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Showing posts with label others. Show all posts

DxO Optics Pro V4.2 Reference Manual

DxO Optics Pro V4.2 Reference Manual

DxO Optics Pro’s precise, calibrated corrections are based on unique algorithms derived from actual measurements made on real camera bodies and lenses. Thousands of test measurements are made on each body and lens combination, with every permutation of shooting parameters.

This is why the whole DxO Optics Pro system operates using what are called ‘Correction Modules’, each unique and specific to a particular body / lens combination; for this reason, you need to make sure you have the right module(s) for the bodies and/or lenses you use. All this means that DxO Optics Pro produces extremely accurate actual corrections of measured phenomena, instead of just subjective (and often impossibly time-consuming) manual approximations.

In addition, this new version 4 of the software also includes a number of corrections that are not camera-specific, so you can make the most of other images too, and some adjustments, going beyond purely correction, that you can perform manually for creative effect.

A simple workflow
The way the DxO Optics Pro workflow is organized is perhaps worth explaining briefly. You start by creating a new ‘project’, which you can name and save, and into which you will assemble the pictures you wish to process at this time. You can then click on the “Process Now” button to start processing the images with DxO automatic presets. Alternatively, you can work on preview images to define your own corrections or adjustments. And it’s worth underlining that your original image files are left untouched, they are never altered in any way, deleted, or overwritten, so your precious originals are 100% safe at all times!

What makes DxO Optics Pro even more powerful and ergonomic, is that some or all of your chosen settings can be saved as one or more ‘presets’ that can be applied across a whole series of images — but still leaving you the possibility of making further manual adjustments too, of course! Even without the use of any manual settings at all, DxO Optics Pro can process your images fully automatically, for guaranteed improved results every time!

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TUCIT – X The Ultimate Camera Interval Timer Manual

TUCIT – X The Ultimate Camera Interval Timer Manual

Inventory
1 Tucit - X comes with a plug-in infra-red lamp on a cable, a small piece of velcro, a 9 volt battery holder, a copy of this manual and 2 laminated menu summaries.
2 If your camera is to be controlled by an electrical switch you will need to acquire and attach an appropriate plug to Tucit’s blue lead.
The Name
1 TUCIT stands for The Ultimate Camera Interval Timer. Pronounce it like ‘bucket’ and the X like ‘ex’.

What Can Tucit - X Do?
1 Tucit - X is built for kite aerial photography (kap) and is also used in balloon aerial photography and various other applications.
2 Tucit provides you with 3 alternative ways to trigger your camera; infra-red ‘wireless’ controls or electrical contact switches or servos providing finger actions.
3 It provides control signals for model aeroplane servos to give you panning and tilting movements.
4 Tucit - X allows you to set virtually any interval between pictures and you can have countdown periods from 2 seconds upwards.
5 It can provide double wake-up signals for cameras which fall into sleep mode after long intervals. And, for example for film cameras, you can set a limit to the number of pictures taken each time.
6 A rig moves menu provides a number of movement options for camera rigs with either pan or pan and tilt servos. These include panning with occasional vertical lookdowns as well as three and four level panning.
7 There is a batch mode which lets you take pictures in groups - like panoramas with resting periods in between. And there’s a series mode which may help your camera to take bracketed exposures – i.e. a series of 3 pictures between every move. Alternatively it can hold down (delay) finger shutters to take burst or bracketed shots.
8 There is also a kap session menu so that you can achieve multiple objectives whilst your camera is in the air. Or just use it to stop pictures and tilt upwards for landing.

Bipolar/Monopolar Temperature Controller Model TC-202A User’s Manual

Bipolar/Monopolar Temperature Controller Model TC-202A User’s Manual

The Bipolar/Monopolar Temperature Controller (Model TC-202A) is designed to be used with several micro-incubators supplied by Harvard Apparatus Inc.These models include the Open Perfusion Micro-Incubator (Model PDMI-2), Patch Slice Micro-Incubator (Model PSMI),Leiden Static Micro-Incubator (Model LU-CB1) Leiden Closed Perfusion Micro-Incubator (Model LU-CPC-CEH) and Brain/Tissue Slice System (Model BSC-BU).

