EGU23-10785
https://doi.org/10.5194/egusphere-egu23-10785
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Humic-like substances in residential biofuel use emissions from the northwestern Himalayan region, India

Prashant Rawat1, Sebastien Bau2, and Sayantan Sarkar1
Prashant Rawat et al.
  • 1INDIAN INSTITUTE OF TECHNOLOGY MANDI, SCENE, Kamand, India (d21112@students.iitmandi.ac.in, sayantan@iitmandi.ac.in )
  • 2Laboratory of Aerosol Metrology, Institut National de Recherche et de Sécurité, France (sebastien.bau@inrs.fr)

Indoor biofuel use for cooking/heating purposes is potentially a significant source of fine-mode aerosols in the Indian Himalayan region, with important implications for ambient atmospheric processes. Incomplete combustion of biofuels leads to emission of absorbing aerosols such as elemental carbon (EC), brown carbon (BrC) and humic-like substances (HULIS), which can affect climate via direct as well as indirect forcing.  However, profiles of these aerosols in indoor microenvironments are poorly studied, especially from the Indian Himalayan region. Here, we report size-segregated light absorption properties (absorption coefficient; babs_aq) of aqueous brown carbon (BrCaq) for cow dung cake (CDC), firewood (WD), charcoal (CC), kerosene (KS) and liquified petroleum gas (LPG) combustion in indoor settings from two northwest Himalayan states (Uttarakhand and Himachal Pradesh). We further characterize BrC composition using excitation emission matrix (EEM) fluorescence spectroscopy coupled with parallel factor (PARAFAC) analysis. Size-segregated samples (>2.5 µm, 2.5-1 µm, 1-0.5 µm, 0.5-0.25 µm and <0.25 µm) were collected during indoor cooking activities which showed PM levels exceeding Indian ambient PM2.5 standard by 8-460 times, with CDC showing the highest PM concentration in all size ranges. Size distribution profile of the fuels showed trimodal distributions with one peak in the Aitken nuclei mode (0.05 μm for CDC, WD and LPG; 0.06 μm for CC and KS) and the other two in the accumulation mode (0.22 and 2.03 μm for CDC, 0.21 μm and 2.1 μm for WD, 0.24 and 1.91 μm for KS, and 0.17 and 0.83 μm for CC). PM size distribution across kitchen and fuel types was characterized by more than 50% concentration in the Greenfield Gap region (0.1-2 μm)., CDC showed highest babs_365 for all size ranges combined (2245±357 Mm-1) compared to other fuels while LPG showed the lowest (190±46 Mm-1). BrCaq in the lowest size fraction showed greater babs compared to other size ranges in all fuels except KS. High values of babs ratio (>5) for300-400 nm (babs_300_400) to 400-500 nm (babs_400_500) wavelength range suggested the presence of HULIS in CDC and WD samples while other fuels exhibited values below 2.6. The lower size fractions (<0.5 µm) of CDC and WD were characterized by higher babs_300_400/babs_400_500 values (6.9±1.6 for CDC and 7.4±2.8 for WD) than upper size ranges (3.2±0.8 for CDC and 2.3±0.5 for WD), indicating a dominance of HULIS components in finer aerosol. Upon analysis of EEMs coupled with PARAGAC, three major chromophoric categories in BrCaq of CDC and WD samples were observed: two types of HULIS components with varying degree of conjugation and one type of protein-like substances (PRLIS). HULIS was the dominant chromophore type in lower size fractions (<0.5 µm) of CDC and WD samples (70±4% for CDC and 61±6% for WD) while for upper size fractions its contribution was relatively lower (50±10% for CDC and 36±9% for WD). Finally, BrCaq from CDC and WD emissions exhibited direct climate forcing potential equivalent to EC (relative radiative forcing (RRF): 91-98%), confirming that indoor biofuel emissions are indeed significant sources of climate forcing agents in the Indian Himalayan context.

How to cite: Rawat, P., Bau, S., and Sarkar, S.: Humic-like substances in residential biofuel use emissions from the northwestern Himalayan region, India, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-10785, https://doi.org/10.5194/egusphere-egu23-10785, 2023.