Middle-Atmosphere Temperature Monitoring Addressed with a Constellation of CubeSats Dedicated to Climate Issues

Philippe Keckhut LATMOS/IPSL, UVSQ, Université Paris-Saclay, Sorbonne Université, CNRS/INSU, Guyancourt, France

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Alain Hauchecorne LATMOS/IPSL, UVSQ, Université Paris-Saclay, Sorbonne Université, CNRS/INSU, Guyancourt, France

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Mustapha Meftah LATMOS/IPSL, UVSQ, Université Paris-Saclay, Sorbonne Université, CNRS/INSU, Guyancourt, France

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Sergey Khaykin LATMOS/IPSL, UVSQ, Université Paris-Saclay, Sorbonne Université, CNRS/INSU, Guyancourt, France

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Chantal Claud Laboratoire de Météorologie Dynamique, Ecole Polytechnique, CNRS/INSU, Palaiseau, France

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Pierre Simoneau ONERA, Chemin de la Hunière, Palaiseau, France

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Abstract

While meteorological numerical models extend upward to the mesopause, mesospheric observations are required for leading simulations and numerical weather forecasts and climate projections. This work reviews some of the challenges about temperature observation requirements and the limiting factors of the actual measurements associated with atmospheric tides. A new strategy is described here using a limb-scattering technique that is based on previous experiments in space. Such observations can be used with cube satellites. Technical issues are the large dynamic range (4 orders of magnitude) required for the measurements, the accuracy of the limb pointing, and the level of stray light. The technique described here will expect accuracy of 1–2 K with a vertical resolution of 1–2 km. A constellation of 100 platforms could provide temperature observations with space (100 km) and time (3 h) resolutions recommended by the World Meteorological Organization, and tidal issues could be resolved with a minimum of 3–5 platforms with specific orbit maintained to avoid drifts.

© 2021 American Meteorological Society. For information regarding reuse of this content and general copyright information, consult the AMS Copyright Policy (www.ametsoc.org/PUBSReuseLicenses).

Corresponding author: Philippe Keckhut, keckhut@latmos.ipsl.fr

Abstract

While meteorological numerical models extend upward to the mesopause, mesospheric observations are required for leading simulations and numerical weather forecasts and climate projections. This work reviews some of the challenges about temperature observation requirements and the limiting factors of the actual measurements associated with atmospheric tides. A new strategy is described here using a limb-scattering technique that is based on previous experiments in space. Such observations can be used with cube satellites. Technical issues are the large dynamic range (4 orders of magnitude) required for the measurements, the accuracy of the limb pointing, and the level of stray light. The technique described here will expect accuracy of 1–2 K with a vertical resolution of 1–2 km. A constellation of 100 platforms could provide temperature observations with space (100 km) and time (3 h) resolutions recommended by the World Meteorological Organization, and tidal issues could be resolved with a minimum of 3–5 platforms with specific orbit maintained to avoid drifts.

© 2021 American Meteorological Society. For information regarding reuse of this content and general copyright information, consult the AMS Copyright Policy (www.ametsoc.org/PUBSReuseLicenses).

Corresponding author: Philippe Keckhut, keckhut@latmos.ipsl.fr
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