TimTrack is an algorithm for tracking charged particles using data from detectors. It estimates the parameters of a "SAETA", which defines a particle track using 6 parameters. TimTrack uses a least squares method to minimize the differences between measured and predicted values from a model. It can handle data from various detector geometries by defining appropriate configuration and data matrices. The method provides a matrix solution that is fast to compute and easy to implement.
The document discusses the Trasgo Project, which aims to develop an affordable and high-performance timing and tracking detector. It describes the key aspects of Trasgo, including its use of timing resistive plate chambers for high time resolution, a timing and tracking board for data acquisition and reconstruction, and a fast track reconstruction algorithm. Potential applications of Trasgo that are mentioned include cosmic ray detection for research in astroparticle physics, dosimetry, and studying correlations between cosmic rays and climate change. Examples are given of how Trasgo could provide more accurate information about air shower properties compared to using surface detectors alone.
TimTrack is an algorithm for tracking charged particles using data from detectors. It estimates the parameters of a "SAETA", which defines a particle track using 6 parameters. TimTrack uses a least squares method to minimize the differences between measured and predicted values from a model. It can handle data from various detector geometries by defining appropriate configuration and data matrices. The method provides a matrix solution that is fast to compute and easy to implement.
1. Timtrack is a tracking algorithm that uses a least squares method to estimate the parameters of tracks (called SAETAs) passing through detector planes.
2. A SAETA contains 6 parameters that define a track: two coordinates at a reference plane, two projected slopes, time at the reference plane, and velocity.
3. Timtrack works directly with detector measurements like coordinates and times. It allows the SAETA parameters to vary to minimize the difference between measured and predicted values across detector planes.
The document discusses calibration of the tanks at the Pierre Auger Observatory. It describes a three step calibration process: 1) adjusting PMT voltages to equalize signals, 2) setting trigger thresholds to achieve 100Hz single rates at 150 channels, and 3) using charge histograms to determine peak charge values accurately. Understanding the tank response to inclined muons is important for analyzing inclined showers, which provide additional statistics and composition information. Measuring muon flux and properties directly is needed to validate simulation models used in the analysis of inclined events.
The document discusses the development of sealed resistive plate chambers (sRPCs) as a more flexible alternative to gas ionization detectors that do not require a gas system. Several prototype sRPCs were constructed and two were tested with radioactive sources, though two failed on the first day with little response. Signals from the functioning chambers increased over time, and high voltage had to be decreased to avoid streamers but with reduced gain. Further testing is needed to evaluate resolution, efficiency, isolation, and alternative gas mixtures to better understand aging effects in sRPCs.
The document summarizes a simulation of extensive air showers (EAS) using the AIRES code. Key points:
1) Simulations were run for primaries of protons, carbon, iron, and gamma rays with energies of 1015 eV in the "knee" region to study EAS characteristics.
2) Variables like energy, arrival time, production height, and identity of secondaries were recorded. Results showed differences in lateral distribution and time profiles between primaries.
3) Further analysis of observables like particle counts, arrival times, and azimuthal/zenith angles at different distances from the core is planned to better understand correlations with primary properties. Multivariate analysis techniques may help reveal hidden
This document discusses signal coupling in multi-conductor timing RPC detectors. It provides theoretical models and experimental results on pad, strip, double-strip, and multi-strip detector configurations. Simulations show cross-talk levels below 3% and cluster sizes of 1 can be achieved in optimized multi-strip designs, with time resolutions around 110 ps even for double hits. Experimental measurements on long multi-strip detectors validated the simulations. Further optimization may still improve performance.
The document discusses the front-end electronics (FEE) developed for the timing RPCs used in the HADES experiment. The FEE consists of daughter boards (DBOs) connected to the RPC cells that amplify and digitize signals, and mother boards (MBOs) that interface between the DBOs and data acquisition system. The FEE achieves a time resolution of less than 17 ps using a charge-to-width algorithm to encode timing and charge information. Testing shows the FEE performs well and could be adapted for use in the TRASGO detector with some modifications to reduce power consumption.
The document discusses the Trasgo Project, which aims to develop an affordable and high-performance timing and tracking detector. It describes the key aspects of Trasgo, including its use of timing resistive plate chambers for high time resolution, a timing and tracking board for data acquisition and reconstruction, and a fast track reconstruction algorithm. Potential applications of Trasgo that are mentioned include cosmic ray detection for research in astroparticle physics, dosimetry, and studying correlations between cosmic rays and climate change. Examples are given of how Trasgo could provide more accurate information about air shower properties compared to using surface detectors alone.
