Turbulence regimes over the Amazon Forest

Abstract

Our goal is the detailed characterization of turbulence regimes at the ATTO tower site. This includes both nighttime (very stable or weakly stable) and daytime (mixed or forced convection). We will characterize them in terms of parameters that are external to the planetary boundary layer (PBL), such as large-scale wind forcing, radiative processes, roughness and thermal surface properties. This is important because internal parameters, commonly used for that purpose, are affected by the same problems that make turbulence regime determination difficult, such as the lack of turbulence in the very stable case or its peculiar geometry in free convection. With this analysis, we will also address the effects of the turbulence regimes in the vertical profiles of concentration and fluxes of the different chemical species that are measured at the ATTO tower. We will then compare the relationships found with analyses we performed at other places. Our aim is to generalize the dependence of the turbulence regimes on parameters that are external to the PBL in a quasi-universal way. The final goal is to implement the general relationships found between fluxes and gradients of mean quantities in numerical schemes for the interaction between the forest and the atmosphere.

Objectives

Our main goals are:

  • To obtain a more realistic characterization of atmospheric turbulence regimes as a function of parameters that are external to the planetary boundary layer, such as large-scale winds, radiative processes and surface properties, both for daytime and nighttime conditions at the ATTO site
  • To compare the results found with those obtained at other sites, with different surface cover, to find universal controls
  • To identify how the turbulence regimes the scalar mean concentration and fluxes of the different scalars sampled at the ATTO towerTo establish similarity relationships based on parameters that are external to the planetary boundary layer, based on the analysis described in the previous points
  • To implement the results in numerical schemes that represent the interaction between the surface and the atmosphere
  • To form human resources through participation in graduate and undergraduate programs

Team

  • Luis Gustavo Nogueira Martins, Universidade Federal de Santa Maria, Santa Maria, RS, Brazil;
  • Claudio Teichrieb, Universidade Federal de Santa Maria, Santa Maria, RS, Brazil;
  • Mauricio Ilha de Oliveira, Universidade Federal de Santa Maria, Santa Maria, RS, Brazil;
  • Stefan Wolff, Max Planck Institute for Chemistry, Mainz, Germany;
  • Hartwig Harder, Max Planck Institute for Chemistry, Mainz, Germany;
  • Christopher Pohlker, Max Planck Institute for Chemistry, Mainz, Germany;
  • Cléo Quaresma Dias Jr., Instituto Federal do Pará, Belém, PA, Brazil;
  • Luca Mortarini, Consiglio Nazionale delle Ricerche, Turin, Italy;
  • Daiane Brondani, Università degli Studi di Urbino, Urbino, Italy
  • Antonio Ocimar Manzi, Instituto Nacional de Pesquisas Espaciais, São José dos Campos, SP,  Brazil;
  • Felipe Denardin Costa, Universidade Federal do Pampa, Alegrete, RS, Brazil;
  • Rafael Maroneze, Universidade Federal do Pampa, Alegrete, RS, Brazil;Franciano Puhales, Universidade Federal de Santa Maria, Santa Maria, RS, Brazil;
  • Anne Mendonça, Instituto Nacional de Pesquisas da Amazônia, Manaus, AM, Brazil