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Katia Lamer
,
Edward P. Luke
,
Brian Walsh Jr.
,
Steven Andrade
,
Zackary Mages
,
Zeen Zhu
,
Erin Leghart
,
Bernat P. Treserras
,
Ann Emrick
,
Pavlos Kollias
,
Andrew Vogelmann
, and
Martin Schoonen

Abstract

The Brookhaven National Laboratory Center for Multiscale Applied Sensing (CMAS) aims to address environmental equity needs in the context of a changing climate. As a first step toward this goal, the center developed a one-of-a-kind observatory tailored to the study of highly heterogeneous urban environments. This article describes the features of the mobile observatory that enable its rapid deployment either on or off the power grid, as well as its instrument payload. Beyond its unique design, the observatory optimizes data collection within the obstacle-laden urban environment using a new smart sampling paradigm. This setup facilitated the collection of previously poorly documented environmental properties, including wind profiles throughout the atmospheric column. The mobile observatory captured unique observations during its first few intensive observation periods. Vertical air motion and infrared temperature measurements collected along the faces of the supertall One Vanderbilt skyscraper in Manhattan, NY, reveal how solar and anthropogenic heating affect wind flow and thus the venting of heat, pollution, and contaminants in urban street canyons. Also, air temperature measurements collected during travel along a 150-km transect between Upton and Manhattan, NY, offer a high-resolution view of the urban heat island and reveal that temperature disparities also exist within the city across different neighborhoods. Ultimately, the datasets collected by CMAS are poised to help guide equitable urban planning by highlighting existing disparities and characterizing the impact of urban features on the urban microclimate with the goal of improving human comfort.

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Pavlos Kollias
,
Mark A. Miller
,
Edward P. Luke
,
Karen L. Johnson
,
Eugene E. Clothiaux
,
Kenneth P. Moran
,
Kevin B. Widener
, and
Bruce A. Albrecht

Abstract

The U.S. Department of Energy Atmospheric Radiation Measurement (ARM) Program operates millimeter-wavelength cloud radars in several climatologically distinct regions. The digital signal processors for these radars were recently upgraded and allow for enhancements in the operational parameters running on them. Recent evaluations of millimeter-wavelength cloud radar signal processing performance relative to the range of cloud dynamical and microphysical conditions encountered at the ARM Program sites have indicated that improvements are necessary, including significant improvement in temporal resolution (i.e., less than 1 s for dwell and 2 s for dwell and processing), wider Nyquist velocities, operational dealiasing of the recorded spectra, removal of pulse compression while sampling the boundary layer, and continuous recording of Doppler spectra. A new set of millimeter-wavelength cloud radar operational modes that incorporate these enhancements is presented. A significant change in radar sampling is the introduction of an uneven mode sequence with 50% of the sampling time dedicated to the lower atmosphere, allowing for detailed characterization of boundary layer clouds. The changes in the operational modes have a substantial impact on the postprocessing algorithms that are used to extract cloud information from the radar data. New methods for postprocessing of recorded Doppler spectra are presented that result in more accurate identification of radar clutter (e.g., insects) and extraction of turbulence and microphysical information. Results of recent studies on the error characteristics of derived Doppler moments are included so that uncertainty estimates are now included with the moments. The microscale data product based on the increased temporal resolution of the millimeter-wavelength cloud radars is described. It contains the number of local maxima in each Doppler spectrum, the Doppler moments of the primary peak, uncertainty estimates for the Doppler moments of the primary peak, Doppler moment shape parameters (e.g., skewness and kurtosis), and clear-air clutter flags.