TimTrack is an algorithm for tracking charged particles using data from detectors. It estimates the parameters of a "SAETA", which defines a particle track using 6 parameters. TimTrack uses a least squares method to minimize the differences between measured and predicted values from a model. It can handle data from various detector geometries by defining appropriate configuration and data matrices. The method provides a matrix solution that is fast to compute and easy to implement.
1. Timtrack is a tracking algorithm that uses a least squares method to estimate the parameters of tracks (called SAETAs) passing through detector planes.
2. A SAETA contains 6 parameters that define a track: two coordinates at a reference plane, two projected slopes, time at the reference plane, and velocity.
3. Timtrack works directly with detector measurements like coordinates and times. It allows the SAETA parameters to vary to minimize the difference between measured and predicted values across detector planes.
The document discusses calibration of the tanks at the Pierre Auger Observatory. It describes a three step calibration process: 1) adjusting PMT voltages to equalize signals, 2) setting trigger thresholds to achieve 100Hz single rates at 150 channels, and 3) using charge histograms to determine peak charge values accurately. Understanding the tank response to inclined muons is important for analyzing inclined showers, which provide additional statistics and composition information. Measuring muon flux and properties directly is needed to validate simulation models used in the analysis of inclined events.
The document discusses the development of sealed resistive plate chambers (sRPCs) as a more flexible alternative to gas ionization detectors that do not require a gas system. Several prototype sRPCs were constructed and two were tested with radioactive sources, though two failed on the first day with little response. Signals from the functioning chambers increased over time, and high voltage had to be decreased to avoid streamers but with reduced gain. Further testing is needed to evaluate resolution, efficiency, isolation, and alternative gas mixtures to better understand aging effects in sRPCs.
The document summarizes a simulation of extensive air showers (EAS) using the AIRES code. Key points:
1) Simulations were run for primaries of protons, carbon, iron, and gamma rays with energies of 1015 eV in the "knee" region to study EAS characteristics.
2) Variables like energy, arrival time, production height, and identity of secondaries were recorded. Results showed differences in lateral distribution and time profiles between primaries.
3) Further analysis of observables like particle counts, arrival times, and azimuthal/zenith angles at different distances from the core is planned to better understand correlations with primary properties. Multivariate analysis techniques may help reveal hidden
This document discusses signal coupling in multi-conductor timing RPC detectors. It provides theoretical models and experimental results on pad, strip, double-strip, and multi-strip detector configurations. Simulations show cross-talk levels below 3% and cluster sizes of 1 can be achieved in optimized multi-strip designs, with time resolutions around 110 ps even for double hits. Experimental measurements on long multi-strip detectors validated the simulations. Further optimization may still improve performance.
The document discusses the front-end electronics (FEE) developed for the timing RPCs used in the HADES experiment. The FEE consists of daughter boards (DBOs) connected to the RPC cells that amplify and digitize signals, and mother boards (MBOs) that interface between the DBOs and data acquisition system. The FEE achieves a time resolution of less than 17 ps using a charge-to-width algorithm to encode timing and charge information. Testing shows the FEE performs well and could be adapted for use in the TRASGO detector with some modifications to reduce power consumption.
This document discusses the relationship between cosmic rays, solar activity, and climate/weather patterns. It begins by outlining how solar wind modulates cosmic rays, which influence cloud formation by acting as cloud condensation nuclei. Studies of Forbush decreases have provided evidence this mechanism works in the real atmosphere. The author then discusses how cosmic ray flux variations from our galactic position may have influenced past climate changes. Finally, the document analyzes correlations between solar activity and climate variability patterns like the NAO and weather types in Galicia, Spain. The overall evidence suggests solar activity modulates cosmic rays in ways that influence global and regional climate and weather patterns.
The document presents work on the MIDAS project which aims to identify particle masses using multiple sampling. It outlines results from initial MATLAB simulations showing electrons can be distinguished from muons and protons below 500 MeV. A Geant4 simulation using the SETA environment was also developed to model the TRASGO detector in more detail. Further simulations are needed but combining velocity, chi-squared values with additional information like timing may allow ambiguous particles to be discriminated.
The document discusses calibration of the tanks at the Pierre Auger Observatory. It describes a three step calibration process: 1) adjusting PMT voltages to obtain the same signal for a vertical muon, 2) setting the trigger threshold to obtain a 100Hz single particle rate at 150 channels, and 3) using charge histograms to determine the signal produced by a vertical muon. Calibration information like histograms of baseline, pulse height, and charge are provided with event data. Analysis of inclined showers is also discussed, noting they are important for composition studies and increasing statistics. Understanding the tank response to inclined muons is crucial, but has not been directly measured.
This document discusses characteristics of extensive air showers initiated by cosmic rays, including:
1) Shower characteristics like size, timing, energies, densities, and rates are intrinsic properties that must be accounted for in cosmic ray detector design and interpretation of data.
