EGU26-128, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-128
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Monday, 04 May, 10:45–12:30 (CEST), Display time Monday, 04 May, 08:30–12:30
 
Hall X1, X1.14
Sources and formation pathways of particulate nitrate over the western India: Insights through δ15N and δ18O isotopes
Chandrima Shaw1, Neeraj Rastogi1, Ritwick Mandal2, and Prasanta Sanyal2
Chandrima Shaw et al.
  • 1Physical Research Laboratory, Ahmedabad 380009, India (chandrimashaw@gmail.com) (nrastogi@prl.res.in)
  • 2Indian Institute of Science Education and Research Kolkata, Mohanpur 741246, India. (ritwickmandalrm@gmail.com) (psanyal@iiserkol.ac.in)

Oxides of Nitrogen (NOx) are key precursors of tropospheric ozone and particulate nitrate (NO3-), both of which contribute to air quality degradation and climate forcing. NOx is oxidized to nitric acid (HNO3), which partitions into particulate NO3-, an important component of PM2.5. The formation of HNO3 and ultimately NO3- occurs through multiple chemical pathways and is influenced by atmospheric chemistry as well as meteorological parameters like temperature, relative humidity, and boundary layer dynamics. India has been recognised a global hotspot for NOx emission, owing to rapid urbanization and population growth. Major sources of NOx include emissions from traffic, agriculture, biomass burning, and combustion. Despite being a major contributor of NOx, large uncertainties exist in regional emission inventories due to limited observational constraints. Stable isotopic signature of particulate NO3- serves as an excellent tool to understand its formation pathways and sources of its precursor.  Here, we have applied a dual-isotope (δ15N and δ18O) approach to understand seasonal and diurnal variations in NO3- formation pathways and NOx sources over Ahmedabad, an urban megacity in western India, during winter and summer. In winter, overall particulate NO3- formation was driven mainly by the OH oxidation pathway (P1, 61.9 ± 7%) and N2O5 hydrolysis (P2, 24.6 ± 6%), with smaller contributions from VOC-derived (P3, 7.6 ± 4%) and ClNO2 pathways (P4, 5.9 ± 3%). However, strong diurnal contrasts were evident, with P1 accounting for 69.4 ± 5% during the day and P2 increasing to 32.8 ± 7% at night, reflecting enhanced photochemical activity during day and nocturnal buildup of N2O5 under cooler, low-light conditions at night. In summer, NO3- formation was dominated by the OH pathway throughout the day and night (67.5 ± 7%), with no significant diurnal variability. This seasonal shift was attributed to elevated boundary layer height and enhanced atmospheric mixing, which stabilized particulate NO3-, which was particularly associated with stable non-volatile cations. Source apportionment of NOx using the Bayesian model (MixSIAR) revealed no significant diurnal differences within either season; however, a distinct seasonal pattern in NOx sources was observed. In winter, traffic was the largest contributor (46.7 ± 19%), followed by soil emissions (24.4 ± 12%), biomass burning (18.0 ± 9%), and coal-fired power plants (10.9 ± 8%). In summer, soil-related emissions increased to 38.4 ± 12% due to temperature-enhanced microbial activity and volatilization from urban waste, livestock areas, and fertilized land, while traffic remained a dominant source (40.1 ± 17%). Biomass burning and power plant contributions remained lower but persistent across both seasons. Together, these results provided the first dual-isotope-based evidence from western India showing how meteorology and emission processes jointly influence NO3- formation and NOx source, thus offering critical observational insight needed to improve regional nitrogen budgets and air quality mitigation strategies.

How to cite: Shaw, C., Rastogi, N., Mandal, R., and Sanyal, P.: Sources and formation pathways of particulate nitrate over the western India: Insights through δ15N and δ18O isotopes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-128, https://doi.org/10.5194/egusphere-egu26-128, 2026.