This is a talk for the Hablemos de ALMA (Let's Speak about ALMA) internal outreach series where the first project of the ALMA 2030 Roadmap, the Wideband Sensitivity Upgrade (WSU) is described.
In this talk the expected science benefits are discussed first by John Carpenter; then complexities of Systems Engineering and why those processes will be needed are talked about by Juande Santander-Vela; and finally, the Project Management issues of this upgrade are considered by Carla Crovari.
This version of the talk took place on the ALMA Santiago Central Office (SCO) on August 19th, 2022.
Trabalho sobre terapia gênica feito por alunos da E.E. Paulo Freire de Canarana-MT, onde são apresentados os conceitos, características e afins da transgenia.
Em 1896, o francês Henri Becquerel descobriu a radioatividade, ele estudava os efeitos da luz solar sobre determinados materiais fluorescentes, como o minério de urânio. À espera da melhora do tempo, que se apresentava nublado, guardou a amostra do minério numa gaveta. Ao retirá-la, alguns dias mais tarde, Becquerel observou que a pedra havia emitido radiações mesmo no escuro e obteve a primeira prova da existência da radioatividade natural.
Radiação é a propagação espacial de energia através de partículas ou ondas. A radiação eletromagnética e uma forma de energia que se propaga com a combinação dos campos elétricos e magnéticos.
A radioatividade, por sua vez, é a propriedade de certos elementos químicos de altos peso atômicos (urânio, tório, rádio, césio etc...) de emitir espontaneamente energia e partículas subatômicas.
Trabalho sobre terapia gênica feito por alunos da E.E. Paulo Freire de Canarana-MT, onde são apresentados os conceitos, características e afins da transgenia.
Em 1896, o francês Henri Becquerel descobriu a radioatividade, ele estudava os efeitos da luz solar sobre determinados materiais fluorescentes, como o minério de urânio. À espera da melhora do tempo, que se apresentava nublado, guardou a amostra do minério numa gaveta. Ao retirá-la, alguns dias mais tarde, Becquerel observou que a pedra havia emitido radiações mesmo no escuro e obteve a primeira prova da existência da radioatividade natural.
Radiação é a propagação espacial de energia através de partículas ou ondas. A radiação eletromagnética e uma forma de energia que se propaga com a combinação dos campos elétricos e magnéticos.
A radioatividade, por sua vez, é a propriedade de certos elementos químicos de altos peso atômicos (urânio, tório, rádio, césio etc...) de emitir espontaneamente energia e partículas subatômicas.
Rate and Performance Analysis of Indoor Optical Camera Communications in Opti...Willy Anugrah Cahyadi
It is a summary of my dissertation for the Ph.D. degree. The main topic is optical camera communication (OCC), which was being standardized under the revision to IEEE 802.15.7-2011 standard in 2018.
Overview of Integrated Detector Electronics products including Application Specific Integrated Circuits, ROICs and low noise amplifiers for radiation detection.
Development of a High Performance Optical Cesium Beam Clock for Ground Applic...ADVA
At the VIII International “Metrology of Time and Space” Symposium in St. Petersburg, Patrick Berthoud revealed the latest results in the development of Oscilloquartz’s high-performance optical cesium beam clock.
Probing the atmosphere - new radar & lidar technologies for remote sensing of...CLIC Innovation Ltd
MMEA (The Measurement, Monitoring and Environmental Efficiency Assessment) research program final seminar presentation by Dr. Ari-Matti Harri, Finnish Meteorological Institute
This project seeks to design innovative tools to measure in vivo biomechanical parameters of joint prostheses, orthopaedic implants, bones and ligaments. These tools, partly implanted, partly external, will record and analyze relevant information in order to improve medical treatments. An implant module includes sensors in order to measure the forces, temperature sensors to measure the interface frictions, magneto-resistance sensors to measure the 3D orientation of the knee joint as well as accelerometers to measure stem micro-motion and impacts. An external module, fixed on the patient.s body segments, includes electronic components to power and to communicate with the implant, as well as a set of sensors for measurements that can be realized externally.