A micro-incubation system from Harvard Apparatus consists of the Temperature Controller (TC-202A),a micro-incubator (one of the above) of choice,a 35 mm plastic Petri dish or reusable cover slip dish (LU-CSD, MSC-TD or MSC-PTD) and an associated pumping system.Such a system allows complete environmental conditioning along with excellent micro-mechanical access for electrodes or micropipettes, all with optimum optical access.

A proportional temperature controller is basically a source of electric current whose magnitude is determined by comparing a desired target temperature with its current value. The TC-202A’s output is proportional to the difference in temperature between the desired and the current value. This type of system avoids the electrical noise of suddenly turning current on and off, unlike less expensive controllers. When using the TC-202A in the Biphasic mode, the current will spontaneously reverse direction when the current temperature is too high; in short,it can also cool when used with Peltier elements.(PDMI-2/PSMI)

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GE4000 User Manual

GE4000 User Manual

The GE4000 series of cameras are sensitive, 5 frames per second, 11 megapixel, Gigabit Ethernet cameras based on the Kodak KAI-11002 CCD sensor.

Supported Features
Imaging Modes
free-running, external trigger, fixed rate, software trigger
Fixed Rate Control
0.001 fps to maximum frame rate
External Trigger Delay 0 to 60 seconds in 1 microsecond increments
External Trigger Event rising edge, falling edge, any edge, level high, level low
Exposure Time
140 microseconds to 60 seconds in 1 microsecond increments
Gain
0 to 25dB
Region of Interest (ROI) independent x and y control with 1 pixel resolution***
Horizontal Binning
1 to 8 pixels
Vertical Binning
1 to full resolution of sensor***
Pixel Formats
Mono8, Mono16*, Bayer8, Bayer16
Sync Out Modes
trigger ready, trigger input, exposing, readout, imaging, strobe, GPO

The General Purpose I/O port uses a Hirose HR10A-10R-12SB connector on the camera side. The mating cable connector is Hirose HR10A-10P-12P. This connector can be purchased from Prosilica or from http://www.digikey.com.
See Addendum for more detail.
DO NOT EXCEED 5.5V ON SIGNAL INPUTS.
All inputs and outputs are galvanically isolated from the internal camera circuitry.

TRIGGER INPUT
This input signal allows the camera to be synchronized to some external event. The camera can be programmed to trigger on the rising or falling edge of this signal. The camera can also be programmed to capture an image at some programmable delay time after the trigger event.

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ST-402 Operating Manual

ST-402 Operating Manual

Congratulations and thank you for buying one of our ST-402 cooled CCD cameras. The ST-402 has the following features:
• Uses Kodak’s microlensed, blue enhanced KAF-0402ME CCD with 765 x 510 9-micron square pixels.
• 16-bit A/D converter with correlated double sampling running at 1.8 megahertz.
• Temperature regulated Thermo-Electric (TE) cooling with 25C delta for reduction in CCD dark current.
• Single board, small, compact design with internal shutter allowing exposures down to 40 milliseconds that makes taking dark frames a trivial task.
• USB 2 interface yielding up to 1.2 megapixels per second download rates but full backward compatibility with USB 1.1 computers at 400 kilopixels per second.
• Input power requirements of 10.0 – 14.5 Volts DC at 1 Amp through the new center-positive locking power jack.
• Telescope interface with four optically isolated normally open signals on the industry standard RJ-11 jack.
• T-Thread based mechanical interface that supports a variety of nosepieces and adapters.
• Optional 4-position filter wheel with parfocal Red, Green, Blue and Clear filters.
• Powerful yet intuitive CCDOps software for image acquisition and processing.

