NASA Jet Propulsion Laboratory California Institute of Technology JPL Home Earth Solar System Stars & Galaxies Science & Technology Bring the Universe to You JPL Email News RSS Podcast Video
Follow this link to skip to the main content

Home
Research
Research Topics List
spacer
Earth Sciences
spacer
Planetary Sciences
spacer
Astrophysics & Space Sciences
spacer
Exploration & Observational Systems
spacer
Software & Computing Systems
Strategic Technology Directions
Guidelines for Ethics in Research
Laboratories and Facilities
Opportunities
Community
News and Events
ST icon
Office of the Chief Scientist and Chief Technologist
Research

Earth Sciences

Average Rating: 4 / 5 (6 ratings)
  •   star rating help
    How Do I Rate This?
    The blue stars show the average user rating for this item. To add your own rating, move your cursor over the stars to highlight them in gold, and click to show your rating. One star highlighted is the lowest rating, all five is the highest. Once you have rated an item, your rating is added to the average.
Atmospheric Science
Atmospheric Science

Atmospheric science at JPL is conducted by a diverse set of researchers who track ozone recovery, quantify tropospheric pollutants such as aerosols, ozone, and carbon
monoxide, and develop state-of-the-art atmospheric models. All of these efforts complement each other as instrument, lab study, and modeling teams collaborate to improve their measurements and understandings of current atmospheric conditions.


The study of Earth's environment and its preservation and improvement are at the heart of spaceborne experiments. Flight experiment scientists are:

  • Studying hurricanes and other aspects of weather from orbiting spacecraft in order to better understand these phenomena
  • Measuring cloud properties and aerosol particles in the atmosphere and mapping vegetated and icy areas
  • Observing stratospheric ozone to characterize depletion and the resulting ozone hole
  • Mapping the global distribution of water vapor, the most abundant of the greenhouse gases, in order to understand its effect on climate change
  • Mapping the global distribution of the water vapor isotope, HDO, an indicator of atmospheric dynamic and the water cycle
  • Mapping tropospheric ozone distribution to study global air quality
  • Mapping global carbon dioxide columns to constrain regional sources and sinks of CO2
  • Measuring fundamental spectroscopic and kinetic parameters that are critical to the interpretation of the remotely sensed data


Remote Sensing Observations

JPL is responsible for the integrity and analysis of the data that returns to earth from various instrument on NASA’s A-Train constellation of earth observing spacecrafts. Many of these spacecrafts have on-board instruments that, using various techniques, remotely observe the earth’s atmosphere.

Tropospheric Emission Spectrometry

Work performed in this area is centered on the data returned from the Tropospheric Emission Spectrometer (TES) experiment on the EOS-Aura satellite. TES is an infrared Fourier Transform Spectrometer designed to make global measurements of tropospheric ozone and its chemical precursors.

Air pollution species that TES measures include ozone and CO, as well as ammonia (NH3) and methanol. Global mid-tropospheric CO2 measurements have been derived from TES, as well as the instantaneous radiative forcing of ozone, and global methane fields. Water vapor isotope, HDO, measurements are used to study the water cycle and atmospheric dynamics.

TES mesaurements
Ozone and Carbon Monoxide measurements from the TES instrument

Microwave Atmospheric Science

Microwave instruments are used to obtain information about the chemistry, hydrology, and dynamics of Earth's atmosphere. Its overall goal is to produce information that is needed for understanding and protecting the health of our atmosphere - using the unique capabilities and infrastructure provided by JPL and NASA. Research in this area is 'anchored' on the Microwave Limb Sounder (MLS) experiments, which were initiated at JPL in the early 1970s - starting with aircraft, progressing through balloon and then satellite instruments.

MLS measurements
EOS MLS measurements of ozone loss during the 2004-05 Arctic winter

The first MLS satellite experiment was on the Upper Atmosphere Research Satellite (UARS), launched in 1991 to assess the chlorine threat to stratospheric ozone. The second, EOS MLS, is on the EOS Aura satellite, launched July 15 2004, with an expected operational lifetime of at least five years. The overall objectives of EOS MLS are to:

  1. Track recovery of ozone layer chemistry
  2. Provide information on how atmospheric composition affects climate
  3. Provide information on pollution in the upper troposphere

The EOS MLS measures many more chemical species than were possible with the first MLS, due to infusion of new submillimeter technology developed at JPL.

Aerosol and Cloud Science

The MISR instrument on board the Terra spacecraft collects multi-angle as well as multi-spectral data never before obtained by satellite instruments. The additional information contained in these data make it possible to set limits on particle size and composition, as well as aerosol amount, measured over ocean. The data is also be used to derive aerosol properties in the atmosphere over heterogeneous land and dense dark vegetation. Researchers use different methods to derive aerosol properties over different types of surface.

MISR also significantly adds to current understanding of clouds and solar radiation in several ways, but its most important contributions will be to provide more accurate estimates of cloud albedo. MISR's nine cameras span much of the range of angles over which cloud reflectivity varies. The albedo retrieved by MISR are expected to be ten times more accurate than those obtained from similar measurements with only a single camera looking straight down.


In Situ Atmospheric Measurements

JPL makes many in situ measurements of the atmosphere and is able to routinely support field campaigns. Many scientists conducting studies with in situ instruments are active in validation and other campaigns that take place several times a year. Balloons are able to lift their payloads about 99.7% of the earth’s atmosphere so that they can more accurately measure vertical profiles of atmospheric gases.

