Jan 15 – 17, 2024
Institute of Nuclear Physics PAN, Cracow Poland
Europe/Warsaw timezone

Session

The CREDO Collaboration Meeting

Jan 17, 2024, 9:30 AM
Institute of Nuclear Physics PAN, Cracow Poland

Institute of Nuclear Physics PAN, Cracow Poland

Conveners

The CREDO Collaboration Meeting: Science I

  • There are no conveners in this block

The CREDO Collaboration Meeting: Science II

  • There are no conveners in this block

The CREDO Collaboration Meeting: Guest Physics Talks

  • There are no conveners in this block

The CREDO Collaboration Meeting: Institutional members review / introduction

  • Piotr Homola (Institute of Nuclear Physics PAN)

The CREDO Collaboration Meeting: Task Leaders Reports

  • Piotr Homola (Institute of Nuclear Physics PAN)

The CREDO Collaboration Meeting: Organization Road Map - The CREDO Bylaws

  • Piotr Homola (Institute of Nuclear Physics PAN)

The CREDO Collaboration Meeting: Closing

  • Robert Kaminski (Insititute of Nuclear Physics PAN)
  • David Álvarez Castillo (Institute of Nuclear Physics PAS)

The CREDO Collaboration Meeting: Discussion

  • Piotr Homola (Institute of Nuclear Physics PAN)

Presentation materials

There are no materials yet.

  1. Oleksandr Sushchov (INP PAS)
    1/17/24, 9:30 AM

    Cosmic rays are anticipated to give rise to cascades of product particles during their journey through space, resulting from interactions with fields, radiation, and matter. These phenomena, collectively known as cosmic-ray ensembles (CRE), are expected to exhibit variations in shapes, sizes, and constituents. Comprehensive studies of CRE necessitate an alternative approach to cosmic ray...

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  2. Łukasz Bibrzycki (AGH University of Krakow)
    1/17/24, 9:50 AM

    The recent, ongoing as well as planned CREDO ML research activities will be discussed. So far CREDO ML focused on the analysis of individual cosmic ray events including the filtering of artifacts and hardware noise and attepmts to associate event shapes with particular particle types. In terms of ML methodologies these were supervised binary and multi-class problems, respectively. We also...

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  3. Simon Liebing (Institute of Theoretical Physics, TU Bergakademie Freiberg. Freiberg, Germany)
    1/17/24, 10:20 AM

    The author statistically evaluates the public data from the CREDO science project.[1]
    Starting from observations on the live website data, some effects will be investigated looking through the whole available data set.
    Especially I will focus on how long users and devices contribute.
    There an interesting divergence between live data and stored data is observed.
    Another effect which can be...

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  4. Noemi Zabari (Astroteq.ai & CREDO.science)
    1/17/24, 10:40 AM

    This research endeavors to forecast earthquakes with a magnitude of 6 or greater within a 1000 km radius from three cosmic ray stations, employing machine learning methodologies. Our approach incorporates a feature store library for streamlined data preparation, encompassing 360 hours of cosmic ray data and the time elapsed since the last earthquake. Utilizing a feature store library and a...

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  5. Antonio Napolitano (University of Napoli Parthenope, Italy)
    1/17/24, 11:30 AM

    Antonio Napolitano
    Department of Engineering
    University of Napoli “Parthenope”, Italy

    https://sites.google.com/site/antnapol
    antonio.napolitano@uniparthenope.it

    Presentation of the main research topic related to CREDO collaboration at the University of Napoli “Parthenope”, Italy:

    **Exploitation of Cyclostationarity and its Generalizations for Science Data...

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  6. Dr Piotr Homola (Institute of Nuclear Physics PAN)
    1/17/24, 12:00 PM

    I'll report on progress with understanding the physics of the cosmo-seismic correlations. The main observations associated with the effect point to the role of both solar magnetism and lunar gravitational forces, although the latter does not appear to have a tidal character. In addition we observe a clear appearance of the sidereal day periodicity in both cosmic ray and earthquake data. None...

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  7. Dr Aneta Wojnar (Universidad Complutense, Madrid, Spain)
    1/17/24, 2:30 PM

    I will briefly explore the connection between modified
    theories of gravity and models based on the generalized uncertainty
    principle. This connection enables the examination of gravity proposals
    through tabletop experiments. Using the Landau model of liquid helium as
    an illustrative example, we will delve into the details. Additionally, I
    will demonstrate the application of Earth seismic...