This equipment is designed to help the surgeon with the alignment or positioning phase during surgery. After surgery, by providing excessive wear and micro-motion information about the prosthesis, it will allow to detect any early migration and potentially avoid later failure. During rehabilitation, it will provide useful outcomes to evaluate in vivo joint function. The tools provided can also be implanted during any joint surgery in order to give the physician the information needed to diagnose future disease such as ligament insufficiency, osteoarthritis or prevent further accident. The proposed nanosystems are set to improve the efficiency of healthcare, which is both a benefit to the patient and to society. Although the scientific and technical developments proposed in this project can be applied to all orthopaedic implants, the technological platform which is being built as a demonstrator is limited to the case of knee prosthesis. In addition, by reaching the minimum size achievable thanks to clever packaging techniques and also by reducing, or even removing, the cumbersome battery, it paves the way for a new generation of autonomous implantable medical devices.
Similar to Hablemos de ALMA — Wideband Sensitivity Upgrade (20)
The Square Kilometre Array telescopes have recently started their construction phase, after years of pre-construction effort. The new SKA Observatory (SKAO) intergovernmental organisation has been created, and the start of construction (T0) has already happened. In this talk we summarise the construction progress in our facility, and the role that software development, and in particular the development of our TANGO-based control system, is playing.
The Square Kilometre Array (SKA), even in its first phase (SKA Phase 1, or SKA1) will be the largest ground-based astronomical facility ever built, with unprecedented sensitivity in the frequency ranges for local to highly redshifted HI, and future expansion up to 25 GHz. The range of science cases that the SKA telescopes will cater for will also be the largest of any research facility, from the Epoch of Reionization (EoR) and the Cosmic Down (CD), to tests of Einstein’s General Relativity, to finding all detectable pulsars in the Milky Way, and helping with the Cradle of Life case for Astrobiology. In this talk we will go through the different science cases, with emphasis in those with the most cosmological significance, such as EoR, CD, and probing General Relativity. (Talk presented at CosmoAndes 2018.)
The Square Kilometre Array Organisation (SKAO) is in the process to start construction of what will be the largest research facility in the world, with two radio interferometers generating each one petabyte of data per day, which will be distributed by a network of SKA Regional Centres (SRCs). Construction is expected to start after the establishment of the SKA Observatory Inter-Governmental Organisation by mid 2021, and last for around 6 years after that. However, we are already prototyping the software development processes that will help us align the work of around 150 full-time equivalent people around the world. In this talk we will show what are the current agile software development processes at SKAO, how we are already leveraging the Scaled Agile Framework (SAFe®) to provide alignment across the world-wide community of developers and other contributors, and how we will be managing the full software lifecycle of it during construction and beyond.
Systems Engineering (SE) is the set of processes and documentation required for successfully realising large-scale engineering projects, but the classical approach is not a good fit for software-intensive projects, especially when the needs of the different stakeholders are not fully known from the beginning, and requirement priorities might change. The SKA is the ultimate software-enabled telescope, with enormous amounts of computing hardware and software required to perform its data reduction. We give an overview of the system and software engineering processes in the SKA1 development, and the tension between classical and agile SE.
This set of slides introduce the TANGO control system for the SKA telescopes, using analogies between tango dancing and the paradigms of the TANGO control system.
The talk was given in the context of the Engineering Q&A talks of the SKA Organisation.
Talk given as part of the Bluedot Festival. Tries to emphasise the current trends in Citizen Science, how are they powered by the same ICT innovation that powers other industries, and how curation and metadata are key both for professional and citizen scientist, and facilities to perform that will be needed.
The Square Kilometre Array is currently undergoing the Preliminary Design Reviews for its composing elements, and is thus at a critical point on its way to becoming ready for construction starting in 2018. In this talk we will provide an overview of the SKA, its composing elements, and their status, with emphasis on the Telescope Manager and the Science Data Processor, respectively the Monitoring & Control system, and Pipeline. We will see how do they compare with their ALMA equivalents, and how is the SKA similar/different from ALMA.