Mark IV Interferometer

A Mark IV interferometer team uses a mid-infrared Fourier transform interferometer to measure the atmosphere using the Sun as a source. The Mark IV interferometer can be deployed in a stratospheric balloon gondola, on aircraft, or on the ground.

Balloon OH (BOH) measurements

This instrument mounted on a balloon uses a heterodyne radiometer to detect thermal emission from the OH radical in the Earth's stratosphere. BOH is deployed in a stratospheric balloon gondola and is used to validate OH measurements made by the Microwave Limb Sounder (MLS) instrument on the Aura satellite.

Submillimeter Limb Sounder (SLS) instrument

SLS uses a cryogenic heterodyne radiometer to detect thermal emission from multiple molecules near 640 GHz in the Earth's stratosphere. SLS is deployed in a stratospheric balloon gondola or on aircraft.

Mark IV Profiles
Figure above shows profiles of normalized Potential Vorticity (sPV) for the dates and locations of various MkIV balloon flights

LIDAR Measurements

LIDAR is used by groups at JPL to measure tropospheric and stratospheric temperature, ozone and water. Instrumentation is housed at Table Mountain and in Hawaii.

The LIDAR group has expertise in remote sensing instrumentation, and retrievals as well as atmospheric science. There are close ties with the MLS project, the TES project, the OCO project, and the Network for Detection of Stratospheric Change.

LIDAR seasonal measurements
The 5-year ozone climatology shows a very well pronounced annual cycle around 15 km characterized by a maximum in late winter/spring, and a minimum in late summer/fall. (Figure on the left is TMO, right is TMF.)




Laboratory Studies and Modeling

Laboratory Studies
This activity involves the use of state-of-the-art experimental techniques to measure kinetic, photochemical and spectroscopic parameters related to elementary atmospheric processes. Rate coefficients, cross sections and quantum yields are measured using methods such as laser photolysis, discharge-flow and steady-state photolysis combined with high-sensitivity detection methods such as molecular beam mass spectrometry, long-path UV-visible-NIR absorption, diode laser wavelength modulation spectroscopy and laser-induced fluorescence.

Particular importance is placed on processes that play important roles in polar ozone depletion, long-term trends in stratospheric ozone at mid-latitudes, the oxidizing potential of the troposphere, and the formation of oxidants in urban and regional environments.

Quantitative spectroscopy is another key focus of the laboratory studies program. JPL’s Molecular Spectroscopy Team takes measurements of molecules from the microwave through the ultraviolet spectral regions to measure spectroscopic parameters of atmospheric molecules with extremely high precision and accuracy. These parameters are required for the measurement of atmospheric composition and structure by NASA remote sensing instruments for studies in Earth and planetary sciences, astrobiology and astrophysics.

Modeling

In this area, computer models of atmospheric processes are developed and used to interpret data from satellite and field measurements, as prognostic tools to understand long-term changes in climate and composition, and to diagnose elementary processes in atmospheric transport and chemistry.

GEOS-Chem CO2
CO2 at 30 hPa during Apr 2003, as modeled by GEOS-Chem

For tropospheric studies, researchers use three-dimensional chemical transport models that incorporate winds derived from weather models. In combination with detailed emission inventories of trace gases, these models have been used to study long-range pollution transport, to determine the effects of biomass burning on global air quality, and to derive budgets of the production and loss of trace gases and estimate their dependence on natural and anthropogenic sources. Many of these model studies use global measurements of trace gases from space to constrain the model calculations. These models are also used in satellite validation studies, where they provide a platform for comparing ground-based, aircraft, and satellite measurements. Stratospheric modeling efforts use many of the same tools and techniques to understand the dynamical and chemical processes that lead to stratospheric ozone depletion as well as to study the budgets of ozone and other trace gases in the important transition region between the troposphere and stratosphere.

At regional and cloud-resolving scales, a fully coupled aerosol-chemistry-meteorology model (WRF-Chem) has been used to simulate the emission, transport, mixing, and chemical transformation of trace gases and aerosol-cloud interactions. Both direct and indirect effects of aerosols are included in the model and are shown to have significant impacts on clouds and precipitation. The model results are compared closely with satellite observations, and we are exploring ways to establish a framework for the application of satellite data to the evaluation and improvement of model parameterizations.



Contacts

Michelle Santee - Management Contact
E-Mail: Michelle.Santee@jpl.nasa.gov
Phone: 818.354.9424

Dong Wu - Aerosols and Clouds
E-Mail: Dong.L.Wu@jpl.nasa.gov
Phone: 818.393.1954

Joao Teixeira - Climate Physics
E-Mail: Joao.Teixeira@jpl.nasa.gov
Phone: 818.354.2762

Geoffrey Toon - Atmospheric Observations
E-Mail: Geoffrey.Toon@jpl.nasa.gov
Phone: 818.354.8259

Stanley Sander - Lab Studies and Modeling
E-Mail: Stanley.P.Sander@jpl.nasa.gov
Phone: 818.354.2625

John Worden - Tropospheric Emission Spectroscopy
E-Mail: John.R.Worden@jpl.nasa.gov
Phone: 818.393.7122


Links

Site Manager:  Brian Knosp
Webmasters:  Cornell Lewis, Maryia Davis

JPL Clearance:  CL#08-4147