EGU2020-4091
https://doi.org/10.5194/egusphere-egu2020-4091
EGU General Assembly 2020
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Aeolus: ESA’s wind mission. Status and future challenges

Tommaso Parrinello1, Anne Grete Straume2, Jonas Von Bismark1, Sebastian Bley1, Viet Duc Tran3, Peggy Fischer1, Thomas Kanitz2, Denny Wernham2, Thorsten Fehr2, Emilio Alvarez2, Oliver Reitebuch4, and Isabell Krisch4
Tommaso Parrinello et al.
  • 1ESA/ESRIN, Frascati, Italy
  • 2ESA/ESTEC, Noordwijk, The Netherlands
  • 3ESA/ESOC, Darmstadt, Germany
  • 4DLR, Oberpfaffenhofen, Germany

The European Space Agency (ESA)’s wind mission, Aeolus, was launched on 22 August 2018. Aeolus is a member of the ESA Earth Explorer family and its main objective is to demonstrate the potential of Doppler wind Lidars in space for improving weather forecast and to understand the role of atmospheric dynamics in climate variability. Aeolus carries a single instrument called ALADIN: a high sophisticated spectral resolution Doppler wind Lidar which operates at 355 which is the first of its kind to be flown in space. It provides profiles of single horizontal line-of-sight winds (primary product) in near-real-time (NRT), and profiles of atmospheric backscatter and extinction. The instrument samples the atmosphere from about 30 km down to the Earth’s surface, or down to optically thick clouds. The required precision of the wind observations is 1-2.5 m/s in the troposphere and 3-5 m/s in the stratosphere while the systematic error requirement be less than 0.7 m/s. The mission spin-off product includes information about aerosol and cloud layers. The satellite flies in a polar dusk/dawn orbit (6 am/pm local time), providing ~16 orbits per 24 hours with an orbit repeat cycle of 7 days. Global scientific payload data acquisition is guaranteed with the combined usage of Svalbard and Troll X-band receiving stations.

The status of the Aeolus mission will be provided, including its performance assessment, planned operations and exploitation in the near future. This comprises the outcome of the instrument in its early operation phase, calibration and validation activities and a general review of the main scientific findings. Scope of the paper is also to inform about the programmatic highlights and future challenges.

How to cite: Parrinello, T., Straume, A. G., Von Bismark, J., Bley, S., Tran, V. D., Fischer, P., Kanitz, T., Wernham, D., Fehr, T., Alvarez, E., Reitebuch, O., and Krisch, I.: Aeolus: ESA’s wind mission. Status and future challenges , EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-4091, https://doi.org/10.5194/egusphere-egu2020-4091, 2020.

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  • CC1: Comment on EGU2020-4091, Gail Skofronick-Jackson, 05 May 2020

    Nice Presentation! Gail Skofronick Jackson

    • AC1: Reply to CC1, Tommaso Parrinello, 05 May 2020

      Thank you so much

  • CC2: MRD threshold, Peter Knippertz, 05 May 2020

    Nice presentation. Could you please explain what the MRD threshold is and how it is determined for Aeolus?

    Thanks!

    • AC2: Reply to CC2, Anne Grete Straume-Lindner, 06 May 2020

      Hi Peter, do you mean the L2B wind (HLOS component) random and systematic error requirements? These are: Random errors (precision): 1 m/s (0-2 km altitude) and 2.5 m/s (2-16 km altitude). Above 16 km it is desired to achieve 3-5 m/s. Unknown systematic errors (bias): 0.7 m/s. The Aeolus Mission Requirements Document (MRD) can be found e.g. here:

      • AC3: Reply to AC2, Anne Grete Straume-Lindner, 06 May 2020

        I see that web links cannot be posted here. The Aeolus MRD is available on the ESA Aeolus web site and the Aeolus AO CAL/VAL call site.