In a project of the complexity of the SKA, it is very important to be very observant of the different requirements for the SKA telescopes, and how they are implemented by the different sub-systems. And because the design of the SKA is evolving, the need to assess the impact of design changes, and potential trade-offs, is more relevant than ever. In this talk I will present how the SKA Organisation is leading the Systems Engineering work of the different consortia, and how we are using Model Based Systems Engineering (MBSE) to integrate the design inputs from the sub-systems, and be able to keep a Systems view that ensures that the element designs are sound, and really comply with the stringent requirements posed by the SKA.
Building a National Virtual Observatory: The Case of the Spanish Virtual Obse...Joint ALMA Observatory
Talk at the presentation workshop for the Chilean Virtual Observatory (ChiVO; http://www.chivo.cl/workshop-program), on lessons that can be learned from the development of the Spanish Virtual Observatory, and how ChiVO has already applied most of them.
Wf4Ever: Scientific Workflows and Research Objects as tools for scientific in...Joint ALMA Observatory
Astronomers are being drowned in data: facilities like ALMA currently provide datasets in the Gigabyte range, and increasing, while facilities like the LSST and the SKA will generate datasets large enough so that data download, even of the reduced datasets, will not be feasible. In this talk we will introduce the concept of Scientific Workflows, as software tools that allow for the easy exploration of both local and remote datasets and processing services, and of Research Objects, which encapsulate all relevant aspects of a scientific experiment, and allow for its quantitative and qualitative assessment, enable reuse with proper attribution, and linkage to publications, among others. The AstroTaverna plugin, with astronomy-specific for workflow creation, was also presented in this ALMA Weekly Seminar.
How e-Science tools are needed for the new data intensive science, specifically targeted to the Square Kilometre Array. Talk given at the Special Symposium 15 on Data Intensive Astronomy, held during the General Assembly Meeting of the International Astronomical Union in Bejing, 2012.
Introduction to the problem of spatial indexing for spherical coordinate systems, as those used in astronomy. Part of the virtual observatory course by Juan de Dios Santander Vela, as imparted for the MTAF (Métodos y Técnicas Avanzadas en Física, Advanced Methods and Techniques in Physics) Master at the University of Granada (UGR).
How future astronomy projects will generate enormous amounts of data, and what does that mean for astronomical data processing. Part of the virtual observatory course by Juan de Dios Santander Vela, as imparted for the MTAF (Métodos y Técnicas Avanzadas en Física, Advanced Methods and Techniques in Physics) Master at the University of Granada (UGR).
Introducción a los sistemas gestores de bases de datos: orígenes y clases. Parte del curso de Observatorio Virtual impartido por Juan de Dios Santander Vela, dentro del máster MTAF (Métodos y Técnicas Avanzadas en Física) de la Universidad de Granada (UGR).
Role of data models in the Virtual Observatory, and overview of IVOA data models. Part of the virtual observatory course by Juan de Dios Santander Vela, as imparted for the MTAF (Métodos y Técnicas Avanzadas en Física, Advanced Methods and Techniques in Physics) Master at the University of Granada (UGR).
Description of the VOTable data format, VO semantic tools (UCDs, UTypes), and VO protocols. Part of the virtual observatory course by Juan de Dios Santander Vela, as imparted for the MTAF (Métodos y Técnicas Avanzadas en Física, Advanced Methods and Techniques in Physics) Master at the University of Granada (UGR).
Description of the Virtual Observatory architecture, and IVOA documents that make it explicit. Part of the virtual observatory course by Juan de Dios Santander Vela, as imparted for the MTAF (Métodos y Técnicas Avanzadas en Física, Advanced Methods and Techniques in Physics) Master at the University of Granada (UGR).
