EEE article

EEE article

Also this year, the EEE Project is participating in the International Cosmic Day organized by DESY, which will be held on November 26, coinciding with the in-person meeting at the Centro Fermi for the schools involved in the EEE Project. Schools that cannot attend in person will be able to follow and participate in the event online. ICD is an opportunity for us to deepen our study of cosmic rays and exchange our experience with students from all over the world.

On this page, you will find the preliminary agenda and instructions for the analysis to be carried out.

In particular, we propose students to analyze data collected by some EEE telescopes and/or POLAR detectors installed in Ny Ålesund (Svalbard) during the period from April to May 2024, when the detectors observed a decrease in the muon rate caused by a spectacular Solar Flare (Forbush effect).

The data to be analyzed and the details for the analysis are provided below.


By November 19, the schools participating in the EEE Project can send the results of their studies to This email address is being protected from spambots. You need JavaScript enabled to view it. in the form of a presentation (.ppt or .pdf) and simultaneously a summary of their analysis on a single page according to the template you can find here (the template is not mandatory and can be modified, but the report must fit on an A4 page).

Preliminary agenda:

  • 10:00 AM Welcome to the Schools

  • 10:10 AM Seminar (Dr. A. Oliva, INFN Bologna)

  • 11:00 AM Schools' reports on data analysis

  • 11:50 AM Conclusion of the event

Proposed analysis, data and instructions:

On this occasion, we will have data acquired by the following detectors:
EEE telescopes running with the new eco-friendly gas mixture:

  • BOLO-02 (Bologna)

  • CAGL-01 (Cagliari)

  • LAQU-01 (L'Aquila)

  • VICE-01 (Vicenza)

POLAR detectors:

  • POLA-01 (Ny Ålesund)

  • POLA-02 (Bologna)

  • POLA-03 (Ny Ålesund)

  • POLA-04 (Ny Ålesund)

  1. The available data for all the detectors listed cover the time period from April 1, 2024 to May 15, 2024.
  2. The data is available in both CSV format (to be analyzed using Excel or similar software) and ROOT format (to be analyzed with ROOT).
  3. The proposed analysis can be done on one or more datasets.
  4. The provided instructions are to be considered as a starting point for the analysis and are based on using Excel (recommended choice).

The analysis concerns the study of the Forbush effect connected to the exceptional solar storm on May 10, which lit up the Italian skies with a fiery red glow (news Centro Fermi, SIF Prima Pagina)—a phenomenon observed both by POLAR detectors and some EEE telescopes operating with the new eco-friendly gas mixture.

  • Download the data (currently not available, for more information send an e-mail to This email address is being protected from spambots. You need JavaScript enabled to view it..

  • Use the instructions [download instructions] as a starting point for the analysis.

  • Once the analysis is complete, send the report as a .ppt file (max size 3 MB) to This email address is being protected from spambots. You need JavaScript enabled to view it. together with a one-page summary following the template found here (max size 2 MB).

For clarifications, please contact This email address is being protected from spambots. You need JavaScript enabled to view it..

Good work!

On November 22, 2022, the EEE Project will participate in the International Cosmic Day organized by link. As always, the ICD is an event that allows us to deepen the study of cosmic rays and to exchange our experience with that of students from all over the world. Also this year, students, teachers, and researchers will come together to study cosmic rays.

For this edition of the ICD, the EEE Project has prepared an online meeting during which, alongside presentations by researchers engaged in the study of cosmic rays, students will be able to present the results of their analyses. On this page, you will find the meeting agenda and details for joining. In particular, we encourage students to study the variation of cosmic ray flux as a function of the latitude where the measurement is taken.

The data to be analyzed and the instructions for the analysis are provided below.

By November 15, the EEE Project Schools that wish to participate can send the results of their studies to This email address is being protected from spambots. You need JavaScript enabled to view it. in the form of a presentation (ppt or pdf) and simultaneously a one-page summary of their analysis(the important thing is that the report fits on one A4 page).

