GSFC Code 916: Atmospheric Chemistry and
Dynamics Branch [menu bar image map]

Two-dimensional Modelling

The Goddard Space Flight Center (GSFC) two-dimensional (2D) model is used in the Atmospheric Chemistry and Dynamics Branch to help understand the physical and chemical processes related to ozone changes in the stratosphere and mesosphere (middle atmosphere). The model domain extends from the south pole to the north pole in latitude and from the ground to about 90 kilometers in altitude. The model includes chemistry (about 40 photodissociation processes and about 110 chemical reactions) involving 52 different atmospheric constituents, vertical and meridional winds, and diffusion processes.

This computer model is used to simulate natural and humankind-related changes in middle atmospheric ozone. Natural ozone changes that have been studied include those related to the 27-day solar rotation, the 11-year solar cycle, solar proton events, relativistic electron precipitations, interannual dynamical variations, volcanic eruptions, supernovae explosions, and gamma-ray bursts. Humankind-related changes that have been studied include those related to the chlorofluorocarbon and halon increases, the nuclear explosion tests in the early 1960s, Space Shuttle and Titan IV rocket launches, a proposed fleet of high speed civil transport planes that would fly in the stratosphere, and the proposed test flights of the National Aerospace Plane.

The model simulation is a realization of our theory of middle atmospheric processes. Comparison of the 2D model output and observational data can therefore either support that theory if there is a good agreement, or point to deficiencies that need to be resolved if there are discrepancies. Sometimes the theoretical understanding is lacking and the comparison serves to revise the theory and the model. Disagreements between the model simulation and data can also be due to problems with the data such as remote sensing retrieval errors. The iterative comparison and revision of models such as the GSFC 2D model and observations is what drives middle atmospheric science forward.

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Stratospheric ozone is affected by anthropogenically caused chlorine and bromine increases, solar cycle ultraviolet flux variations, and the changing sulfate aerosol abundance due to several volcanic eruptions. A study was recently completed, which included all three of these variations, with the GSFC 2D model to predict ozone variations over the 1979 to 1994 period. The model captures much of the variability and downward trend in total ozone that is measured by the Total Ozone Mapping Spectrometer (TOMS) instruments, on Nimbus 7 and on Meteor 3, over this time period.

The model simulations predict a decrease in total ozone of about 4% from 1979 to 1994 due to the chlorine and bromine increases. The changing sulfate aerosol abundances can also significantly affect total ozone with the Mt. Pinatubo eruption computed to cause a decrease in global ozone by about 3% in 1992. Solar ultraviolet flux variations cause increases and decreases in total ozone with computed changes of about 1% from solar maximum to minimum.

Model predictions for the future indicate that total ozone should start to recover from its lowest levels by the late 1990's. Future measurements of ozone are crucial to help quantify the recovery process.

For further discussion of past, present and future trends in ozone see Jackman, et al. (J. Geophys. Res., 101, 28,753-28,767, 1996).

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Observations of ozone by the Solar Backscatter UltraViolet (SBUV) and SBUV/2 instruments also indicate substantial changes in ozone during the period January 1979 to December 1993. The percentage changes in ozone over this time period are illustrated as trends per decade in the top figure above.

These ozone changes are believed to be caused by the increasing chlorine and bromine in the atmosphere over that 15 year time period from humans' production of chlorofluorocarbons (CFCs) and halons. The GSFC 2D model has been used to compute the ozone changes caused by the humankind-produced CFCs and halons over the 1979-93 time period.

The decadal trends predicted from the GSFC 2D model over this time period are given for two different model simulations (Models 1 and 2) in the lower two figures. Model 1 uses standard chemistry while Model 2 includes an added chemical reaction and leads to a smaller downward trend in the upper stratosphere (35-50 km) than computed in Model 1. Both Models 1 and 2 have similarities with the trends calculated from the SBUV and SBUV/2 observations, however, both Models 1 or 2 reveal some differences when compared to the observations.

(This is Figure 1 in Chandra et al. [1995])

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Selected Publications

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Principal Investigator

Charles H. Jackman, NASA GSFC

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Co-Investigator

Eric L. Fleming, Science Systems and Applications, Inc.


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Last Updated: 9 December 2004
Author: Charles Jackman (jackman@assess.gsfc.nasa.gov)
Web Curator: Leslie R. Lait (Hughes STX) (lrlait@ertel.gsfc.nasa.gov)
Responsible NASA organization/official: Dr. P. K. Bhartia, Atmospheric Chemistry and Dynamics Branch/Head