Description of the elements and purpose of the IVOA, the International Virtual Observatory Alliance. Part of the virtual observatory course by Juan de Dios Santander Vela, as imparted for the MTAF (Métodos y Técnicas Avanzadas en Física, Advanced Methods and Techniques in Physics) Master at the University of Granada (UGR).
Overview of the virtual observatory course by Juan de Dios Santander Vela, and part of the MTAF (Métodos y Técnicas Avanzadas en Física, Advanced Methods and Techniques in Physics) Master at the University of Granada (UGR).
The use of Nauplii and metanauplii artemia in aquaculture (brine shrimp).pptxMAGOTI ERNEST
Although Artemia has been known to man for centuries, its use as a food for the culture of larval organisms apparently began only in the 1930s, when several investigators found that it made an excellent food for newly hatched fish larvae (Litvinenko et al., 2023). As aquaculture developed in the 1960s and ‘70s, the use of Artemia also became more widespread, due both to its convenience and to its nutritional value for larval organisms (Arenas-Pardo et al., 2024). The fact that Artemia dormant cysts can be stored for long periods in cans, and then used as an off-the-shelf food requiring only 24 h of incubation makes them the most convenient, least labor-intensive, live food available for aquaculture (Sorgeloos & Roubach, 2021). The nutritional value of Artemia, especially for marine organisms, is not constant, but varies both geographically and temporally. During the last decade, however, both the causes of Artemia nutritional variability and methods to improve poorquality Artemia have been identified (Loufi et al., 2024).
Brine shrimp (Artemia spp.) are used in marine aquaculture worldwide. Annually, more than 2,000 metric tons of dry cysts are used for cultivation of fish, crustacean, and shellfish larva. Brine shrimp are important to aquaculture because newly hatched brine shrimp nauplii (larvae) provide a food source for many fish fry (Mozanzadeh et al., 2021). Culture and harvesting of brine shrimp eggs represents another aspect of the aquaculture industry. Nauplii and metanauplii of Artemia, commonly known as brine shrimp, play a crucial role in aquaculture due to their nutritional value and suitability as live feed for many aquatic species, particularly in larval stages (Sorgeloos & Roubach, 2021).
The ability to recreate computational results with minimal effort and actionable metrics provides a solid foundation for scientific research and software development. When people can replicate an analysis at the touch of a button using open-source software, open data, and methods to assess and compare proposals, it significantly eases verification of results, engagement with a diverse range of contributors, and progress. However, we have yet to fully achieve this; there are still many sociotechnical frictions.
Inspired by David Donoho's vision, this talk aims to revisit the three crucial pillars of frictionless reproducibility (data sharing, code sharing, and competitive challenges) with the perspective of deep software variability.
Our observation is that multiple layers — hardware, operating systems, third-party libraries, software versions, input data, compile-time options, and parameters — are subject to variability that exacerbates frictions but is also essential for achieving robust, generalizable results and fostering innovation. I will first review the literature, providing evidence of how the complex variability interactions across these layers affect qualitative and quantitative software properties, thereby complicating the reproduction and replication of scientific studies in various fields.
I will then present some software engineering and AI techniques that can support the strategic exploration of variability spaces. These include the use of abstractions and models (e.g., feature models), sampling strategies (e.g., uniform, random), cost-effective measurements (e.g., incremental build of software configurations), and dimensionality reduction methods (e.g., transfer learning, feature selection, software debloating).
I will finally argue that deep variability is both the problem and solution of frictionless reproducibility, calling the software science community to develop new methods and tools to manage variability and foster reproducibility in software systems.
Exposé invité Journées Nationales du GDR GPL 2024
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
ANAMOLOUS SECONDARY GROWTH IN DICOT ROOTS.pptxRASHMI M G
Abnormal or anomalous secondary growth in plants. It defines secondary growth as an increase in plant girth due to vascular cambium or cork cambium. Anomalous secondary growth does not follow the normal pattern of a single vascular cambium producing xylem internally and phloem externally.
This presentation explores a brief idea about the structural and functional attributes of nucleotides, the structure and function of genetic materials along with the impact of UV rays and pH upon them.
