Space Science Reviews

, Volume 125, Issue 1, pp 417–430

Early Data from Aura and Continuity from Uars and Toms

Authors

    • NASA Goddard Space Flight Center
  • M. R. Schoeberl
    • NASA Goddard Space Flight Center
  • A. R. Douglass
    • NASA Goddard Space Flight Center
  • P. K. Bhartia
    • NASA Goddard Space Flight Center
  • J. Barnett
    • Oxford University
  • R. Beer
    • Jet Propulsion Laboratory
  • J. Waters
    • Jet Propulsion Laboratory
  • M. Gunson
    • Jet Propulsion Laboratory
  • L. Froidevaux
    • Jet Propulsion Laboratory
  • J. Gille
    • University of Colorado
  • P. F. Levelt
    • Royal Netherlands Meteorological Institute
Article

DOI: 10.1007/s11214-006-9074-1

Cite this article as:
Hilsenrath, E., Schoeberl, M.R., Douglass, A.R. et al. Space Sci Rev (2006) 125: 417. doi:10.1007/s11214-006-9074-1

Abstract

Aura, the last of the large EOS observatories, was launched on July~15, 2004. Aura is designed to make comprehensive stratospheric and tropospheric composition measurements from its four instruments, HIRDLS, MLS, OMI and TES. These four instruments work in synergy to provide data on ozone trends, air quality and climate change. The instruments observe in the nadir and limb and provide the best horizontal and vertical resolution ever achieved from space. After over one year in orbit the instruments are nearly operational and providing data to the scientific community. We summarize the mission, instruments, and initial results and give examples of how Aura will provide continuity to earlier chemistry missions.

Keywords

satellite observationsatmospheric composition

Copyright information

© Springer Science+Business Media, Inc. 2006