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Pavlos Kollias
,
Eugene E. Clothiaux
,
Thomas P. Ackerman
,
Bruce A. Albrecht
,
Kevin B. Widener
,
Ken P. Moran
,
Edward P. Luke
,
Karen L. Johnson
,
Nitin Bharadwaj
,
James B. Mead
,
Mark A. Miller
,
Johannes Verlinde
,
Roger T. Marchand
, and
Gerald G. Mace
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A Focus On Mixed-Phase Clouds

The Status of Ground-Based Observational Methods

Matthew D. Shupe
,
John S. Daniel
,
Gijs de Boer
,
Edwin W. Eloranta
,
Pavlos Kollias
,
Charles N. Long
,
Edward P. Luke
,
David D. Turner
, and
Johannes Verlinde

The phase composition and microphysical structure of clouds define the manner in which they modulate atmospheric radiation and contribute to the hydrologic cycle. Issues regarding cloud phase partitioning and transformation come to bear directly in mixed-phase clouds, and have been difficult to address within current modeling frameworks. Ground-based, remote-sensing observations of mixed-phase clouds can contribute a significant body of knowledge with which to better understand, and thereby more accurately model, clouds and their phase-defining processes. Utilizing example observations from the Mixed-Phase Arctic Cloud Experiment (M-PACE), which occurred at the Department of Energy (DOE) Atmospheric Radiation Measurement (ARM) Program's Climate Research Facility in Barrow, Alaska, during autumn 2004, we review the current status of ground-based observation and retrieval methods used in characterizing the macrophysical, microphysical, radiative, and dynamical properties of stratiform mixed-phase clouds. In general, cloud phase, boundaries, ice properties, liquid water path, optical depth, and vertical velocity are available from a combination of active and passive sensors. Significant deficiencies exist in our ability to vertically characterize the liquid phase, to distinguish ice crystal habits, and to understand aerosol-cloud interactions. Further validation studies are needed to evaluate, improve, and expand our retrieval abilities in mixed-phase clouds.

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Michael P. Jensen
,
James H. Flynn
,
Laura M. Judd
,
Pavlos Kollias
,
Chongai Kuang
,
Greg Mcfarquhar
,
Raj Nadkarni
,
Heath Powers
, and
John Sullivan
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Virendra P. Ghate
,
Pavlos Kollias
,
Susanne Crewell
,
Ann M. Fridlind
,
Thijs Heus
,
Ulrich Löehnert
,
Maximilian Maahn
,
Greg M. McFarquhar
,
Dmitri Moisseev
,
Mariko Oue
,
Manfred Wendisch
, and
Christopher Williams
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J. Rémillard
,
A. M. Fridlind
,
A. S. Ackerman
,
G. Tselioudis
,
P. Kollias
,
D. B. Mechem
,
H. E. Chandler
,
E. Luke
,
R. Wood
,
M. K. Witte
,
P. Y. Chuang
, and
J. K. Ayers

Abstract

A case study of persistent stratocumulus over the Azores is simulated using two independent large-eddy simulation (LES) models with bin microphysics, and forward-simulated cloud radar Doppler moments and spectra are compared with observations. Neither model is able to reproduce the monotonic increase of downward mean Doppler velocity with increasing reflectivity that is observed under a variety of conditions, but for differing reasons. To a varying degree, both models also exhibit a tendency to produce too many of the largest droplets, leading to excessive skewness in Doppler velocity distributions, especially below cloud base. Excessive skewness appears to be associated with an insufficiently sharp reduction in droplet number concentration at diameters larger than ~200 μm, where a pronounced shoulder is found for in situ observations and a sharp reduction in reflectivity size distribution is associated with relatively narrow observed Doppler spectra. Effectively using LES with bin microphysics to study drizzle formation and evolution in cloud Doppler radar data evidently requires reducing numerical diffusivity in the treatment of the stochastic collection equation; if that is accomplished sufficiently to reproduce typical spectra, progress toward understanding drizzle processes is likely.