Deep Behavioral Phenotyping in Systems Neuroscience for Functional Atlasing a...Ana Luísa Pinho
Functional Magnetic Resonance Imaging (fMRI) provides means to characterize brain activations in response to behavior. However, cognitive neuroscience has been limited to group-level effects referring to the performance of specific tasks. To obtain the functional profile of elementary cognitive mechanisms, the combination of brain responses to many tasks is required. Yet, to date, both structural atlases and parcellation-based activations do not fully account for cognitive function and still present several limitations. Further, they do not adapt overall to individual characteristics. In this talk, I will give an account of deep-behavioral phenotyping strategies, namely data-driven methods in large task-fMRI datasets, to optimize functional brain-data collection and improve inference of effects-of-interest related to mental processes. Key to this approach is the employment of fast multi-functional paradigms rich on features that can be well parametrized and, consequently, facilitate the creation of psycho-physiological constructs to be modelled with imaging data. Particular emphasis will be given to music stimuli when studying high-order cognitive mechanisms, due to their ecological nature and quality to enable complex behavior compounded by discrete entities. I will also discuss how deep-behavioral phenotyping and individualized models applied to neuroimaging data can better account for the subject-specific organization of domain-general cognitive systems in the human brain. Finally, the accumulation of functional brain signatures brings the possibility to clarify relationships among tasks and create a univocal link between brain systems and mental functions through: (1) the development of ontologies proposing an organization of cognitive processes; and (2) brain-network taxonomies describing functional specialization. To this end, tools to improve commensurability in cognitive science are necessary, such as public repositories, ontology-based platforms and automated meta-analysis tools. I will thus discuss some brain-atlasing resources currently under development, and their applicability in cognitive as well as clinical neuroscience.
Phenomics assisted breeding in crop improvementIshaGoswami9
As the population is increasing and will reach about 9 billion upto 2050. Also due to climate change, it is difficult to meet the food requirement of such a large population. Facing the challenges presented by resource shortages, climate
change, and increasing global population, crop yield and quality need to be improved in a sustainable way over the coming decades. Genetic improvement by breeding is the best way to increase crop productivity. With the rapid progression of functional
genomics, an increasing number of crop genomes have been sequenced and dozens of genes influencing key agronomic traits have been identified. However, current genome sequence information has not been adequately exploited for understanding
the complex characteristics of multiple gene, owing to a lack of crop phenotypic data. Efficient, automatic, and accurate technologies and platforms that can capture phenotypic data that can
be linked to genomics information for crop improvement at all growth stages have become as important as genotyping. Thus,
high-throughput phenotyping has become the major bottleneck restricting crop breeding. Plant phenomics has been defined as the high-throughput, accurate acquisition and analysis of multi-dimensional phenotypes
during crop growing stages at the organism level, including the cell, tissue, organ, individual plant, plot, and field levels. With the rapid development of novel sensors, imaging technology,
and analysis methods, numerous infrastructure platforms have been developed for phenotyping.
Richard's aventures in two entangled wonderlandsRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
DERIVATION OF MODIFIED BERNOULLI EQUATION WITH VISCOUS EFFECTS AND TERMINAL V...Wasswaderrick3
In this book, we use conservation of energy techniques on a fluid element to derive the Modified Bernoulli equation of flow with viscous or friction effects. We derive the general equation of flow/ velocity and then from this we derive the Pouiselle flow equation, the transition flow equation and the turbulent flow equation. In the situations where there are no viscous effects , the equation reduces to the Bernoulli equation. From experimental results, we are able to include other terms in the Bernoulli equation. We also look at cases where pressure gradients exist. We use the Modified Bernoulli equation to derive equations of flow rate for pipes of different cross sectional areas connected together. We also extend our techniques of energy conservation to a sphere falling in a viscous medium under the effect of gravity. We demonstrate Stokes equation of terminal velocity and turbulent flow equation. We look at a way of calculating the time taken for a body to fall in a viscous medium. We also look at the general equation of terminal velocity.
