Earth  ID: 5175

TEMPO - Nitrogen Dioxide Air Pollution Over North America - Additional Views

The Tropospheric Emissions: Monitoring of Pollution (TEMPO) instrument measures sunlight reflected and scattered off the Earth’s surface, clouds and the atmosphere. Gases in the atmosphere absorb the sunlight, and the resulting spectra are then used to determine the amounts of several gases in the Earth’s atmosphere, including nitrogen dioxide. The amount of nitrogen dioxide is provided as a “column density”, defined as the total number of nitrogen dioxide molecules in a column of air above a square centimeter on the Earth’s surface. The tropospheric column density is the amount of nitrogen dioxide in the lower part of the atmosphere, from the surface to about 10 km in altitude. In polluted regions, most of that nitrogen dioxide is located near the ground.

Because TEMPO is in a geostationary orbit, the instrument can continuously observe North American pollution during daylight hours. The instrument makes more frequent but only partial scans when part of the continent is dark, focusing on just the East (sunrise) or West (sunset).

In North America, nitrogen dioxide is primarily produced from burning fossil fuels for transportation, power generation and industrial activity, as well as from wildfires. Nitrogen dioxide plays an important role in the formation of ground-level ozone and particulate matter pollution, and is itself a toxic gas. These pollutants are harmful to both human and ecosystem health.

TEMPO is a collaboration between the Smithsonian Astrophysical Observatory at the Center for Astrophysics | Harvard & Smithsonian, and the NASA Langley Research Center. More information about the TEMPO mission can be found at:

Older Version

Visualization Credits

Kel Elkins (USRA): Visualizer
Laurence Schuler (ADNET Systems, Inc.): Technical Support
Ian Jones (ADNET Systems, Inc.): Technical Support
Trent L. Schindler (USRA): Visualizer
Cindy Starr (Global Science and Technology, Inc.): Visualizer
Caroline Nowlan (Center for Astrophysics | Harvard & Smithsonian): Scientist
Xiong Liu (Center for Astrophysics | Harvard & Smithsonian): Scientist
Katie Jepson (KBR Wyle Services, LLC): Producer
Please give credit for this item to:
NASA's Scientific Visualization Studio

Data provided by the Smithsonian Astrophysical Observatory at the Center for Astrophysics | Harvard & Smithsonian.

Short URL to share this page:

NASA Science >> Earth
SVS >> Pollution