UVProbe is multifunctional, easy-to-use software supplied as standard with Shimadzu UV-VIS Spectrophotometers. The UVProbe is connected to the LabSolutions system, which is known for its capabilities in complying with ER/ES regulations. Enables safe, reliable management of data.Not only can UV data be managed, but the comprehensive management of LC, GC, and FTIR data can also be accomplished.In addition, When combined with CLASS-Agent, it provides powerful support for Part 11 compatibility.
Uv Probe Software Free 18
Uv Probe Software Free DownloadDownload > =2sIi3wresizing a measurement is essentially a rewriting of the measurement type. a typical entry might be to record the time at a specific depth, then a certain distance later, record that distance. (the distance can be relative or absolute.) you can change the measurement type by selecting the measurement type on the measurement type menu and then renumbering or deleting the items on the measurement type menu or by using the sliders on the measurement type menu. to have the measurement re-entered or re-read, simply press the [enter] button.for example, if you entered the time as the measurement, and the length is 5cm, the measurement type would be changed from time to length (5cm). if you enter the distance as the measurement, and the length is 5cm, the measurement type would be changed to length (5cm). as you can measure distance at the x,y, and z measurement types, there were additional custom parameter types that can be entered or reread, such as wavelength.as an example, after you select x and y measurement types, press [enter] to reread the measurement type. as you can distance measurement, there were additional custom parameter types you can record as you proceed with the laboratory log.24 28 introduction photometric data acquisition using the readaui module a right to read the data from the photometric data acquisition using the readaui function. a right to browse the photometric data of the date. a right to cancel the readaui function. selected waveband a right to select the wavelength to be used for the photometric data. selected image type a right to select the image type to be used for the photometric data. continue editing a right to confirm the edited values by selecting the apply button. this button is not available when performing photometric data acquisition using the readaui function. 65a90a948d -istri-lagi-bikin-video-bokep-pribadi3gp -friend-request-full-movie-720p -saath-saath-hain-movie-free-download-hindi-hd -man-3-dubbed-in-hindi-download-mp4
\r\n\tThanks to its unique optical design the Cary 60 UV-Vis spectrophotometer is immune to the distorting effect of room light. Room light immunity enables measurements outside the sample compartment using fiber optic probes. It also allows easy operation of the Cary 60 with an open sample compartment and reduces the risk of compromised data due to handling mistakes.
Kor Software is designed to interface with both EXO and ProDIGITAL (DSS) instruments, including the new ProSwap Logger. Use Kor Software to view live data, import/export recorded data, calibrate sensors, manage handheld settings, set up deployments, and more! This software is included on a USB flash drive that ships with all new instruments, and the latest version can be found here on the website.
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.
It is strongly recommended to update KorDSS to v1.7.4.0, as it features support for all released probe/cable assemblies. This version of KorDSS must be used when updating ProDSS instrument firmware to v1.2.10.
Note: Older MultiLab 4010-1 units can be updated with the latest version of 4010-1W firmware. This firmware allows for the use of wireless MultiLab sensors, the IDS 4100 ProBOD polarographic probe, and the FDO 4410 sensor.
Our flexible sensor design incorporates two vertically stacked sensors to allow the independent discrimination of strain and pressure (Fig. 1b). This is a unique aspect of our technology, because strain gauges and nanocomposite-based strain sensors mounted on a flexible membrane are intrinsically sensitive to both strain and pressure. The strain is determined by measuring the capacitance change between two thin-film comb electrodes sliding relative to each other. They are sandwiched between two stretchable elastomer layers. Meanwhile, pressure is measured with a thin, flexible capacitor with our previously reported microstructured elastic dielectric layer for high sensitivity8,16, while both substrates supporting the top and bottom electrodes, respectively, are bonded on only one side to the stretchable package. This design allows the pressure sensor to be free of the influence of strain.