1. John Carpenter, JAO Observatory Scientist
Juande Santander, JAO Development System Engineer
Carla Crovari, JAO Development Project Manager
ALMA 2030 First Project
Wideband Sensitivity Upgrade
3. ALMA and new facilities
ALMA
TMT 30 meter
ESO 39 meter
JWST
Nancy Grace Roman
Telescope
ngVLA
GMT 25 meter
Vera Rubin Telescope
4. 1
THE ALMA
DEVELOPMENT
ROADMAP
J. Carpenter, D. Iono, L. Testi, N. Whyborn, A. Wootten, N. Evans
(The ALMA Development Working Group)
Approved by the Board by written procedure pursuant Art. 11 of the Board’s Rules of Procedure
Need upgrades for better science, synergy
with these facilities
5. From the ALMA 2030 Development Program, approved by the ALMA Board in 2017-2018 (1)
(1) “The ALMA Development Roadmap”, Doc #: AEDM 2018-017-O
The Wideband Sensitivity Upgrade
program, is the set of projects that
will enable ALMA:
• To broaden the receiver IF
bandwidth up to a factor four
(x4), and
• To upgrade the associated
electronics and correlator
First one, the Wideband Sensitivity Upgrade
6. Wideband Sensitivity Upgrade: Overview
Upgrade of the bandwidth and throughput of the ALMA system with improved sensitivity
- better receivers
- collect and transport more data
- process more data
Correlator
@ AOS
Archives
Data processing
@ SCO
Astronomers
Antennas Receivers Back end
Upgrade!
7. ALMA 2030 new Challenges
• Planning, designing, and executing the expansion projects, at the same time as operations
continue – as much as possible
• Core systems of the Observatory will be updated, preparing for a much higher data flow.
• We need…
- A systemic approach, together with a thorough identification of the systems that need to
be updated
- Careful planning and a dedicated follow up: we want the complete chain of upgrades
together with the current operation to be successful!
8. Dedicated Roles
ALMA 2030 Roadmap Co-author Joined June 2022 Joined March 2022
John Carpenter,
Observatory Scientist
Juande Santander-Vela,
JAO Development
Systems Engineer
Carla Crovari,
JAO Development
Project Manager
10. Wideband Sensitivity Upgrade: Overview
• Available bandwidth
• Correlated bandwidth
• Observing speed 2-4 times more stations available for you to listen to!
11. Wideband Sensitivity Upgrade: Overview
• Available bandwidth
• Correlated bandwidth
• Observing speed
WSU will have many times more frequency coverage!
Record up to 68 times more stations at the same time!
12. Wideband Sensitivity Upgrade: Overview
• Available bandwidth
• Correlated bandwidth
• Observing speed
Increase in Band 6 observing speed with ALMA 2030
Observing mode Increase in speed over current system*
Continuum 4.8x (with goal of 9.6x)
Spectral line 2.25-4.7x
Increase in observing speed results from
• improved receiver temperatures
• improved digital efficiency
• wider bandwidth (continuum)
Spectral scans will see further speed increases due to larger correlated bandwidth.
* To reach same sensitivity as current system with single tuning
13. Wideband Sensitivity Upgrade: Overview
• Available bandwidth
• Correlated bandwidth
• Observing speed
Listen to the radio station to more remote locations!
14. The power of molecular spectroscopy in disks
• ALMA continuum images traces the solid particles (“dust”) in the disk.
