Published September 2016 | Version Published + Accepted Version + Supplemental Material
Journal Article Open

Investigation of a potential HCHO measurement artifact from ISOPOOH

  • 1. ROR icon Goddard Space Flight Center
  • 2. ROR icon University of Maryland, Baltimore County
  • 3. ROR icon Harvard University
  • 4. ROR icon California Institute of Technology
  • 5. ROR icon University of Wisconsin–Madison

Abstract

Recent laboratory experiments have shown that a first generation isoprene oxidation product, ISOPOOH, can decompose to methyl vinyl ketone (MVK) and methacrolein (MACR) on instrument surfaces, leading to overestimates of MVK and MACR concentrations. Formaldehyde (HCHO) was suggested as a decomposition co-product, raising concern that in situ HCHO measurements may also be affected by an ISOPOOH interference. The HCHO measurement artifact from ISOPOOH for the NASA In Situ Airborne Formaldehyde instrument (ISAF) was investigated for the two major ISOPOOH isomers, (1,2)-ISOPOOH and (4,3)-ISOPOOH, under dry and humid conditions. The dry conversion of ISOPOOH to HCHO was 3 ± 2 % and 6 ± 4 % for (1,2)-ISOPOOH and (4,3)-ISOPOOH, respectively. Under humid (relative humidity of 40–60 %) conditions, conversion to HCHO was 6 ± 4 % for (1,2)-ISOPOOH and 10 ± 5 % for (4,3)-ISOPOOH. The measurement artifact caused by conversion of ISOPOOH to HCHO in the ISAF instrument was estimated for data obtained on the 6 September 2013 flight of the Studies of Emissions and Atmospheric Composition, Clouds and Climate Coupling by Regional Surveys (SEAC4RS) campaign. Prompt ISOPOOH conversion to HCHO was the source of < 4 % of the observed HCHO, including in the high-isoprene boundary layer. Time-delayed conversion, where previous exposure to ISOPOOH affects measured HCHO later in the flight, was conservatively estimated to be < 10 % of observed HCHO, and is significant only when high ISOPOOH sampling periods immediately precede periods of low HCHO.

Additional Information

© Author(s) 2016. This work is distributed under the Creative Commons Attribution 3.0 License. Received: 13 Jun 2016 – Published in Atmos. Meas. Tech. Discuss.: 16 Jun 2016; Revised: 12 Aug 2016 – Accepted: 15 Aug 2016 – Published: 16 Sep 2016. F. N. Keutsch and J. C. Rivera-Rios were supported by the National Science Foundation (AGS 1628491, 1628530, 1247421, 1321987). J. M. St. Clair, G. M. Wolfe, and T. F. Hanisco were supported by NASA (NNH12ZDA001N-UACO). M. J. Kim was supported by the National Science Foundation (AGS PRF 1524860).

Attached Files

Published - amt-9-4561-2016.pdf

Accepted Version - nihms952688.pdf

Supplemental Material - amt-9-4561-2016-supplement.pdf

Files

amt-9-4561-2016-supplement.pdf

Files (10.4 MB)

Name Size
md5:2c9382ee72c105d33b6774003394f396
9.3 MB Preview Download
md5:349db7d737a6ea2f8e9a356d398cdfed
799.3 kB Preview Download
md5:3e379ee716b18cfee69feec645fa437d
347.2 kB Preview Download

Additional details

Identifiers

PMCID
PMC5889939
Eprint ID
71311
Resolver ID
CaltechAUTHORS:20161020-090716797

Funding

NSF
AGS-1628491
NSF
AGS-1628530
NSF
AGS-1247421
NSF
AGS-1321987
NASA
NNH12ZDA001N-UACO
NSF Atmospheric and Geospace Sciences Fellowship
AGS-1524860

Dates

Created
2016-10-20
Created from EPrint's datestamp field
Updated
2022-04-14
Created from EPrint's last_modified field

Caltech Custom Metadata