2) Models can be used to understand shower development and determine physical parameters from air shower data, but depend on hadronic interactions and primary particle composition which introduce uncertainties.
3) The energy and altitude of detection affect what can be observed, with higher energy air showers penetrating further and being detectable at higher altitudes.
The document discusses field-programmable gate arrays (FPGAs) and their potential use as tracking devices. It provides an overview of FPGA technology, including programmable logic blocks, interconnects, embedded memory and hard processor cores. The document compares FPGAs to application-specific integrated circuits (ASICs) and discusses performance, design effort required, and example applications of FPGAs.
The document provides an overview of the HADES RPC ToF Wall cosmic ray commissioning project. It discusses (1) the instrumentation of the 6 RPC sectors and initial cosmic ray testing, (2) the collection of approximately 50 days of cosmic ray data totaling 895 GB, and (3) preliminary analysis of cosmic ray tracks using the TimTrack algorithm, including reconstructed position and time results. The aim is to validate the RPC detector performance before data taking with particle beams begins.
The document summarizes the development of a large area sealed RPC detector for use in cosmic ray experiments and outreach activities. A 1 square meter first prototype was built in August 2009 using a modular design of 4mm acrylic and 2mm glass layers with external readout electrodes. Initial performance testing shows a background current that is hypothesized to come from trapped air or material outgassing that is expected to reduce after further cleaning cycles.
TimTrack is a software for tracking charged particles that uses C language for its speed and flexibility. It uses linear algebra libraries like LAPACK and Intel IPP for numerical computations like solving systems of linear equations. TimTrack version 2.0 implements a new algebra version for faster variance-covariance matrix calculations. Future versions will parallelize computations using OpenMP, MPI, and GPUs with CUDA to further improve performance for large particle datasets.
The TRB was developed as a general purpose platform for time-to-digital converters (TDCs) and fast data acquisition for nuclear physics experiments with thousands of channels. It provides integrated TDC, data acquisition, and local computing capabilities in a modular design that can be directly mounted on detectors. Measurements showed time resolutions of 40 picoseconds for 128 channels and 16 picoseconds for 32 channels. The TRB has been successfully used in several experiments and more developments are planned to further improve performance and reduce costs.
The document discusses the development of sealed resistive plate chambers (sRPCs) as a more flexible alternative to gas ionization detectors that do not require a gas system. Several prototype sRPCs were constructed and two were tested with radioactive sources, finding that signals and current increased over time but that high voltage had to be reduced to avoid streamers at the cost of gain. Further work is needed to characterize the resolution and efficiency of sRPCs over time and to improve their construction and evaluate different gas mixtures to reduce aging effects.
This document discusses the relationship between cosmic rays, solar activity, and climate/weather patterns. It outlines that solar wind modulates cosmic rays entering the atmosphere, which act as cloud condensation nuclei and affect cloud formation. Studies have found correlations between cosmic ray flux decreases during solar events and decreases in cloud cover. The document then discusses how this proposed mechanism may influence climate through impacts on cloud radiative forcing. It analyzes links between various climate patterns like the North Atlantic Oscillation and weather types with rainfall and temperature in Galicia, Spain, and how these correlations have changed over time with solar activity levels.
This document discusses signal coupling in multi-conductor highly inhomogeneous HF environments like multi-strip timing RPC detectors. It summarizes simulations and measurements of cross-talk and time resolution in multi-strip RPC detectors of various lengths from 20cm to 100cm. Optimization techniques like differential signaling and shielding were able to reduce cross-talk to below 3% and achieve cluster sizes of around 1, with a modest degradation of time resolution to 110ps mainly affecting the first neighbor strips. Further optimization may still be possible.
The document summarizes a simulation of extensive air showers (EAS) using the AIRES code. Key results include:
1) Simulations of EAS were conducted for primaries of protons, carbon, iron, and gamma rays with energies of 1015 eV in the "knee" region.
2) Observables like particle type, arrival time, zenith angle, and azimuthal angle were recorded for electrons and muons at varying distances from the shower core.
3) Preliminary analysis of arrival times and angular distributions shows differences between primaries that could help identify the primary particle.
4) Further multivariate analysis of correlations between observables may provide hidden insights into the primary cosmic ray
The document discusses estimating a saeta (trajectory) using a linear model, where available data Y is modeled as a function of known quantities X and unknown parameters that determine the saeta plus some errors. It describes how to obtain the estimator for the parameters and its properties. It then poses three questions about estimating a saeta under different references, imposing restrictions like going through the origin, and combining information from multiple estimated saetas.
