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Roll vortices in the planetary boundary layer: A review

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TLDR
Roll vortices may be loosely defined as quasi-two-dimensional organized large eddies with their horizontal axis extending through the whole planetary boundary layer (PBL), and their indirect manifestation is most obvious in so-called cloud streets as can be seen in numerous satellite pictures as mentioned in this paper.
Abstract
Roll vortices may be loosely defined as quasi two-dimensional organized large eddies with their horizontal axis extending through the whole planetary boundary layer (PBL). Their indirect manifestation is most obvious in so-called cloud streets as can be seen in numerous satellite pictures. Although this phenomenon has been known for more than twenty years and has been treated in a review by one of us (R.A.Brown) in 1980, there has been a recent resurgence in interest and information. The interest in ocena/land-atmosphere interactions in the context of climate modeling has led to detailed observational and modeling efforts on this problem. The presence of rolls can have a large impact on flux modelling in the PBL. Hence, we shall review recent advances in our understanding of organized large eddies in the PBL and on their role in vertical transport of momentum, heat, moisture and chemical trace substances within the lowest part of the atmosphere.

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Citations
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Numerical Simulation of the Quasi-Stationary Snowband Observed over the Southern Coastal Area of the Sea of Japan on 16 January 2001

TL;DR: In this article, a meso-β-scale convective snow band was observed in the coastal area of eastern Hokuriku district, middle part of Japan, and numerical simulations of this snowband were performed using a nonhydrostatic cloud resolving model (NHM), with a horizontal grid size of 1 km.
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A Dual-Doppler Radar Study of Longitudinal-Mode Snowbands. Part I: A Three-Dimensional Kinematic Structure of Meso-γ-Scale Convective Cloud Systems within a Longitudinal-Mode Snowband

TL;DR: In this article, the three-dimensional kinematic structures and organization processes of meso-γ-scale (∼20 km) convective cloud systems were studied in detail.
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Remote Measurement of Turbulent Wind Spectra by Heterodyne DopplerLidar Technique

TL;DR: In this paper, both spatial averaging and error contribution to the wind spectra can be modeled starting from the transmitted laser pulse characteristics and signal processing parameters, so that their effect can be predicted.
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Roll Circulations in the Convective Region of a Simulated Squall Line

TL;DR: In this article, the authors show that the convective region of squall lines will sometimes overturn as quasi-horizontal convective rolls, where individual convective cells often have long-lived, undiluted cores that entrain primarily on the sides of the rolls.
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On the influence of sea‐ice inhomogeneities onto roll convection in cold‐air outbreaks

TL;DR: In this article, the authors used large-eddy simulations (LES) to model roll convection within the convective atmospheric boundary layer (CBL) during strong cold-air outbreaks (CAO).
References
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Coherent Motions in the Turbulent Boundary Layer

TL;DR: In this paper, the role of coherent structures in the production and dissipation of turbulence in a boundary layer is characterized, summarizing the results of recent investigations, and diagrams and graphs are provided.
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Perturbed Free Shear Layers

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A Large-Eddy-Simulation Model for the Study of Planetary Boundary-Layer Turbulence

TL;DR: In this paper, a new large-eddy-simulation (LES) model code which uses a mixed pseudospectral finite-difference method was developed and tested with a simple vortex flow and with the Wangara day-33 data.
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A simple model of the atmospheric boundary layer; sensitivity to surface evaporation

TL;DR: In this paper, a simple formulation of the boundary layer is developed for use in large-scale models and other situations where simplicity is required, where some resolution is possible within the boundary layers, but where the resolution is insufficient for resolving the detailed boundary-layer structure and overlying capping inversion.
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Numerical Investigation of Neutral and Unstable Planetary Boundary Layers

TL;DR: In this article, numerical integrations are presented for a neutrally stratified planetary boundary layer containing a passive scalar, and for three unstable cases with upward heat flux, assuming the air is assumed unsaturated.