Published Ryan Schonert on April 11, 2019
I recently had the opportunity to attend my first PittCon meeting. Unlike other specialized conferences I’ve attended in the past, PittCon is well-attended by scientists of multiple disciplines, and it’s exciting to see the challenges and solutions being discussed by researchers from all over the world. However, fuels analysis was still the focus of many presentations, and as you may already know, GC-VUV is a rising star in this field. I got to present two research projects: one on VUV Verified Hydrocarbon Analysis (VHA), and another on the use of GC-MS to help supplement the VUV absorbance spectral library. In case you couldn’t make it, here’s what you missed:
ASTM D8071, hydrocarbon type analysis of gasoline using GC-VUV, has already proven itself a reliable alternative to ASTM D6730, detailed hydrocarbon analysis of gasoline using GC-FID (DHA), delivering PIONA results with a GC run under 34 minutes. However, many applications still use DHA because of its ability to speciate the large number of compounds in gasoline. With ASTM D8071, we take advantage of GC-VUV’s ability to spectrally deconvolve coelutions and quantify PIONA classes, but the method isn’t designed to provide speciation of everything in gasoline. For those who want the speed and reliability of GC-VUV while maintaining speciation, VHA is the answer. VHA provides full speciation of as many as 150 compounds in gasoline, making up approximately 90% of most gasolines, while still providing accurate PIONA data needed for gasoline analysis. All of this is achieved in a GC run of approximately 50 min, making it a very useful alternative to DHA (Figure 1).
GC-MS used to supplement the VUV spectral library:
GC-VUV has proven itself a worthy complementary technique with GC-MS. GC-MS is helpful to GC-VUV, too. The NIST mass spectral library, for example, has many decades of entries over the VUV library. We can take advantage of GC-MS and use it to build out the VUV spectral library. Normally, new compounds are added to the VUV spectral library by purchasing reference materials, collecting their spectra with GC-VUV, and establishing their response factors relative to a known compound, such as benzene. However, as outlined in ASTM D8071, most PIONA compounds will have shared class-based response factors; for example, isoparaffins have a relative response factor of 0.781. This means that if we can obtain spectra, we can often make entries for new PIONA compounds without purchasing any reference materials! This combination GC-MS/GC-VUV concept has already been demonstrated on multiple occasions. For example, several olefins were added to the library using samples with high olefin content (Figure 2).