TimTrack is a software for tracking charged particles. It uses C language for its speed and flexibility. Previous versions used LAPACK or Intel IPP libraries for linear algebra operations. The newest version TimTrack v2.0 uses LAPACK and is 23.6 seconds faster than earlier versions for tracking 1 million particles. Future plans include parallelizing with OpenMP, MPI, and implementing on GPUs using CUDA.
1. The document discusses methods for estimating and analyzing saetas (linear models). It proposes estimating a saeta under a new reference frame by applying the appropriate transformation to the estimated saeta coefficients.
2. Once a saeta is estimated, it can be restricted to pass through the origin by applying a linear restriction to the model estimation. The restriction can be tested with an F-test.
3. When two saetas are estimated from different data sets, the best overall saeta can be determined by testing whether the two saetas are equal.
Este documento describe los rayos cósmicos, incluyendo su interacción con la atmósfera terrestre, su composición y espectro de energía, y los métodos para estudiarlos. También presenta el proyecto Trasgo, el cual propone desarrollar un detector de rastreo de partículas basado en cámaras de placas resistivas para proporcionar información adicional sobre las partículas de alta energía.
Este documento describe los rayos cósmicos y su estudio mediante cascadas atmosféricas. Detalla la historia del descubrimiento de los rayos cósmicos, su composición y espectro energético. Explica cómo se forman y desarrollan las cascadas atmosféricas y cómo se pueden medir para caracterizar las partículas primarias. Finalmente, menciona algunos experimentos históricos y actuales y las técnicas que utilizan para estudiar las cascadas y los rayos cósmicos.
The TRASGO project aims to develop an innovative cosmic ray detector based on timing RPCs. The detector, called TRASGO, will be able to measure particle timing, tracking, and identification. It will consist of timing RPC planes with 100ps time resolution, a fast tracking algorithm called TimTrack, and a particle identification method called MIDAS. An array of 10-50 TRASGO detectors called MEIGA will be installed to study cosmic rays around the knee and test simulation packages. The MEIGA collaboration has been formed between universities in Spain and Portugal to develop the detectors and carry out the cosmic ray measurements.
This document discusses the relationship between cosmic rays, solar activity, and climate/weather patterns. It begins by outlining how solar wind modulates cosmic rays, which influence cloud formation by acting as cloud condensation nuclei. Studies of Forbush decreases have provided evidence this mechanism works in the real atmosphere. The author then discusses how cosmic ray flux variations from our galactic position may have influenced past climate changes. Finally, the document analyzes correlations between solar activity and climate variability patterns like the NAO and weather types in Galicia, Spain. The overall evidence suggests solar activity modulates cosmic rays in ways that influence global and regional climate and weather patterns.
The document presents work on the MIDAS project which aims to identify particle masses using multiple sampling. It outlines results from initial MATLAB simulations showing electrons can be distinguished from muons and protons below 500 MeV. A Geant4 simulation using the SETA environment was also developed to model the TRASGO detector in more detail. Further simulations are needed but combining velocity, chi-squared values with additional information like timing may allow ambiguous particles to be discriminated.
The document discusses calibration of the tanks at the Pierre Auger Observatory. It describes a three step calibration process: 1) adjusting PMT voltages to obtain the same signal for a vertical muon, 2) setting the trigger threshold to obtain a 100Hz single particle rate at 150 channels, and 3) using charge histograms to determine the signal produced by a vertical muon. Calibration information like histograms of baseline, pulse height, and charge are provided with event data. Analysis of inclined showers is also discussed, noting they are important for composition studies and increasing statistics. Understanding the tank response to inclined muons is crucial, but has not been directly measured.
This document discusses characteristics of extensive air showers initiated by cosmic rays, including:
1) Shower characteristics like size, timing, energies, densities, and rates are intrinsic properties that must be accounted for in cosmic ray detector design and interpretation of data.
2) Models can be used to understand shower development and determine physical parameters from air shower data, but depend on hadronic interactions and primary particle composition which introduce uncertainties.
3) The energy and altitude of detection affect what can be observed, with higher energy air showers penetrating further and being detectable at higher altitudes.
The document discusses field-programmable gate arrays (FPGAs) and their potential use as tracking devices. It provides an overview of FPGA technology, including programmable logic blocks, interconnects, embedded memory and hard processor cores. The document compares FPGAs to application-specific integrated circuits (ASICs) and discusses performance, design effort required, and example applications of FPGAs.
The document provides an overview of the HADES RPC ToF Wall cosmic ray commissioning project. It discusses (1) the instrumentation of the 6 RPC sectors and initial cosmic ray testing, (2) the collection of approximately 50 days of cosmic ray data totaling 895 GB, and (3) preliminary analysis of cosmic ray tracks using the TimTrack algorithm, including reconstructed position and time results. The aim is to validate the RPC detector performance before data taking with particle beams begins.
