01 Jul 2022
01 Jul 2022

Evolution of squall line variability and error growth in an ensemble of LES

Edward Groot and Holger Tost Edward Groot and Holger Tost
  • Institut für Physik der Atmosphäre, Johannes Gutenberg Universität, Johannes-Joachim-Becher-Weg 21, Mainz, Germany

Abstract. Squall lines represent an organized form of atmospheric convection that link processes occurring at the small end of the mesoscale and processes ocurring at the large end of the mesoscale. This study analyses the initial condition sensitivity of idealized squall lines in an LES ensemble. The ensemble spread of the squall lines is evaluated using passive tracers, an ensemble sensitivity analysis, other statistical tools and an error growth metric. Analysing gravity wave dynamics, convective initiation, squall line relative motion and updraft/downdraft characteristics and transport, a chain of interacting processes is identified.

From the convective point of view ensemble spread is rooted in a secondary phase of convective initiation (30–35 min) a few km ahead of the squall line. Contrasts in the amount secondary initiation arise within the ensemble, as vertical velocity varies at the location of convective initiation within the ensemble due to differences in gravity wave amplitude and phase. Immediately after the secondary phase of initiation (30–45 min), the cold pool accelerates to velocities of 2–4 m/s (ensemble envelope).

With the spread in secondary convective initiation, upward mass transport is disturbed, which also affects downdraft mass fluxes. Furthermore, once accelerated (30–40 minutes), the cold pool nearly maintains its propagation speed in each ensemble member. It is shown that part of the errors occurring after 45–85 minutes are explained by the cold pool velocity and a correction for cold pool velocity removes a substantial fraction of the spread. A coherent anomaly of the circulation within the squall line, which is consistent with extra upward mass transport, exists during this phase of the evolution. It is proposed that the identified chain of interactions may be explained by a common mode of variability, which determines a substantial portion of the ensemble spread in the stage after 30–85 minutes in many diagnostics.

Based on a non-monotonic relation between initial conditions and local vertical velocities that cause secondary initiation, one can argue that an intrinsic limit of predictability exists, as Melhauser and Zhang (2012) do.

Edward Groot and Holger Tost

Status: final response (author comments only)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2022-515', Anonymous Referee #1, 08 Jul 2022
  • RC2: 'Comment on egusphere-2022-515', Anonymous Referee #2, 01 Aug 2022
  • AC1: 'AC: response to RC1 and RC2', Edward Groot, 20 Sep 2022
  • AC2: 'AC: response to RC1 and RC2', Edward Groot, 20 Sep 2022

Edward Groot and Holger Tost

Data sets

Output data and namelist - README file ’Evolution of squall line variability and error growth in an ensemble of LES’ Groot, Edward

Edward Groot and Holger Tost


Total article views: 406 (including HTML, PDF, and XML)
HTML PDF XML Total Supplement BibTeX EndNote
313 78 15 406 35 10 5
  • HTML: 313
  • PDF: 78
  • XML: 15
  • Total: 406
  • Supplement: 35
  • BibTeX: 10
  • EndNote: 5
Views and downloads (calculated since 01 Jul 2022)
Cumulative views and downloads (calculated since 01 Jul 2022)

Viewed (geographical distribution)

Total article views: 374 (including HTML, PDF, and XML) Thereof 374 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
Latest update: 29 Nov 2022
Short summary
Thunderstorm systems play an important role in the dynamics of the Earth’s atmosphere and some of them form a well organised line: squall lines. Simulations of such squall lines with very small initial perturbations are compared to an unperturbed control simulation. The evolution of perturbations and processes amplifying them are analysed. It is shown that the formation of new secondary thunderstorm cells (after the initial primary cells) directly ahead of the line affects the spread strongly.