54 research outputs found
Exploration of a Polarized Surface Bidirectional Reflectance Model Using the Ground-Based Multiangle Spectropolarimetric Imager
Accurate characterization of surface reflection is essential for retrieval of aerosols using downward-looking remote sensors. In this paper, observations from the Ground-based Multiangle SpectroPolarimetric Imager (GroundMSPI) are used to evaluate a surface polarized bidirectional reflectance distribution function (PBRDF) model. GroundMSPI is an eight-band spectropolarimetric camera mounted on a rotating gimbal to acquire pushbroom imagery of outdoor landscapes. The camera uses a very accurate photoelastic-modulator-based polarimetric imaging technique to acquire Stokes vector measurements in three of the instrument's bands (470, 660, and 865 nm). A description of the instrument is presented, and observations of selected targets within a scene acquired on 6 January 2010 are analyzed. Data collected during the course of the day as the Sun moved across the sky provided a range of illumination geometries that facilitated evaluation of the surface model, which is comprised of a volumetric reflection term represented by the modified Rahman-Pinty-Verstraete function plus a specular reflection term generated by a randomly oriented array of Fresnel-reflecting microfacets. While the model is fairly successful in predicting the polarized reflection from two grass targets in the scene, it does a poorer job for two manmade targets (a parking lot and a truck roof), possibly due to their greater degree of geometric organization. Several empirical adjustments to the model are explored and lead to improved fits to the data. For all targets, the data support the notion of spectral invariance in the angular shape of the unpolarized and polarized surface reflection. As noted by others, this behavior provides valuable constraints on the aerosol retrieval problem, and highlights the importance of multiangle observations.NASAJPLCenter for Space Researc
Scientific Objectives, Measurement Needs, and Challenges Motivating the PARAGON Aerosol Initiative
Aerosols are involved in a complex set of processes that operate across many spatial and temporal scales. Understanding these processes, and ensuring their accurate representation in models of transport, radiation transfer, and climate, requires knowledge of aerosol physical, chemical, and optical properties and the distributions of these properties in space and time. To derive aerosol climate forcing, aerosol optical and microphysical properties and their spatial and temporal distributions, and aerosol interactions with clouds, need to be understood. Such data are also required in conjunction with size-resolved chemical composition in order to evaluate chemical transport models and to distinguish natural and anthropogenic forcing. Other basic parameters needed for modeling the radiative influences of aerosols are surface reflectivity and three-dimensional cloud fields. This large suite of parameters mandates an integrated observing and modeling system of commensurate scope. The Progressive Aerosol Retrieval and Assimilation Global Observing Network (PARAGON) concept, designed to meet this requirement, is motivated by the need to understand climate system sensitivity to changes in atmospheric constituents, to reduce climate model uncertainties, and to analyze diverse collections of data pertaining to aerosols. This paper highlights several challenges resulting from the complexity of the problem. Approaches for dealing with them are offered in the set of companion papers
Identification of Functional Toxin/Immunity Genes Linked to Contact-Dependent Growth Inhibition (CDI) and Rearrangement Hotspot (Rhs) Systems
Bacterial contact-dependent growth inhibition (CDI) is mediated by the CdiA/CdiB family of two-partner secretion proteins. Each CdiA protein exhibits a distinct growth inhibition activity, which resides in the polymorphic C-terminal region (CdiA-CT). CDI+ cells also express unique CdiI immunity proteins that specifically block the activity of cognate CdiA-CT, thereby protecting the cell from autoinhibition. Here we show that many CDI systems contain multiple cdiA gene fragments that encode CdiA-CT sequences. These “orphan” cdiA-CT genes are almost always associated with downstream cdiI genes to form cdiA-CT/cdiI modules. Comparative genome analyses suggest that cdiA-CT/cdiI modules are mobile and exchanged between the CDI systems of different bacteria. In many instances, orphan