Summary of Contents for Princeton Instruments NIRvana-LN
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NIRvana-LN™ Camera System 4411-0145 Issue April 20, 2016...
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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...
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C.3 Remove Camera Mounting Plate and Cover from IsoPlane 320....107 C.4 Mount the NIRvana-LN on the IsoPlane 320 ......108 Appendix D: WinX/LightField Cross Reference .
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Mounting NIRvana-LN to an IsoPlane 320..... .108 Figure C-6: NIRvana-LN Mounted to an IsoPlane 320 ..... .109...
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Related Documentation........9 Table 2-1: NIRvana-LN Rear-Panel Connectors ......17 Table 2-2: Standard NIRvana-LN Camera System Cables .
This manual provides users with information necessary to install a NIRvana-LN camera and place it in operation. Topics include a detailed description of the NIRvana-LN camera as well as the installation, applications, cleaning, and specifications of the camera system.
1.3 Document Organization This manual is organized as follows: Chapter 1, About this Manual • Briefly describes the NIRvana-LN family of detectors; details the structure of this manual; and documents environmental, storage, and cleaning requirements. Chapter 2, NIRvana-LN Camera System •...
Includes two alphabetically sorted tables (WinX to LightField and LightField to WinX) that cross reference terms used in the two applications. Warranty and Service • Provides the Princeton Instruments warranty and customer support contact information. 1.4 Conventions Used in this Manual The following conventions are used throughout this manual: ®...
™ NIRvana -LN System Manual Issue 4 WARNING! If the equipment is damaged, the protective grounding could be disconnected. Do not use damaged equipment until its safety has been verified by authorized personnel. Disconnecting the protective earth terminal, inside or outside the apparatus, or any tampering with its operation is also prohibited.
Chapter 1 About this Manual 1.6.1 Detector Observe the following precautions when working with the Detector: If the equipment is damaged, the protective grounding could be disconnected. Do • not use damaged equipment until its safety has been verified by authorized personnel.
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This chapter provides an introduction to, and overview information about, Princeton Instruments’ NIRvana-LN camera system. Figure 2-1 shows those items that are typically included as part of a standard NIRvana-LN Camera System. Figure 2-1: NIRvana-LN Camera System: Standard Items OWER UPPLY WITH...
Read rate, binning information, and regions of interest for NIRvana-LN cameras are some of the parameters that are configured using the data acquisition software on the host computer.
2.1.1 InGaAs FPA Sensor The NIRvana-LN camera incorporates a 640 x 512 (20 x 20 μm pixels) InGaAs focal plane array (FPA) that is equipped with a four-port readout. The sensor’s excellent response and outstanding sensitivity in the 0.8 μm -1.55 μm spectrum make it particularly well suited for Near Infrared II window/Short Wave Infrared (SWIR) region imaging applications.
The standard upright Dewar holds 2.2 liters of liquid nitrogen (LN.) All-directional and end-on Dewar inserts are available. 2.2 Spectrometer Support The NIRvana-LN easily mounts to the IsoPlane SCT-320 spectrograph. Refer to Appendix C, IsoPlane 320 Mounting, on page 105 for information about mounting the NIRvana-LN to a spectrograph.
[9.8 ft] 2.5 Certificate of Performance Each NIRvana-LN camera is shipped with a Certificate of Performance which states that the camera system has been assembled and tested according to approved Princeton Instruments procedures. It documents the camera’s performance data as measured during the testing of the NIRvana-LN and lists the following camera- and customer-specific information: •...
Other optional items may be available. For complete information about available options for the NIRvana-LN camera system, contact Princeton Instruments. 2.7.1 Application Software Princeton Instruments offers a number of data acquisition software packages for use with NIRvana-LN camera systems, including: ® LightField •...
WinView and WinSpec take full advantage of the versatility of the NIRvana-LN camera and even enhance it by making integration of the detection system into larger experiments or instruments an easy, straightforward endeavor.
2.8.1 Camera Although there is no periodic maintenance that needs to be performed on a NIRvana-LN camera, users are advised to wipe it down with a clean damp cloth from time to time. This operation should only be done on the external surfaces and with all covers secured. In dampening the cloth, use clean water only.
