- IN32A-03: TEMPO at Night
-
NOLA CC
Author(s):Generic 'disconnected' Message
James Carr, Carr Astronautics Corporation (First Author, Presenting Author)
Heesung Chong, Center for Astrophysics | Harvard & Smithsonian
Xiong Liu, Center for Astrophysics | Harvard & Smithsonian
John Houck, Center for Astrophysics | Harvard & Smithsonian
Virginia Kalb, NASA Goddard Space Flight Center
Zhuosen Wang, University of Maryland College Park/NASA Goddard Space Flight Center
Houria Madani, Carr Astronautics Corporation
Daniel Lindsey, NOAA/NESDIS/GOES-R
Steven Miller, Colorado State Univ-CIRA
Sergey Marchenko, SSAI
Zhixin Xue, University of Iowa
Jun Wang, the University of Iowa
Dong Wu, Climate and Radiation Laboratory, NASA/GSFC
David Flittner, NASA Langley Research Center
Kelly Chance, Center for Astrophysics | Harvard & Smithsonian
NASA’s TEMPO instrument operates over the equator at 91ºW longitude from a commercial communications satellite. During daytime, it measures the concentrations of trace gases and pollutants in the atmosphere. At night, it collects images of city lights, aurorae, moonlit clouds, gas flares, light from ships, and lightning. TEMPO makes a spectrum of the light from each pixel, and this enables a host of applications such as spectral classification of city lights to map usage of LED, high pressure sodium, and other types of artificial lighting, which has implications for health, ecology, and light pollution mitigation. Many spectral features can be seen in the spectra of aurorae, night glow, and lightning, and the temperature of gas flares can be measured.
Scientific DisciplineNeighborhoodType
Enter Note
Go to previous page in this tab
Session