• ALMA molecular line images traces the gas:
- chemistry and the chemical compositions of planets
- 3D velocity and temperature structure of disks
- detect embedded planets through velocity distortions
Dust
HD 163296
Öberg et al. (2021)
15. The ALMA 2030 Advantage
Band 6v2 IF=12 GHz
SiO
J=5-4
c-C3H2
6(0,6)-5(1,5)
HC3N
J=24-23
C17
O
J=2-1
H2CO
3(2,1)-2(2,0)
C15
N
N=2-1
H2S
2(2,0)-2(1,1)
c-C3H2
3(3,0)-2(2,1)
SO
3Σ 6(5)-5(4)
SO2
11(1,11)-10(0,10)
c-C3H2
5(2,3)-4(3,2)
13CS
J=5-4
C34S
J=5-4
HC3N
J=28-27
t-HCOOH
11(2,10)-10(2,9)
SO
3Σ 2(3)-3(2)
SO
3Σ 8(9)-8(8)
SO
3Σ 5(6)-4(5)
c-C3H2
5(3,3)-4(2,2)
HC18O+
J=3-2
HC3N
J=25-24
H2CS
7(0,7)-6(0,6)
CS
J=5-4
HC3N
J=27-26
CN
N=2-1
t-HCOOH
10(4,6)-9(4,5)
H2CO
3(1,2)-2(1,1)
c-C3H2
4(3,2)-3(2,1)
c-C3H2
3(2,1)-2(1,2)
H2CS
7(1,6)-6(1,5)
SO2
10(5,5)-11(4,8)
NO
J=5/2-3/2
DCO+
J=3-2
… and up to 40 additional spectral windows!
16. The WSU benefits all ALMA projects!
Outflow
SiO
Envelope
DCO+
Protostar
Envelope
Disk
Outflow
Formation of individual stars Star formation across galaxies Origins of the first galaxies
z=9.11
17. Mentimeter question!
Will the system you work in be updated for the WSU project?
• Yes
• No, but the system I work in will be impacted
• No
• I don’t know
Correlator
@ AOS
Archives
Data processing
@ SCO
Astronomers
Antennas Receivers Back end
Upgrade!
Go to menti.com
and use code
1706 7017
27. ALMA
Environmental
Specifications
ALMA System
General Safety
Design
Specification
ALMA Product
Assurance
Requirements
ALMA Product
Tree
ALMA Policy
Document: Use of
Metric and SI
Units
Requirements
and guidelines for
identification and
labeling of ALMA
equipment
ALMA Power
Quality
(Compatibility
Levels)
Specification
ALMA System
Electro-magnetic
Compatibility
(EMC)
Requirements
Standards for AC
Plugs, Socket-
Outlets, and
Couplers
ALMA System
Electrical Design
Requirements
ALMA Documen-
tation Standards
ALMA Documen-
tation Control
Plan
ALMA Coordinate
Systems
Specification
Interface Control
Document
Management
Plan
Seismic Design
Specifications
(AOS & OSF)
ALMA System
Technical
Requirements
28.
29.
30.
31.
32.
33.
34.
35.
36.
37.
38.
39. These are only the specifications that
will need to change because of the
ALMA 2030 Roadmap!
40. Did you know that there are more than
85,000 documents in the ALMA Elecronic
Document Management System?
41. How do we make sure we have the right
specifications updated…
42. How do we make sure we have the right
specifications updated…
…and the right updates?
44. «Systems Engineering is a transdisciplinary approach
and means to enable the realization of successful
systems.
Successful systems must satisfy the needs of their
customers, users and other stakeholders.»
This definition and diagrams in the presentation from the
Systems Engineering Book of Knowledge (SEBoK)
45. Key Elements of Systems Engineering
Users/Stakeholders
indicate
needs
Systems Engineers
elicit
needs
Development Teams
specify
system
Implement
system
checks system
maturity and
lifecycle
System
provided to
Environment
Interacts
46. Key Elements of Systems Engineering
Users/Stakeholders
indicate
needs
Systems Engineers
elicit
needs
Development Teams
specify
system
Implement
system
checks system
maturity and
lifecycle
System
provided to
Environment
Interacts
Systems Engineering focuses on
ensuring that the pieces work together
to achieve the objectives of the whole
47. Key Elements of Systems Engineering
Users/Stakeholders
indicate
needs
Systems Engineers
elicit
needs
Development Teams
specify
system
Implement
system
checks system
maturity and
lifecycle
System
provided to
Environment
Interacts
Main role of the Systems Engineering function
is as connective tissue and translation layer
across the different stakeholders
throughout the life of the system.
