Abstract. Retrievals of total column NO2 (TCNO2) are compared for 14 sites
from the Ozone Measuring Instrument (OMI using OMNO2-NASA v3.1) on the AURA
satellite and from multiple ground-based PANDORA spectrometer instruments
making direct-sun measurements. While OMI accurately provides the daily
global distribution of retrieved TCNO2, OMI almost always
underestimates the local amount of TCNO2 by 50 % to 100 % in polluted
areas, while occasionally the daily OMI value exceeds that measured by
PANDORA at very clean sites. Compared to local ground-based or aircraft
measurements, OMI cannot resolve spatially variable TCNO2 pollution
within a city or urban areas, which makes it less suitable for air quality
assessments related to human health. In addition to systematic
underestimates in polluted areas, OMI's selected 13:30 Equator crossing time
polar orbit causes it to miss the frequently much higher values of
TCNO2 that occur before or after the OMI overpass time. Six discussed
Northern Hemisphere PANDORA sites have multi-year data records (Busan,
Seoul, Washington DC, Waterflow, New Mexico, Boulder, Colorado, and Mauna Loa),
and one site in the Southern Hemisphere (Buenos Aires, Argentina). The first
four of these sites and Buenos Aires frequently have high TCNO2
(TCNO2 > 0.5 DU). Eight additional sites have shorter-term
data records in the US and South Korea. One of these is a 1-year data
record from a highly polluted site at City College in New York City with
pollution levels comparable to Seoul, South Korea. OMI-estimated air mass
factor, surface reflectivity, and the OMI 24 km × 13 km FOV (field of view)
are three factors that can cause OMI to underestimate TCNO2. Because of
the local inhomogeneity of NOx emissions, the large OMI FOV is the most
likely factor for consistent underestimates when comparing OMI TCNO2 to
retrievals from the small PANDORA effective FOV (measured in m2)
calculated from the solar diameter of 0.5∘.