are connected to the  
spectrograph and detector.  
3. Turn on the power to the spectrograph and the detector.  
4. Start the application software.  
5. Loosen the rotation adjustment screws (see Figure 2-9) enough that you can rotate the  
detector. The mounting plate holes are slotted to allow about 4° of rotational positioning.  
6. If background subtraction is an available function, acquire a background to be applied  
while data are acquired.  
7. Turn on the light source and begin continuous data acquisition.  
8. While viewing the data being acquired, rotate the detector until you obtain the sharpest  
peaks or, if in imaging mode, the spectral lines are perpendicular in the image.  
9. Tighten the mounting screws.  
10. Confirm that the data still show sharp peaks or perpendicular spectral lines.  
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2.8.4 Focusing the Spectrometer  
The basic actions for focusing the spectrometer  
are listed below. This general procedure  
assumes that you have already mounted the  
array detector to the exit port of the  
spectrograph and that there is a light source at  
the entrance port. Refer to Chapter 3 of this  
manual for detailed LightField and WinSpec  
instructions for performing this function. For  
other application software, refer to that  
software’s manual or help file.  
Micrometer Compartment  
1. Using a 9/64” hex wrench, unscrew the four  
screws that secure the Micrometer  
Compartment cover (see Figure 2-10).  
2. Set the screws aside.  
3. Remove the Micrometer Compartment  
cover and set it aside.  
Figure 2-10. Micrometer Compartment Location  
4. Using a 5/64” hex wrench, loosen the locking set screw shown in Figure 2-11.  
5. While continuously acquiring data from a spectral line source, adjust the micrometer  
until the half width of the peak is at a minimum. Note that as focus is improved, the  
intensity of the spectral line will increase. It is important to adjust the acquisition time to  
keep the entire spectral line on scale.  
6. Tighten down the locking set screw.  
7. Place the Micrometer Compartment cover on the spectrograph. Replace and tighten all of  
the cover screws.  
Locking Set Screw  
Figure 2-11. Micrometer Locking Set Screw  
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Chapter 3  
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19  
2.8.5 Height Adjustment of Image Plane  
Note: This procedure should only be attempted by someone experienced in  
aligning optical components and assemblies.  
2.8.5.1 Overview  
During the manufacturing process, the IsoPlane focal plane is  
factory-aligned so that it is precisely centered on the optical  
axis. However, in some instances when a CCD camera is  
attached, the center pixel of the CCD camera may be located  
slightly above or below the optical axis of the spectrograph.  
In most applications this is not critical: however, if it is  
important to have the exit focal plane image precisely  
centered on the CCD, the height of the exit beam can be  
adjusted using the procedure in this section.  
Set Screw  
Cap Screw  
If you have an optical fiber and fiber adapter that can  
precisely center the beam at the center of the IsoPlane  
focal plane, then that can be used as a guide in positioning  
the exit focal plane. If the IsoPlane is equipped with a  
Figure 2-12. Height Adjustment Screws  
standard 3 mm manual entrance slit or optional 3 mm  
motorized entrance slit, you can also install the supplied 4 mm high slit baffle and use the 4mm  
high image as a guide in positioning the exit focal plane. The adjustment is made by adjusting  
the pair of push-pull vertical alignment screws as shown in Figure 2-12.  
2.8.5.2 Data Acquisition Mode  
During this adjustment procedure, the detector should be running in continuous mode so an image of  
the source is displayed in the acquisition software. Continuous operation is necessary to provide  
active feedback of the light source position as adjustments are being made. We recommend using a  
mercury lamp with a center wavelength of 546.075 nm however other light sources and center  
wavelengths can be used.  
2.8.5.3 Required Tools  
5/32” hex wrench  
3/32” hex wrench  
2.8.5.4 Adjustment Procedure  
1. Remove the Micrometer Compartment cover (Figure 2-10) to access the height adjustment  
2. Determine if the image is HIGH or LOW on the detector array.  
a. If the image is HIGH, alternately loosen the Cap Screw and tighten the Set Screw until  
the image is centered about the center row of the camera.  
Notes:  
1. CAUTION: ONLY ADJUST THE CAP AND SET SCREWS INDICATED IN Figure 2-12.  
ADJUSTMENTS TO OTHER SCREWS MAY RESULT IN SEVERE MISALIGNMENT OF  
THE INSTRUMENT.  
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2. Adjustments to the Cap and Set Screws should be small, approximately 1/8th-turn or less.  
3. If the Cap Screw is adjusted 1/8th-turn in a counter-clockwise direction, then the Set Screw should  
be adjusted 1/8th-turn in a clockwise direction.  
4. If the initial adjustment does not move the image far enough on the CCD, repeat the adjustments  
to the Cap and Set Screws as stated in Notes a.2 and a.3 above.  
5. Several small adjustments are recommended.  
6. At the end of the procedure the Cap and Set Screws should be tight.  
b. If the image is LOW, alternately loosen the Set Screw and tighten Cap Screw until the  
image is centered.  
Notes:  
1. CAUTION: ONLY ADJUST THE SET AND CAP SCREWS AS INDICATED IN Figure 2-12.  
ADJUSTMENTS TO OTHER SCREWS MAY RESULT IN SEVERE MISALIGNMENT OF  
THE INSTRUMENT.  
2. Adjustments to the Set and Cap Screws should be small, approximately 1/8th-turn or less.  
3. If the Set Screw is adjusted 1/8th-turn in a counter-clockwise direction, then the Cap Screw  
should be adjusted 1/8th-turn in a clockwise direction.  
4. If the initial adjustment does not move the image far enough on the CCD, repeat the adjustments  
to the Set and Cap Screws as stated in Notes b.2 and b.3 above.  
5. Several small adjustments are recommended.  
6. At the end of the procedure the Set and Cap Screws should be tight.  
2.9 Single Point Detector Mounting Instructions  
Single point detectors (such as the PD-438) mount directly to  
the optional exit slit with mounting plate assembly of the  
IsoPlane monochromator. Because the outcoming beam path  
exits from the focusing mirror at 15 degrees to the housing, the  
slit assembly is secured to a tapered mounting plate at the  
exit port.  
1. Position the detector so its labels are upright (the  
optical axis is not vertically centered).  
2. Mount the detector directly to the exit slit assembly  
(already mounted to the tapered mounting plate at the  
exit port) so its four mounting holes align correctly  
with the tapped mounting holes of the slit assembly.  
3. Insert the four 8-32 mounting screws and use a 9/64”  
hex wrench to tighten the screws.  
4. The detector should now be mounted correctly.  
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Chapter 3  
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21  
2.10 Spectrometer Calibration  
Refer to the application software manual or the software help for information on calibrating the  
data pixels with wavelengths.  
2.11 Slit Width Adjustments in the Model 716-1 Manual Bilateral  
Slit and the 716-MS Kinematic Slit  
The slit width of each bilateral slit assembly (716 type) is adjustable from 0.010 millimeters to  
3 millimeters (10 to 3,000 µm) by a micrometer knob located on the top of the slit housing. The  
micrometer knob is graduated in 0.010 millimeter (10 µm) increments.  
