Wet chemical surface ozone measurements during POLARSTERN cruise ANT-I/3 (PS01) in 1982/83

DOI

On the outward journey, European air masses, loaded by photochemically produced ozone, may have partly influenced the measurements in clean air. As simultaneously measured low concentrations of Krypton-85 (which only has anthropogenic sources) show, the high ozone mixing ratios at 0-5°N cannot be explained by photochemical formation, but must be of natural origin. On the return journey, the ITCZ was at 6°S and was weak. This explains the very low ozone values of only 4 ppb at times, caused by the photolysis of ozone.The ozone device was housed in the crow's nest, to avoid ship-polluted interference. At later cruises, the instrument was placed near the weather station, because the maintenance in the crow’s nest was impractical and the new air intake at the uppermost railing turned out to be suitable as well. As a precaution, the air pump was changed nine times during the trip. At the end of the last section, the pump wobbled a little, resulting in a five percent loss of production, which could be corrected

Positions partly approximate

Identifier
DOI https://doi.org/10.1594/PANGAEA.944269
Related Identifier References https://doi.org/10.2312/BzP_0014_1983
Related Identifier References https://doi.org/10.48433/BzPM_0760_2022
Metadata Access https://ws.pangaea.de/oai/provider?verb=GetRecord&metadataPrefix=datacite4&identifier=oai:pangaea.de:doi:10.1594/PANGAEA.944269
Provenance
Creator Winkler, Peter
Publisher PANGAEA
Publication Year 2022
Rights Creative Commons Attribution 4.0 International; https://creativecommons.org/licenses/by/4.0/
OpenAccess true
Representation
Resource Type Dataset
Format text/tab-separated-values
Size 747 data points
Discipline Earth System Research
Spatial Coverage (-43.150W, -22.900S, -11.700E, 37.600N)
Temporal Coverage Begin 1983-03-26T01:00:00Z
Temporal Coverage End 1983-04-23T05:00:00Z