Dynamics of diabatically forced anticyclonic plumes in the stratosphere

Author:

Podglajen Aurélien1ORCID,Legras Bernard1ORCID,Lapeyre Guillaume1ORCID,Plougonven Riwal1ORCID,Zeitlin Vladimir1ORCID,Brémaud Vincent1ORCID,Sellitto Pasquale23ORCID

Affiliation:

1. LMD/IPSL, École Polytechnique, Institut Polytechnique de Paris ENS, PSL Université, Sorbonne Université, CNRS Palaiseau France

2. Univ Paris Est Créteil and Université Paris Cité CNRS, LISA Créteil France

3. Istituto Nazionale di Geofisica e Vulcanologia Osservatorio Etneo Catania Italy

Abstract

AbstractA new class of vortices has been observed in the stratosphere following extreme wildfires (Canada 2017, Australia 2020) and volcanic eruptions (Raikoke 2019). These vortices are long‐lived mesoscale anticyclones (hundreds to 1,000 km in diameter) trapping plumes of aerosols and combustion/volcanic compounds. Owing to their unusual composition, these anticyclonically trapped plumes (ATPs) are associated with a significant radiative heating, which fuels their ascent through the stratosphere. This article investigates the dynamics of ATPs using two complementary approaches: analytically, in a potential vorticity (PV) perspective, and through idealised numerical simulations with the Weather Research and Forecasting (WRF) model. In both cases, we consider the vortical flow forced by a heating Lagrangian tracer. By reformulating the problem in the potential radius–potential temperature coordinate system introduced for tropical cyclones, we first clarify that ATP formation is concomitant with the injection of air into the stratosphere at extratropical latitudes. Then, we derive a set of simplified one‐dimensional equations describing the subsequent evolution of the flow after the injection. The equation obtained for the tracer is a variant of the classical Burgers' equation. In qualitative agreement with the three‐dimensional WRF simulations, this theoretical model predicts that ATPs develop an upper tracer front associated with sustained near‐zero anticyclonic PV, followed by a smooth tracer tail of cyclonic PV. Radiative relaxation of the temperature perturbations induced by the anticyclone and the presence of an initial PV anomaly tend to stabilise ATPs during their ascent. Finally, we note that the theory predicts a similar relationship between the plume and anticyclonic PV for cooled ATPs, which is supported by three‐dimensional simulations and may apply to the 2022 Hunga volcanic plume.

Funder

Agence Nationale de la Recherche

Publisher

Wiley

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