Also this year, the best presentation will be awarded a Cosmic Box!!!

Agenda

10:00 AM – Welcome to the Schools
10:10 AM – Seminar to be decided
11:00 AM – Schools' reports on data analysis
11:30 AM – Cosmic ray flux vs. latitude
11:50 AM – Event conclusion

Connection instructions for the meeting:
To get more information about the event consult the Indico Agenda clicking this link

Proposed analysis, data, and instructions

On this occasion, we will use data recently acquired by the POLA-02 detector on board the Amerigo Vespucci. We will particularly try to study the variation of cosmic ray flux with latitude. We will have two sets of data acquired during two port stops, one in Ancona and one in Durres, as well as the entire dataset collected during the whole voyage.

 

IMG 7983

 

Available data:


The data are in .csv files that can be analyzed using Excel (recommended choice and basis for the provided instructions) or similar spreadsheet programs.

  • Download the data (compressed folder containing three .csv files).
  • Use the instructions (download instructions) as a starting point for the analysis.
  • Once the analysis is complete, please send the report as a .ppt file (maximum size 3 MB) to This email address is being protected from spambots. You need JavaScript enabled to view it. together with a one-page summary of the analysis according to the template found here (maximum report size 2 MB).

For clarifications, contact This email address is being protected from spambots. You need JavaScript enabled to view it..

Good work!!!

On November 10, 2021, the EEE Project will participate again in the International Cosmic Day organized by DESY. Once again, the ICD represents an opportunity for us to deepen the study of cosmic rays and to exchange our experience with that of students around the world.

The strict safety and COVID-19 contagion prevention rules will partially limit contacts and the physical sharing of experiences.

For the ICD 2021 edition, the EEE Project has prepared an online meeting during which, together with presentations by researchers engaged in the study of cosmic rays, students will be able to present the results of their analyses. On this page you will find the meeting agenda and connection details. In particular, we propose that students to use data sed acquired by POLA-01 detector on the Nanuq boat on the 30th of July 2018 to study the muon's rate depending on the zenital angle of incidence.

The data to be analyzed and the details for the analysis are provided below.

By November 3, the EEE Project Schools that intend to participate can send the results of their studies to This email address is being protected from spambots. You need JavaScript enabled to view it. in the form of a presentation (.ppt or .pdf) and at the same time a summary of their analysis on a single A4 page.

Agenda

10:00 AM Welcome to the Schools
10:10 AM Muonic tomografy of Etna vulcan (Dr. Giuseppe Gallo)
10:50 AM Schools' reports on data analysis
              Scacchi High School (Bari)
              Galvani High School (Bologna)

11:15 AM Welcome from the Outreach Cosmic Ray Activities (OCRA) - Bari
              Scacchi High School (Bari)

              IIS Staffa (Trinitapoli)

11:30 AM Cosmic ray flux vs. direction (Prof. Daniele de Gruttola, Dott.ssa Cristina Ripoli)


11:50 AM Conclusion of the event

 

 

Instructions for Connection to the meeting:

To correctly connect to the meeting and view the event timetable, connect to the Indico Agenda of the Fermi Center at this link.

Proposed analysis, data and instructions

On this occasion, we will use the data acquired by the POLA-01 detector on board the Nanuq on July 30, 2018; during that expedition, the boat ran aground and tilted in such a way that it was possible to study the muon rate as a function of the zenith angle of arrival. For a review of the POLA-01 detector, please refer to the following presentation.

Data available:

The data are in a .csv file type, so they can be analyzed using Excel (recommended choice and on which the provided instructions are based) or similar calculation programs. You will have three data sets available and can decide whether to analyze one or more.

  • Download the data (data currently unavailable, contact This email address is being protected from spambots. You need JavaScript enabled to view it.)
  • Use the instructions (download the instructions) as a starting point for the analysis.
  • Once the analysis is complete, send the report in the form of a .ppt file (maximum size 3 MB) to This email address is being protected from spambots. You need JavaScript enabled to view it.

