the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Performance analysis of the NanoScan SMPS and the Mini WRAS Ultrafine Aerosol Particle Size Spectrometers
Abstract. In aerosol science, there is an increasing interest to perform mobile measurements to obtain number size distribution of ultrafine particles (UFP), using portable instruments based on unipolar charging and size segregation by electrical particle mobility. Applications of such measurements range from ambient and indoor aerosol studies to source identification in work environments. However, knowledge on the actual measurement uncertainties of these portable instruments under various conditions has been limited. This investigation presents results from an intercomparison workshop conducted at the World Calibration Center for Aerosol Physics (WCCAP) in Leipzig, Germany, in January 2020. Manufacturers and users were invited to have their portable instruments tested and compared against reference instrumentation for particle number size distributions (PNSD) and total particle number concentration (PNC). In particular, the performances and uncertainties of the NanoScan SMPS (Scanning Mobility Particle Sizer) Model 3910 (TSI Inc.) and the Mini Wide Range Aerosol Spectrometer (WRAS) Model 1371 (Grimm Aerosol Technik) were investigated extensively against the WCCAP Mobility Particle Size Spectrometers (MPSS) and Condensation Particle Counters (CPC). A total of 11 TSI NanoScan SMPS and 4 GRIMM Mini WRAS instruments were characterized for ambient aerosols as well as lab-generated aerosols.
The workshop results affirm that the portable instruments must be serviced and calibrated annually or prior field studies to provide measurements within the given uncertainties. It should be noted that users should carry out timely service, maintenance and calibration of portable instruments at their facilities. During initial inspection, non-serviced NanoScan SMPS instruments overestimated a dominant ultrafine aerosol mode by 120 % at around 80 nm. Maintenance and servicing improved the performance. Overall, the performance of NanoScan SMPS instruments improved for the ultrafine aerosol mode while the PNC in the fine aerosol mode still overestimated by up to 80 %. The latter effect seems to be systematically related to the unipolar charging of particles, and the reduced sensitivity of electrical particle mobility with increasing particle size above 200 nm. Due to shift in the second mode of bimodal distribution, particles are overcounted around 100 nm. With regard to the integral PNC, some of the NanoScan SMPS found to be in good agreement (i.e. within 20 %) compared to the reference CPC. In addition, a reasonably good unit-to-unit agreement within ±20 % was found for NanoScan SMPS instruments. The Mini WRAS instruments, after proper cleaning and servicing, provided improved results within ±15 % deviation in PNC in the ultrafine aerosol mode. Overall, most of the GRIMM Mini WRAS instruments (operating with software version 10.0) agrees well with PNC (i.e. 10–50 %) when the ultrafine mode was dominant. Conversely, PNC of the fine aerosol mode was systematically underestimated by 60 % above 100 nm. Except for one instrument, the integral PNC of the GRIMM Mini WRAS spectrometers were within an uncertainty range of ±20 % compared to the reference CPC. Additionally, it is important for users to note that the Mini WRAS performed significantly better when using software version 10.0 compared to version 8.2.
The workshop results suggest that despite the above-mentioned uncertainties, these portable instruments are suited for mobile ultrafine particle measurements to detect relative differences in the PNSD such as source apportionment studies of ultrafine particles at work places or outdoors near sources.
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RC1: 'Comment on amt-2022-155', Anonymous Referee #1, 01 Jun 2022
The comment was uploaded in the form of a supplement: https://amt.copernicus.org/preprints/amt-2022-155/amt-2022-155-RC1-supplement.pdf
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AC1: 'Reply on RC1', Ajit Ahlawat, 02 Sep 2022
The comment was uploaded in the form of a supplement: https://amt.copernicus.org/preprints/amt-2022-155/amt-2022-155-AC1-supplement.pdf
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AC1: 'Reply on RC1', Ajit Ahlawat, 02 Sep 2022
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RC2: 'Comment on amt-2022-155', Anonymous Referee #2, 21 Jun 2022
The comment was uploaded in the form of a supplement: https://amt.copernicus.org/preprints/amt-2022-155/amt-2022-155-RC2-supplement.pdf
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AC2: 'Reply on RC2', Ajit Ahlawat, 02 Sep 2022
The comment was uploaded in the form of a supplement: https://amt.copernicus.org/preprints/amt-2022-155/amt-2022-155-AC2-supplement.pdf
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AC2: 'Reply on RC2', Ajit Ahlawat, 02 Sep 2022
Status: closed
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RC1: 'Comment on amt-2022-155', Anonymous Referee #1, 01 Jun 2022
The comment was uploaded in the form of a supplement: https://amt.copernicus.org/preprints/amt-2022-155/amt-2022-155-RC1-supplement.pdf
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AC1: 'Reply on RC1', Ajit Ahlawat, 02 Sep 2022
The comment was uploaded in the form of a supplement: https://amt.copernicus.org/preprints/amt-2022-155/amt-2022-155-AC1-supplement.pdf
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AC1: 'Reply on RC1', Ajit Ahlawat, 02 Sep 2022
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RC2: 'Comment on amt-2022-155', Anonymous Referee #2, 21 Jun 2022
The comment was uploaded in the form of a supplement: https://amt.copernicus.org/preprints/amt-2022-155/amt-2022-155-RC2-supplement.pdf
-
AC2: 'Reply on RC2', Ajit Ahlawat, 02 Sep 2022
The comment was uploaded in the form of a supplement: https://amt.copernicus.org/preprints/amt-2022-155/amt-2022-155-AC2-supplement.pdf
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AC2: 'Reply on RC2', Ajit Ahlawat, 02 Sep 2022
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