Summertime
Photochemical Ozone Formation in Santiago de Chile.
Not exact matches
A detailed
ozone model budget analysis was performed with simultaneous observations of O3, HCl, H2O, CH4, NO, and NO2 from the Halogen Occultation Experiment (HALOE) on the Upper Atmosphere Research Satellite (UARS) under conditions with the strongest
photochemical control of
ozone.
On the contrary, the use of currently recommended
photochemical parameters leads to insufficient
ozone destruction in the model.
Recently, additional
ozone production mechanisms have been proposed to resolve the
ozone deficit problem, which arises from greater
ozone destruction than production in several
photochemical models of the upper stratosphere and lower mesosphere.
VOCs, sunlight and nitrogen oxides react to produce high levels of
ozone and
photochemical smogs.
Oxidized nitrogen becomes part of
photochemical smog and
ozone and is a major component of the infamous PM 2.5, particulate matter less than 2.5 microns in diameter that decreases visibility and is harmful when inhaled because it can penetrate deeply into the lungs.
Tracking the
ozone lets us track the
photochemical processes taking place in the Martian atmosphere.
The findings are timely because the Environmental Protection Agency is developing stricter regulations for ground - level
ozone, a primary component in
photochemical smog.
«Free oxygen [O2] in the atmosphere is required to form a protective layer of
ozone [O3], which can shield methane from
photochemical destruction,» Reinhard said.
The
ozone season is selected because it is the part of the year with highest temperatures and strongest solar radiation and thus the time when
photochemical reactions of
ozone precursor gases are most likely to produce high
ozone levels (Rice, 2014).
SO2 in the air will also eat
ozone and contribute to
photochemical smog.
Due to the important role of
ozone in driving temperature changes in the stratosphere as well as radiative forcing of surface climate, several different groups have provided databases characterizing the time - varying concentrations of this key gas that can be used to force global climate change simulations (particularly for those models that do not calculate
ozone from
photochemical principles).
Even so, it has not been regarded as a threat to the
ozone layer, because its typical lifetime in the atmosphere before it is broken down in
photochemical reactions is only about five months.
This while the
photochemical reactions are different but the mechanism involved in warming their atmosphere is similar to our oxygen -
ozone system.
Smog consists of: -
Ozone (O3) * (formed from the
photochemical reaction of Nitrogen dioxide (NO2) + Hydrocarbons)- Particulate matter (PM - 10) * - Sulfur dioxide (SO2) * * Air Pollution is already regulated in the: 1970 Clean Air Act (Amended: 1977, 1990)- Water Pollution is already regulated in the Federal Water Pollution Control Act (Amended: Clean Water Act of 1977, Water Quality Act of 1987)
Joanna Haigh and colleagues now show that these spectral variations — when incorporated into a radiative -
photochemical model — lead to decreases in
ozone below 45 kilometres and increases above.
Langmann, B., and S.E. Bauer, 2002: On the importance of reliable background concentrations of
ozone for regional scale
photochemical modelling.
Our results, simulated with a radiative -
photochemical model, are consistent with contemporaneous measurements of
ozone from the Aura - MLS satellite, although the short time period makes precise attribution to solar effects difficult.
US EPA, 1996: Air quality criteria for
ozone and related
photochemical oxidants.