For clarifications contact This email address is being protected from spambots. You need JavaScript enabled to view it.


Good work!!

On November 4, 2020, the EEE Project will participate again in the International Cosmic Day organized by DESY. Once again, the ICD represents an opportunity for us to deepen the study of cosmic rays and to exchange our experience with that of students around the world.

The strict safety and COVID-19 contagion prevention rules will partially limit contacts and the physical sharing of experiences.

For the ICD 2020 edition, the EEE Project has prepared an online meeting during which, together with presentations by researchers engaged in the study of cosmic rays, students will be able to present the results of their analyses. On this page you will find the meeting agenda and connection details. In particular, we propose that students study the seasonal modulation of the muon rate, using data acquired by the Polar family of detectors between July 2019 and July 2020.

In addition to data analysis activities, during the meeting there will be a presentation by Dr. Carmelo Pellegrino regarding the KM3Net experiment, an underwater network of detectors hunting for neutrinos, and an intervention by Dr. Francesco Noferini, relating to the observation with Polar detectors of the seasonal effect in the cosmic ray flux.

The data to be analyzed and the details for the analysis are provided below.

By November 2, the EEE Project Schools that intend to participate can send the results of their studies to This email address is being protected from spambots. You need JavaScript enabled to view it. in the form of a presentation (.ppt or .pdf) and at the same time a summary of their analysis on a single A4 page.

Agenda

3:00 PM Welcome to the Schools
3:10 PM The KM3NeT experiment (Dr. Carmelo Pellegrino)
3:50 PM Schools' reports on data analysis
              Staffa High School (Trinitapoli)
              Regina Margherita High School (Salerno)
              A. Volta High School (Reggio Calabria)
Other schools' analysis for consultation
              Scorza High School Cosenza, Galvani High School Bologna, Cavour High School                Rome, Pacioli High School Sant'Anastasia
4:30 PM The seasonal effect in the Cosmic Ray flux with Polar detectors (Dr. Francesco Noferini)
4:55 PM Conclusion of the event

 

 

Instructions for Connection to the meeting:

To correctly connect to the meeting and view the event timetable, connect to the Indico Agenda of the Fermi Center at this link.

Proposed analysis, data and instructions

On this occasion, we will use data acquired by the Polar detectors between July 2019 and July 2020 to study the trend of the muon rate and evaluate the possible "seasonal effect": the change in average atmospheric conditions implies a change in the measured flux.

Data available:

The data are in a .csv file type, so they can be analyzed using Excel (recommended choice and on which the provided instructions are based) or similar calculation programs. You will have three data sets available and can decide whether to analyze one or more.

  • Download the data (data currently unavailable, contact This email address is being protected from spambots. You need JavaScript enabled to view it.)
  • Use the instructions (download the instructions) as a starting point for the analysis.
  • Once the analysis is complete, send the report in the form of a .ppt file (maximum size 3 MB) to This email address is being protected from spambots. You need JavaScript enabled to view it.

For clarifications contact This email address is being protected from spambots. You need JavaScript enabled to view it.


Good work!!

Also this year, the EEE Project participates in the International Cosmic Day (ICD) organized by DESY, which will be held on November 26, together with the in-person meeting at the Centro Fermi of the EEE Project schools. Schools that cannot attend in person will be able to follow and participate in the event online. The ICD is an occasion that allows us to deepen the study of cosmic rays and to exchange our experience with that of students around the world.

On this page, you will find the preliminary agenda and the instructions for the analysis to be carried out.

In particular, we propose to the students an analysis of data acquired by some EEE telescopes and/or POLAR detectors installed in Ny Alesund (Svalbard) during the period from April to May 2024, when the detectors observed a decrease in the muon rate due to a spectacular Solar Flare (Forbush effect).

The data to be analyzed and the details for the analysis are provided below.


