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Observations of the infrared solar spectrum from space by the ATMOS experiment.

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Remote sensing of the Earth's atmosphere from space with high-resolution Fourier-transform spectroscopy: development and methodology of data processing for the Atmospheric Trace Molecule Spectroscopy experiment.

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Pressure sounding of the middle atmosphere from ATMOS solar occultation measurements of atmospheric CO(2) absorption lines.

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Updated: Jun 11, 2026

Early Detection of Cyanobacterial Blooms and Associated Cyanotoxins using Fast Detection Strategy
07:13

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Published on: February 25, 2021

ATMOS data processing and science analysis methods.

R H Norton, C P Rinsland

    Applied Optics
    |June 29, 2010
    PubMed
    Summary
    This summary is machine-generated.

    The Atmospheric Trace Molecule Spectroscopy (ATMOS) instrument captured over 1500 solar spectra in 1985. This data enabled detailed studies of both the solar and Earth's upper atmospheres.

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    Area of Science:

    • Atmospheric science
    • Solar physics
    • Spectroscopy

    Background:

    • The Atmospheric Trace Molecule Spectroscopy (ATMOS) instrument is a high-speed Fourier transform spectrometer.
    • It operates in the mid-infrared range (2.2-16 micrometers).

    Purpose of the Study:

    • To describe the data processing pipeline for ATMOS telemetry data.
    • To detail the analysis software and methods for atmospheric and solar studies.
    • To introduce the ATMOS data analysis facility.

    Main Methods:

    • Recorded over 1500 solar spectra at approximately 0.0105-cm(-1) resolution.
    • Acquired spectra during high sun (solar atmosphere) and low sun (Earth's upper atmosphere) conditions.
    • Utilized a Fourier transform spectrometer operating in the mid-IR.

    Main Results:

    • Successfully converted telemetry data into analyzable spectra.
    • Developed and applied analysis software for atmospheric and solar studies.
    • Established a functional ATMOS data analysis facility.

    Conclusions:

    • The ATMOS instrument's first mission provided valuable spectral data.
    • The developed methods and facility are crucial for analyzing atmospheric and solar spectra.
    • This work lays the foundation for further research using ATMOS data.