Chapter 3: Installation Overview Figure 3-1 illustrates a typical NIRvana-LN system diagram for imaging applications. Figure 3-1: System Diagram: NIRvana-LN Imaging Application 100-240 GigE Power 100-240 Supply Power GigE Cable Detector F-Mount and Lens EXPERIMENT Figure 3-2 illustrates a typical NIRvana-LN system diagram for spectrographic applications.
With the power supply disconnected from the detector, connect one end of the Ethernet cable to the GigE connector on the rear of the NIRvana-LN and the other end to the Ethernet port on the host computer. Connect the power supply to the NIRvana-LN.
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Chapter 3 Installation Overview Table 3-1: Installation Overview (Sheet 2 of 2) Action Refer to: Adjust the rotational alignment for the best image or spectral lines. When using LightField, use the function. Section 5.5, Rotational • Align Spectrometer Alignment, on page 46 When using WinSpec/32, use the function.
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During the unpacking, check the system components for possible signs of shipping damage. If there are any, notify Princeton Instruments and file a claim with the carrier. If damage is not apparent but detector or controller specifications cannot be achieved, internal damage may have occurred in shipment.
30° limit, you may have the wrong type of Dewar. Contact the factory. 4.3.3 Detector Power The NIRvana-LN detector receives its power from the power supply, which in turn plugs into a source of AC power. CAUTION! The plug on the line cord supplied with the system should be compatible with the line-voltage outlets in common use in the region to which the system is shipped.
Contact the factory to confirm specific requirements. The specifications listed are the MINIMUM required for a NIRvana-LN system. A faster computer with 2 GB (or more) RAM and a fast hard drive (e.g., 10,000 rpm,) will greatly improve system performance during live mode operations.
™ NIRvana -LN System Manual Issue 4 4.4.2 WinView/32 and WinSpec/32 Host Computer Requirements When running WinView/32 or WinSpec/32 data acquisition software, the host computer must meet, or exceed, the following specifications: 32-Bit Operating System • Windows 7. — ® 2 GHz Pentium 4 (minimum);...
InstallShield Wizard dialog. Figure 4-1: Typical LightField Installation Wizard Dialog After the installation has been completed, reboot the host computer. Connect the NIRvana-LN system components to the host computer and apply power. Launch LightField and activate it according to on-screen instructions. REFERENCES:...
™ NIRvana -LN System Manual Issue 4 4.5.2 Install WinSpec/32 Perform the following procedure to install WinSpec/32 on the host computer: NOTES: Install the GigE Adapter card BEFORE installing the WinSpec/32 application software. Leave the interface cable disconnected from the detector until you have installed WinSpec/32.
Chapter 4 System Setup Click Next > to continue with the installation, and follow on-screen prompts. Once the installation has been completed, connect the detector to the host computer and turn on the detector’s power supply. Reboot the host computer. Windows will automatically detect the newly-installed GigE card.
[0.254 mm]. Because of this, an image area or a focus set at room temperature will change as a detector cools. The NIRvana-LN is designed so the optical center of an array is offset at room temperature. Now, when a detector cools to operating temperature, the optical center of the array is at the center of the nose.
4.8 Configure Default Parameters in LightField Perform the following procedure to configure LightField with default system parameters: Verify the NIRvana-LN (and spectrograph, if this is a spectroscopy system) is connected to the host computer and that the detector (and spectrograph) power supply is turned on.
™ NIRvana -LN System Manual Issue 4 When the Camera Detection Wizard - Welcome dialog is displayed, the checkbox for manual configuration should remain unselected. See Figure 4-4. Figure 4-4: Typical Camera Detection Wizard - Welcome Dialog Click Next> to continue. Continue to follow on-screen prompts to complete the initial hardware setup.
LN, which can cause severe injury. NIRvana-LN detectors use liquid nitrogen to reduce the temperature of the array. The liquid nitrogen is stored in a Dewar that is enclosed in a vacuum jacket for minimal external thermal losses.
-LN System Manual Issue 4 4.10.1 Fill Procedure Perform the following procedure to fill the Dewar on a NIRvana-LN detector: 1. Loosen the retaining nut a few turns, then remove the LN Dewar port cap by pulling it straight out. See Figure 4-5.