By November 19, the schools of the EEE Project can send the results of their studies to This email address is being protected from spambots. You need JavaScript enabled to view it. in the form of a presentation (.ppt or .pdf) and simultaneously a summary of their analysis on a single page according to the template found here (the template is not mandatory and can be changed; the important thing is that the report fits on one A4 page).

Preliminary Agenda

  • 10:00 Welcome to the Schools

  • 10:10 Seminar (Dr. A. Oliva, INFN Bologna)

  • 11:00 Schools' reports on data analysis

  • 11:50 Event conclusion

Proposed analysis, data, and instructions

For this occasion, we will have available data acquired by the following detectors:
EEE telescopes operating with the new eco-friendly gas mixture

  • BOLO-02 (Bologna)

  • CAGL-01 (Cagliari)

  • LAQU-01 (L'Aquila)

  • VICE-01 (Vicenza)

POLA-R detectors

  • POLA-01 (Ny Alesund)

  • POLA-02 (Bologna)

  • POLA-03 (Ny Alesund)

  • POLA-04 (Ny Alesund)

The data available for all the detectors listed above cover the period from April 1, 2024, to May 15, 2024.
The data are available both in csv format (analysis via Excel or similar tools) and in root format (analysis via ROOT).
The proposed analysis can be carried out on one or more data sets.
The instructions provided are to be considered the starting point of the analysis and are based on the use of Excel (recommended choice).

The analysis regards the study of the Forbush effect connected to the exceptional solar storm of May 10, which lit up the Italian skies with a fiery red phenomenon (see Centro Fermi newsSIF Prima Pagina) and was observed by both POLA-R detectors and some EEE telescopes operating with the new eco-friendly gas mixture.

  • Download the data: zip folder containing csv and root files for the detectors listed in the period April 1 to May 15, 2024.

  • Use the instructions (download instructions) as a starting point for the analysis.

  • Once the analysis is completed, send the report as a .ppt file (maximum size 3 MB) to This email address is being protected from spambots. You need JavaScript enabled to view it. together with the summary on a single page according to the template found here (maximum size 2 MB).

For clarifications, contact This email address is being protected from spambots. You need JavaScript enabled to view it.

Good work!!!

For information regarding participation in the Extreme Energy Events Project please send an email to:

 This email address is being protected from spambots. You need JavaScript enabled to view it.

or

This email address is being protected from spambots. You need JavaScript enabled to view it.

 

On November 21, 2023, the EEE Project participates in the International Cosmic Day organized by DESY. As always, the ICD represents an event that allows us to deepen the study of cosmic rays and to exchange our experience with that of students from all over the world. Also this year students, professors and researchers are coming together to study cosmic rays.
For this edition of the ICD the EEE Project has prepared an online meeting during which students will be able to present the results of their analyses. On this page you will find the preliminary agenda.

In particular we propose an analysis to study the coincidences between the POLAR detectors installed in Ny Alesund (Svalbard).

 

The data to be analyzed and the details for the analysis are provided below.

By November 10, the EEE Project Schools that intend to participate can send the results of their studies to This email address is being protected from spambots. You need JavaScript enabled to view it. in the form of a presentation (.ppt or .pdf) and at the same time a summary of their analysis on a single page according to the template that you find here (it is not mandatory to be used and can be changed, the important thing is that the report fits on A4).
This year too, the best presentation will be rewarded with a Cosmic Box!!!

 

Agenda

Ore 10:00 Welcome to the Schools

Ore 10:10 Seminar: L’universo che l’occhio non vede: Acceleratori cosmici di alta energia (Prof. P. Blasi)

Ore 11:00 Reports from the Schools

  1. Liceo Scacchi - Bari
  2. Liceo Banzi Bazoli - Lecce
  3. Liceo Galvani - Bologna
  4. Liceo Da Procida - Salerno
  5. Liceo Scorza - Cosenza

Ore 11:50 Conclusions 


Connection Instructions:

Link zoom: https://cern.zoom.us/j/67581280130?pwd=Qm1pSEFjNGtDSEpKMDFhblFYTlVpUT09

 

 

Proposed analysis, data and instructions

This year we are going to analyse the data collected by iPOLA-01 POLA-03 POLA-04 detectors at Ny Alesund (Svalbard).The data files contain the coincidences between POLA-01 and POLA-04 and POLA-04 e POLA-03. We will estimate the number of coincidences per day and also the variation of this number with the distance between the detectors distances.