The OIP (Optical Image Profiler) is a direct push fluorescence detector tool used for the delineation of non-aqueous phase liquid (NAPL) hydrocarbon fuels and oils. The OIP-UV probe is designed with UV and visible light sources which are directed out a sapphire window. As the optical image probe is advanced into the subsurface, the UV light source will induce fluorescence of the fuel polycyclic aromatic hydrocarbons (PAHs). This fluorescence is captured by an onboard camera which operates at 30 images per second. Images are saved throughout the advancement of the log and still photos are taken using UV and visible light sources each rod addition as well as at operator chosen depths. Soil fluorescence images (20 per ft) are saved throughout the log and can be reviewed in Direct Image Viewer after the log is complete. The OIP-G is available for heavier fuel or oil products.
The OIP-UV is a tool for mapping light non-aqueous phase liquids (LNAPL), residual LNAPL, and light oils. The OIP-UV system utilizes a 275nm ultraviolet (UV) light emitting diode (LED) to produce fluorescence from the polycyclic aromatic hydrocarbons (PAHs) contained in fuels and light oils. The UV light is directed out a sapphire window in the side of the probe (Figure 1) onto the soil. When LNAPL level fuels are present, the PAH molecules will absorb the UV light energy and shortly afterwards emit a light photon (fluorophore) which is the resultant fluorescence. Directly behind the sapphire window, the onboard camera captures images of the soil and any fluorescence produced by hydrocarbon contaminants present. The acquisition software analyzes each pixel of the images taken for the presence of color typical of fuel fluorescence. If there is no fuel present in the formation, or it is not in high enough concentration, then the returned camera image will appear black or dark under the UV light source. The OIP acquisition software logs percent area fluorescence with depth. The OIP-UV probe contains a visible as well as UV LEDs. The visible images are useful for determination of soil color, texture and occasionally confirming the presence of fuel or oil LNAPL globules.
The camera within the OIP probe operates at 30 frames per second with the log % area fluorescence (%AF) value being an average of all the images taken over a 0.05ft (1.5cm) interval. As the log is reviewed in Direct Image Viewer, the user can click on the log and a green line will show up across the log which corresponds to a specific depth. The image saved from that depth will display if the OIP Image Display graph is shown. In Figure 2 the depth of the displayed saved image is 24.20ft, it is a UV image with the actual image being displayed in the "captured" image section. The "analyzed" image indicates which pixels within the image display fluorescent color consistent with the color expected for fuel fluorescence. There are two colors that may show up in the analyzed image: red which corresponds to the darker blue colors of the image and green which corresponds to areas of high brightness either due to very low color saturation or high brightness of the image. This is used in an attempt to isolate out possible false mineral fluorescence. The overlaid image takes both the captured image and analyzed image and overlays them so the operator can identify areas that are being counted as fluorescence. Images are saved as the probe is moving for every 0.05ft. The red dots on the right side column of the image display graph are depths that "Still Images" were taken. This will contain both UV and visible light still images on the OIP-UV probe. The OIP-G fluorescence detector probe takes images using a 520nm green laser diode and an infrared LED.
The OIP system software saves 20 images per foot (65 per meter), an example portion of the saved images that an OIP-UV log would contain is shown in Figure 3. These images are saved as the OIP-UV probe is advanced into the subsurface with a typical OIP log containing hundreds of images and being a few hundred mb in size depending upon terminal log depth and amount of color present in the images. Where there is no NAPL or residual NAPL present the images are black, where hydrocarbon NAPL is present blue fluorescence is seen within the images.
The OIP-G log in Figure 5 was performed on a creosote site in the northeast US. The OIP-G probe, which induces fluorescence utilizing a 520nm green laser diode (LD), returns a fluorescence image in the orange-red color range as depicted in the saved images from 10-20ft in the right column of the log. The red dots are the saved still images which are taken with the 520nm green LD and an infrared (IR) LED.
When the probe is stopped to add rods, still images will be captured with both available light sources in the OIP probe. Still images can be captured at any time an operator desires by stopping the probe advancement and selecting a button in the software. The process only takes a few seconds to complete and probe advancement can resume. These still images provide greater image clarity and an opportunity to look at the soil and fuel under visible light. Visible images provide the investigator an opportunity to observe soil color and texture in-situ. Occasionally when hydrocarbon NAPL is present in a saturated sand formation NAPL globules are evident in both the UV and visible images (Figure 6). 2ff7e9595c
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