Getting Started
In addition to this truly fine Operating Manual, the ST-402 package includes the following items:
ST-402 Camera – The camera body is 4 x 5 x 2 inches with a T-Thread adapter on the front cover. 1 ¼ Inch T-Thread Nosepiece – This screws into the front of the camera for telescope work and includes a soft rubber cap for keeping out the dust when not in use. Optional 2 Inch Nosepiece and Visual Back adapters are available from SBIG. In addition a screw-in T-to-C adapter is available for use with C-Mount camera lenses or C-Mount adapters.

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PriorLux - PriorLab Manual W2968 Issue B

PriorLux - PriorLab Manual W2968 Issue B

The PriorLab and PriorLux upright compound microscopes are high quality instruments equipped with high resolution, chromatically corrected optics for excellent image quality. The robust construction and hard wearing materials ensure long lasting and trouble free operation. The instrument can be used with a number of accessories allowing brightfield, dark ground, phase contrast and polarising contrast observations. For documentation, both instruments are available with a trinocular head which permits mounting of a video or digital camera system.

The PriorLab / PriorLux is shipped in protective bags within a pre-formed container. Each component should be carefully unpacked and checked, cutting rather than tearing the plastic bags. The head (binocular or trinocular) should be fitted to the dovetail on top of the stand and locked in place with the head locking screw. The eyepieces then just drop into the eyepiece tubes at the front of the head, these should be pushed in as far as they will go. Remove each objective lens from its protective “pot” and screw into the free positions on the nosepiece. Move the stage and the condenser carrier to the highest position and insert the condenser from underneath with the diaphragm control facing to the front. This is locked in position with the clamping screw, which is fitted from the side.

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Movable Top Plate (MTP) User Manual

Movable Top Plate (MTP) User Manual

You are now the owner of a Scientifica Movable Top Plate (MTP). Once set up the MTP will provide you with a stable platform from which to carry out your experiments.
Remember:
To get the best performance out of your platform you must set it up correctly. Please follow the steps in this manual to ensure the platform is set up in accordance with manufacturers guidelines.
Special shipping brackets are provided for your MTP to prevent damage during shipment.
Step 1.
Remove the shipping brackets using the Hex Key provided.
Step 2.
Setting the correct length of your platform leg.
It is absolutely essential that you ensure the legs are all the same height. Any differences in leg length will reduce the smoothness of the stage motion and damage the bearings.
A digital vernier caliper has been provided to make this process easy.
It is important to ensure that the platform height is set to correct focal point of your microscope.
(This information should be supplied by your microscope Manufacturer – Olympus, Zeiss, Leica, Nikon). Once you have decided on the correct height, use the digital calipers to ensue that all four of the MTP legs are the same height. This can be checked by measuring the gap between the top of the locking ring to underside of the top of leg.

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ZenithStar 80 Instruction Manual

ZenithStar 80 Instruction Manual

This simple step-by-step instruction manual is designed to provide you with a better understanding of how to use your new telescope. It will also guide you through how to maintain the ZenithStar 80 and operate it at its utmost capabilities. Please carefully familiarize yourself with your telescope parts and its functions before operation.

During daytime usage and night time observation, depending on your range of application, you have many choices for precision eyepieces with different magnifications.

Your new ZenithStar 80 is exceptionally suitable for nebulae, clusters, large galaxies and comets: we therefore suggest you use low power, wide-angle eyepieces for best results. Viewing the moon and planets at up to 120x (power) is quite impressive too at stable seeing. You can easily locate an object in its surrounding with lower magnification, and then gradually zoom-in with higher power eyepieces for maximum close-up and vivid details.

The largest field of view is covered by 12x low power wide-angle eyepieces. Do not exceed the suggested maximum magnification of 120x as the seeing might deteriorate so that nothing is gained in terms of perceiving more and better details. To calculate the magnification of your telescope, divide the telescope focal length in mm (480) by the eyepiece focal length. For example, a 25 mm focal length eyepiece will produce 480/25 = 19x.

Be sure to operate with a stable tripod. Other options include German equatorial mounts, which are used by most amateur astronomers for precise tracking stability. Optional WO mounting rings and plates, and 2″ diagonal mirror or erecting prism are highly recommended for high-quality images. Though this telescope is not specifically designed for astrophotography it can yield very good results when used together with the necessary equipment. Please refer to our Accessories Chart on page 03 for more details on the photo equipment you need.