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P. Kollias
,
N. Bharadwaj
,
E. E. Clothiaux
,
K. Lamer
,
M. Oue
,
J. Hardin
,
B. Isom
,
I. Lindenmaier
,
A. Matthews
,
E. P. Luke
,
S. E. Giangrande
,
K. Johnson
,
S. Collis
,
J. Comstock
, and
J. H. Mather
Full access
P. Kollias
,
N. Bharadwaj
,
E. E. Clothiaux
,
K. Lamer
,
M. Oue
,
J. Hardin
,
B. Isom
,
I. Lindenmaier
,
A. Matthews
,
E. P. Luke
,
S. E. Giangrande
,
K. Johnson
,
S. Collis
,
J. Comstock
, and
J. H. Mather

Abstract

Improving our ability to predict future weather and climate conditions is strongly linked to achieving significant advancements in our understanding of cloud and precipitation processes. Observations are critical to making these advancements because they both improve our understanding of these processes and provide constraints on numerical models. Historically, instruments for observing cloud properties have limited cloud–aerosol investigations to a small subset of cloud-process interactions. To address these challenges, the last decade has seen the U.S. DOE ARM facility significantly upgrade and expand its surveillance radar capabilities toward providing holistic and multiscale observations of clouds and precipitation. These upgrades include radars that operate at four frequency bands covering a wide range of scattering regimes, improving upon the information contained in earlier ARM observations. The traditional ARM emphasis on the vertical column is maintained, providing more comprehensive, calibrated, and multiparametric measurements of clouds and precipitation. In addition, the ARM radar network now features multiple scanning dual-polarization Doppler radars to exploit polarimetric and multi-Doppler capabilities that provide a wealth of information on storm microphysics and dynamics under a wide range of conditions. Although the diversity in wavelengths and detection capabilities are unprecedented, there is still considerable work ahead before the full potential of these radar advancements is realized. This includes synergy with other observations, improved forward and inverse modeling methods, and well-designed data–model integration methods. The overarching goal is to provide a comprehensive characterization of a complete volume of the cloudy atmosphere and to act as a natural laboratory for the study of cloud processes.

Free access
Holger Siebert
,
Kai-Erik Szodry
,
Ulrike Egerer
,
Birgit Wehner
,
Silvia Henning
,
Karine Chevalier
,
Janine Lückerath
,
Oliver Welz
,
Kay Weinhold
,
Felix Lauermann
,
Matthias Gottschalk
,
André Ehrlich
,
Manfred Wendisch
,
Paulo Fialho
,
Greg Roberts
,
Nithin Allwayin
,
Simeon Schum
,
Raymond A. Shaw
,
Claudio Mazzoleni
,
Lynn Mazzoleni
,
Jakub L. Nowak
,
Szymon P. Malinowski
,
Katarzyna Karpinska
,
Wojciech Kumala
,
Dominika Czyzewska
,
Edward P. Luke
,
Pavlos Kollias
,
Robert Wood
, and
Juan Pedro Mellado

Abstract

We report on the Azores Stratocumulus Measurements of Radiation, Turbulence and Aerosols (ACORES) campaign, which took place around Graciosa and Pico Islands/Azores in July 2017. The main objective was to investigate the vertical distribution of aerosol particles, stratocumulus microphysical and radiative properties, and turbulence parameters in the eastern North Atlantic. The vertical exchange of mass, momentum, and energy between the free troposphere (FT) and the cloudy marine boundary layer (MBL) was explored over a range of scales from submeters to kilometers. To cover these spatial scales with appropriate measurements, helicopter-borne observations with unprecedented high resolution were realized using the Airborne Cloud Turbulence Observation System (ACTOS) and Spectral Modular Airborne Radiation Measurement System–Helicopter-Borne Observations (SMART-HELIOS) instrumental payloads. The helicopter-borne observations were combined with ground-based aerosol measurements collected at two continuously running field stations on Pico Mountain (2,225 m above sea level, in the FT), and at the Atmospheric Radiation Measurement (ARM) station on Graciosa (at sea level). First findings from the ACORES observations we are discussing in the paper are as follows: (i) we have observed a high variability of the turbulent cloud-top structure on horizontal scales below 100 m with local temperature gradients of up to 4 K over less than 1 m vertical distance, (ii) we have collected strictly collocated radiation measurements supporting the relevance of small-scale processes by revealing significant inhomogeneities in cloud-top brightness temperature to scales well below 100 m, and (iii) we have concluded that aerosol properties are completely different in the MBL and FT with often-complex stratification and frequently observed burst-like new particle formation.

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