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Continuous hissing indicates that the vacuum in the Dewar jacket is probably inadequate. In this case, first remove all LN from the Dewar and allow the Dewar to warm up to room temperature. Then contact Princeton Instruments Customer Support for further instructions. Refer to Contact Information on page 120 for complete information.
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This chapter provides a step-by-step procedure for placing an imaging or spectroscopy system in operation for the first time when using Princeton Instruments’ LightField 64-bit data acquisition software. The intent of this procedure is to gain basic familiarity with the operation of the system and to show that it is functioning properly.
Upon data transfer, the data are displayed and/or stored via the application software. This sequence is illustrated by the block diagram shown in Figure 5-1. Figure 5-1: Light Path Block Diagram for NIRvana-LN Systems Incoming Photons Camera InGaAs Array Analog to Digital Converter...
Shutter Internal Slit Shutter • A shutter mounted internally has an external shutter connector in the sidewall of the spectrograph. Connect a shutter cable from the NIRvana-LN Shutter connector to that connector. Power ON the camera and fill the Dewar.
Available Devices area. In Figure 5-2, the detector being used is a NIRvana-LN: 640 and the spectrograph is an IsoPlane. Figure 5-2: Typical LightField Available Devices Area Drag the icons into the Experiment Devices area. See Figure 5-3.
Chapter 5 LightField First Light Procedure Experiment Settings stack to the left now displays several expanders. Because this is a new experiment, the default settings for the detector are active. Status bar at the bottom of the window displays an icon for temperature status which reports the current temperature and whether the set temperature has been reached.
If the camera is LN-cooled, the Dewar should be filled while the camera is ON. Launch LightField and drag the icons for the NIRvana-LN and the IsoPlane into the area.
REFERENCES: Refer to the IsoPlane User Manual supplied with the spectrograph for complete information. Perform the following procedure to focus the NIRvana-LN with an IsoPlane SCT-320 spectrograph: Remove the cover from the Micrometer Compartment. Use a 3/32” hex wrench to loosen the locking set screw.
™ NIRvana -LN System Manual Issue 4 5.7 Data Collection Perform the following procedure to begin acquiring data: After the system has been rotationally aligned and focused, stop running in Alignment mode. Make any required changes to the experiment’s setup and software parameters. Changes may include adjusting exposure time, setting up an entrance slit shutter, changing timing mode to External Sync, and/or lowering the target temperature.
This chapter provides a step-by-step procedure for placing a spectroscopy system in operation for tthe first time when using Princeton Instruments’ WinSpec/32 data acquisition software. The intent of this procedure is to gain basic familiarity with the operation of the system and to show that it is functioning properly.
Upon data transfer, the data are displayed and/or stored via the application software. This sequence is illustrated by the block diagram shown in Figure 6-1. Figure 6-1: Light Path Block Diagram for NIRvana-LN Systems Incoming Photons Camera InGaAs Array Analog to Digital Converter...
Shutter 6.2 Power On Sequencing The NIRvana-LN camera must be powered on before WinX/32 is launched in order to establish and maintain communication between the NIRvana-LN camera and the host computer. If WinX/32 is launched before the NIRvana-LN has been powered on, many of the functions will be disabled.
™ NIRvana -LN System Manual Issue 4 Connect the shutter cable between the entrance slit shutter and the NIRvana-LN connector. Shutter • External Slit Shutter A shutter assembly mounted externally to the spectrograph has shutter cable that plugs into the connector.
Chapter 6 WinSpec/32 and WinView/32 First Light Procedure From the WinSpec/32 menu bar, select Setup —> Detector Temperature Configure the detector temperature parameters as indicated in Table 6-2. Table 6-2: WinSpec/32 Target Temperature Configuration Parameter Value Notes Target Temperature -190°C This information is read from the camera.
Select the grating to be moved, and set it to an appropriate position. For example, when using a NeAr lamp, set the grating to 763.51 nm. NOTE: The spectral range of a NIRvana-LN is 900 nm to 1600 nm at -190°C. Turn on the light source at the spectrograph entrance slit.