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JTS-Rotator SPH Manual

JTS-Rotator SPH Manual

JTS-Rotator SPH, produced by Esaypano, is designed for professional shooting of high quality image, including rotator and bracket. JTS-Rotator allows photographer to take sequential constant-angle shots around a single axis with the nodal point of camera and lens in line with the center of panoramic rotation. JTS-Rotator has several advantages in taking pictures:
Supports top and bottom images shooting;
Supports adjusting vertically and horizontally, fore-and-aft adjusting as well; Easy to carry about, with total weight of less than 1.5kg; Wear well again abrasion, made of alloyed material together with strong screws and accurate calibration; Not necessary to repeat calibration setup after you have made correct alignment of optical axis and nodal point

Structure of Rotator
Three jamming screws allow photographer to fix and rotate the rotator more easily with one for locking completely and other two for horizontal every 45 and 60 degree rotating respectively. A slight “click” will help photographer to know how many degree you have rotated without the need to look at the calibration while taking photos from different angles horizontally.

For example, if you don’t need to shoot image from different angles horizontally, please fix the screw “LOCK” only with other two loosening; if you want to get full circular or full frame image, you may need to tighten 60-degree jamming screw and loose the other two, one “click” saying 60 degree while two for 120 degree and three 180 degree; if you want to shoot drum image, 45-degree jamming screw will help you in the same way as 60-degree jamming screw.

The screw on the top of the rotator is used to fix the bracket, which is an indispensable part of JTS-Rotator SPH, and which is a critical part in shooting image successfully.

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Pixagent ITP Version 2.0 User Manual

Pixagent ITP Version 2.0 User Manual

Thank you for downloading ITP version 2.0! ITP is a powerful workflow solution for digital photographers and provides a wide variety of features to help you to get your work done faster. In addition to this functionality, ITP 2.0 is also much easier to set up than any product before it - allowing users of all levels to be up and running in no time. This manual provides detailed instructions on the administration and use of this extensive package, for both Standard and Professional editions. Note that this document is designed as a reference manual, if you are looking for step-by-step instructions you should look at the accompanying setup guides available on our website.

This version is being supplied in two separate editions - standard and professional. The standard edition is provided as freeware, and may be used without payment - it covers the basic functionality needed to get wireless transmission working. The professional version is a commercial product, and may only be used by individuals who have purchased a licence from Pixagent. It offers a host of powerful functions such as memory card synchronization, full-screen live image review, slideshows and more - if you would like to try these features, there is a 30-day free demo period available on download. Please read on for more details!

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ExpoCap Instructions Custom White Balance Aid

ExpoCap Instructions Custom White Balance Aid

Before using your new ExpoCap Custom White Balance Aid, please refer to your camera manual for specific instructions on how to set a custom white balance.

IMPORTANT: Do not point your camera directly at the sun without the ExpoCap installed. Direct sunlight may damage or destroy your camera’s image sensor.

Custom White Balance (WB)
Setting a custom white balance on your digital camera will help you get better color under many difficult lighting conditions. Using the ExpoCap to help set the custom white balance is simply the quickest and easiest way to help your camera capture richer, more beautiful colors.

Installation
Squeeze the two buttons on the exterior of the filter ring and insert the ExpoCap into the threaded recess in front of your camera lens. To remove the ExpoCap, simply reverse this action.

Stacking ExpoCap With Other Filters
The ExpoCap can be installed and used as intended over other camera filters, such as Skylight or Polarizing filters. Note that any color characteristics introduced by filters stacked with the ExpoCap during the custom white balance procedure will be neutralized in the process. If color correction from a filter is desired, then the custom white balance must be taken without the desired filter in place.

Proper Exposure
It is essential to obtain a proper exposure while setting a custom WB. Failure to do so may result in the inability to set a correct balance. The most convenient way to obtain a proper exposure through the ExpoCap is to use an automatic exposure (AE) setting such as the “P” “S” or “A” modes.