The data

The data are in .csv format and you can use Excel or similar (our instructions are based on Excel).

- Download the data: .zip folder containing four .csv files, one relating to the coincidences between POLA-01 and POLA-04 and three relating to the coincidences between POLA-03 and POLA-04; NB: for easier data management with Excel, the coincidences between POLA-03 and POLA-04 have been divided into 3 .csv files and the information from the three files must therefore be merged for analysis (see instructions).

NB: Correct POLA-01 POLA-04 coincidence file

- Use the instructions (dowload instructions in italian) as starting point for the anlysis.

-Send theil report as .ppt file (max 3 MB) to This email address is being protected from spambots. You need JavaScript enabled to view it. together with the one page summary (template max 2 MB).

For further info contact This email address is being protected from spambots. You need JavaScript enabled to view it.

Good luck!!!

 

Il 21 novembre 2023 il Progetto EEE partecipa all’ International Cosmic Day organizzato da DESY. Come sempre l'ICD rappresenta un appuntamento che ci permette di approfondire lo studio dei raggi cosmici e di scambiare la nostra esperienza con quella degli studenti di tutto il mondo.
Per questa edizione dell’ICD il Progetto EEE ha preparato un meeting online durante il quale gli studenti potranno presentare i risultati delle loro analisi.

In questa pagina trovate l’agenda preliminare e le indicazione per l'analisi da svolgere.

In particolare proponiamo agli studenti di un'analisi sui dati dei rivelatori POLAR installati a Ny Alesund (Svalbard).

I dati da analizzare ed i dettagli per l’analisi sono forniti di seguito.

Entro il 10 novembre le Scuole del Progetto EEE possono inviare i risultati dei loro studi a This email address is being protected from spambots. You need JavaScript enabled to view it. in forma di presentazione (.ppt o .pdf) e contestualmente un riassunto della loro analisi in un’unica pagina secondo il template che trovate qui (non è da usare obbligatoriamente e si può cambiare, l’importante è che il report stia in un A4).
Anche quest’anno  la presentazione migliore sarà premiata con una Cosmic Box !!!

Agenda

Ore 10:00 Benvenuto alle Scuole

Ore 10:10  L’universo che l’occhio non vede: Acceleratori cosmici di alta energia (Prof. P. Blasi)

Ore 11:00 Report delle scuole sull’analisi Dati

  1. Liceo Scacchi - Bari
  2. Liceo Banzi Bazoli - Lecce
  3. Liceo Galvani - Bologna
  4. Liceo Da Procida - Salerno
  5. Liceo Scorza - Cosenza

Ore 11:50 Conclusione dell’evento

Istruzioni per la Connessione al meeting:

Link zoom: https://cern.zoom.us/j/67581280130?pwd=Qm1pSEFjNGtDSEpKMDFhblFYTlVpUT09


Analisi proposta, dati e istruzioni

In questa occasione useremo i dati acquisitidai rivelatori POLA-01 POLA-03 POLA-04 installati presso la staizone scientifica internazionale di Ny Alesund (Isole Svalbard). Avremo a disposizioni due file dati che contengono rispettivamente le coincidenze tra i rivelatori POLA-01 e POLA-04 e POLA-04 e POLA-03; l'analisi consiste nel valutare il numero di coincidenze al giorno e nello stimare la variazione di tale numero con la distanza dei rivelatori

I dati a disposizione:

I dati sono  in due file di tipo .csv (quindi analizzabili utilizzando Excel scelta consigliata e sulla quale si basano le istruzioni fornite o programmi di calcolo simili) e contenuti in una cartella compress.