WinSpec/32 and WinView/32 First Light Procedure 6.6 Verify Shutter Operation Perform the following procedure to verify the shutter is operating properly and light is being received at the NIRvana-LN camera: From the WinSpec/32 menu bar, select to begin data Acquisition —> Focus acquisition.
6.7 Rotational Alignment Perform the following procedure to rotationally align a NIRvana-LN camera: Mount a Princeton Instruments light source such as the IntelliCal light source in front of the entrance slit of the spectrograph. With the spectrograph properly connected to the computer, turn the power on, wait for the spectrograph to initialize.
REFERENCES: Refer to the IsoPlane User Manual supplied with the spectrograph for complete information. Perform the following procedure to focus the NIRvana-LN with an IsoPlane SCT-320 spectrograph: Remove the cover from the Micrometer Compartment. Use a 3/32” hex wrench to loosen the locking set screw.
™ NIRvana -LN System Manual Issue 4 6.9 Acquire Data Perform the following procedure to begin acquiring data: After the system has been rotationally aligned and focused, stop running in Focus mode. Make any required changes to the experiment’s setup and software parameters. Changes may include: •...
Chapter 6 WinSpec/32 and WinView/32 First Light Procedure 6.10 Shut Down Procedure Perform the following procedure to shut down the system: Carefully empty the Dewar and store the liquid 1. For liquid nitrogen cooled systems: nitrogen that has been removed. CAUTION! Because of the low operating temperatures, cryogenically-cooled detectors must always remain powered ON when Liquid Nitrogen...
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At the end of the exposure time, the array is read out and cleaning starts again. NOTE: The NIRvana-LN camera has a minimum exposure time of: • 100 μs in 250 kHz mode; •...
Another way to prevent light from falling on the array during readout is to use a 25 mm external shutter which is typically used at a Princeton Instruments supplied spectrograph entrance slit. This shutter can then be controlled by the camera and is...
Exposure and Signal 7.4 Cooling the Array The detector in the NIRvana-LN is cryogenically-cooled. Although the detector can be operated at temperatures in the range of -175°C to -194°C, pixel gain and offset corrections are optimal when the camera is at its default temperature of -190°C. Generally speaking, the lower the array temperature, the lower the dark current and, therefore, the greater the sensitivity.
™ NIRvana -LN System Manual Issue 4 The deepest operating temperature for a system depends on the array size and packaging; and the time required to achieve lock can vary over a considerable range, depending on such factors as the detector type, array type, ambient temperature, etc. Once lock occurs, it is okay to begin focusing.
Chapter 7 Exposure and Signal Figure 7-3: Typical WinSpec/32 Automatic Background Subtraction Dialog NOTES: Although a pattern is repeatable, its profile will change from temperature setting to temperature setting. Therefore, both the background data and the experiment data MUST be acquired at the same locked temperature. In situations where uncorrected/raw data is required, perform background subtraction as a post-acquisition process.
™ NIRvana -LN System Manual Issue 4 7.6 Flatfield Correction The application of Flatfield Correction compensates for any non-uniformity of illumination sources and/or non-uniformity of the InGaAs detector. Applying a flatfield correction is a three-step process: A reference flatfield image must be acquired and saved; •...
Thus, to minimize dark signal effects, the detector temperature should be set for the lowest temperature within the recommended range for the detector. For NIRvana-LN, a default temperature of -190ºC provides the best performance.
The gain choice should be based on the signal intensity. 7.10.1 Region of Interest (ROI) NIRvana-LN supports Region of Interest (ROI) or area selection. While there will be no increase in readout speed, there will be a reduction in the size of the data set.
ADC offset, also known as baseline offset, provides another way of dealing with dark signal. By offsetting the baseline signal, much of the background is ignored during conversion. For the NIRvana-LN, this offset is set at the factory and is not configurable. REFERENCES: For additional information, refer to Section 7.8, Dark...
-LN System Manual Issue 4 All NIRvana-LN arrays have been tested for uniformity and do not exhibit any vignetting (i.e., reduction of response,) at the extreme ends of the array. If a reduction in response is measured across the array, it may be the result of one or more of the following conditions: Water condensation has occurred on the edges of the Dewar window.