How to Set a Custom WB Using ExpoCap
Install the ExpoCap on the end of the lens. Set your camera to an AE mode, set your focus to manual (your camera may not respond in auto focus with the disc installed), then press the shutter release button. Select or save this setting or the resulting image as the reference for your custom white balance. You must set a different custom white balance for each change in lighting.

Where to Aim the Camera
The best results are obtained by standing near, or in similar lighting as your subject and pointing the camera back towards the position from which you will take the picture. In other words, the same color of light falling on your subject must also strike the front surface of the ExpoDisc. See the following examples for tips in some common lighting conditions.
Artificial Light
1. Single Light Source. Aim the camera towards the light source.
2. Dual Light Source. Aim the camera midway between the lights

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Multi-Sensor Core Logger Manual

Multi-Sensor Core Logger Manual

This introduction presents an overview of the capabilities and features of the Multi-Sensor Core Logger (MSCL). Itdescribes the major features of the logging systems and outlines variations that occur between different generations of logging systems. The organisation and use of this manual are described, notational conventions safety symbols and abbreviations are explained.

The Multi-Sensor Core Logger (MSCL)
The Geotek Multi-Sensor Core logger has been built for a range of users since 1989. During that time the logging system has inevitably evolved with significant improvements being made to the simplicity of the mechanical arrangements, the effectiveness of the sensors and in particular with the sophistication of the software. Consequently there are a number of slightly different systems in use. Despite this natural evolution Geotek has been conscious of the need to update older systems so that important new features can be incorporated. This is particularly true with the software, which has been designed to function on all systems with only minor modifications to the electronics and hardware. If you find features described in this manual that do not seem to apply to your system then contact Geotek directly for an assessment of the upgrade potential.

Types of Logging Systems
Single Section - Whole Cores - Core Boat
Early versions of the logger moved the core sections through the sensor systems using a core boat in which each whole core section was placed. Each core section was logged individually. Data files were subsequently manually concatenated by the user within a spreadsheet.

Single Section - Whole Cores - Core Pusher - Long Belt
Later versions of the logger did not have a core boat. They moved individual whole core sections through the sensor systems by using a core pusher to push individual core sections (lying on plastic rails) through the system. This was achieved using a long belt that went around the complete length of the track, through the sensor systems and was attached to the core pusher.

Multiple Sections - Whole Cores - Core Pusher - Short Belt
Recent versions of the logger have maintained the core pusher principle but have a short belt which allows the pusher only to move along the right hand section. Cores are passed through the complete sensor array by butting adjacent cores together. In this way a continuous core logging process is achieved with continuous data sets for a complete core.

Multiple Sections - Split Cores - Core Pusher - Short Belt or Ball-screw
The most versatile logging system is now the split core logging system that is floor mounted and measures p-wave Velocity and Gamma Density either horizontally through whole cores or vertically through whole or split cores. It features a moving vertical slide onto which is mounted the upper p-wave transducer (either the older type that required water coupling or the new Acoustic Rolling Contact (ARC) type). This automated vertical slide enables the measurements to be performed on horizontally split cores as well as whole rounds. With this system there is a large degree of flexibility that enables other sensor systems to be attached.

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ADB Potenza Remote Instruction Manual

ADB Potenza Remote Instruction Manual

Programming Remote Control
Your remote control can handle several devices. However, first you have to set up your remote control for your equipment. You can do this in one of the following ways:
Brand Setup
First, find the manufacturer of your equipment on the Brand Codes list. If the manufacturer’s brand is not listed, go to Automatic
Search below. To set up your remote control follow these steps:
1. Turn the device on.
2. Press TV / AUD / DVD / AUX / STB depending on what mode you want to handle and then hold RCU SETUP until the device key blinks twice.
3. Enter one of the codes from the list. If the code was correct the mode key blinks twice. If not, the key emits one long blink. Then, you will have to repeat steps 2 and 3 until entering the correct code.
4. Press POWER. If the device has turned off, you have chosen the right code. If none of the codes work, try Automatic Search.