Each clockwise revolution of the micrometer knob increases the slit width 0.25 millimeters  
(250 µm). For maximum reproducibility, the slit width should be set in a clockwise direction  
(increasing slit widths) each time it is changed. Refer to the drawing below.  
The micrometer knob should not be rotated below a reading of 0.00 or above 3.00. A micrometer  
setting of less than 0.010 millimeters (10 µm) should not be used, because a stop is provided to  
prevent the slit jaws from contacting each other.  
Note: Damage May Be Done If Slit Jaws Are Opened Wider Than 3.0 mm.  
Slit Width Micrometer Settings  
Slit Width Adjustable from  
10 Micrometers to 3000 Micrometers (3 mm)  
Figure 2-13. Slit Width Setting:  
200 Micrometers (0.200 mm)  
Figure 2-14. Slit Width Setting:  
1380 Micrometers (1.38 mm)  
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2.12 Slit Width Adjustments in the Model 718-1 Motorized 3mm Slit  
The Model 718-1 motorized slit assembly is a self-calibrating, 10 µm to 3 mm  
adjustable bilateral slit. Stepping-motor-controlled adjustments are made in 1 µm  
increments over the full range. The Model 718-12 motorized slit assembly is a  
self calibrating, 10 µm to 12mm adjustable bilateral slit. Stepping-motor  
controlled adjustments are made in 5 µm increments over the full range.  
Full control of the slit, including automated bandpass setting, is integrated  
into LightField® and SpectraSense™ software. The slit motor is only  
energized when you send the command via the software to control it. When  
the power to a spectrograph is turned off, the slit remains in the position to  
which it was last set. This position is stored in nonvolatile memory allowing slit position to be  
maintained with power on or off.  
2.13 Internal Shutter Installation/Removal  
An IsoPlane may be ordered with an optional internal shutter at the entrance slit.  
This shutter is controlled either by a detector via a shutter cable from the  
detector’s Shutter connector to the Shutter connector on the IsoPlane or by an  
Shutter Control box (Model SHC-EXT) available from Princeton Instruments.  
2.13.1Installing an Internal Shutter  
1. Using a 9/64” hex wrench, unscrew the four socket head screws that secure the Turret  
Compartment cover to the top of the IsoPlane. Lift the cover and screws off of the  
IsoPlane and set them aside.  
2. Remove the grating turret. If you are not sure how to do this, refer to Section 2.14 Turret  
Screws  
3. Use extreme care so as not to touch the grating surfaces.  
4. Mount the shutter assembly on the two socket head screws above  
the entrance slit. You may need to back out the screws about five  
turns.  
5. Use the 9/64” hex wrench to tighten down the screws.  
6. Connect the shutter cable to the connector in the floor of the  
IsoPlane. Make sure the connector on the cable  
Shutter  
aligns with the connector in the floor.  
Shutter Cable  
Connector  
7. Re-install the grating turret. If you are not sure  
how to do this, refer to Section 2.7 Turret  
8. Place the Turret Compartment cover on the  
spectrograph. Replace and tighten all of the  
cover screws.  
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Chapter 3  
SCT 320 Operation  
23  
2.13.2Removing an Internal Shutter  
If you are planning to use a PI-MAX detector (or other detector without an external shutter  
control connector) and the IsoPlane has an internal shutter, you will either have to remove the  
shutter or control the shutter via a Princeton Instruments SHC-EXT external shutter control box  
if one is available. This is because there is no way for these detectors to keep the shutter open or  
to open the shutter during an acquisition. The following instructions step through the removal  
process.  
1. Using the 9/64” hex wrench, unscrew the four  
Shutter  
socket head screws that secure the Turret  
Shutter Cable  
Connector  
Compartment cover to the top of the IsoPlane.  
Lift the cover and screws off of the IsoPlane  
and set them aside.  
2. Remove the grating turret. If you are not sure  
how to do this, refer to Section 2.14 Turret  
3. Use extreme care so as not to touch the  
grating surfaces.  
Screws  
4. After removing the turret and placing it in a safe location, reach  
into the compartment and unplug the connector on the shutter  
cable from the connector mounted to the base of the IsoPlane by  
pulling it straight up.  
5. Using the 9/64” hex wrench, loosen but do not remove the two  
hex head socket screws that secure the shutter housing to the wall  
of the IsoPlane.  
6. Lift up and pull out on the shutter to remove it.  
7. Store it in a safe location.  
8. Re-install the grating turret. If you are not sure how to do this, refer to Section 2.7 Turret  
9. Place the Turret Compartment cover on the spectrograph. Replace and tighten all of the  
cover screws.  
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IsoPlane® SCT 320 Manual  
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2.14 Turret Removal  
CAUTION  
1. The optical surfaces in the spectrograph are extremely delicate and can be permanently damaged by  
contact with solid objects as well as with most liquids and aerosols.  
2. DO NOT TOUCH optical surfaces with anything. Wear thin protective powderless gloves to  
minimize damage from body oils if you accidentally touch any optical surface, especially the grating.  
3. Avoid talking or sneezing near optical surfaces. Do not breathe directly on them.  
The following procedure is recommended for removing the grating turret from the IsoPlane’s  
Turret Compartment. Observe proper optical handling procedures.  
1. Scan the instrument to Grating #1 and a Center Wavelength of 0 nm.  
2. Using the 9/64” hex wrench, remove the four Turret Compartment cover screws and remove  
the cover.  
3. Loosen the Center Torque Screw (see Figure 2-15).  
4. Use extreme care so as not to touch the grating surfaces. Grasp the Center Torque Screw  
and lift the grating turret straight up off the grating spindle assembly (see Figure 2-16). If the  
turret cannot be lifted up, you may need to loosen the Center Torque Screw more.  
5. Put the removed grating turret assembly into the protective container it was shipped in.  
Center Torque Screw  
Figure 2-15. Center Torque Screw  
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Chapter 3  
SCT 320 Operation  
25  
Figure 2-16. Lift Turret up out of the Turret Compartment  
6. If you are not installing/removing a shutter assembly or installing a different turret, replace  
and secure the Turret Compartment cover.  
2.15 Turret Interchange  
Read and follow the instructions in this section only if you have ordered more than one turret for the  
IsoPlane. Otherwise, you never have to interchange turrets.  
The IsoPlane is supplied with one on-axis mounted triple grating turret assembly, but you may  
order up to three (3) grating turrets for the spectrograph. If you have multiple turrets (2 or 3), the  
built-in sensing mechanism will auto-identify for the software which grating turret is installed.  
You may, however, want to label the turrets (for example, with the spectral range used).  
CAUTION  
1. The optical surfaces in the spectrograph are extremely delicate and can be permanently damaged by  
contact with solid objects as well as with most liquids and aerosols.  
