Measurements of industrial emissions of alkenes in Texas using the solar occultation flux method
Journal article, 2010

Solar occultation flux (SOF) measurements of alkenes have been conducted to identify and quantify the largest emission sources in the vicinity of Houston and in SE Texas during September 2006 as part of the TexAQS 2006 campaign. The measurements have been compared to emission inventories and have been conducted in parallel with airborne plume studies. The SOF measurements show that the hourly gas emissions from the large petrochemical and refining complexes in the Houston Ship Channel area and Mount Belvieu during September 2006 corresponded to 1250 +/- 180 kg/h of ethene and 2140 +/- 520 kg/h of propene, with an estimated uncertainty of about 35%. This can be compared to the 2006 emission inventory value for ethene and propene of 145 +/- 4 and 181 +/- 42 kg/h, respectively. On average, for all measurements during the campaign, the discrepancy factor is 10.2(+ 8,-5) for ethene and 11.7(+ 7,-4) for propene. The largest emission source was Mount Belvieu, NE of the Houston Ship Channel, with ethene and propene emissions corresponding to 440 +/- 130 kg/h and 490 +/- 190 kg/h, respectively. Large variability of propene was observed from several petrochemical industries, for which the largest reported emission sources are flares. The SOF alkene emissions agree within 50% with emissions derived from airborne measurements at three different sites. The airborne measurements also provide support to the SOF error budget.

Spectroscopy

Author

Johan Mellqvist

Chalmers, Department of Radio and Space Science, Optical Remote Sensing

Jerker Samuelsson

Chalmers, Department of Radio and Space Science, Optical Remote Sensing

John Johansson

Chalmers, Earth and Space Sciences, Optical Remote Sensing

Claudia Rivera

Chalmers, Department of Radio and Space Science, Optical Remote Sensing

B. Lefer

S. Alvarez

J. Jolly

Journal of Geophysical Research

0148-0227 (ISSN)

Vol. 115

Subject Categories

Meteorology and Atmospheric Sciences

Atom and Molecular Physics and Optics

DOI

10.1029/2008JD011682

More information

Created

10/7/2017