Automatic Search
Automatic Search should only be undertaken if none of the brand codes works or your brand name is not listed. Use the Automatic Search option.
1. Switch on your device. Then press appropriate mode key, for example TV if you want to set up a TV.
2. Press and hold RCU SETUP until the mode key blinks twice.
3. Press 9 9 1. The mode key blinks twice.
4. Aim the remote at the device and press POWER.
5. Press CH + and CH- repeatedly until the device is switched off.
6. Press POWER to turn the TV on.
7. Next, press RCU SETUP to store the code for your device. The mode key blinks twice. Your remote control is now programmed to operate your TV set.
8. To search codes for other devices repeat steps 1 through 7, but substitute the TV key with the appropriate one for the mode you are searching for.

Finding Your Code
If you want to know what code operates your device, you can obtain it with the Device Code option. To find out the code, follow these instructions:
1. Switch on your device. Then press appropriate mode key, for example TV if you want to set up a TV.
2. Press and hold the RCU SETUP until the mode key blinks twice.
3. Press 9 9 0. The mode key blinks twice.
4. For the first digit of your code, press 1 and count the number of times the key blinks (e.g. 2 blinks = 2). If the light does not blink, the digit is 0. For the second digit press 2 and count the number of blinks. Do the same for the remaining digits.
5. To check for other device codes, repeat the above steps, but substitute the TV key with the appropriate one for the device you are checking.

Using Learning
Your remote control includes a learning feature. It means you can transfer some unique functions from the remote control of other device to this remote control.
1. Press RCU SETUP until the last selected mode key blinks twice. Then press 9 7 5.
2. Press the mode key. For example to transfer a function from DVD remote control press DVD.
3. Press the key on which the function will be stored.
4. Place your remote control and the device remote control (e.g. your DVD remote control) head-to-head, about 5 centimeters / 2 inches apart.
5. On the device remote, press and hold the key to be learned. The target remote control will blink rapidly and turn off. Keep holding the key on the device remote control until the device key on the target remote blinks twice.
6. If the learning failed, the device key emits one long blink. You will have to repeat step 5.

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KR-V9090 Instruction Manual

KR-V9090 Instruction Manual

Compared to standard remote controls, the remote control supplied with this receiver has several operation modes. These modes enable the remote control to control other audio/video components. In order to effectively use the remote control it is important to read the operating instructions and obtain a proper understanding of the remote control and how to switch its operation modes (etc.). Using the remote control without completely understanding its design and how to switch the operation modes may result in incorrect operations.

True home theater sound
This receiver incorporates a wide variety of surround modes to bring you maximum enjoyment from your video software. Select a surround mode according to your equipment or the software you are going to play and enjoy!
Dolby Pro Logic & Dolby 3 Stereo
This surround system reproduces theater-like surround sound from video software marked

The PRO LOGIC mode uses the built-in directivity enhancer circuit to control the Left, Center, Right and Surround channel audio signals and reproduce a real sense of sound motion . The 3 STEREO mode uses the directivity enhancer circuit to provide proper acoustic positioning and a real sense of sound motion even when only the front and center speakers are used.

New DSP surround modes
The DSP (Digital Signal Processor) used for this receiver incorporates a variety of high quality adjustable sound fields, like “ARENA”, “JAZZ CLUB” and “STADIUM”, to add the “presence” associated with an arena, jazz club or stadium to the original signal. It is compatible with almost any kind of program source.

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Multiple Wavelength Multiviewer Operation Manual

Multiple Wavelength Multiviewer Operation Manual

The Multiviewer is a complete system for multispectral imaging. It allows two images to be collected simultaneously using Princeton Instruments CCD or ICCD cameras. It features high throughput dichroic optics and UV wavelength operation as an option. Princeton Instruments multiple wavelength Multiviewer system offers the following features:
• One image projected in dual wavelengths simultaneously on a single CCD or ICCD
• No filter wheel delays and no shot-to-shot variation
• No parallax. All images are taken from the same perspective
• UV operation to 200 nm (optional)
• High throughput dichroic optics
• Low stray light

Performance Considerations
The Multiviewer design allows an image to be acquired at two different wavelengths simultaneously. With a gated intensified camera, both images can be acquired in as little as 5 nanoseconds. This means that even transient events can now be recorded at multiple wavelengths. This eliminates problems of shot-to-shot variability that occur when recording a transient event at multiple wavelengths by recording successive occurrences. With a Multiviewer, the complete multispectral image is acquired in a single shot.