- Scaricare i dati: cartella .zip contenente quattro file .csv uno relativo alle coincidenze tra POLA-01 e POLA-04 e tre relativi alle coincidenze tra POLA-03 e POLA-04; NB: per una più semplice gestione dei dati con Excel le coincidenze tra POLA-03 e POLA-04 sono state divise in 3 file .csv e vanno quindi unite le informazioni dei tre file per l'analisi (vedere le istruzioni).

NB: File corretto coincidenze POLA-01 POLA-04

- Utilizzare le istruzioni (scarica le istruzioni) come punto di partenza per l’analisi.

- Una volta completata l’analisi inviare il report in forma di file .ppt (dimensione massima 3 MB) a This email address is being protected from spambots. You need JavaScript enabled to view it. unitamente al riassunto in un’unica pagina secondo il template che trovate qui (dimensione massima del report 2 MB).

Per chiarimenti contattare This email address is being protected from spambots. You need JavaScript enabled to view it.

Buon Lavoro!!!

2025

Conferenza/Evento Sito Conferenza Tipologia Contributo Speaker   Titolo    
Link Contributo
Incontri di Fisica delle Alte Energie (IFAE 2025), Cagliari (Italia), 9-11 Aprile Link Poster C.Ripoli

Osservazione della variazione Forbush nel flusso dei cosmici per mezzo della rete dei telescopi del progetto Extreme Energy Event

 
European Geoscience Union (EGU) Conference, Vienna, 27 Aprile- 2 Maggio   Link Talk M.Schroen      
High latitude muon and neutron observation of the Forbush decrease during the May 2024 solar storms
 
European Geoscience Union (EGU) Conference, Vienna, 27 Aprile- 2 Maggio Link Talk O.Pinazza
Observation of the Forbush decrease during the May 2024 solar storms with different muon and neutron detectors in 
the high-latitude site of the Svalbard archipelago
 
26th International Workshop on Radiation Imaging Detectors, Bratislava, 6-10 Luglio   Link Poster C.Ripoli
Cosmic ray measurements with compact scintillator telescopes and SiPM readout
 

 

 

International Cosmic Ray Conference (ICRC), Ginevra, 15-24 Luglio  Link Poster O.Pinazza
High latitude muon and neutron observation of the Forbush decrease during the May 2024 solar storms
 
International Cosmic Ray Conference (ICRC), Ginevra, 15-24 Luglio Link Poster P.La Rocca Measurement campaigns of the cosmic ray flux at different latitudes within the Extreme Energy Events Project  
International Cosmic Ray Conference (ICRC), Ginevra, 15-24 Luglio Link Talk F.Nozzoli      
Characterization of the Piedicastello Tunnels as a Potential Underground Laboratory for Astroparticle Physics in Trento, Italy
 
International Cosmic Ray Conference (ICRC), Ginevra, 15-24 Luglio Link Poster L.Ghezzer      
Analysis of annual periodicities in the muon rate measured by the EEE detectors installed at the high-latitude site of Ny-Ȧlesund
 

11th Congresso SIF, Palermo, 22-26 Settembre  

Link Talk C.Ripoli      
Osservazione dell'evento Forbush di Maggio 2024 con i rivelatori a Ny-Alesund e con la rete di telescopi MRPC
 

 