cdiA-CT/cdiI modules are fused to full-length cdiA genes in other bacterial species. Examination of cdiA-CT/cdiI modules from Escherichia coli EC93, E. coli EC869, and Dickeya dadantii 3937 confirmed that these genes encode functional toxin/immunity pairs. Moreover, the orphan module from EC93 was functional in cell-mediated CDI when fused to the N-terminal portion of the EC93 CdiA protein. Bioinformatic analyses revealed that the genetic organization of CDI systems shares features with rhs (rearrangement hotspot) loci. Rhs proteins also contain polymorphic C-terminal regions (Rhs-CTs), some of which share significant sequence identity with CdiA-CTs. All rhs genes are followed by small ORFs representing possible rhsI immunity genes, and several Rhs systems encode orphan rhs-CT/rhsI modules. Analysis of rhs-CT/rhsI modules from D. dadantii 3937 demonstrated that Rhs-CTs have growth inhibitory activity, which is specifically blocked by cognate RhsI immunity proteins. Together, these results suggest that Rhs plays a role in intercellular competition and that orphan gene modules expand the diversity of toxic activities deployed by both CDI and Rhs systems
An Integrated Approach for Characterizing Aerosol Climate Impacts and Environmental Interactions
Aerosols exert myriad influences on the earth's environment and climate, and on human health. The complexity of aerosol-related processes requires that information gathered to improve our understanding of climate change must originate from multiple sources, and that effective strategies for data integration need to be established. While a vast array of observed and modeled data are becoming available, the aerosol research community currently lacks the necessary tools and infrastructure to reap maximum scientific benefit from these data. Spatial and temporal sampling differences among a diverse set of sensors, nonuniform data qualities, aerosol mesoscale variabilities, and difficulties in separating cloud effects are some of the challenges that need to be addressed. Maximizing the long-term benefit from these data also requires maintaining consistently well-understood accuracies as measurement approaches evolve and improve. Achieving a comprehensive understanding of how aerosol physical, chemical, and radiative processes impact the earth system can be achieved only through a multidisciplinary, inter-agency, and international initiative capable of dealing with these issues. A systematic approach, capitalizing on modern measurement and modeling techniques, geospatial statistics methodologies, and high-performance information technologies, can provide the necessary machinery to support this objective. We outline a framework for integrating and interpreting observations and models, and establishing an accurate, consistent, and cohesive long-term record, following a strategy whereby information and tools of progressively greater sophistication are incorporated as problems of increasing complexity are tackled. This concept is named the Progressive Aerosol Retrieval and Assimilation Global Observing Network (PARAGON). To encompass the breadth of the effort required, we present a set of recommendations dealing with data interoperability; measurement and model integration; multisensor synergy; data summarization and mining; model evaluation; calibration and validation; augmentation of surface and in situ measurements; advances in passive and active remote sensing; and design of satellite missions. Without an initiative of this nature, the scientific and policy communities will continue to struggle with understanding the quantitative impact of complex aerosol processes on regional and global climate change and air quality
MITS: the Multi-Imaging Transient Spectrograph for SOXS
The Son Of X-Shooter (SOXS) is a medium resolution spectrograph R~4500
proposed for the ESO 3.6 m NTT. We present the optical design of the UV-VIS arm
of SOXS which employs high efficiency ion-etched gratings used in first order
(m=1) as the main dispersers. The spectral band is split into four channels
which are directed to individual gratings, and imaged simultaneously by a
single three-element catadioptric camera. The expected throughput of our design
is >60% including contingency. The SOXS collaboration expects first light in
early 2021. This paper is one of several papers presented in these proceedings
describing the full SOXS instrument
Optical design of the SOXS spectrograph for ESO NTT
An overview of the optical design for the SOXS spectrograph is presented.
