EGU26-640, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-640
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Friday, 08 May, 09:55–10:05 (CEST)
 
Room E2
Assesssement of Trace Gases Variability and Satellite Retrieval Accuracy using Pandora Observations in the Central Himalayas
Mukesh Kumar1,2, Manish Naja1, Prajjwal Rawat3, Priyanka Srivastava1, Hiroshi Tanimoto4, and Jim Crawford3
Mukesh Kumar et al.
  • 1Aryabhatta Research Institute of Observational Sciences Nainital, Atmospheric Sciences, Nainital, India (mukeshkumar@aries.res.in; manish@aries.res.in; priyanka@aries.res.in)
  • 2Indian Institute of Technology, Roorkee, India (mukeshsharma342225@gmail.com)
  • 3NASA Langley Research Center, Hampton, VA, United States (prajjwal.rawat@nasa.gov; james.h.crawford@nasa.gov)
  • 4National Institute of Environmental Studies, Tsukuba, Japan (tanimoto@nies.go.jp)

For the first time, a Pandora spectrometer has been deployed in the central Himalayan region as part of the Pandora Global Network (PGN), at ARIES, Nainital (29.36°N, 79.36°E; 1970 m a.s.l.), a high-altitude remote site in South Asia where Pandora coverage has been negligible; however, pollutant concentrations across South Asia remain very high. Although the site is elevated, it is located adjacent to the Indo-Gangetic Plains (IGP) and is therefore affected by the transport of pollutants from the IGP.

The instrument retrieves column densities of key trace gases, ozone (O3), nitrogen dioxide (NO2), and formaldehyde (HCHO), including their total column (TO3, TNO2, THCHO) and lower-tropospheric column (LTrNO2, LTrHCHO) amounts, suitable for validation of satellite observations in this complex mountain topology. Analysis of observations from January 2024 to June 2025 shows clear seasonality, with elevated springtime columns (TNO2: 4-5 × 10¹⁵ molecules cm⁻²; LTrNO2: 1 ± 0.1 × 10¹⁵ molecules cm⁻²; LTrHCHO: 0.8 ± 0.1 × 10¹⁶ molecules cm⁻²) and reduced values in the summer–monsoon period (LTrNO2: ~0.3 ± 0.05 × 10¹⁵ molecules cm⁻²; LTrHCHO: ~0.2 × 10¹⁶ molecules cm⁻²). The seasonal cycle of column NO2 agrees with surface in-situ NOy, though their diurnal patterns differ: column NO₂ increasing steadily from morning until the evening period, while surface NOy peaks around midday and column HCHO shows maximum value during daytime (12-13 hours IST), followed by a decline toward evening.

Pandora observations were also used to evaluate the performance of GEMS and TROPOMI satellite products for O3 and NO2 over a complex mountainous environment. For total column ozone, both GEMS and TROPOMI capture the day-to-day variability (R² = 0.98 for both satellites against Pandora). However, GEMS exhibits a systematic underestimation of about 15 ± 5 DU, while TROPOMI shows good agreement during the spring season but overestimates ozone by approximately 10 DU in other seasons. Similarly, both satellites represent the daily variability of TNO2 reasonably well (R² = 0.71 for GEMS and 0.78 for TROPOMI). However, both instruments generally overestimate TNO2. In contrast, the performance for LTrNO2 is considerably poorer, with R² values of only 0.17 (GEMS) and 0.28 (TROPOMI). Thus, showing low sensitivity of satellite retrievals for NO2 in the lower troposphere.  These results highlight the crucial role of high-quality ground-based measurements such as Pandora in validating satellite retrievals and advancing our understanding of trace gas behaviour in complex terrain.

How to cite: Kumar, M., Naja, M., Rawat, P., Srivastava, P., Tanimoto, H., and Crawford, J.: Assesssement of Trace Gases Variability and Satellite Retrieval Accuracy using Pandora Observations in the Central Himalayas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-640, https://doi.org/10.5194/egusphere-egu26-640, 2026.