Even for slowly moving subjects, simultaneous imaging provides an advantage. While the morphology of a subject may not change very quickly, the intensity at an individual pixel can change abruptly due to slow movement of a sharp edge across the pixel. Ratio images created from successive frames taken at different wavelengths often contain artifacts due to this effect. Simultaneous dual-wavelength imaging eliminates this ambiguity.

Whether a system is designed for operation on transient or slowly changing subjects, the elimination of moving filter systems improves overall system reliability. Since the Multiviewer has no moving parts, the reliability is much higher. The passive design also requires no computer control and has no power requirements.

Get pdf Multiple Wavelength Multiviewer Operation Manual

PocketWizard MultiMAX Owner’s Manual

PocketWizard MultiMAX Owner’s Manual

The PocketWizard MultiMAX is a microprocessor-based radio slave system that uses advanced digital signaling to increase triggering range, reliability and reject radio noise from other sources. Since is utilizes Transceiver technology, it is both a transmitter and a receiver all in one. It is the most innovative and advanced wireless solution in the photographic industry.

As a stand-alone unit, the MultiMAX offers precision special effects functions not available in any wireless triggering device. It incorporates integrated Trigger Time Control software, True Trigger Confirmation and Selective Quad Triggering, all of which offer solutions to photographic challenges that hinder today’s photographer’s creativity. Unparalleled in features and performance, the PocketWizard MultiMAX is more than just a radio slave.

The MultiMAX displays remaining battery life with a 3 segment battery icon in the upper left corner of the LCD:
3 segments displayed = batteries are fresh/new
2 segments displayed = batteries are good
1 segment displayed = replace batteries soon
0 segments displayed = install fresh/new batteries immediately

With one set of standard Alkaline batteries the MultiMAX will operate for approximately 60 hours. When using Intervalometer or Multipop modes exclusively, battery life can be 200 – 300 hours. This time may vary depending on temperature, battery type, and the quality of batteries used. Extensive use of back light, speaker, or extended trigger contact times will consume the batteries at a faster rate.

The MultiMAX continually regulates the battery power which gives excellent performance throughout the life of the batteries. The unit will continue to function normally until the batteries are nearly exhausted.

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MobileTSM User Guide

MobileTSM User Guide

Getting Ready to Use MobileTSM
Bluetooth Setting
For the serial Bluetooth device (Promi), it needs to be charge so that it has the sufficient power to do your survey measurement. It is provide with its own power charger which you just need to plug in to the Bluetooth device. Remember also to check whether the communication between two Bluetooth is still connect or disconnect by navigate to My Bluetooth Places icon and search for the generic serial that you are using. The generic serial will tell you whether is disconnect or connected

Pairing a New Bluetooth Device
Before you start using a Bluetooth device, you need to pair up your Bluetooth devices; the USB Bluetooth (to be attached to the Tablet PC) between the serial Bluetooth attachment (to be attached to the total station). Pairing the devices allow you to avoid entering access information each time a connection is attempted. Paired devices share a unique link key, which they exchange each time they connect.
1. To start initiating your Bluetooth pairing, click on the
Start > Bluetooth Manager shown at above Note: Remember to plug in your USB Bluetooth into the Tablet PC and make sure the other Bluetooth device is ON before doing any pairing. The Bluetooth icon in your system tray will be in white colour once plugged in.
2. Click on the New menu > Connect!. A Connection Wizard screen will show up.
3. Click the Explore a Bluetooth device then click Next to continue the process.
4. A Bluetooth Connection Wizard: Explore a Bluetooth device screen will come out as follow. To select a device, tap inside the device selection box above.
5. After the list inside Bluetooth Browser screen appears as following, choose a device. Tap Next to continue or Back to return to the previous screen. To exit without completing the connection, tap Cancel.