• Shutter Trigger 8.1 Shutter Control Modes When an external entrance slit shutter is being controlled by NIRvana-LN, shutter operation can be coordinated with the experiment. Available shutter control modes for Full Frame operation are: Normal; • Disable Opened {Always Open};...
TRIGGER IN AUX I/O rear of the camera. See Figure 8-1. Figure 8-1: Rear Panel Connectors on NIRvana-LN Detector When configuring the trigger input, consider the following criteria: Pulse Height • 0 to +3.3 V logic levels (TTL-compatible).
Chapter 8 Experiment Synchronization 8.2.1 Free Run {No Response} In this mode, there is no external triggering or the camera ignores external triggers, and all settings are obtained from the setup parameters, making the duration of each exposure time constant and the interval times between exposures constant. NOTE: In this timing mode, all shutter modes behave the same way.
™ NIRvana -LN System Manual Issue 4 Figure 8-3: Timing Diagram: External Sync {Readout Per Trigger} RIGGER GNORED GNORED TRIG RIGGER ESET XPOSURE 8.2.3 Bulb Trigger {Expose During Trigger Pulse} When } timing is selected, the camera Bulb Trigger Expose During Trigger Pulse exposure is determined by an external trigger received on the signal through TRIGGER IN...
Fast operation is primarily intended for collecting real-time sequences of experimental data where timing is critical and events cannot be missed. Once the NIRvana-LN has sent the start command by the computer, all frames are collected without further intervention from the computer.
™ NIRvana -LN System Manual Issue 4 Figure 8-5: Fast Mode Operation Flowchart Start (Fast Mode) Computer programs camera with exposure and binning parameters. Start Acquisition command sent from computer to camera. Cleans Performed 1 Frame collected as per timing mode.
Chapter 8 Experiment Synchronization 8.4 TTL OUT Control The TTL-compatible logic level output (0 to +3.3 V ) from the TTL Out connector on the AUX I/O cable can be used to monitor camera status and control external devices. NOTE: By default, TTL OUT is active HIGH.
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™ NIRvana -LN System Manual Issue 4 Additional related signals and configuration settings include: • Logic 1 Always High is always pulled HIGH (1). TTL OUT • Wait for Trigger Waiting For Trigger goes HIGH (1) when the camera is ready to acquire and is waiting for an TTL OUT external trigger from the signal before exposing the CCD.
Typically, data readout operations are destructive in nature. That is, once the collected data are read, a cleaning operation is initiated, and the data are cleared from the FPA. In addition to standard readout operation, NIRvana-LN systems support Non-Destructive Readout (NDRO.) NDRO provides the ability to read data collected without initiating a clean operation making it possible to monitor an experiment’s progress without...
™ NIRvana -LN System Manual Issue 4 Figure 9-2: Typical LightField NDRO Configuration Parameters CAUTION! The configuration values for both Exposure Time and NDRO Period can be changed dynamically (i.e., while an experiment is in progress.) However, if Save NDRO Frames is enabled, and one (or both) of these values are changed while an Experiment is in progress, the experiment/application may crash if there is insufficient disk space.
Chapter 9 Non-Destructive Readout Frame Tracking must be enabled when using NDRO. By default, LightField automatically enables Frame Tracking when NDRO is enabled. However, if Frame Tracking is manually disabled, an Experiment Conflict is reported and displayed within LightField. See Figure 9-4.
™ NIRvana -LN System Manual Issue 4 9.3 Monitoring Experiment Progress An NDRO experiment’s progress is monitored and displayed using several criteria: • Progress Circle Once an experminent has been started, the Progress Circle is displayed to the right of the three (3) Experiment Control buttons. See Figure 9-5.
Chapter 9 Non-Destructive Readout • Number of Frames Indicator Indicates how many frames have been completed with respect to the total number of Destructive Readout frames to be captured. Progress is indicated: — Numerically (e.g., 1 of 8 Frames, 2 of 30 Frames, etc.) —...
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Chapter 10: Troubleshooting WARNING! Do not attach or remove any cables while the NIRvana-LN system is powered on. Recommended troubleshooting guidelines are available for many issues that may occur while working with a NIRvana-LN system. Refer to Table 10-1 for additional information.