2. DO NOT TOUCH optical surfaces with anything. Wear thin protective powderless gloves to  
minimize damage from body oils if you accidentally touch any optical surface, especially the grating.  
3. Avoid talking or sneezing near optical surfaces. Do not breathe directly on them.  
The following procedure is recommended for interchanging grating turrets. Observe proper  
optical handling procedures.  
1. Locate the storage container with the new grating turret to be installed.  
2. Become familiar with the components as labeled on Figure 2-17, Figure 2-19, Figure 2-20,  
3. Scan the instrument to Grating #1 and a Center Wavelength of 0 nm.  
4. Using the 9/64” hex wrench, remove the four Turret Compartment cover screws and remove  
the cover. Become familiar with the grating turret and its components.  
5. Loosen the Center Torque Screw (see Figure 2-17).  
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IsoPlane® SCT 320 Manual  
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6. Use extreme care so as not to touch the grating surfaces. Grasp the Center Torque Screw  
and lift the grating turret straight up off the grating spindle assembly (see Figure 2-18). If the  
turret cannot be lifted up, you may need to loosen the Center Torque Screw more.  
7. Put the removed grating turret assembly into the protective container it was shipped in (align  
the post and hole). Tighten the Center Torque screw and then use a 3/32” hex wrench to  
tighten the three set screws on the bottom of the container (about 1 turn).  
8. Before removing the replacement grating turret from its shipping container, use a 3/32” hex  
wrench to loosen the three set screws on the bottom of the container (about 1 turn).  
9. Then remove the cover from the shipping container, grasp the Center Torque Screw and turn  
it counter-clockwise until the turret can be lifted straight up.  
10. Locate the hole near the edge between gratings on the grating turret assembly (see Figure 2-19).  
11. Locate the vertical post on the Grating Spindle Assembly (see Figure 2-20).  
12. Position the grating turret on the grating spindle so the hole in the turret assembly aligns with  
the post in the turret assembly as shown in Figure 2-21.  
13. Make sure the turret is properly seated.  
14. Tighten the Center Torque Screw until it clicks. This sets the torque on the spindle correctly.  
Note: You cannot overtighten this screw. It designed to slip once the correct torque is attained.  
15. Place the Turret Cover on the spectrograph. Replace and tighten all of the cover screws.  
16. Put the removed grating turret into the storage container: align the hole in the grating turret  
assembly with the vertical post on the bottom plate of the shipping container, and tighten the  
Center Torque Screw until it clicks. Replace the plastic cover and store the container in a safe  
location.  
17. If the IsoPlane’s power supply is on, re-start the IsoPlane to allow auto-identification of the  
new grating turret. If the power supply is off, the auto-identification will occur the next time  
you turn the supply on.  
Center Torque Screw  
Figure 2-17. Center Torque Screw  
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Chapter 3  
SCT 320 Operation  
27  
Figure 2-18. Lift Turret up out of the Turret Compartment  
Hole  
Figure 2-19. Location of Hole on Turret Grating Assembly  
Post  
Figure 2-20. Location of Post on Grating Spindle Assembly  
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IsoPlane® SCT 320 Manual  
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Aligned  
Hole and Post  
Figure 2-21. Turret Installed (Hole and Post Aligned)  
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Chapter 3 Operation  
3.1 Introduction  
This chapter reviews how to enable the control of an IsoPlane and Princeton Instruments detector  
by either the LightField (64-bit) or WinSpec (32-bit) software. This chapter also points out how  
to perform alignment using the software. Further information about operating the system can be  
found in the appropriate software manual or help file.  
Warnings:  
1. A PyLoN with an internal shutter or a SPEC-10 with an internal shutter CANNOT be used with an  
IsoPlane spectrograph.  
2. If the detector has a flange mount and has an internal shutter, DO NOT USE the Shutter connector  
to drive a shutter internal to an IsoPlane. If both the detector and spectrograph have shutters, the  
IsoPlane shutter will have to be removed or a Princeton Instruments SHC-EXT Shutter Control Box  
can be used to control the opening and closing of the IsoPlane’s internal shutter. See Internal  
3.2 Pre-Operation Checks  
Before starting the operating software (LightField or WinSpec, for example), confirm that:  
The detector is mounted to the IsoPlane.  
The detector and IsoPlane are connected to the computer via the appropriate  
communications cables.  
The detector and IsoPlane are powered on.  
If the detector is LN-cooled, the Dewar has been filled.  
3.3 Initialization  
When power is turned ON to the IsoPlane, it initializes to a wavelength of 0.0 nm for grating  
number 1. If the power is switched OFF and then ON again to the IsoPlane, it will re-initialize.  
Initialization gives the system a reference, or starting position to keep track of wavelength  
position, grating location, and other parameters. Alternative start-up parameters can be  
programmed if the factory defaults are not suitable (see Appendix A).  
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3.4 LightField  
Start LightField after making sure the detector and IsoPlane are connected to the computer and  
are turned on. When LightField boots it will look for available devices and will load their icons  
in the Available Devices panel. Before you can design a new experiment or run an existing one,  
the appropriate device icons must be dragged into the Experiment Devices panel. Once there is  
at least one device, the Experiment Settings panel will be populated with expanders for groups  
of experiment settings.  
Note: If the IsoPlane (SCT-320) icon is the only device in the Experiment Devices panel, the  
Spectrograph expander will be the only expander in the list. When you drag a detector into the panel, the  
Calibration expander and all of the detector- related expanders will be displayed.  
3.4.1 Define the Detector and Spectrograph  
Figure 3-1. LightField Available Devices panel  
1. After LightField opens, you should see an icon representing your detector in the  
Available Devices area. In the figure above, the detector is a PIXIS:100B eXcelon®.  
2. Drag the icon into the Experiment Devices area.  
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Chapter 3  
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31  
Figure 3-2. LightField Experiment Settings stack and Experiment Devices panel  
3. Note that the Experiment Settings stack on the left now displays several expanders.  
Because this is a new experiment, the default settings for the detector will be active. The  
Status bar (at the bottom of the window) displays an icon for temperature status.  
Temperature status reports the current temperature and whether the set temperature has  
been reached. Clicking on the icon, opens the Sensor expander which is where the set  
temperature can be changed.  
4. On the Shutter expander, select Shutter Mode: Normal (see Figure 3-2).  
5. Open the Spectrometer expander, select the appropriate grating (see Figure 3-2). In this  
case, the 300g/mm (Blaze: 750) grating was selected and the center wavelength was set  
to 500 nm for a mercury lamp. Use 0.0 nm if using a broadband source.  
Hint: Overhead fluorescent lights produce a mercury spectrum. Use a white card tilted at 45  
degrees in front of the entrance slit to reflect overhead light into the spectrograph. Select 500 nm  
as the spectral line.  