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Wi-Pics Operations Manual

Wi-Pics Operations Manual

Wi-Pics TM was designed with the philosophy that photographers should be free to devote their time and attention to capturing great images, without being disk-jockeys or couriers for flash memory cards. Wi-Pics TM replaces a photographer’s CompactFlash™ storage card during digital image capture.

After Wi-Pics TM has been powered-on, it emulates the behavior of a typical CompactFlash™ memory card. Image files recorded by the camera are stored on an internal hard disk drive, or on supplemental CompactFlash™ storage cards inserted into the Wi-Pics TM unit by the user. When the software in Wi-Pics TM detects the recording of an image by the camera, the image can be transmitted to a remote workstation or server via the unit’s wireless or wired network interfaces.

Wi-Pics™ is a patent-pending network appliance designed to allow any Type II CompactFlash TM compatible digital camera to transmit images via wireless and wired networks. Use of Wi-Pics™ requires no modification of camera hardware or firmware, and does not impact camera buffer performance or battery life. What makes Wi-Pics unique from other wireless options is its data association.

Data association is the ability to rename files with critical search data at the moment of capture and to place that data into the EXIF header of a JPEG file. Wi-Pics™ solves the problem of moving images from Point A to Point B, while adding the capability to easily search and retrieve images directly after they are captured.

Wi-Pics™ provides photographers with connectivity to transfer their images instantly and automatically to a remote server or workstation, and simultaneously provides redundant backup image storage.

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Keeler Slit Lamp Instructions

Keeler Slit Lamp Instructions

Keeler Slit Lamps are instruments designed to give a very high level of performance. In order to ensure you gain the maximum benefits from your Keeler Slit Lamp we suggest that you read this instruction manual carefully before assembly or use. Please be sure to check all warning or rating labels on your Slit Lamp.

Main features of Keeler Slit Lamps
• Keeler Slit Lamps are combination of outstanding optical performance combined with elegant yet functional design.
• Quality optics to reduce eye fatigue and to ensure clear crisp images.
• X-Y-Z base with single joystick control.
• Stereo microscope body with magnifications of x10 and x16, x6 to x40 or x6 to x33 zoom depending on model.
• Accessories for attaching digital cameras, cctv cameras, teaching tube. Tonometers.
• Tilt facility 5°, 10°, 15°, 20° (Tower illumination systems only).
• Optional filters, diffusers.
• Optional measuring eyepieces.

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Charge Preamplifiers ICP 100/110/120 Operators Manual

Charge Preamplifiers ICP 100/110/120 Operators Manual

The Charge Preamplifiers ICP1×0 are used for piezoelectric transducers with charge output. These types of transducers are frequently given preference over ICP® compatible transducers because of their smaller dimensions and their higher dynamic range. Sometimes high temperature at the measuring point does not allow electronic circuits near to this place. The Charge Preamplifiers ICP1×0 have an ICP® compatible voltage output with low impedance. The output signal can be transmitted over long distances using inexpensive coaxial cables. The ICP1×0 is supplied by constant current via the output cable. Therefore, a special cable for power supply is not required.

Function
The abbreviation ICP® means “Integrated Circuit Piezoelectric”. It has been established be- tween many other brand names as
industrial standard for piezoelectric transducers. The integrated circuit of the Charge Preamplifier transforms the charge signal of the piezo ceramics, with its very high impedance and high sensitivity against interference, into a voltage signal with low impedance. This signal may be transmitted and processed much easier than the high impedance charge signal.

The distinguishing feature of the integrated circuits for impedance transformation is, that power supply and measuring signal are transmitted via the same cable. Figure 1 shows the circuit diagram. For easy separation of the low impedance output signal from the power supply, the amplifier circuit is supplied with constant current. This constant current has to be fed into the measuring line.

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