Preprints
https://doi.org/10.5194/egusphere-2024-2874
https://doi.org/10.5194/egusphere-2024-2874
20 Sep 2024
 | 20 Sep 2024

Fluorescence properties of long-range transported smoke: Insights from five-channel lidar observations over Moscow during the 2023 wildfire season

Igor Veselovskii, Mikhail Korenskiy, Nikita Kasianik, Boris Barchunov, Qiaoyun Hu, Philippe Goloub, and Thierry Podvin

Abstract. The fluorescence lidar at the Prokhorov General Physics Institute (Moscow) was utilized to study transported smoke during the wildfire season from May to September 2023. The lidar system, based on a tripled Nd:YAG laser, performs fluorescence measurements  at wavelengths of 438, 472, 513, 560, and 614 nm. This configuration enables the assessment of the spectral dependence of fluorescence backscattering from the planetary boundary layer (PBL) to the upper troposphere and lower stratosphere (UTLS). The fluorescence capacity of smoke, defined as the ratio of fluorescence backscattering to aerosol backscattering at the laser wavelength, exhibits significant variation in the UTLS, with changes of up to a factor of 3. This variation is likely indicative of differences in the relative concentration of organic compounds within the smoke. Analysis of more than 40 smoke episodes enabled an evaluation of the height dependence of smoke fluorescence properties. Observations reveal that the fluorescence capacity generally increases with altitude, suggesting a higher concentration of organic compounds in the UTLS compared to the lower troposphere. Additionally, the measurements consistently show differences in the fluorescence spectra of smoke and urban aerosol. Urban aerosol fluorescence tends to decrease gradually with wavelength, whereas the peak of smoke fluorescence is observed at the 513 or 560 nm channels. This spectral distinction provides an effective means of separating smoke from urban aerosol. The technique was applied to events where smoke from the upper troposphere descended into the PBL and mixed with urban particles, demonstrating its utility in distinguishing between these aerosol types.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this preprint. The responsibility to include appropriate place names lies with the authors.
Igor Veselovskii, Mikhail Korenskiy, Nikita Kasianik, Boris Barchunov, Qiaoyun Hu, Philippe Goloub, and Thierry Podvin

Status: final response (author comments only)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2024-2874', Anonymous Referee #1, 22 Oct 2024
  • RC2: 'Comment on egusphere-2024-2874', Anonymous Referee #2, 04 Nov 2024
Igor Veselovskii, Mikhail Korenskiy, Nikita Kasianik, Boris Barchunov, Qiaoyun Hu, Philippe Goloub, and Thierry Podvin
Igor Veselovskii, Mikhail Korenskiy, Nikita Kasianik, Boris Barchunov, Qiaoyun Hu, Philippe Goloub, and Thierry Podvin

Viewed

Total article views: 364 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
199 25 140 364 2 5
  • HTML: 199
  • PDF: 25
  • XML: 140
  • Total: 364
  • BibTeX: 2
  • EndNote: 5
Views and downloads (calculated since 20 Sep 2024)
Cumulative views and downloads (calculated since 20 Sep 2024)

Viewed (geographical distribution)

Total article views: 342 (including HTML, PDF, and XML) Thereof 342 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 14 Nov 2024
Download
Short summary
A fluorescence lidar was utilized to study transported smoke during the wildfire season from May to September 2023. The lidar performs fluorescence measurements at 5 wavelengths. Observations reveal that the fluorescence capacity increases with altitude, suggesting higher concentration of organic compounds in the UTLS compared to the lower troposphere. And urban aerosol fluorescence tends to decrease with wavelength, while the peak of smoke fluorescence is observed at 513 or 560 nm channels.