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IsoPlane® SCT 320 Manual  
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3.4.2 Perform Alignment  
Because the detector is mounted directly to the mounting plate on the IsoPlane, the rotational  
alignment and focusing operations are different from the way these operations are performed for  
an Acton SP Series spectrograph. The following information assumes that you are familiar with  
the locations of the mounting plate, Micrometer Compartment, and the locking set screw. If not,  
refer to earlier sections of this manual.  
1. Mount a light source such as a Princeton Instruments Hg and Ne/Ar Dual Switchable  
light source in front of the entrance slit.  
2. With the IsoPlane properly connected to the computer, turn the power on, wait for the  
spectrograph to initialize.  
3. With the detector mounted to the spectrograph and connected to the computer, turn on the  
power and wait for the detector to initialize. If the detector is LN-cooled, the Dewar  
should be filled.  
4. Start the application software. Because you are using LightField, you will need to drag the  
icons for the detector and the IsoPlane into the Experiment Devices area.  
5. Set the spectrograph to 500 nm if using a mercury source or to 0.0 nm if using a  
broadband source.  
6. Wait until the detector locks at its default temperature.  
7. Using a 9/64” hex wrench, loosen the four screws at the corners of the detector mounting plate.  
8. Select the Align Spectrometer function from the Experiment menu to open the  
Spectrometer Alignment dialog. This dialog describes the changes that LightField will  
make to the current setup to assist you in performing rotational alignment of the array to  
the spectrograph's optics. When you click on the Begin button, the modifications are  
made and continuous live data will be displayed as you rotate the detector.  
Figure 3-3. Spectrometer Alignment dialog  
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Chapter 3  
SCT 320 Operation  
33  
9. Click on the peak you will be monitoring for the alignment. This will display the data  
cursor, which you can position at the top of the peak. Since the data cursor spans the  
ROIs (graphs), you can use the data cursor as your vertical reference.  
10. Slowly rotate the camera until the peaks align in all of the ROIs.  
Alternatively, you can acquire an image, display the large data cursor, and compare the  
vertical bar to the line shape on the screen. Rotate the detector until the line shape on the  
screen is parallel with the vertical bar.  
11. After completing the rotational alignment, click on the Stop button.  
12. Re-tighten the four mounting plate screws.  
13. Using a 9/64” hex wrench, remove the cover from the Micrometer Compartment.  
14. Using a 3/32” hex wrench, loosen the micrometer locking set screw (see Figure 2-11).  
15. Click on Run, and while continuously acquiring data, adjust the micrometer until you  
maximize the intensity level and minimize the FWHM of a selected peak or peaks. Note  
that the Peak Find function (for the graph selected by the cursor) is automatically turned  
on to help you identify peaks and view FWHM widths.  
Figure 3-4. Alignment Helper: Before and After Rotational Alignment  
16. Tighten down the locking set screw.  
17. Place the Micrometer Cover on the spectrograph. Replace and tighten all of the cover  
screws.  
18. Stop acquisition.  
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IsoPlane® SCT 320 Manual  
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3.5 WinSpec  
Start WinSpec after making sure the detector and IsoPlane are connected to the computer and are  
turned on. WinSpec should find the detector and present a dialog for selecting the detector for  
your experiment. Before you can use the IsoPlane, you must tell WinSpec that it is the  
spectrograph you will be using.  
3.5.1 Select the Detector  
Note: If the detector is LN-cooled, the Dewar should be filled while the detector is ON.  
1. If this is the first time you have installedWinSpec/32 and a supported detector, the Camera  
Detection wizard will run automatically. Otherwise, if you installing a new detector type, click on  
the Launch Camera Detection Wizard… button on the Controller/CCD tab to start the wizard.  
2. On the Welcome dialog (Figure 3-5), leave the checkbox unselected and click on Next.  
Figure 3-5. Camera Detection Wizard - Welcome dialog  
3. Follow the instructions on the dialogs to perform the initial hardware setup: this wizard enters  
default parameters on the Hardware Setup dialog tabs and gives you an opportunity to  
acquire a test image to confirm the system is working.  
4. If the detector is LN-cooled, fill the Dewar while the detector is powered ON.  
3.5.2 Define the Spectrograph  
1. From the Main menu bar, open the Spectrograph menu, and select Define.  
Figure 3-6. Define Spectrograph dialog  
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Chapter 3  
SCT 320 Operation  
35  
2. On the Define Spectrograph dialog (Figure 3-6), click on the Install/Remove  
Spectrograph button.  
3. On the Install/Remove Spectrograph dialog, scroll down the list of supported  
spectrographs, click on Acton SCT320, click on the Install Selected Spectrograph  
button, and then click on OK to return to the Define Spectrograph dialog.  
Figure 3-7. Install/Remove Spectrograph dialog  
Figure 3-8. Define Spectrograph dialog: Acton SCT320 is Active Spectrograph  
4. To confirm that WinSpec recognizes the spectrograph, click on Do Hardware Initialize.  
You should hear the turret moving.  
5. Now that you have identified the spectrograph to WinSpec, your next steps should be to  
align the spectrograph optics to the detector. See 3.5.3 Perform Alignmenton the next  
page.  
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3.5.3 Perform Alignment  
The initial alignment described in this section assumes that you have already connected and  
turned on the detector and spectrograph, have opened WinSpec, and identified the detector and  
spectrograph. After you have aligned the optics the first time, you may want to repeat the process  
to fine tune the alignment.  
1. Mount a light source such as a Princeton Instruments Hg and Ne/Ar Dual Switchable  
light source in front of the entrance slit.  
2. From the Main menu bar, open the Spectrograph menu, select Move, choose the grating  
to be move, and then set it to 500 nm if using a mercury lamp or to 0.0 nm if using a  
broadband source.  
Figure 3-9. Move Spectrograph dialog: Gratings tab  
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Chapter 3  
SCT 320 Operation  
37  
3. Set the slit to 10 µm at a minimum. If necessary, adjust the Exposure Time to maintain  
optimum (near full-scale) signal intensity.  
4. Wait until the detector locks at its default temperature. If the detector is LN-cooled, it  
should have been filled after the detector was powered ON.  
5. Turn on Focus mode.  
6. Adjust the rotation alignment. First, use a 9/64” hex wrench to loosen the four screws at  
the corners of the detector mounting plate. While watching a live display of the spectrum  
displayed as a graph, select a peak to monitor and then rotate the detector (up to 4 degrees  
of rotation are possible). The peak will go from broad to narrow and back to broad. Leave  
the detector rotation set for the narrowest achievable peak.  
Alternatively, take an image, display the horizontal and vertical cursor bars, and compare  
the vertical bar to the line shape on the screen. Rotate the detector until the line shape on  
the screen is parallel with the vertical bar.  
Another technique is to set up three ROIs (one at the top, middle, and bottom of the  
array) with 10 rows binned for each via the Experiment Setup|ROIs tab, Then change  
the data display via the Display Layout dialog, so that 3d Graph is selected (General  
tab), the Z Axis Endpoints (3D Layout tab) are %X = 0 and % Y = 40, and the Save as  
Default check box is checked. Click on OK. While running in Focus mode, you should  
see three stacked graphs. Aligning the large cursor with a prominent peak, rotate the  
detector until the peak aligns with the cursor in all three ROIs.  