The document summarizes the development of a large area sealed RPC detector for use in cosmic ray experiments and outreach activities. A 1 square meter first prototype was built in August 2009 using a modular design of 4mm acrylic and 2mm glass layers with external readout electrodes. Initial performance testing shows a background current that is hypothesized to come from trapped air or material outgassing that is expected to reduce after further cleaning cycles.
TimTrack is a software for tracking charged particles that uses C language for its speed and flexibility. It uses linear algebra libraries like LAPACK and Intel IPP for numerical computations like solving systems of linear equations. TimTrack version 2.0 implements a new algebra version for faster variance-covariance matrix calculations. Future versions will parallelize computations using OpenMP, MPI, and GPUs with CUDA to further improve performance for large particle datasets.
The TRB was developed as a general purpose platform for time-to-digital converters (TDCs) and fast data acquisition for nuclear physics experiments with thousands of channels. It provides integrated TDC, data acquisition, and local computing capabilities in a modular design that can be directly mounted on detectors. Measurements showed time resolutions of 40 picoseconds for 128 channels and 16 picoseconds for 32 channels. The TRB has been successfully used in several experiments and more developments are planned to further improve performance and reduce costs.
The document discusses the development of sealed resistive plate chambers (sRPCs) as a more flexible alternative to gas ionization detectors that do not require a gas system. Several prototype sRPCs were constructed and two were tested with radioactive sources, finding that signals and current increased over time but that high voltage had to be reduced to avoid streamers at the cost of gain. Further work is needed to characterize the resolution and efficiency of sRPCs over time and to improve their construction and evaluate different gas mixtures to reduce aging effects.
This document discusses the relationship between cosmic rays, solar activity, and climate/weather patterns. It outlines that solar wind modulates cosmic rays entering the atmosphere, which act as cloud condensation nuclei and affect cloud formation. Studies have found correlations between cosmic ray flux decreases during solar events and decreases in cloud cover. The document then discusses how this proposed mechanism may influence climate through impacts on cloud radiative forcing. It analyzes links between various climate patterns like the North Atlantic Oscillation and weather types with rainfall and temperature in Galicia, Spain, and how these correlations have changed over time with solar activity levels.
This document discusses signal coupling in multi-conductor highly inhomogeneous HF environments like multi-strip timing RPC detectors. It summarizes simulations and measurements of cross-talk and time resolution in multi-strip RPC detectors of various lengths from 20cm to 100cm. Optimization techniques like differential signaling and shielding were able to reduce cross-talk to below 3% and achieve cluster sizes of around 1, with a modest degradation of time resolution to 110ps mainly affecting the first neighbor strips. Further optimization may still be possible.
The document summarizes a simulation of extensive air showers (EAS) using the AIRES code. Key results include:
1) Simulations of EAS were conducted for primaries of protons, carbon, iron, and gamma rays with energies of 1015 eV in the "knee" region.
2) Observables like particle type, arrival time, zenith angle, and azimuthal angle were recorded for electrons and muons at varying distances from the shower core.
3) Preliminary analysis of arrival times and angular distributions shows differences between primaries that could help identify the primary particle.
4) Further multivariate analysis of correlations between observables may provide hidden insights into the primary cosmic ray
The document discusses estimating a saeta (trajectory) using a linear model, where available data Y is modeled as a function of known quantities X and unknown parameters that determine the saeta plus some errors. It describes how to obtain the estimator for the parameters and its properties. It then poses three questions about estimating a saeta under different references, imposing restrictions like going through the origin, and combining information from multiple estimated saetas.
TimTrack is a software for tracking charged particles. It uses C language for its speed and flexibility. Previous versions used LAPACK or Intel IPP libraries for linear algebra operations. The newest version TimTrack v2.0 uses LAPACK and is 23.6 seconds faster than earlier versions for tracking 1 million particles. Future plans include parallelizing with OpenMP, MPI, and implementing on GPUs using CUDA.
1. The document discusses methods for estimating and analyzing saetas (linear models). It proposes estimating a saeta under a new reference frame by applying the appropriate transformation to the estimated saeta coefficients.
2. Once a saeta is estimated, it can be restricted to pass through the origin by applying a linear restriction to the model estimation. The restriction can be tested with an F-test.
3. When two saetas are estimated from different data sets, the best overall saeta can be determined by testing whether the two saetas are equal.
Este documento describe los rayos cósmicos, incluyendo su interacción con la atmósfera terrestre, su composición y espectro de energía, y los métodos para estudiarlos. También presenta el proyecto Trasgo, el cual propone desarrollar un detector de rastreo de partículas basado en cámaras de placas resistivas para proporcionar información adicional sobre las partículas de alta energía.