™ NIRvana -LN System Manual Issue 4 10.2 Camera1 (or Similarly Named Device) in Camera Name Field When the Camera Detection Wizard installs a new camera, the camera is automatically named Camera#, where # = 1, 2 , 3, ..., depending on the number of cameras detected. This name appears in the title bar on the Hardware Setup dialog, as well as the on the Hardware Setup|Controller/Camera tab.
Hardware Setup dialog. See Figure 10-3 Figure 10-3: Updated Camera Name on Hardware Setup Dialog Hardware Setup: Camera1 Controller/Camera Display Cleans Camera Name Hardware Setup: NIRvana-LN Camera1 Controller/Camera Display Cleans Camera Type: PI 640 x 512 Camera Name:...
™ NIRvana -LN System Manual Issue 4 10.3 Cooling Troubleshooting This section provides recommended troubleshooting guidelines for cooling-related issues. 10.3.1 Temperature Lock cannot be Achieved or Maintained. Possible causes could include: • The vacuum has deteriorated and needs to be refreshed. •...
Chapter 10 Troubleshooting 10.4 Data Overrun Due to Hardware Conflict Message Displayed If this dialog appears when acquiring a test image, acquiring data, or running in focus mode, check the array size and then check the DMA buffer size. A large array (e.g., a 2048x2048 array,) requires a larger DMA buffer larger setting than that for a smaller array (e.g., a 512x512 array.) Figure 10-4: Data Overrun Due to Hardware Conflict Dialog...
Issue 4 10.6 Ethernet Network is Not Accessible When the Princeton Instruments software is installed, all Intel Pro/1000 interface card drivers found on the host computer are updated with the Intel Pro/1000 Grabber Adapter (Vision High-Performance IP Device) driver provided by Pleora Technologies, Inc. If this computer is connected to an Ethernet network via an Intel Pro/1000 card that does not use the Pleora driver, the network connection will be broken.
Chapter 10 Troubleshooting 5. Once the driver installation has been completed, it may be necessary to reboot the computer. If prompted for a reboot, select: • Yes to reboot the host computer immediately, or • NO to delay rebooting the computer until a later time. When delaying the reboot, dismiss/close the eBUS Driver Installation Tool dialog.
™ NIRvana -LN System Manual Issue 4 10.7 Program Error Message Displayed Figure 10-7 illustrates the dialog that may be displayed when attempting to acquire a test image, acquire data, or run in focusing mode and the DMA buffer size is too small. A large array (e.g., a 2048x2048 array,) requires a larger setting than that for a smaller array (e.g., a 512x512 array.) Figure 10-7: Typical Program Error Dialog...
Dewar window even at very wide angles (e.g., > f/1.5.) If vignetting is observed, it is possible that your experiment exceeds these angular constraints. Princeton Instruments measures the array response with a collimated uniform light source to prevent such false bias results.
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• Power Supply Weight: 4 lb (1.8 kg) A.2 Power Specifications All DC voltages required by NIRvana-LN cameras are generated by an external power supply and then delivered to the camera using a custom power cable. Refer to Table A-1 for input power specifications for the external NIRvana-LN Power Supply.
™ NIRvana -LN System Manual Issue 4 A.3 Environmental Specifications Refer to Table A-2 for environmental specifications for the NIRvana-LN system. Table A-2: NIRvana-LN Environmental Specifications Specification Parameter Minimum Nominal Maximum Storage Temperature -20C — +55C Operating Temperature 5ºC —...
Rise Time 100 Duration The AUX I/O connector is located on the rear of the NIRvana-LN chassis. It is a female, DB26, high-density connector. Figure A-1 illustrates the pinout of the AUX I/O connector, viewed from the rear panel of the NIRvana-LN chassis, with each contact/pin identified by its pin number.
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™ NIRvana -LN System Manual Issue 4 Table A-4: AUX I/O Connector Pinout and Signal Descriptions (Sheet 2 of 3) Pin # Signal Name Signal Description System digital ground. Any external circuitry intended to interface with the trigger control signals must reference this ground connection. READOUT MON Active high.