7. After completing the rotational alignment, tighten the four mounting plate screws.  
8. Remove the cover from the Micrometer Compartment.  
9. Using a 3/32” hex wrench, loosen the locking set screw.  
10. While continuously acquiring data, adjust the micrometer until you maximize the  
intensity level and minimize the FWHM of a selected peak or peaks.  
11. Tighten down the locking set screw.  
12. Place the Micrometer Cover on the spectrograph. Replace and tighten all of the cover  
screws.  
13. Then stop acquisition.  
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Appendix A Using the Monochromator Control Software  
A.1 Introduction  
As has been previously mentioned in this manual, the Acton IsoPlane spectrograph can be  
controlled using Princeton Instruments’ LightField, WinSpec, or SpectraSense software. It can  
also controlled from a computer using the supplied Monochromator Control software via the  
RS-232 or USB interface. The information on how to do this is provided in this appendix.  
A.2 Install the Monochromator Control Software  
Use the install disk shipped with the monochromator to install that software on your computer.  
The icon for this software on your computer screen is labeled MonoControl.  
A.2.1 Monochromator Control Application Software  
The Monochromator Control software is a stand-alone Acton software program for basic  
scanning and calibration. Utilities for grating updates and communications are also included.  
Normally, the software is installed in the directory C:\Program Files\Princeton  
Instruments\MonoControl. This directory contains the subdirectories Bin and Data. The Bin  
directory contains the executable code for the program.  
Upon installation, a Monochromator Control icon is usually placed on the desktop for starting  
the software. If this icon is not on the desktop, check for the program in the Windows Start  
menu\Programs or go directly to the MonoControl\Bin directory and start the software there.  
When the Monochromator Control software loads, there is a main screen with selections for  
monochromator operation and for various setup functions. (If the buttons are grayed out, exit the  
program, connect the IsoPlane, wait for it to initialize, and then restart the program.) Click on the  
Operation button and a screen will come up which allows for basic control of the  
monochromator wavelength. All functions of this software are described in the Monochromator  
Control software manual supplied on the Monochromator Control software install CD.  
A.3 Connecting the IsoPlane to the Computer  
The IsoPlane is designed for operation by computer using RS-232 or USB, control that enables  
wavelength scanning at a pre-set linear scan rate, change of scanning speeds, grating selection,  
rapid GOTO wavelength positioning, change of grating turrets, and “jog” wavelength  
positioning. Refer to the Monochromator Control software for Windows for operation with a  
computer.  
A.4 Controlling the IsoPlane Spectrograph at the Command  
Level  
Although it requires more programming on the user’s part, the spectrograph can also be  
controlled with direct commands through its USB 1.1 port or RS-232 port. The same command  
set, listed below, is used for both RS-232 and USB.  
Commands can be sent as single commands or grouped in strings of commands. All commands are  
single words (contain no spaces) and all commands in a string are separated by at least one space.  
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Parameters, if needed, precede the command and are separated from the command by at least one  
space (e.g., 546.07 GOTO).  
For RS-232 operation, the port set-up is 9600 baud, 8 data bits, 1 stop bit and no parity. A convenient  
tool for trying out this mode of operation is the program HyperTerminal supplied with the Windows  
operating system. The USB 1.1 port with the driver supplied also shows up as and is treated like a  
com port – although a very fast one. All commands or strings of commands must be terminated with  
a carriage return (0D hex). The spectrograph responds to a command when the command has been  
completed by returning the characters OK followed by carriage return and line feed (hex ASCII  
sequence 20 6F 6B 0D 0A). The default condition is to echo each character that is sent to the  
spectrograph with the RS-232 interface and to not echo the commands when using the USB  
interface. When sending a command or string of commands, it is important to wait for the  
spectrograph to complete the processing of that command string before sending another command.  
A.4.1 Spectrograph Wavelength Movement Commands  
GOTO  
Goes to a destination wavelength at maximum motor speed. Accepts  
destination wavelength in nm as a floating point number with up to 3  
digits after the decimal point or whole number wavelength with no  
decimal point.  
<GOTO>  
NM  
Same as GOTO (For compatibility with software written for previous  
Acton SP series models.)  
Goes to a destination wavelength at constant nm/min rate specified by last  
NM/MIN command. Accepts destination wavelength in nm as a floating  
point number with up to 3 digits after the decimal point or whole number  
wavelength with no decimal point.  
<NM>  
>NM  
Same as NM (For compatibility with software written for Acton SP series  
models.)  
Similar to NM except it returns control to user immediately rather than  
waiting for completion of spectrograph wavelength move. Can be used  
with ?NM or MONO-?DONE below. This command must be terminated  
with MONO-STOP listed below.  
Note: Use the NM command when communication with the monochromator  
during the scan is not required.  
?NM  
Returns present wavelength in nm to 0.01nm resolution with units nm  
appended.  
e.g., ?NM 300.00 nm  
MONO-?DONE  
MONO-STOP  
Used with >NM command to determine if monochromator has reached the  
destination. Returns 0 if move is not complete, 1 if move is complete.  
Stops the monochromator wavelength move after use of the >NM  
command.  
NM/MIN  
Sets the scan rate in nm/min to 0.01 nm/min resolution with units nm/min.  
?NM/MIN  
Returns present scan rate in nm/min to 0.01 nm/min resolution with units  
nm/min.  
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Appendix A  
Using the Monochromator Control Software  
41  
A.4.2 Grating Control Commands  
GRATING  
Places specified grating in position to the wavelength of the wavelength  
on the present grating. Up to nine (9) gratings are allowed on three (3)  
turrets. This command takes a grating number from 1 - 9.  
IMPORTANT NOTE: This command assumes that the correct turret is specified  
by the TURRET command. For example, using grating numbers 1, 4 and 7 will  
place the first grating on the installed turret into that position and call up the  
parameters for the grating number specified.  
?GRATING  
Returns the number of gratings presently being used numbered 1 - 9.  
?GRATINGS  
Returns the list of installed gratings with position groove density and  
blaze. The present grating is specified with an arrow.  
TURRET  
Specifies the presently installed turret or the turret to be installed.  
e.g., if installing the second turret, issue the command 2 TURRET to  
insure using the correct parameters.  
?TURRET  
Returns the correctly installed turret numbered 1 - 3.  
The following command is used for grating installation by Acton part number:  
INSTALL  
Installs new grating parameters into the non-volatile memory of the  
IsoPlane monochromator. Uses the part number of the grating to specify  
the parameters.  
e.g., 1-120-500 5 INSTALL places a 1200 g/mm grating blazed at 500 nm  
into the second grating position on turret number 2.  
The following commands are used for grating installation by grating parameters:  
SELECT-GRATING Specifies the grating number to be installed 1 - 9.  