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  8. Mikhail Kovalyov
    1/17/24, 3:00 PM

    I'm going to explain why why earthquakes are affected by tidal forces and then showing how quakes correlate with UAPs, using recent paper https://www.nature.com/articles/s41598-023-49527-x. In the end, I would mention the 10.1-10.2 year lunar periodicity as a reference to the cosmo-seismic effect reported in https://doi.org/10.1016/j.jastp.2023.106068.

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  9. Eduardo de la Fuente Acosta (Departamento de Física, CUCEI, Universidad de Guadalajara, México)
    1/17/24, 3:40 PM

    PeVatrons are natural particle accelerators that can accelerate particles with energies of up to 1 PeV. Although the term PeVatron was coined by the High Energy Stereoscopic System (HESS) collaboration in 2016 through the analysis of the galactic center, its era began in 2021 thanks to the discovery of ultra-high energy gamma-ray sources by highly sensitive observatories such as the High...

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  10. José Manuel Vaquero (Universidad de Extremadura)
    1/17/24, 4:30 PM

    In this contribution, we present to the CREDO community the SpES (Space & Earth Sciences) research group of the University of Extremadura, which is a member of the CREDO consortium. This research group attempts to make significant advances in Earth sciences using a global perspective. Its main research areas are Solar-Terrestrial Physics, Climatology, Meteorology, and History and Teaching...

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  11. Ms Klaudia Tajthi
    1/17/24, 4:40 PM

    Presentation of Experyment Science Center in Gdynia. Since 2021 we are participating in citizen science collaborating with Institute of Oceanology Polish Academy of Science. I will tell about our experience in citizen science and about our plans connected with CREDO.

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  12. Robert Nowakowski (PTMA)
    1/17/24, 4:50 PM

    PTMA as an organization has been an official member of the CREDO consortium since September 2022. Members of the Society give lectures and demonstrations of detection stations during internal PTMA meetings, science picnics and festivals, astronomical events and sky observing.

    From 2023, the CREDO.science promotion is also carried out as part of the international space education project...

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  13. Dr Marcin Piekarczyk (AGH University of Krakow)
    1/17/24, 4:55 PM

    Presentation of AGH University of Krakow as an institutional member of the CREDO research collaboration. Discussing the role of the university, identifying the researchers involved in the collaboration, with particular emphasis on current and planned CREDO-related activities and future potential contributions to CREDO.

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  14. Prof. Tadeusz Wibig
    1/17/24, 5:00 PM

    We would like to give a brief overview of the idea behind the CREDO-Maze project realised at the University of Lodz and summarise its status today. For some time now, we have been testing and continuously improving the design of the detectors and their electronics, adding various components that may not be necessary for CREDO itself, but may be useful for other purposes, including education....

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  15. Prof. Robert Kaminski (Insititute of Nuclear Physics PAN)
    1/17/24, 5:15 PM
  16. David Álvarez Castillo (Institute of Nuclear Physics PAS), Dr Noemi Zabari
    1/17/24, 5:20 PM
  17. Marcin Piekarczyk (AGH University of Krakow)
    1/17/24, 5:25 PM
  18. Krystian Batyjewski
    1/17/24, 5:30 PM

    Are we one step away from tokenizing the CREDO detector?
    Will the creation of a micro-payment system using Blockchain technology
    and rewarding active CREDO app's users with CREDO tokens contribute
    to the popularization and significant increase in the power of the detector?

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  19. Dmitriy Beznosko (Bard College New Orleans)
    1/17/24, 5:35 PM

    The use of the AI can bolster the community involvement in the science that also carries the educational aspect of learning about the LLM and can include local high schools to produce the materials for the learning of the metal networks. Additional school involvement can be in the forms of hosting simple hardware solutions as additional data collection stations, some of that may start under...

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  20. 1/17/24, 5:40 PM

    We will discuss the first draft of the CREDO Bylaws which would be the first step on the CREDO Organizational Road Map: https://docs.google.com/document/d/1pLpV3cPLvRpgYXowGbJs7WAqzqCFFk5vc6avjx9Vu9g/edit?usp=sharing
    Feel free to comment & suggest edits also before and after the session.

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  21. Mr Marek Więckowski (Polish Society of Amateur Astronomers (PTMA))

    PTMA as an organization has been an official member of the CREDO consortium since September 2022. Members of the Society give lectures and demonstrations of detection stations during internal PTMA meetings, science picnics and festivals, astronomical events and sky observing.

    Go to contribution page
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