4.4 Article

Atmospheric Abundance of PM2.5 Carbonaceous Matter and Their Potential Sources at Three High-Altitude Glacier Sites over the Indian Himalayan Range

期刊

ACS EARTH AND SPACE CHEMISTRY
卷 6, 期 12, 页码 2919-2928

出版社

AMER CHEMICAL SOC
DOI: 10.1021/acsearthspacechem.2c00216

关键词

PM2; 5; Himalayan glacier aerosol; carbonaceous matters; char-EC and soot-EC; secondary organic aerosol; biomass burning

资金

  1. SERB, India [EMR/2015/000928, CRG/2022/003926]
  2. DST FIST, India [SR/FST/CSI-259/2014 (c)]
  3. UGC-SAP-DRS-II, India program [F- 540/7/DRS-II/2016 (SAP-I)]
  4. SERB (India) [EMR/2015/000928]

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This study examines the concentrations of PM2.5 mass and carbonaceous species in the Indian Himalayan glacier region during the summer and winter periods. Different seasonal variations and sources of PM2.5 and carbonaceous species are found at the three investigated sites. High-temperature OC4 is the most prevalent carbon fraction, and biomass burning is suggested to be the predominant source of carbon in one of the sites.
This study inspects the concentrations of fine particulate matter (PM2.5) mass and carbonaceous species, including organic carbon (OC) and elemental carbon (EC), as well as their thermal fractions in the Indian Himalayan glacier region at the western Himalayan region (WHR; Thajiwas glacier, 2799 m asl), central Himalayan region (CHR; Gomukh glacier, 3415 m asl), and eastern Himalayan region (EHR; Zemu glacier, 2700 m asl) sites, throughout the summer and winter periods of 2019-2020. Ambient PM2.5 samples were collected on quartz fiber filters using a low-volume sampler, followed by carbon (OC and EC) quantification using the IMPROVE_A thermal/optical reflectance methodology. Different seasonal variations in PM2.5 and carbonaceous species levels were found at all three sites investigated. Averaged PM2.5 mass ranged 55-87 mu g m-3 with a mean of 55.45 +/- 16.30 mu g m-3 at WHR, 86.80 +/- 35.73 mu g m-3 at CHR, and 72.61 +/- 24.45 mu g m-3 at EHR. Among the eight carbon fractions, high-temperature OC4 (evolved at 580 degrees C in the helium atmosphere) was the most prevalent carbon fraction, followed by low-temperature OC2 (280 degrees C) and EC1 (580 degrees C at 2% oxygen and 98% helium). Char-EC representing incomplete combustion contributed to 56, 67, and 53% of total EC, whereas soot EC contributed to 38, 26, and 43% of total EC in WHR, CHR, and EHR, respectively. The measured OC/EC ratios imply the presence of secondary organic carbon, whereas char-EC/soot-EC ratios suggested that biomass burning could be the predominant source of carbon at CHR, whereas coal combustion and vehicular emission might be dominant sources at WHR and EHR sites.

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