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Optical Characteristics of Atmospheric Aerosol Based on the Results of Measurements near St. Petersburg from 2016 to 2021. / Шпак, Кристина Андреевна; Небосько, Евгений Юрьевич; Ионов, Дмитрий Викторович.

в: Izvestiya - Atmospheric and Oceanic Physics, Том 60, № 5, 10.07.2024, стр. 523–532.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Шпак, КА, Небосько, ЕЮ & Ионов, ДВ 2024, 'Optical Characteristics of Atmospheric Aerosol Based on the Results of Measurements near St. Petersburg from 2016 to 2021', Izvestiya - Atmospheric and Oceanic Physics, Том. 60, № 5, стр. 523–532. https://doi.org/10.1134/S0001433824700518

APA

Vancouver

Author

Шпак, Кристина Андреевна ; Небосько, Евгений Юрьевич ; Ионов, Дмитрий Викторович. / Optical Characteristics of Atmospheric Aerosol Based on the Results of Measurements near St. Petersburg from 2016 to 2021. в: Izvestiya - Atmospheric and Oceanic Physics. 2024 ; Том 60, № 5. стр. 523–532.

BibTeX

@article{1609868112d54567b516ceb5dd240bf9,
title = "Optical Characteristics of Atmospheric Aerosol Based on the Results of Measurements near St. Petersburg from 2016 to 2021",
abstract = "This paper presents the results of measurements of the optical characteristics of aerosol particles using a solar photometer and nephelometer from 2016 to 2021 obtained at the atmospheric monitoring station in Peterhof (59.88° N, 29.83° E). The measurements are compared with the MERRA-2 reanalysis data. It isshown that interseasonal variability is observed in the region, characterized by low values of the Angstrom exponent in winter and high values in the warm season. The backscatter fraction has a similar—but less pronounced—seasonal cycle. The average value of the turbidity coefficient for the period is less than 0.10, which makes it possible to determine the observation station as a background one. Using the HYSPLIT model, the origin of air masses forming the atmospheric air state at the observation station is determined when the limitingvalues of the measured scattering coefficients (<10 and >70) and the Angstrom exponent (<1) are realized. Air masses coming from the northwest correspond to clean and humid air from the marine area and are manifested in the minimum values of the measured parameters. The maximum values of the scattering coefficient are associated with fine aerosol entering the atmosphere both from regional emissions sources (urban pollution from the territory of St. Petersburg) and as a result of transboundary transport from southwestern directions.",
author = "Шпак, {Кристина Андреевна} and Небосько, {Евгений Юрьевич} and Ионов, {Дмитрий Викторович}",
year = "2024",
month = jul,
day = "10",
doi = "10.1134/S0001433824700518",
language = "English",
volume = "60",
pages = "523–532",
journal = "Izvestiya - Atmospheric and Oceanic Physics",
issn = "0001-4338",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "5",

}

RIS

TY - JOUR

T1 - Optical Characteristics of Atmospheric Aerosol Based on the Results of Measurements near St. Petersburg from 2016 to 2021

AU - Шпак, Кристина Андреевна

AU - Небосько, Евгений Юрьевич

AU - Ионов, Дмитрий Викторович

PY - 2024/7/10

Y1 - 2024/7/10

N2 - This paper presents the results of measurements of the optical characteristics of aerosol particles using a solar photometer and nephelometer from 2016 to 2021 obtained at the atmospheric monitoring station in Peterhof (59.88° N, 29.83° E). The measurements are compared with the MERRA-2 reanalysis data. It isshown that interseasonal variability is observed in the region, characterized by low values of the Angstrom exponent in winter and high values in the warm season. The backscatter fraction has a similar—but less pronounced—seasonal cycle. The average value of the turbidity coefficient for the period is less than 0.10, which makes it possible to determine the observation station as a background one. Using the HYSPLIT model, the origin of air masses forming the atmospheric air state at the observation station is determined when the limitingvalues of the measured scattering coefficients (<10 and >70) and the Angstrom exponent (<1) are realized. Air masses coming from the northwest correspond to clean and humid air from the marine area and are manifested in the minimum values of the measured parameters. The maximum values of the scattering coefficient are associated with fine aerosol entering the atmosphere both from regional emissions sources (urban pollution from the territory of St. Petersburg) and as a result of transboundary transport from southwestern directions.

AB - This paper presents the results of measurements of the optical characteristics of aerosol particles using a solar photometer and nephelometer from 2016 to 2021 obtained at the atmospheric monitoring station in Peterhof (59.88° N, 29.83° E). The measurements are compared with the MERRA-2 reanalysis data. It isshown that interseasonal variability is observed in the region, characterized by low values of the Angstrom exponent in winter and high values in the warm season. The backscatter fraction has a similar—but less pronounced—seasonal cycle. The average value of the turbidity coefficient for the period is less than 0.10, which makes it possible to determine the observation station as a background one. Using the HYSPLIT model, the origin of air masses forming the atmospheric air state at the observation station is determined when the limitingvalues of the measured scattering coefficients (<10 and >70) and the Angstrom exponent (<1) are realized. Air masses coming from the northwest correspond to clean and humid air from the marine area and are manifested in the minimum values of the measured parameters. The maximum values of the scattering coefficient are associated with fine aerosol entering the atmosphere both from regional emissions sources (urban pollution from the territory of St. Petersburg) and as a result of transboundary transport from southwestern directions.

U2 - 10.1134/S0001433824700518

DO - 10.1134/S0001433824700518

M3 - Article

VL - 60

SP - 523

EP - 532

JO - Izvestiya - Atmospheric and Oceanic Physics

JF - Izvestiya - Atmospheric and Oceanic Physics

SN - 0001-4338

IS - 5

ER -

ID: 126625050