Early data from Aura and continuity from UARS and TOMS

E. Hilsenrath; M. R. Schoeberl; A. R. Douglass; P. K. Bhartia; J. Barnett; R. Beer; J. Waters; M. Gunson; L. Froidevaux; J. Gille; P. F. Levelt

doi:10.1007/s11214-006-9074-1

Early data from Aura and continuity from UARS and TOMS

E. Hilsenrath, M. R. Schoeberl, A. R. Douglass, P. K. Bhartia, J. Barnett, R. Beer, J. Waters, M. Gunson, L. Froidevaux, J. Gille, P. F. Levelt

Atmospheric Chemistry Observations & Modeling Administrative Office

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

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.

Original language	English
Pages (from-to)	417-430
Number of pages	14
Journal	Space Science Reviews
Volume	125
Issue number	1-4
DOIs	https://doi.org/10.1007/s11214-006-9074-1
State	Published - Apr 2006

Keywords

Atmospheric composition
Satellite observations

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10.1007/s11214-006-9074-1

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title = "Early data from Aura and continuity from UARS and TOMS",

abstract = "Aura, the last of the large EOS observatories, was launched on July\textasciitilde{}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 = "Atmospheric composition, Satellite observations",

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doi = "10.1007/s11214-006-9074-1",

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T1 - Early data from Aura and continuity from UARS and TOMS

AU - Hilsenrath, E.

AU - Schoeberl, M. R.

AU - Douglass, A. R.

AU - Bhartia, P. K.

AU - Barnett, J.

AU - Beer, R.

AU - Waters, J.

AU - Gunson, M.

AU - Froidevaux, L.

AU - Gille, J.

AU - Levelt, P. F.

PY - 2006/4

Y1 - 2006/4

N2 - 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.

AB - 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.

KW - Atmospheric composition

KW - Satellite observations

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SP - 417

EP - 430

JO - Space Science Reviews

JF - Space Science Reviews

IS - 1-4

ER -

Early data from Aura and continuity from UARS and TOMS

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