Impact of Gravity Waves on the Middle Atmosphere of Mars: A Non‐Orographic Gravity Wave Parameterization Based on Global Climate Modeling and MCS Observations. Issue 3 (10th March 2020)

• Record Type: Journal Article
• Authors: Gilli, G.; Forget, F.; Spiga, A.; Navarro, T.; Millour, E.; Montabone, L.; Kleinböhl, A.; Kass, D. M.; McCleese, D. J.; Schofield, J. T.
• Is Part Of: Journal of geophysical research. Volume 125:Issue 3(2020)
• Page Start: n/a
• Page End: n/a
• Publication Date: 2020-03-10
• Subjects: general circulation model -- Mars middle atmosphere -- non‐orographic gravity waves -- thermal tides -- Mars Climate Database; Planets -- Periodicals; Geophysics -- Periodicals; 559.9
• DOI: 10.1029/2018JE005873
• Languages: English
• ISSNs: 2169-9097

Abstract

Abstract: The impact of gravity waves (GW) on diurnal tides and the global circulation in the middle/upper atmosphere of Mars is investigated using a general circulation model (GCM). We have implemented a stochastic parameterization of non‐orographic GW into the Laboratoire de Météorologie Dynamique (LMD) Mars GCM (LMD‐MGCM) following an innovative approach. The source is assumed to be located above typical convective cells ( ∼ 250 Pa), and the effect of GW on the circulation and predicted thermal structure above 1 Pa ( ∼ 50 km) is analyzed. We focus on the comparison between model simulations and observations by the Mars Climate Sounder (MCS) on board Mars Reconnaissance Orbiter during Martian Year 29. MCS data provide the only systematic measurements of the Martian mesosphere up to 80 km to date. The primary effect of GW is to damp the thermal tides by reducing the diurnal oscillation of the meridional and zonal winds. The GW drag reaches magnitudes of the order of 1 m/s/sol above 10 − 2 Pa in the northern hemisphere winter solstice and produces major changes in the zonal wind field (from tens to hundreds of m/s), while the impact on the temperature field is relatively moderate (10–20 K). It suggests that GW‐induced alteration of the meridional flow is the main responsible for the simulated temperature variation. The results also show that with the GW scheme included, the maximum day‐night temperature difference due to the diurnal tide is around 10 K, and the peak of the tide is shifted toward lower altitudes, in better agreement with MCS observations. Key Points: A stochastic non‐orographic gravity wave (GW) scheme is implemented into the LMD‐MGCM Non‐orographic GW generated above typical convective layers control diurnal tides The implemented GW scheme improves the accuracy of the LMD‐MGCM between 1 and 0.01 Pa in comparison with MCS