Este documento describe los rayos cósmicos y su estudio mediante cascadas atmosféricas. Detalla la historia del descubrimiento de los rayos cósmicos, su composición y espectro energético. Explica cómo se forman y desarrollan las cascadas atmosféricas y cómo se pueden medir para caracterizar las partículas primarias. Finalmente, menciona algunos experimentos históricos y actuales y las técnicas que utilizan para estudiar las cascadas y los rayos cósmicos.
The TRASGO project aims to develop an innovative cosmic ray detector based on timing RPCs. The detector, called TRASGO, will be able to measure particle timing, tracking, and identification. It will consist of timing RPC planes with 100ps time resolution, a fast tracking algorithm called TimTrack, and a particle identification method called MIDAS. An array of 10-50 TRASGO detectors called MEIGA will be installed to study cosmic rays around the knee and test simulation packages. The MEIGA collaboration has been formed between universities in Spain and Portugal to develop the detectors and carry out the cosmic ray measurements.
Taking AI to the Next Level in Manufacturing.pdfssuserfac0301
Read Taking AI to the Next Level in Manufacturing to gain insights on AI adoption in the manufacturing industry, such as:
1. How quickly AI is being implemented in manufacturing.
2. Which barriers stand in the way of AI adoption.
3. How data quality and governance form the backbone of AI.
4. Organizational processes and structures that may inhibit effective AI adoption.
6. Ideas and approaches to help build your organization's AI strategy.
Digital Marketing Trends in 2024 | Guide for Staying AheadWask
https://www.wask.co/ebooks/digital-marketing-trends-in-2024
Feeling lost in the digital marketing whirlwind of 2024? Technology is changing, consumer habits are evolving, and staying ahead of the curve feels like a never-ending pursuit. This e-book is your compass. Dive into actionable insights to handle the complexities of modern marketing. From hyper-personalization to the power of user-generated content, learn how to build long-term relationships with your audience and unlock the secrets to success in the ever-shifting digital landscape.
Have you ever been confused by the myriad of choices offered by AWS for hosting a website or an API?
Lambda, Elastic Beanstalk, Lightsail, Amplify, S3 (and more!) can each host websites + APIs. But which one should we choose?
Which one is cheapest? Which one is fastest? Which one will scale to meet our needs?
Join me in this session as we dive into each AWS hosting service to determine which one is best for your scenario and explain why!
Let's Integrate MuleSoft RPA, COMPOSER, APM with AWS IDP along with Slackshyamraj55
Discover the seamless integration of RPA (Robotic Process Automation), COMPOSER, and APM with AWS IDP enhanced with Slack notifications. Explore how these technologies converge to streamline workflows, optimize performance, and ensure secure access, all while leveraging the power of AWS IDP and real-time communication via Slack notifications.
Ivanti’s Patch Tuesday breakdown goes beyond patching your applications and brings you the intelligence and guidance needed to prioritize where to focus your attention first. Catch early analysis on our Ivanti blog, then join industry expert Chris Goettl for the Patch Tuesday Webinar Event. There we’ll do a deep dive into each of the bulletins and give guidance on the risks associated with the newly-identified vulnerabilities.
HCL Notes and Domino License Cost Reduction in the World of DLAUpanagenda
Webinar Recording: https://www.panagenda.com/webinars/hcl-notes-and-domino-license-cost-reduction-in-the-world-of-dlau/
The introduction of DLAU and the CCB & CCX licensing model caused quite a stir in the HCL community. As a Notes and Domino customer, you may have faced challenges with unexpected user counts and license costs. You probably have questions on how this new licensing approach works and how to benefit from it. Most importantly, you likely have budget constraints and want to save money where possible. Don’t worry, we can help with all of this!
We’ll show you how to fix common misconfigurations that cause higher-than-expected user counts, and how to identify accounts which you can deactivate to save money. There are also frequent patterns that can cause unnecessary cost, like using a person document instead of a mail-in for shared mailboxes. We’ll provide examples and solutions for those as well. And naturally we’ll explain the new licensing model.
Join HCL Ambassador Marc Thomas in this webinar with a special guest appearance from Franz Walder. It will give you the tools and know-how to stay on top of what is going on with Domino licensing. You will be able lower your cost through an optimized configuration and keep it low going forward.
These topics will be covered
- Reducing license cost by finding and fixing misconfigurations and superfluous accounts
- How do CCB and CCX licenses really work?
- Understanding the DLAU tool and how to best utilize it
- Tips for common problem areas, like team mailboxes, functional/test users, etc
- Practical examples and best practices to implement right away
How to Get CNIC Information System with Paksim Ga.pptxdanishmna97
Pakdata Cf is a groundbreaking system designed to streamline and facilitate access to CNIC information. This innovative platform leverages advanced technology to provide users with efficient and secure access to their CNIC details.
