Preprints
https://doi.org/10.5194/amt-2022-224
https://doi.org/10.5194/amt-2022-224
 
03 Aug 2022
03 Aug 2022
Status: a revised version of this preprint was accepted for the journal AMT and is expected to appear here in due course.

Satellite observations of gravity wave momentum flux in the mesosphere / lower thermosphere (MLT): feasibility and requirements

Qiuyu Chen1, Konstantin Ntokas1, Björn Linder2, Lukas Krasauskas1, Manfred Ern1, Peter Preusse1, Jörn Ungermann1, Erich Becker3, Martin Kaufmann1, and Martin Riese1 Qiuyu Chen et al.
  • 1Institute of Energy and Climate Research (IEK-7: Stratosphere), Forschungszentrum Jülich, Jülich, Germany
  • 2Department of Meteorology, Stockholm University, Stockholm, Sweden
  • 3Northwest Research Associates Inc., Boulder, CO, USA

Abstract. In the recent decade it became evident that we need to revise our picture of how gravity waves (GWs) reach the mesosphere and lower thermosphere (MLT). This has consequences for not just the properties of the GWs itself, but in particular for the global circulation in the MLT. Information on spectral distribution, direction and zonal mean GW momentum flux is required to test the theoretical and modeling findings. In this study, we propose a constellation of two CubeSats for observing mesoscale GWs in the MLT region by means of temperature limb sounding in order to derive such constraints. Each CubeSat deploys a highly miniaturized spatial heterodyne interferometer (SHI) for the measurement of global oxygen atmospheric band emissions. From these emissions, the 3-D temperature structure can be inferred. We propose to obtain four independent observation tracks by splitting the interferograms in the center and thus gaining 2 observation tracks for each satellite. We present a feasibility study of this concept based on self-consistent, high-resolution global model data. This yields a full chain of end-to-end (E2E) simulation incorporating 1) orbit simulation; 2) airglow forward modelling; 3) tomographic temperature retrieval; 4) 3-D wave analysis; and 5) GW momentum flux (GWMF) calculation. The simulation performance is evaluated by comparing the retrieved zonal-mean GWMF with that computed directly from the model wind data. A major question to be considered in our assessment is the minimum number of tracks required for the derivation of 3D GW parameters with sufficient accuracy. In particular, our simulations show that the GW polarization relations are still valid in the MLT region and can thus be employed for inferring GWMF from the 3--D temperature distributions. Based on the E2E simulations for gaining zonal-mean climatologies of GW momentum flux, we demonstrate that our approach is robust and stable, given a four-track observation geometry and the expected instrument noise under nominal operation conditions. Using phase-speed-direction spectra we show also that the properties of individual wave events are recovered when employing four tracks. Finally, we discuss the potential of the proposed observations to address current topics in the GW research. We outline for which investigations ancillary data are required to answer science questions.

Qiuyu Chen et al.

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on amt-2022-224', Anonymous Referee #1, 24 Aug 2022
    • AC1: 'Reply on RC1', Qiuyu Chen, 03 Nov 2022
  • RC2: 'Comment on amt-2022-224', Anonymous Referee #2, 21 Sep 2022
    • AC2: 'Reply on RC2', Qiuyu Chen, 03 Nov 2022

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on amt-2022-224', Anonymous Referee #1, 24 Aug 2022
    • AC1: 'Reply on RC1', Qiuyu Chen, 03 Nov 2022
  • RC2: 'Comment on amt-2022-224', Anonymous Referee #2, 21 Sep 2022
    • AC2: 'Reply on RC2', Qiuyu Chen, 03 Nov 2022

Qiuyu Chen et al.

Qiuyu Chen et al.

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Short summary
Observations of phase-speed – direction spectra and zonal mean net gravity wave momentum flux are required to understand how gravity waves reach the mesosphere / lower thermospshere and how they there interact with the background flow. To this end we propose to fly two CubeSats, each deploying a spatial heterodyne spectrometer for limb observation of the airglow. End-to-end simulations demonstrate that individual gravity waves are retrieved faithfully for the expected instrument performance.