This is a multifunctional, easy-to-use software supplied as standard with Shimadzu UV-VIS Spectrophotometers. When combined with CLASS-Agent, it provides powerful support for Part 11 compatibility. Reports can be created with a free layout of graphs and tables. The thickness and color of graph lines can be changed, and text and diagrams pasted.
Uv probe software free download
KorEXO v2 is optimized for computers and tablets running Windows OS. The software is included on a USB flash drive that ships with all new EXO Systems. Updates to KorEXO Software are downloaded from the YSI website, along with the latest instrument firmware.
You can download and install the latest operating software by following the steps in this section. Minimum computer and operating system requirements needed to run each NanoDrop instrument are described in the installation section.
The OIP probe (model OP6560, Geoprobe Systems) (U.S. Patent Pending) is approximately 525 mm (20.75 in.) in length and has a maximum diameter of about 50 mm (2.0 in.) with a tapered square body design to enhance contact between the formation and probe (Fig. 2). The probe is equipped with a replaceable sapphire window on one side, having an optical opening of approximately 13 mm. This window allows light from a 275-nm ultraviolet light-emitting diode (UV LED) (approx. 3-mW output) or visible light (vis) LED mounted inside the probe to illuminate the formation outside the window. Peak UV intensity is at the center of the window, and intensity drops to about 80% of peak intensity at the edge of the window. Fluorescence induced by the UV light (or reflected light from the vis LED) passes back through the window to a small CMOS camera mounted inside the probe. The CMOS sensor is a Bayer mosaic sensor which excludes most UV wavelength light so that BTEX fluorescence in the UV range is not detected. Images are captured by the camera at a rate of 30 frames per second (fps), but only one image is saved in the log file for every 15 mm (0.05 ft) of log depth. The images are 9.5 mm 7.0 mm in area with resolution of 640 480 pixels (approx. 0.3 megapixels). The images are analyzed at 30 fps in the acquisition software with a two-stage digital filter (U.S. Patent Pending) based on the HSV (hue, saturation, value) color model (Agoston 2005). Light detected by the camera must meet specified HSV criteria to be identified as UV-induced fluorescent light emitted by hydrocarbon contaminants. The first stage filter sets a minimum brightness level, above this level the hue on a given pixel must fall in a specified blue range to be classified as fuel fluorescence. The second stage filter checks for high brightness, low color saturation pixels. Both filters are summed to determine the percent area (pixels) of each image where fluorescent light is detected. The averaged % area of fluorescence for all images analyzed over each 15 mm (0.05 ft) increment of log is plotted on the log graph. Of course, if there is no fluorescence the images are dark. The captured fluorescence and analyzed images are displayed on-screen as the probe is advanced, along with the EC and percent area of fluorescence (%AF) logs (Fig. 3). When advancement is stopped to add another drive rod, the acquisition software automatically captures a still image of both UV-induced fluorescence and visible light. The operator also can stop probe advancement at any depth of interest and capture UV and visible light still images by pressing an icon on the software screen. Still images (Fig. 4) are typically more clear and sharp than images captured, while the probe is being advanced and may be more useful for understanding soil texture and contaminant distribution in the soil matrix. After the log is completed, the file may be reviewed in the log viewing software (Fig. 3). Each of the images captured during the log, including stills, may be reviewed along with the EC and %AF log. The logs, with selected image, or individual images, may be exported and saved for use in reports or presentations.
A trunk line, pre-strung through the drive rods, connects the downhole probe to the electronic interface (Fig. 2) at the surface which is used to operate the OIP system. A Field Instrument (model FI6000, Geoprobe Systems) provides power for and acquires data from the EC dipole on the probe and from the string potentiometer mounted on the direct push machine. The string potentiometer is used to track the depth and rate of probe advancement. The FI6000 outputs multiple channels of data for presentation on a laptop computer via the acquisition software system. The OIP Interface (model OP6100, Geoprobe Systems) provides power to the two LEDs and the CMOS camera in the downhole probe and receives video image feed which is relayed to the laptop computer for analysis in the acquisition software. A summary of the field logging procedure and QA measures are provided below.
The installer will attempt to download any missing components from Microsoft's website if they're not already installed, but if you will be installing this software on a computer without access to the Internet, you can download the .Net Framework 3.5 here and Windows Installer here.Log Display OptionsThe DI Viewer has three log display options which allow the user to display and compare data quickly and easily to get the most information possible. The software automatically recognizes which log type has been chosen to display. Appropriate graph series will be displayed for the chosen log type. Options are available to view different graph series.
The OIP-UV probe uses a UV LED and visible light camera and is suitable for the delineation of fuels such as gasoline, diesel, etc. In addition to the software-filtered images showing percent areal fluorescence, the OIP-UV also provides the client with full-color images of the soils outside the probe window.
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The PASCO Wireless Spectrometer is fully integrated with our user-friendly Spectrometry Software.This free software is compatible with most student devices, enabling lab groups to quickly share and review their data with ease. Also available as a free, fully functional app, PASCO's cross-platform Spectrometry Software improves the efficiency of analyses with features such as: 2ff7e9595c
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