UiPath Test Automation using UiPath Test Suite series, part 6DianaGray10
Welcome to UiPath Test Automation using UiPath Test Suite series part 6. In this session, we will cover Test Automation with generative AI and Open AI.
UiPath Test Automation with generative AI and Open AI webinar offers an in-depth exploration of leveraging cutting-edge technologies for test automation within the UiPath platform. Attendees will delve into the integration of generative AI, a test automation solution, with Open AI advanced natural language processing capabilities.
Throughout the session, participants will discover how this synergy empowers testers to automate repetitive tasks, enhance testing accuracy, and expedite the software testing life cycle. Topics covered include the seamless integration process, practical use cases, and the benefits of harnessing AI-driven automation for UiPath testing initiatives. By attending this webinar, testers, and automation professionals can gain valuable insights into harnessing the power of AI to optimize their test automation workflows within the UiPath ecosystem, ultimately driving efficiency and quality in software development processes.
What will you get from this session?
1. Insights into integrating generative AI.
2. Understanding how this integration enhances test automation within the UiPath platform
3. Practical demonstrations
4. Exploration of real-world use cases illustrating the benefits of AI-driven test automation for UiPath
Topics covered:
What is generative AI
Test Automation with generative AI and Open AI.
UiPath integration with generative AI
Speaker:
Deepak Rai, Automation Practice Lead, Boundaryless Group and UiPath MVP
Fueling AI with Great Data with Airbyte WebinarZilliz
This talk will focus on how to collect data from a variety of sources, leveraging this data for RAG and other GenAI use cases, and finally charting your course to productionalization.
Your One-Stop Shop for Python Success: Top 10 US Python Development Providersakankshawande
Simplify your search for a reliable Python development partner! This list presents the top 10 trusted US providers offering comprehensive Python development services, ensuring your project's success from conception to completion.
TrustArc Webinar - 2024 Global Privacy SurveyTrustArc
How does your privacy program stack up against your peers? What challenges are privacy teams tackling and prioritizing in 2024?
In the fifth annual Global Privacy Benchmarks Survey, we asked over 1,800 global privacy professionals and business executives to share their perspectives on the current state of privacy inside and outside of their organizations. This year’s report focused on emerging areas of importance for privacy and compliance professionals, including considerations and implications of Artificial Intelligence (AI) technologies, building brand trust, and different approaches for achieving higher privacy competence scores.
See how organizational priorities and strategic approaches to data security and privacy are evolving around the globe.
This webinar will review:
- The top 10 privacy insights from the fifth annual Global Privacy Benchmarks Survey
- The top challenges for privacy leaders, practitioners, and organizations in 2024
- Key themes to consider in developing and maintaining your privacy program
OpenID AuthZEN Interop Read Out - AuthorizationDavid Brossard
During Identiverse 2024 and EIC 2024, members of the OpenID AuthZEN WG got together and demoed their authorization endpoints conforming to the AuthZEN API
1. Proyecto
timtrack
timtrack
timtrack
timtrack
timtrack
timtrack timtrack
A Tracking Algorithm for
timtrack TRASGOS
timtrack
timtrack
timtrack
timtrack
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
2. About the TRASGO concept
A TRASGO
(TRAck reconStructinG mOdule)
is a detector able to work stand-alone offering full capabilities of timing and
tracking of charged particles
DAQ Electronics
Network
Power supplies
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
3. About SAETAS
A SAETA (SmAllest sEt of daTA) is the basic unit of information
in the timtrack algorithm and in the TRASGOs concept
A SAETA contains 6 parameters defining a charged particle track
In a cartesian coordinate system:
- X0 and Y0: 2 coordinates at a reference plane
- X’ and Y’ : 2 projected slopes in planes x-z and y-z
- T0 : The time at the reference plane respect a reference time
- V : The velocity
Saeta: s = (X0,X’,Y0,Y’,T0,V)
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
4. About SAETAS
From the mathematical point of view will be better to use:
Saeta: s = (X0,X’,Y0,Y’,T0,1/Vz)
where:
V = Vz · Sqrt(1+X’2+Y’2)
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
5. L
x
z
Saeta
X’ V
X0 T0
Vz
z=0 Y’
Y0 y
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
6. About timtrack
TimTrack is the algorithm developed to estimate SAETAS
1. It is based on a Least Squares Method (LSM)
2. It works directly with the primary data provided by detectors:
- Coordinates:
- Times: it is assumed that:
all times are refered to a common t=0
(all detector are WELL synchronized)
3. It lets free the six elements of a saeta:
(X0, X’, Y0, Y’, T0 and 1/Vz)
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
7. About timtrack
1st. Step
- To define the model, giving the cuantities that are measured
as function of the parameters of the saeta
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
8. x Times
Example Strip-like detector
X-type plane
z
T T’
z=zi
z=0
y
0
0
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
9. x Times
X-type plane
z
T
V T’
X’
X0 T0
z=zi
Y’
z=0
Y0 y
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
10. x Times
X-type plane
T z
T’
X’
V
X0 T0
z=zi
Vz Y’
z=0
Y0 y
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
11. x Times
X-type plane
Ti z
T’i
V
X’
X0 T0
z=zi
Y’
z=0
Y0 y
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
12. x Coordinates
X-type plane
z
Xi V
X’
X0 T0
z=zi
Y’
z=0
Y0 y
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
13. x
Ti
Y-type plane
z
V
X’
X0 T0
z=zi
z=0
Y’ T’i
Y0 Yi y
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
14. About timtrack
1st. Step
- To define the model giving the cuantities to be measured as
function of the parameters of the saeta
Either
or
3 equations (conditions) per plane!