48. Key Elements of Systems Engineering
Users/Stakeholders
indicate
needs
Systems Engineers
elicit
needs
Development Teams
specify
system
Implement
system
checks system
maturity and
lifecycle
System
provided to
Environment
Interacts
But Systems Engineering is also the
process and discipline of thinking about
the system so that project and system
risks are minimized.
49. Key Elements of Systems Engineering
Users/Stakeholders
indicate
needs
Systems Engineers
elicit
needs
Development Teams
specify
system
Implement
system
checks system
maturity and
lifecycle
System
provided to
Environment
Interacts
And to think about the system the
complexity needs to be managed.
50. «Systems Engineering is a transdisciplinary approach
and means to enable the realization of successful
systems.
Successful systems must satisfy the needs of their
customers, users and other stakeholders.»
This definition and diagrams in the presentation from
the Systems Engineering Book of Knowledge (SEBoK)
51. Need to avoid the trap of
being driven by technology
52. But this was not
a successful system!
Too much emphasis on a particular
technology/metric, and not enough
on operational needs
Abandoned because it was
accident prone, and broke a lot
What is this? It is
cool!
53. We start from the beginning:
what do the users need?
Requirements
System
Concept
Concept of
Operations
55. Requirements have a hierarchy
•Science Requirements
- System Requirements
‣ Subsystem Requirements
•Science Use Cases
- System Use Cases
‣ Discipline Use Cases
They sometimes interplay
with each other
Need to make sure we do something
that is not impossibly costly… or
impossibly complex, or finicky.
We need to be risk driven
in our approach
62. WSU Status Update: where we are now
CoSDD: Conceptual System Design Description
SRR: System Requirements Review
63. WSU Status Update: Conceptual System Design
Description (CoSDD) initial Review
• Scope: Data Acquisition Hardware sub-systems , internal Review
• Date: June 22nd and 23rd, 2022
• Main conclusions:
- A Concept needs to be developed for the Software / Data processing/ Data
distribution (new Working Group is needed)
- In good shape to proceed with the System Requirements update
64. WSU Status Update: Working Groups
Front End/ Digitizer Working Group
• Objective: update the Report “ALMA Front-end & Digitizer Requirements Upgrade”,
ALMA-05.00.00.00-0048-A-REP
• Participates: ESG team members plus Engineers from ESO, NRAO, NAOJ.
IF/ Digitizer Working Group
• Objective: analyze possible configurations regarding the Digitizer location
• Participates: ESG team members plus Engineers from ESO, NRAO, NAOJ.
65. ALMA 2030 WSU
05.20.01.20 Changes to
ALMA Chile Infrastructure
40 Front End
52-IF Processor
Subsystem IFPS
53-Data Transmission
Subsystem DTS
54-Fiber Optic Transmission
Subsystem FOTS
57-BE Miscellaneous
Equipment
60-64 antenna correlator (*)
64-ACA Spectrometer
70- Computing (*)
xx - Science Operations
85-88 System Integration
and Verification
80-System Engineering
xx Project Management
90-Science
WSU Status Update: Preliminary
Work Breakdown Structure (WBS)
66. Project Management and System Engineering for the WSU …in
an Observatory in full Operation….and managed by Executives
in different Regions!
Some things to consider:
• Careful Planning and Communications are essential.
• WSU is a set of projects, it is important to keep a systemic view, both among the new projects and with the
operating ALMA system.
• Good identification of stakeholders… and again, effective and well planned communications is required.
67. Project Management and System Engineering for the WSU …in
an Observatory in full Operation….and managed by Executives
in different Regions!
Some things to consider:
• ALMA technical experts are in Operation… collaboration will be needed (already started through Working
Groups participation)…thanks already and in advance!
• Your feedback (ideas, considerations) are and will be very much valued
• We can do it!… with a collaborative spirit, and step by step… we are just beginning….