G/MM  
Specifies groove density of grating to be installed in g/mm.  
e.g., 1200 G/MM  
BLAZE  
Specifies the blaze wavelength and units of the grating to be installed with  
7 characters of the user’s choice. Unlike other commands, this command  
is issued before the parameters. After the command is issued, the IsoPlane  
responds with ““ . Seven characters are then entered (these may be  
numbers, letters, spaces or special characters).  
UNINSTALL  
Used to remove a grating and its parameters from the IsoPlane  
non-volatile memory.  
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IsoPlane® SCT 320 Manual  
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A.4.3 Slit Width Control Commands (for Motorized Slits only)  
SIDE-EXIT-SLIT  
SIDE-ENT-SLIT  
MICRONS  
Designates side exit slit to receive slit control commands.  
Designates side entrance slit to receive slit control commands.  
Sets the slit width for the designated slit in the range of 10 to 3000  
microns to 1 micron resolution.  
?MICRONS  
Returns the slit width setting in microns to the nearest 1 micron.  
A.4.4 Additional Commands  
MONO-EESTATUS Returns setup and grating calibration parameters for all gratings.  
RESTORE-FACTORY-SETTINGS Returns all parameters, including grating calibration  
parameters, to the original factory calibrated settings.  
Notes:  
1. Any gratings installed at a later date (after initially receiving the IsoPlane)  
will be erased from memory using this “restore command”.  
2. This command will overwrite any calibration parameters set by the user.  
MODEL  
SERIAL  
Returns model number of the spectrograph.  
e.g., MODEL SCT-320  
Returns serial number of the spectrograph. Format is 8 digits with the first  
3 digits being the model number.  
e.g., SERIAL 32010121  
The following are the Start-Up parameters and their default values:  
Parameter  
Default  
GRATING  
#1  
WAVELENGTH  
SCAN SPEED  
0.0 nm  
100.0 nm/min  
Table A-1. Start-Up Parameters and Their Default Values  
Each of the above may be changed through the RS-232 port or USB port using the following  
commands. These values are stored in non-volatile memory and will be in effect after the next  
power-up.  
INIT-GRATING  
Selects which of the two gratings on the installed turret the IsoPlane will  
go to after finding 0.0 nm on the first grating.  
e.g., 2 INIT-GRATING selects the second grating as the default.  
INIT-WAVELENGTH Sets an initial wavelength for the IsoPlane after initialization.  
e.g., 435.84 INIT-WAVELENGTH Notice that two digits after the decimal  
point are required.  
INIT-SRATE  
Sets an initial scan rate for the IsoPlane.  
e.g., 500.00 INIT-SRATE Notice that two digits after the decimal point are  
required.  
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Appendix B Spectrograph to Computer Cable  
Connection  
Figure B-1. RS-232 Cable Wiring  
Figure B-2. IsoPlane Cable Connectors  
FILTER  
SHT TTL  
DSP  
Filter driver connection for Acton FA-2448 Filter Wheel.  
SHT TTL connection for TTL control of shutter.  
DSP connection to connect two spectrographs as doubles.  
Com light flashes when communicating with the computer.  
COM  
READY  
Ready light is on when the instrument is ready to operate. (Green light comes on  
after the instrument initializes. Yellow = busy).  
RS-232  
USB  
RS-232 connection to computer.  
USB connection to computer.  
USB HUB USB Hub 1.1 compatible.  
POWER Power connection +5 and +24 Volts.  
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Appendix C Accessories Listing  
Slit Assembly  
SP-716-1  
Bilaterally adjustable ENTRANCE slit assembly for IsoPlane monochromator  
or spectrograph. Micrometer adjustable widths from 10 µm to 3 mm. Supplied  
with interchangeable 4.0 mm and 14.0 mm high baffles.  
Triple Grating Turret  
300-483 Interchangeable triple grating turret for the IsoPlane. Requires gratings.  
Optional second and third turrets.  
Light Sources: Sources with 220 V, 50 Hz area also available in all models.  
MS-416  
Low Pressure Mercury Light Source with power supply and mounting flange  
for Acton series monochromators and spectrographs. Provides output at typical  
mercury wavelengths (line output).  
DS-421  
TS-425  
30 Watt Deuterium Light Source with housing, power supply, mounting flange,  
and light collection mirror. Provides output from 190 to 350 nm.  
30 Watt Tungsten-Halogen Light Source with housing, power supply,  
mounting flange, and light collection mirror. Provides output from 350 nm to >2.0  
µm  
TS-428  
250 Watt Tungsten-Halogen Light Source with housing, AC power supply,  
mounting flange, variable brightness control and light collection mirror. Provides  
output from 350 nm to >2.0 µm.  
TS-428-DC Same as TS-428 with Regulated DC Power Supply.  
TDS-429  
Dual Light Source with 30 watt deuterium & 30 watt tungsten-halogen lamps.  
Includes housing with light collection mirror, mounting flange, and power supply.  
Provides combined output from 190 to >2.0 µm.  
XS-433  
75 Watt Xenon Light Source includes power supply, housing, mounting flange  
and light collection mirror. Provides continuous spectral output from 190 nm to  
750 nm and declining continuum out to 2.6 µm.  
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IsoPlane® SCT 320 Manual  
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Detectors and Accessories: All detectors include mounting flanges for IsoPlane slit  
assemblies.  
PD-438  
Universal Photomultiplier Tube Housing for standard 1 1/8" side window  
photomultiplier tubes. Requires side window PMT, and photometer/power supply  
for operation. Accepts Acton tubes P1, P2 or P3 below, or customer specified 1  
1/8” side window PMTs.  
PD-439  
PD-471  
Same as PD-438 above, also includes integrated light tight shutter.  
Photomultiplier Tube Housing for 1 /8-inch tubes with built in HV supply. Only  
for SpectraHub.  
P1  
Side Window Photomultiplier Tube (or equivalent) for wavelength region 185-  
650 nm.  
Fits PD-438, PD-439, or PD-471 housing.  
P2  
Side Window Photomultiplier Tube (or equivalent) for wavelength region from  
185-900 nm. Fits PD-438, PD-439, or PD-471 housing.  
P3  
Side Window Photomultiplier Tube (or equivalent) for wavelength region from  
300-1100 nm. Fits PD-438, PD-439, or PD-471 housing.  
SI-440  
SI-440-UV  
General-purpose Single Channel Detector with a 10 mm diameter active area  
for use from 400 to 1100 nm. Enclosed in housing with the BNC connector.  
Single Channel Detector with a UV-enhanced, 10 mm diameter active area for  
use from 200 to 1100 nm operation.  
ID-441  
InGaAs Detector, includes pre-amplifier, uncooled version.  
ID-441-C  
InGaAs Detector, includes pre-amplifier, cooled version, requires either Model  
442-1A thermoelectric cooling for operation.  
442-1 A  
Thermoelectric cooling for ID-441 detectors.  