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
15. About timtrack
2nd. Step
- To build the function S to be minimized
x
V
X’ n planes
X0 T0
Y’
Y0 y
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
16. About timtrack
2nd. Step
- S is a sum over n planes:
K = X or Y
K = Y or X
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
17. About timtrack
2nd. Step
- The expansion of the S function is:
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
18. About timtrack
2nd. Step
- That can be written in a more compact way:
where:
Saeta
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
19. About timtrack
K (configuration Matrix): depend on the detector layout
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
20. About timtrack
a (vector of reduced data): depend on the data
(They are just weighted sums and differences of the measurements)
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
21. About timtrack
3rd. Step
- To apply to LSM method.
From:
leads to:
As K is definite positive, K has an inverse and:
This equation provides the saeta directly from the data
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
22. About timtrack
3rd. Step
- Set of solutions (is just the Cramer rule):
where:
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
23. About timtrack
Error analysis
- The error matrix is
- Incertitudes can be easily calculated from the K matrix elements
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
24. About timtrack
Comments
- The method can be easily extended when there are correlations
between some of the measurements (e.G.: time readouts)
- Only two planes of strip-like detectors are enough to provide
unambiguously the 6 parameters of a saeta
- The solution has a matrix form: It’s very easy and fast of
implementing on computers
-There are many detector layouts with a K matrix having the
same structure (see next examples)
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
25. About timtrack
Other strip-like detector layouts
(with the same K-matrix structure)
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
26. About timtrack
Strip-like detectors with any shape:
x x
XBack
(X,Y) vs2
vs1
ymin YBack y
y
XFront
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
28. About timtrack
Strip-like detectors with any shape:
where:
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
29. About timtrack
Pads or pixel detectors :
∆Yi
X
∆Xi
Xi
X0 z
zi
z=0
Y0 Yi Y
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
30. About timtrack
Pads or pixel detectors :
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
31. About timtrack
Pads or pixel detectors :
where:
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
32. About timtrack
Other strip-like detector layouts
(with different K-matrix structure)
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
33. About timtrack
Other strip-like detector layouts
(with different K-matrix structure)
L
x
Ki
z
’ V
z=0
y
New transverse coordinates defined by an angle φ:
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
34. About timtrack
Other strip-like detector layouts (with different K-matrix structure)
K x
XBack x
XB Ti’
K
(Xp,Yp) -vs sinφ vs
Kim
X
vs cosφ
Kip
φ
φ
YBack + YFront YF - YB
y Y y
Ki
XF
XFront Ti
K=0 K=0
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
35. About timtrack
Other strip-like detector layouts
(with different K-matrix structure)
Remember:
ci = cos ϕi
si = sin ϕi
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
36. About timtrack
Other strip-like detector layouts
(with different K-matrix structure)
Again:
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
37. About timtrack
Other strip-like detector layouts
(with different K-matrix structure)
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
38. About timtrack
Other strip-like detector layouts
(with different K-matrix structure)
The solution of is (Cramer rules):
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
39. About timtrack
Comments
- The “problem” of the method is that there is an inversion of a
matrix. Sometimes it may give problems (when the matrix is not well
conditioned) but there are a lot of numerical methods to do it
(And it has to be done only once)
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
40. About timtrack
A typical example
2 parallel scintillators
T’2
T’1
y
➱
vs1
➱
➱
vs2
(Yo,Y’,V,T0)
➱
z1 z2 z
L1 T
T1
L2 τ=
T2 vs
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
41. About timtrack
A typical example: 2 parallel scintillators: different properties
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
42. About timtrack
A typical example: 2 parallel scintillators: identical properties
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010
43. The END
Thanks!
Juan A. Garzón: 2nd. Workshop on the Trasgo Project. S. Compostela Feb. 5th-6th. 2010