SOXS (Son Of X-Shooter) is the new wideband, medium resolution (R>4500)
spectrograph for the ESO 3.58m NTT telescope expected to start observations in
2021 at La Silla. The spectroscopic capabilities of SOXS are assured by two
different arms. The UV-VIS (350-850 nm) arm is based on a novel concept that
adopts the use of 4 ion-etched high efficiency transmission gratings. The NIR
(800- 2000 nm) arm adopts the '4C' design (Collimator Correction of Camera
Chromatism) successfully applied in X-Shooter. Other optical sub-systems are
the imaging Acquisition Camera, the Calibration Unit and a pre-slit Common
Path. We describe the optical design of the five sub-systems and report their
performance in terms of spectral format, throughput and optical quality. This
work is part of a series of contributions describing the SOXS design and
properties as it is about to face the Final Design Review.Comment: 9 pages, 9 figures, published in SPIE Proceedings 1070
The VIS detector system of SOXS
SOXS will be a unique spectroscopic facility for the ESO NTT telescope able
to cover the optical and NIR bands thanks to two different arms: the UV-VIS
(350-850 nm), and the NIR (800-1800 nm). In this article, we describe the
design of the visible camera cryostat and the architecture of the acquisition
system. The UV-VIS detector system is based on a e2v CCD 44-82, a custom
detector head coupled with the ESO continuous ow cryostats (CFC) cooling system
and the NGC CCD controller developed by ESO. This paper outlines the status of
the system and describes the design of the different parts that made up the
UV-VIS arm and is accompanied by a series of contributions describing the SOXS
design solutions.Comment: 9 pages, 13 figures, to be published in SPIE Proceedings 1070
The Acquisition Camera System for SOXS at NTT
SOXS (Son of X-Shooter) will be the new medium resolution (R4500 for a
1 arcsec slit), high-efficiency, wide band spectrograph for the ESO-NTT
telescope on La Silla. It will be able to cover simultaneously optical and NIR
bands (350-2000nm) using two different arms and a pre-slit Common Path feeding
system. SOXS will provide an unique facility to follow up any kind of transient
event with the best possible response time in addition to high efficiency and
availability. Furthermore, a Calibration Unit and an Acquisition Camera System
with all the necessary relay optics will be connected to the Common Path
sub-system. The Acquisition Camera, working in optical regime, will be
primarily focused on target acquisition and secondary guiding, but will also
provide an imaging mode for scientific photometry. In this work we give an
overview of the Acquisition Camera System for SOXS with all the different
functionalities. The optical and mechanical design of the system are also
presented together with the preliminary performances in terms of optical
quality, throughput, magnitude limits and photometric properties.Comment: 9 pages, 7 figures, SPIE conferenc
Architecture of the SOXS instrument control software
SOXS (Son Of X-Shooter) is a new spectrograph for the ESO NTT telescope,
currently in the final design phase.
The main instrument goal is to allow the characterization of transient
sources based on alerts. It will cover from near-infrared to visible bands with
a spectral resolution of using two separate, wavelength-optimized
spectrographs. A visible camera, primarily intended for target acquisition and
secondary guiding, will also provide a scientific "light" imaging mode.
In this paper we present the current status of the design of the SOXS
instrument control software, which is in charge of controlling all instrument
functions and detectors, coordinating the execution of exposures, and
implementing all observation, calibration and maintenance procedures.
Given the extensive experience of the SOXS consortium in the development of
instruments for the VLT, we decided to base the design of the Control System on
the same standards, both for hardware and software control.
We illustrate the control network, the instrument functions and detectors to
be controlled, the overall design of SOXS Instrument Software (INS) and its
main components. Then, we provide details about the control software for the
most SOXS-specific features: control of the COTS-based imaging camera, the
flexures compensation system and secondary guiding.Comment: 8 pages, 5 figure
SOXS Control Electronics Design
SOXS (Son Of X-Shooter) is a unique spectroscopic facility that will operate
at the ESO New Technology Telescope (NTT) in La Silla from 2020 onward. The
spectrograph will be able to cover simultaneously the UV-VIS and NIR bands
exploiting two different arms and a Common Path feeding system. We present the
design of the SOXS instrument control electronics. The electronics controls all
the movements, alarms, cabinet temperatures, and electric interlocks of the
instrument. We describe the main design concept. We decided to follow the ESO
electronic design guidelines to minimize project time and risks and to simplify
system maintenance. The design envisages Commercial Off-The-Shelf (COTS)
industrial components (e.g. Beckhoff PLC and EtherCAT fieldbus modules) to
obtain a modular design and to increase the overall reliability and
maintainability. Preassembled industrial motorized stages are adopted allowing
for high precision assembly standards and a high reliability. The electronics
is kept off-board whenever possible to reduce thermal issues and instrument
weight and to increase the accessibility for maintenance purpose. The
instrument project went through the Preliminary Design Review in 2017 and is
currently in Final Design Phase (with FDR in July 2018). This paper outlines
the status of the work and is part of a series of contributions describing the
SOXS design and properties after the instrument Preliminary Design Review.Comment: 10 pages, 7 figures, to be publised in SPIE Proceedings 10707-9
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