A.5.1 AUX I/O Cable Each NIRvana-LN system includes an AUX I/O cable that provides convenient access to several system signals. The AUX I/O interface cable is comprised of a male DB26 connector on one end, and five female BNC cables on the other end, each of which provides access to a system signal.
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Figure C-1: IsoPlane SCT-320 Spectroscopy-Mount O-RING C.1 Required Items Refer to Table C-1 for the list of items required to prepare the NIRvana-LN to be used with an IsoPlane 320. Table C-1: Required Items Part Number Description Quantity NIRvana-LN Spectroscopy Mount Kit —...
Figure C-2: Removing F-Mount Adapter from NIRvana-LN Nose EMOVE EMOVE Carefully slide the adapter away from the NIRvana-LN to remove the F-Mount Adapter from the camera. Carefully position the spectroscopy adapter on the nose of the NIRvana-LN. Verify all mounting holes in the adapter align with those on the camera.
Appendix C IsoPlane 320 Mounting C.3 Remove Camera Mounting Plate and Cover from IsoPlane 320 Because the NIRvana-LN includes an integrated mounting plate/flange, the camera mounting plate and shipping cover on the IsoPlane, illustrated in Figure C-3, must first be removed.
Replace the o-ring on the adapter making sure it is fully seated within the groove on the adapter. Align the NIRvana-LN spectroscopic adapter with the entrance to the IsoPlane 320 and carefully slide the camera into place. Figure C-5: Mounting NIRvana-LN to an IsoPlane 320 Carefully rotate the NIRvana-LN until the four (4) mounting thru-holes are aligned with the four (4) threaded mounting inserts on the IsoPlane 320.
Plate and Cover from IsoPlane 320, on page 107 through the four (4) thru-holes on the NIRvana-LN and carefully hand-thread them into the IsoPlane 320 inserts. Use a right-angle 9/64 Allen wrench to tighten the four (4) hex-head screws to secure the NIRvana-LN to the IsoPlane 320.
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Appendix D: WinX/LightField Cross Reference This appendix provides cross reference information for terminology used within the WinX and LightField application software packages. D.1 WinX-to-LightField Terminology Refer to Table D-1 for a list of WinX terms and their corresponding LightField terms. Table D-1: WinX-to-LightField Cross Reference (Sheet 1 of 2) WinX Term LightField Term...
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™ NIRvana -LN System Manual Issue 4 Table D-1: WinX-to-LightField Cross Reference (Sheet 2 of 2) WinX Term LightField Term Logic Out: Shutter Output Signal: Shutter Open Minimum Block Size Final Section Height Normal Shutter Normal (Shutter) Number of Blocks Final Section Count Number of Cleans Number of Clean Cycles...
Appendix D WinX/LightField Cross Reference D.2 LightField-to-WinX Terminology Refer to Table D-2 for a list of LightField terms and their corresponding WinX terms. Table D-2: LightField-to-WinX Term Cross Reference (Sheet 1 of 2) LightField WinX Active Area: Bottom Margin Post-Dummy Rows Parallel to Shift Register Active Area: Left Margin Pre-Dummy Shift Register Columns Active Area: Right Margin...
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™ NIRvana -LN System Manual Issue 4 Table D-2: LightField-to-WinX Term Cross Reference (Sheet 2 of 2) LightField WinX Output Signal: Always High (Inverted) Logic Out: Logic 1 (Inverted) Output Signal: Exposing Logic Out: Expose (Program’d) Output Signal: Reading Out Logic Out: Read Out Output Signal: Shutter Open Logic Out: Shutter...
Instruments will repair or replace, at its sole option, any defective parts, without charge to you. You must deliver the entire product to the Princeton Instruments factory or, at our option, a factory-authorized service center. You are responsible for the shipping costs to return the product to Princeton Instruments.
Issue 4 Sealed Chamber Integrity Limited 12 Month Warranty Princeton Instruments warrants the sealed chamber integrity of all our products for a period of twelve (12) months after shipment. If, at anytime within twelve (12) months from the date of delivery, the detector should experience a sealed chamber failure, all parts and labor needed to restore the chamber seal will be covered by us.
(1) year limited warranty and/or any other warranty, expressed or implied. 3. All warranty service must be made by the Princeton Instruments factory or, at our option, an authorized service center.
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