HALO

WAVEGUIDE

A HALO aircraft mission to explore gravity waves in the polar night jet

Mission status: Scheduled.

Persons in Charge

Mission-PI

Bernd Kaifler, DLR-IPA, Oberpfaffenhofen

Mission coordinator​

tba

Contact point at DLR-FX for this mission:

HALO Deployment Base

Time Period

September – December 2026

Mission phases
  • 14 Sep 26 – 20 Nov 26 || Preparation, Payload integration, EMI testing
  • 23 Nov 26 – 18 Dec 26 || Mission execution
  • Dec 26 || Dismounting of Payload

Project description

Scientific rationale

Atmospheric gravity waves play an important role in the dynamical coupling of the atmosphere. They propagate horizontally and vertically over vast distances and transport energy and momentum. The dissipation of this momentum in the mesosphere drives the global residual circulation which connects both hemispheres and has drastic effects on the thermal structure of the atmosphere. As internal gravity waves are mainly generated in the troposphere, wave generation, propagation and dissipation represent the dominant mechanism which couples the atmosphere from below to above. However, the atmosphere is also coupled from above to below by means of gravity waves. Since gravity waves modify the background flow through wave dissipation and momentum deposition, they influence the propagation of planetary scale waves, thereby affecting the circulation in the troposphere.

Understanding and quantifying these coupling processes is essential for improving both climate models and numerical weather prediction models. However, the details of the involved processes are not yet understood, and parameterizations of gravity waves used in models yield inadequate results so far and are subject to tuning. For example, state-of-the-art general circulation models show that, in particular, gravity wave drag is missing in a latitude belt near 60°S. The missing drag contributes to the so-called cold pole bias observed in climate chemistry models. Many ideas and suggestions have been put forward to explain its existence. Proposed generation mechanisms for the missing gravity waves include fronts and jets in the troposphere, orography from big obstacles (mountain ranges) to small islands in the ocean, secondary wave generation by the multitude of primary waves excited in the troposphere, and stratospheric sources. The latter are least explored due to inherent difficulties in observing the dynamic state of the atmosphere at stratospheric altitudes. Satellite-based instruments have a comparatively low spatial resolution and, most importantly, lack the necessary temporal coverage to detect and track the formation of individual gravity wave packets. On the other hand, ground-based instrumentation is non-existent at southern latitudes near 60°S and sparse in the northern hemisphere. Only in the last years airborne high-resolution remote sensing instruments for the middle atmosphere have become available. During the DEEPWAVE field campaign, stratospheric and mesospheric gravity waves were observed over and in the vicinity of New Zealand. Only one flight to high latitudes (to 63°S) was undertaken during DEEPWAVE. The focus of the SouthTRAC campaign in 2019, which was based from Rio Grande in in the southern part of Argentina, was the southern polar vortex at around 60°S, which was unfortunately decreasing in strength in the latter part of the campaign period. Thus, only during few flights gravity waves were observed to reach stratospheric and lower mesospheric altitudes. Recent observations with a ground-based lidar from South Pole indicate the presence of inertia-gravity waves at the center of the polar vortex, which are generated by a stratospheric source not yet understood.

It is hypothesized that an unexplored stratospheric gravity wave source exists at locations of the polar night jet, which are characterized by significant deviations from a balanced state. In addition, the polar night jet acts as a waveguide for gravity waves: orographic and non-orographic gravity waves are refracted into the polar night jet and are able to propagate over vast distances within the jet. These refracted gravity waves interact with locally generated gravity waves, and increase the gravity wave drag.

More observations of gravity waves in the middle atmosphere at high latitudes are needed in order to answer open questions like: Which local conditions relative to the polar night jet are necessary to effectively excite gravity waves? To what extent do theoretical and numerical models predict potential source regions in terms of horizontal and vertical extent, direction of gravity wave emission, temporal coherence, spectral distribution and wave capturing? Which horizontal dimensions do wave packets that are focused into the polar night jet, achieve? What is the intermittency of gravity wave packets in space and time of and what is their relative contribution to momentum deposition in the mesosphere?

Objectives

The primary goal of the WAVEGUIDE mission is to test the hypotheses and address the questions mentioned in the previous section. In particular, the mission addresses the following scientific objectives:

(1) Investigation of non-orographic internal gravity waves in the vicinity of the polar night jet

(2) Exploration of gravity waves inside the polar vortex and above the pole region

(3) Characterization of gravity wave activity in relation to the spatial and temporal development of the polar vortex for model comparisons

(4) Investigation of mountain wave breaking and secondary wave generation

(5) Case study looking at refraction and horizontal propagation of mountain waves in the stratosphere

(6) Investigation of turbulence in the upper troposphere, lower stratosphere region

Proposal

Long duration, high-altitude flights are conducted to measure the vertical and horizontal distribution of gravity waves at the edge and center of the stratospheric polar vortex in the northern hemisphere. The synergy of downward-looking sensors (e.g. GLORIA) and upward-looking remote sensing instruments (ALIMA) is exploited to resolve the different tropospheric versus stratospheric sources of gravity waves and to investigate their vertical propagation. Momentum fluxes are derived from in-situ measurements (BAHAMAS). Radiosondes are launched to characterize the wind field. Data from ground-based radars and lidars, e.g. in Kühlungsborn (Germany), Kiruna (Sweden), Andenes (Norway), and Sodanyklä (Finland) are utilized to investigate the changing wave propagation conditions when the edge of the polar night jet passes over these stations. The temporal evolution is separated from spatial changes in the structure of the polar night jet by conducting lateral transects as well as overpasses with HALO over the ground-based instruments.

Partners

    • German Aerospace Center, Institute of Atmospheric Physics (DLR-IPA)
    • Forschungszentrum Jülich (FZ Jülich)
    • Karlsruhe Institute of Technology (KIT)

Scientific instruments and payload configuration

  • List of scientific instruments for the mission:

  • ALIMA

    Rayleigh-Doppler lidar | B. Kaifler (DLR-IPA)

  • GLORIA

    Gimballed Limb Observer for Radiance Imaging of the Atmosphere | F. Friedl-Vallon (KIT) & P. Preuße (FZJ)

  • BAHAMAS

    HALO Basic Data Acquisition System | Andreas Giez (DLR-FX)

Cabin and exterior configuration of HALO for the mission

TBA

HALO flights for this mission

Flights are listed by
Aircraft registration | Date | Take-off / Landing (UT) | Total flight time (h) | From / To | Mission #

  • D-ADLR | yyyy-mm-dd | hh:mm:ss – hh:mm:ss | h.hh | CODE – CODE | RF01
  •  

More information

* contact bernd [dot] kaifler [at] dlr [dot] de for access

Press releases, media etc.