search.noResults

search.searching

saml.title
dataCollection.invalidEmail
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
32


Analytical Instrumentation Fuel Analysis by Mid-Infrared Spectroscopy Dr. Roland Aschauer, R&D Director of Eralytics GmbH. www.eralytics.com, office@eralytics.com.


The analysis of fuels, especially gasoline and diesel automotive fuels, by a rapid, accurate, and easy-to-use method which can be applied also in the field is very important for the monitoring of fuel composition and quality at several points in the manufacturing process and distribution chain. Such a method is valuable in laboratories at refineries where fast, accurate results are needed, in small terminal and pipeline laboratories where it is not possible to perform all specified tests but monitoring fuel quality is necessary, at gas stations itself, and in mobile laboratories.


IR spectroscopy is the method of choice for such applications for several reasons discussed below.


Advantages of IR Spectroscopy The IR spectrum contains direct molecular specific information so that many parameters can be determined simultaneously from one measurement. The evaluation of the spectrum that leads to the final results can be performed automatically by microprocessors, so that the instrument can be automated. Thus IR instruments can be operated by personnel that have no background or training in analytical chemistry.


The measurement is very quick in comparison to other analytical methods, in the order of one minute per analysis.


The instruments to measure the IR spectrum can be made very compact, stable, and robust so that they are portable and may be used in harsh conditions and in the field. The IR analysers do not need any gas or other supply, as neither separation steps nor chemical reactions are required prior to the measurement.


No sample preparation is necessary, only an electrical power line is needed.


No other analytical technique combines all these advantages.


Principle of IR Spectroscopy


Infrared (IR) radiation is electromagnetic radiation with a wavelength between 0.7µm and 100µm. This range is further divided in the Near-IR (NIR) range (wavelengths 0.7µm to roughly 4µm), mid-IR (wavelengths 4µm to roughly 20 µm), and far-IR (wavelengths 20µm to 100 µm).


For analytical applications, mostly NIR and mid-IR spectroscopy are used.


In IR spectroscopy, IR radiation in the desired wavelength range is directed through the sample to be analysed, and the intensity of the transmitted radiation is measured as a function of wavelength. The process that leads to attenuation (absorption) of IR radiation by the sample is excitation of vibrations of molecules in the sample.


These vibrations can be excited only by radiation of wavelengths that match the energy difference between the ground and excited vibrational state. These wavelengths are different for different molecules; furthermore there are usually different vibrations in a given molecule. This is why IR spectroscopy allows for the simultaneous determination of many different substances in one sample by one measurement over a certain wavelength range.


If a vibration is excited by radiation of a specific wavelength, then the intensity of the IR radiation passing through the sample at that wavelength


decreases. The more molecules are present, the more vibrations can be excited, and the more the radiation decreases.


Therefore, the concentrations of many different substances can be determined quantitatively by IR spectroscopy.


Application to the Analysis of Fuels Gasoline and Diesel fuels are complex mixtures of many different hydrocarbons and hydrocarbon types. They contain alkanes (paraffins), alkenes (olefins) and aromatics. Moreover, driven in part by the desire to use renewable fuel sources, alcohols and ethers are blended into gasolines, and FAME from vegetable oils is very frequently a component in Diesel fuels. Additionally, additives like MMT to increase octane numbers in gasolines or 2-EHN to increase the cetane number in Diesel fuels are used. Small quantities (<0.1 %) of such additives have a significant effect on some fuel properties. In order to accurately determine the composition of complex mixtures, mid-IR spectroscopy can be very successfully applied to perform a quantitative analysis of gasoline and Diesel fuel.


In gasolines, it is important to know the concentrations of individual compounds, like


benzene, ethanol or MTBE, but also total concentrations of different hydrocarbon types, like olefins and aromatics or the oxygen content. With mid-IR spectroscopy, the lines of individual aromatics (like benzene, toluene, xylenes etc.) and oxygenates (like ethanol, methanol, MTBE, ETBE, etc.) can be resolved and used to calculate the concentrations of each compound, with no or minimal interference from other, chemically similar substances.


These individual lines as well as lines coming from certain hydrocarbon types (like olefins and aromatics) can then be used to calculate also the total concentrations of olefins, aromatics and oxygenates as well as the oxygen content of the gasoline sample.


Some additives like MMT which are present at concentrations typically only around 100 ppm can still be determined with mid-IR spectroscopy since the lines are very strong.


In Diesel fuels, the mid-IR spectrum allows to discriminate between single-nuclear and poly- nuclear aromatics. The FAME concentration can be measured with high accuracy using a very strong line. Unreacted vegetable oil and FAME have different mid-IR spectra, therefore with mid-IR spectroscopy, it is possible to detect if vegetable oil or FAME is present


Annual Buyers’ Guide 2011


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  |  Page 93  |  Page 94  |  Page 95  |  Page 96  |  Page 97  |  Page 98  |  Page 99  |  Page 100  |  Page 101  |  Page 102  |  Page 103  |  Page 104  |  Page 105  |  Page 106  |  Page 107  |  Page 108