SpectraHub SpectraHub data acquisition system, 20-bit A-D converter, single channel  
detector interface. Requires SpectraSense software.  
Microscope Interface  
MicroSpec Microscope Interface enables researchers to perform high quality imaging and  
spectroscopy with a single system. Attaches to a UDP port on an inverted  
microscope and couples to the IsoPlane SCT 320. For more information, refer to  
the MicroSpec data sheet on the Princeton Instruments website.  
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Appendix C  
Accessories Listing  
47  
Filter Wheels and Order Sorting Filter Assemblies  
FA-2448  
Six Position Filter Wheel Assembly. Manual sample indexing, holds up to six  
samples, each 1.0” diameter; automated via SP Control Cable. Can be used with  
the IsoPlane. Requires FA-2448-F Filter Set or customer-supplied filters of  
25 mm (1 inch) diameter and 5 mm or less in thickness.  
FA-2448-1  
Order Sorting Filter Assembly. Includes FA-2448-F Filter Set with 320, 590,  
665, and 715 nm filters mounted in FA-2448 filter wheel. Manual indexing of  
filters for elimination of unwanted second order radiation; automated via SP  
Control Cable. Can be used with the IsoPlane.  
FA-2448-2  
FA-2448-3  
Motorized Six Position Filter Wheel Assembly, with stepping motor and  
FA-2448-4 controller. Enables indexing by computer with RS-232 or USB.  
Requires computer with RS-232 or USB for computerized operation. Set or  
customer-supplied filters of 25 mm (1 inch) diameter and 5 mm or less in thickness.  
Motorized Order Sorting Filter Assembly. Includes FA-2448-F Filter Set with  
320, 590, 665, and 715 nm filters mounted in FA-2448 filter wheel. Enables  
computer controlled indexing of order sorting filters for elimination of unwanted  
second order radiation. Requires computer with RS-232 or USB for operation.  
Requires FA-2448-F Filter Set.  
FA-2448-F  
Order Sorting Filter Set. Includes four filters: 320, 590, 665, and 715 nm.  
Fiber Optic Light Guides: All Fiber optic light guides contain 19 fibers, 200 µm diameter,  
arranged in a line pattern at the slit end, and round at the source end.  
LG-455-020-1 UV-VIS Fiber Optic Bundle 1.0 meter long, for 190 nm to 1100 nm. Requires  
mount.  
LG-455-020-3 UV-VIS Fiber Optic Bundle 3.0 meter long, for 190 nm to 1100 nm. Requires  
mount.  
LG-456-020-1 VIS-NIR Fiber Optic Bundle 1.0 meter long, for 400 nm to 2200 nm. Requires  
mount.  
LG-456-020-1 VIS-NIR Fiber Optic Bundle 3.0 meter long, for 400 nm to 2200 nm. Requires  
mount.  
FC-446-010 Fixed-Position Fiber Adapter is a low-cost solution for positioning fiberoptic  
bundles directly at the entrance port of an IsoPlane spectrograph. Accepts 10 mm  
diameter ferrule.  
FC-446-020 Fiber Coupler with horizontal translation capability for 10 mm diameter fiber  
optic bundle. Accepts 10 mm diameter ferrule.  
FC-446-021 Fiber Coupler with X-Y Micrometer alignment adjustments. Accepts 10 mm  
diameter ferrule.  
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IsoPlane® SCT 320 Manual  
Version 1.B  
FC-446-030 Imaging Fiber Adapter is designed specifically for our imaging spectrographs.  
The all-reflective design eliminates chromatic aberrations and the aspheric mirror  
cancels astigmatism, allowing precise imaging of fibers at the spectrograph  
entrance slit. Includes up/down, left/right screw alignment adjustments. Accepts  
10 mm diameter ferrule. Also includes a 0.75” thick spacer to insert an optional  
FA-2448 series Filter Wheel for order sorting function.  
Connecting Cables  
CC-499-2  
RS232 serial cable, 6 feet (1.82 meters) long, 9-pin female to 9-pin male  
connectors.  
3650-USB-06 USB cable, 6 feet (1.82 meters) long, type A to B connectors.  
If the above cables are not compatible with your system, contact Princeton Instruments for a  
custom cable.  
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Appendix D Gratings for IsoPlane  
Grooves/mm Blaze Wavelength  
Standard Part Mechanical  
Number  
Limit  
50  
150  
150  
150  
300  
300  
300  
300  
600  
600  
600  
600  
600 nm  
500 nm  
800 nm  
1250 nm  
300 nm  
500 nm  
750 nm  
1000 nm  
300 nm  
500 nm  
I3-005-600-P  
I3-015-500-P  
I3-015-800-P  
I3-015-1250-P  
I3-030-300-P  
I3-030-500-P  
I3-030-750-P  
I3-030-1000-P  
I3-060-300-P  
I3-060-500-P  
I3-060-750-P  
I3-060-1000-P  
I3-060-1200-P  
I3-120-300-P  
I3-120-HVIS-P  
I3-120-500-P  
I3-120-750-P  
11.2 µm  
5.6 µm  
2.8 µm  
Notes:  
Blazed Holographic, 190-450 nm,  
optimum range  
††  
Optimum range for this grating is from  
450 nm to the upper mechanical limit  
750 nm  
1000 nm  
1200 nm  
300 nm  
Standard Gratings are 68 X 68 mm.  
600  
1200  
1200  
1200  
1200  
1800  
1800  
2400  
1400 nm  
Holographic VIS ††  
500 nm  
750 nm  
Blazed Holographic UV I3-180-HUV-P  
933 nm  
700 nm  
500 nm  
I3-180-500-P  
I3-240-HVIS-P  
Holographic VIS ††  
Table D-1. Available Gratings  
Ordering Information  
Electronic Orders  
MasterCard / VISA  
Electronic orders accepted with proper  
Company Letterhead and complete contact  
information.  
MasterCard & VISA accepted for purchases.  
Written Orders  
Submit all written orders to our mailing address:  
Fax Orders  
Orders may be placed by fax with written confirmation.  
Please include complete name and address with these  
orders.  
Princeton Instruments  
15 Discovery Way  
Acton, MA 01720 U.S.A.  
FAX: 978-263-5086  
Orders accepted subject to current pricing.  
All orders FOB Princeton Instruments-Acton or shipping charges & insurance added separately.  
All orders subject to new customer approval.  
