search.noResults

search.searching

note.createNoteMessage

search.noResults

search.searching

orderForm.title

orderForm.productCode
orderForm.description
orderForm.quantity
orderForm.itemPrice
orderForm.price
orderForm.totalPrice
orderForm.deliveryDetails.billingAddress
orderForm.deliveryDetails.deliveryAddress
orderForm.noItems
25 Pre-defi ned Method


For convenient routine analysis, the UV7 spectrophotometer contains a pre-defi ned method for the identifi cation of vitamin B12, which includes the spectrum scan and the automatic evaluation of the relevant results. The peaks in the spectrum are identifi ed and their locations are compared to the nominal data, taking into account permitted tolerances.


The absorbance ratios are also automatically calculated and compared to the nominal values so that the fi nal result displays all acceptance criteria for the identifi cation of cyanocobalamin. The method can be edited to suit user requirements.


Using the UV7 Excellence spectrophotometer, cyanocobalamin identifi cation is a simple, fast and effi cient method, with automatic evaluation reducing the risk of error.


Table 1. Acceptance criteria and measured results of a cyanocobalamin sample. References


a measured Vitamin B12 sample. All criteria were fulfi lled, confi rming the identity and purity of cyanocobalamin in the sample.


1. Görög, S. Ultraviolet-visible spectrophotometry in pharmaceutical analysis, 1995, CRC Press.


Read, Share and Comment on this Article, visit: www.labmate-online.com/article New Spectrometer Offers Higher Acquisition Speed for Light Measurement


Ocean Optics has upgraded its Ocean FX miniature spectrometer to now offer an acquisition speed of up to 4,500 scans per second, high-sensitivity CMOS detector performance and integration times as low as 10 µs. With fl exible features to manage saturation intensity, it is suitable for high-intensity LED and light source measurement, laser characterisation, spectral analysis of rapid events and plasma monitoring.


Depending on the performance of the operating system to which it is connected, Ocean FX can acquire up to 4,500 scans per second. This speed allows users to collect more spectral information over shorter periods of time, contributing to better results. The high speed is also useful for capturing rapidly occurring modulation of light output, such as fl icker in LEDs and other sources (see Ocean Optics Application Note:https://oceanoptics.com/ocean-fx-high- speed-applications-in-home-lighting/). The powerful onboard processor holds up to 50,000 spectra in its memory and can perform averaging of up to 5,000 spectra, signifi cantly speeding up transfer times and reducing bandwidth requirements.


Ocean FX is anchored by a high-sensitivity CMOS detector that is responsive from 200-1,100 nm. To account for varying light intensity, its adjustable integration time ranges from 10 seconds down to 10 µs. This ability to integrate over much briefer periods - microseconds instead of milliseconds - avoids saturating the detector in even extremely high-intensity applications. Ocean FX’s interchangeable slits give users the ability to further adjust for differences in light source intensity.


Users can operate the Ocean FX via Gigabit Ethernet, Wi-Fi, USB and now SPI communication protocols. The addition gives OEM users greater design fl exibility, eliminating the need for cables or additional circuitry to convert signals. Ocean FX is available in versions optimised for the UV-Vis (200-850 nm), Vis-NIR (350-1,000 nm) and extended (200-1,025 nm) wavelength ranges. Enhanced-sensitivity, custom and OEM confi gurations are also available.


44502pr@reply-direct.com Laser Gas Detection TDLS Technology


Axetris uses proprietary technology-enhanced TDLS for gas detection. A 0.05 nm narrow bandwidth diode laser beam is used to scan across an absorption band of the target gas, thus performing a high-resolution near infrared absorption measurement.


Laser gas detection, based on Tunable Diode Laser Spectroscopy or TDLS, provides a valid solution to many challenges in environmental gas monitoring and process control.


The TDLS technology offers unique advantages: precise optical, contactless measurements; excellent target gas selectivity; sub ppm-level detectivity for gases such as CH4, NH3, HCl, H2O and CO2; low cost of ownership; high stability, reliability and availability in the fi eld (no regular replacements/ calibration needed).


Axetris’ laser gas sensing modules are a cost effective solution for OEM integrators active in emission control and environmental monitoring. It allows for simple integration due to its self-contained and standalone system design. It also offers hot-gas measurements up to 220°C, which provide a robust sensing solution for highly contaminated gas sample typically for SCR DeNOx and other applications. With these gas sensing modules, Axetris are able to cover a wide range of gas monitoring & detection applications in combustion control, leak detection, breath gas analysis, greenhouse gas monitoring, safety and many more.


45000pr@reply-direct.com


Mass spectrometers for vacuum, gas, plasma and surface science


PITTCON 2018 Visit us on Booth 1360


QGA Gas Analysis System Fast data acquisition


Instruments 8688ad@reply-direct.com WWW.LABMATE-ONLINE.COM


500 measurements/sec Response time to 150 ms Dynamic range PPB


to 100% for Advanced Science W www.HidenAnalytical.com


Microreactor with integrated MS detector


TPD/TPR/TPO and reaction studies


1-20°C/min heating rates


Temperature ramps up to 1000°C


Close-coupled hotzone for 500 ms response


E info@hiden.co.uk


Page 1  |  Page 2  |  Page 3  |  Page 4  |  Page 5  |  Page 6  |  Page 7  |  Page 8  |  Page 9  |  Page 10  |  Page 11  |  Page 12  |  Page 13  |  Page 14  |  Page 15  |  Page 16  |  Page 17  |  Page 18  |  Page 19  |  Page 20  |  Page 21  |  Page 22  |  Page 23  |  Page 24  |  Page 25  |  Page 26  |  Page 27  |  Page 28  |  Page 29  |  Page 30  |  Page 31  |  Page 32  |  Page 33  |  Page 34  |  Page 35  |  Page 36  |  Page 37  |  Page 38  |  Page 39  |  Page 40  |  Page 41  |  Page 42  |  Page 43  |  Page 44  |  Page 45  |  Page 46  |  Page 47  |  Page 48  |  Page 49  |  Page 50  |  Page 51  |  Page 52  |  Page 53  |  Page 54  |  Page 55  |  Page 56  |  Page 57  |  Page 58  |  Page 59  |  Page 60  |  Page 61  |  Page 62  |  Page 63  |  Page 64  |  Page 65  |  Page 66  |  Page 67  |  Page 68  |  Page 69  |  Page 70  |  Page 71  |  Page 72  |  Page 73  |  Page 74  |  Page 75  |  Page 76  |  Page 77  |  Page 78  |  Page 79  |  Page 80  |  Page 81  |  Page 82  |  Page 83  |  Page 84  |  Page 85  |  Page 86  |  Page 87  |  Page 88  |  Page 89  |  Page 90  |  Page 91  |  Page 92