• IsoPlaneis a trademark of Roper Scientific, Inc. •  
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Appendix E Outline Drawings  
Figure E-1. IsoPlane: 320 with Manual Slit Assembly Outline Drawing  
51  
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Figure E-2. IsoPlane: 320 with Motorized Slit Assembly Outline Drawing  
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Appendix F Standard Slit Assembly Drawing  
Figure F-1. Standard Slit Assembly Drawing  
53  
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Appendix G Declaration of Conformity  
DECLARATION OF CONFORMITY  
We, the undersigned  
Manufacturer: Princeton Instruments  
Address, City: 15 Discovery Way, Acton, MA 01720  
Country: USA  
Certify and declare under our sole responsibility that the following apparatus:  
IsoPlane SCT-320 with Power Supply  
Conforms to the emissions requirements of EN61326-1:2006; Clause 7.2:  
CISPR 11 Edition 4: 2003  
CISPR 11 Edition 4: 2003  
IEC 61000-3-2: 2000  
Conducted Emissions, Group 1, Class A  
Radiated Emissions, Group 1, Class A  
Harmonics  
IEC 61000-3-3: 2002  
Flicker  
Conforms to immunity requirements of EN61326-1: 2006 Table 1:  
IEC 61000-4-2: 2001  
IEC 61000-4-3: 2002  
IEC 61000-4-4: 2004  
IEC 61000-4-5: 2001  
IEC 61000-4-6: 2003  
IEC 61000-4-11: 2004  
Electrostatic Discharge 4KV Contact  
Radiated Immunity level 2 3V/m  
EFT/Burst, Power Leads 1KV  
Surge Immunity, Power leads level 2  
Conducted Immunity, Power Leads level 2  
Voltage Dips and Interrupts  
And follows the provisions of:  
EMC Directive 2004/108/EC  
CE Low Voltage Directive 2006/95/EC  
The technical documentation is kept at the following address:  
Company:  
Address, City, State:  
Country:  
Princeton Instruments  
15 Discovery Way, Acton, MA 01720  
USA  
Telephone Number:  
Fax Number:  
+1 800.874.9789/+1 978.263.3584  
+1 978.263.5086  
Name and Position of Person Binding the Manufacturer or his Authorized Representative:  
Michael Case  
Date:  
Signature:  
October 1, 2012  
Engineering Manager  
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Appendix H Certification and Warranty  
Certification  
Princeton Instruments certifies that this instrument was thoroughly tested and found to meet the  
specifications furnished by Princeton Instruments when it was shipped from the factory.  
Warranty  
Princeton Instruments instruments and accessories are warranted for a period of one full year  
from date of delivery to be free from defects in material and to conform to the specifications  
furnished by Princeton Instruments. The company's obligation under this warranty is limited to  
servicing or adjusting an instrument returned to the factory, prepaid, and to repairing or replacing  
at the factory any part or parts thereof. All purchased items carry the original manufacturer’s  
warranty.  
Princeton Instruments shall not be liable for consequential damages resulting from accident,  
alteration, misuse, improper installation, operation on low or excessive voltages or any use in  
violation of the operating instructions furnished by Princeton Instruments.  
If any defect appears within the warranty period, the purchaser shall promptly notify Princeton  
Instruments. No material will be accepted for repair or replacement without prior authorization  
from Princeton Instruments. Upon such authorization and in accordance with instructions of  
Princeton Instruments, parts, materials or equipment for which repair or replacement is requested  
shall be returned to Princeton Instruments for examination, with shipping charges prepaid by the  
purchaser. Final determination as to whether a product or part is actually defective rests with  
Princeton Instruments.  
In such cases where necessary repairs are not covered by this warranty, an estimate of repair  
charges will be submitted to the purchaser before servicing the equipment.  
Princeton Instruments reserves the right to make changes or improvements upon its products  
without imposing any obligations upon itself to install the same upon its products previously  
manufactured.  
This warranty is expressly in lieu of all other obligations or liabilities on the part of Princeton  
Instruments, and Princeton Instruments neither assumes, nor authorizes any other person to  
assume for them, other obligations or liability in connection with the sale of equipment  
manufactured by Princeton Instruments  
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Index  
Monochromator Control application software.................. 39  
Motorized slit ................................................................... 22  
Mounting a detector  
array............................................................................ 16  
PyLoN without shutter................................................ 16  
single point.................................................................. 20  
SPEC-10 LN without shutter ...................................... 16  
three-slotted flange...................................................... 16  
Mounting plate ................................................................. 16  
A-B  
Accessories  
listing of.......................................................................45  
MicroSpec ...................................................................46  
mounting to slit assembly............................................11  
Additional commands.......................................................42  
Adjustment of image plane height ....................................19  
Alignment .........................................................................17  
Application software  
LightField (optional) .....................................................9  
Monochromator Control..............................................39  
SpectraSense (optional)...............................................10  
WinSpec (optional)........................................................9  
O-R  
Ordering information........................................................ 49  
Power supply.................................................................... 11  
Rotational alignment ........................................................ 17  
RS-232  
C
cable ............................................................................ 10  
cable wiring................................................................. 43  
pin assignments........................................................... 10  
port settings................................................................. 11  
Cable connector descriptions............................................43  
Cables  
RS-232 (Part # CC-499-2)...........................................10  
USB Type A to Type B (Part # 3650-USB-06) ...........10  
Calibration light sources ...................................................32  
CameraDetectionwizard.......................................................34  
Certification......................................................................57  
Command level control...............................................10, 39  
Copyright information ........................................................2  
S
Setup procedure, initial ...................................................... 9  
Shutter  
installation................................................................... 22  
removal ....................................................................... 23  
Shutter control box........................................................... 22  
Single point detector  
mounting instructions.................................................. 20  
tapered mounting plate................................................ 20  
Slit  
manual......................................................................... 53  
manual adjustment ...................................................... 21  
motorized .................................................................... 22  
Slit width control commands (motorized slit) .................. 42  
SpectraSense application software ................................... 10  
Standard slit assembly  
D-H  
Description, IsoPlane..........................................................7  
Detectors, rotation of ........................................................37  
Drawing  
IsoPlane with manual slit assembly.............................51  
IsoPlane with motorized slit assembly.........................52  
standard slit assembly..................................................53  
Grating  
availability...................................................................49  
control commands .......................................................41  
drawing ....................................................................... 53  
Supplied interface cables.................................................. 10  
I-L  
Image plane height adjustment .........................................19  
Initial setup procedure ........................................................9  
Interface cables.................................................................10  
IsoPlane, description of.......................................................7  
LightField application software ..........................................9  
Locking set screw...............................................................18  
T-V  
Tapered mounting plate.................................................... 20  
Terminal setup.................................................................. 11  
Turret  
installation................................................... 9, 12, 22, 23  
interchange............................................................ 12, 25  
removal ........................................................... 22, 23, 24  
USB cable ........................................................................ 10  
M-N  
Manual slit adjustment......................................................21  
Mercury spectrum, fluorescent lights................................31  
Micrometer  
W-Z  
compartment................................................................18  
locking set screw...........................................................18  
MicroSpec.........................................................................46  
Model 718 Motorized Slit...................................................22  
Model SHC-EXT..............................................................22  
Warranty........................................................................... 57  
Wavelength movement commands................................... 40  
WinSpec application software............................................ 9  
Wizard, CameraDetection .................................................... 34  
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Contact Princeton Instruments for additional information.  
USA TOLL-FREE +1.877.474.2286 | USA +1.609.587.9797  
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