2024

Conference/Event Conference site Contribution Tyoe Speaker   Title    
Link
13th CRIS-MAC 2024
Cosmic-Ray International Studies and Multi-messenger Astroparticle Conferenc, , 13-21 Giugno
Link Talk O.Pinazza Annual quasiperiodicity in muon rate observed by PolarQuEEEst detectors at 79 N  
13th CRIS-MAC 2024
Cosmic-Ray International Studies and Multi-messenger Astroparticle Conferenc, , 13-21 Giugno
Link Poster C. Ripoli Recent outreach activities of the EEE Project  
110° Congresso Nazionale SIF, Bologna (Italia), Settembre 9 – 13 Link Talk P. La Rocca Partecipazione del Progetto EEE all’International Cosmic Day  
110° Congresso Nazionale SIF, Bologna (Italia), Settembre 9 – 13 LinkLink Talk L.Ghezzer Studio delle variazioni stagionali e pluriennali del flusso dei muoni atmosferici  
110° Congresso Nazionale SIF, Bologna (Italia), Settembre 9 – 13 Link Talk C. Ripoli Measurement of the detection efficiency for cosmic muons of a MRPC detector  
110° Congresso Nazionale SIF, Bologna (Italia), Settembre 9 – 13 Link Talk O. Pinazza Il Progetto Extreme Energy Events espande le sue frontiere  

2023

Conference/Event Conference site Contribution Tyoe
Speaker   Title    
Link
38th International Cosmic Ray Conference (ICRC2023), Nogoya (Japan), July 26 -August  3 Link Talk F. Noferini Recent results from the PolarquEEEst measurement campaign at large geographical latitudes  
24th international Workshop on Radiation Imaging Detectors, Oslo (Norway), June 25-29 Link Poster C. Ripoli Ecological transition for the gas mixtures of the MRPC cosmic ray telescopes of the EEE project  
XVIII International Conference on Topics in Astroparticle and Underground Physics 2023, Wien (Austria), August 28  - September 1 Link Talk C. Ripoli Involving high school teams in the upgrade phase of the Extreme Energy Event project: a review of recent activities  pdf
109° Congresso Nazionale SIF, Salerno (Italy), Septempber 11 – 25 Link Talk C. Ripoli Eco gas mixtures for the MRPC cosmic ray telescopes of the EEE project  Abstract

 

2022

Conference/Event  Site Period Website
Contributio Type Speaker  Contribution Link
66th INFN ELOISATRON WORKSHOP: New gas mixtures for RPC and MRPC detectors  Erice November 20–23 https://agenda.infn.it/event/30846/ Invited Talk Daniele De Gruttola  pdf
66th INFN ELOISATRON WORKSHOP: New gas mixtures for RPC and MRPC detectors Erice November 20–23 https://agenda.infn.it/event/30846/ Invited Talk Cristina Ripoli  pdf
5th Annual International Conference on Education Siviglia Novembre 9–9 https://iated.org/iceri/announcement Talk Silvia Pisano Abstract
RPC 2022  CERN September 26–30  https://indico.cern.ch/event/1123140/ Invited Talk Marcello Abbrescia  pdf
Congresso Nazionale SIF Milano

September12–16

 https://2022.congresso.sif.it/ Talk Maria Paola Panetta Abstract pdf
ICHEP 2022 Bologna

July 6–13

 https://www.ichep2022.it/  Talk Marco Garbibni  pdf
15th Pisa Meeting La Biodola, Isola D'Elba

May 22 – 28

https://www.pi.infn.it/pm/ Poster Edoardo Bossini  pdf
15th Pisa Meeting La Biodola, Isola D'Elba May 22 – 28 https://www.pi.infn.it/pm/ Poster Stefano Grazzi pdf
April Meeting of the American Physical Society New York  April 9 – 12 https://meetings.aps.org/Meeting/APR22/Content/4194 Talk su Invito Luisa Cifarelli Abstract

 

 

Schools with EEE telescope:

CITY; SCHOOL
Altamura (BA) Liceo Cagnazzi
Ancona Liceo Classico C. Rinaldini
Arezzo ITIS G. Galilei
Bari Liceo Scientifico A. Scacchi
Bitetto (BA)  (installation to be completed) Liceo Scientifico E. Amaldi
Bologna Liceo Scientifico E. Fermi
Liceo Classico L. Galvani
Cagliari Liceo Scientifico L.B. Alberti
Liceo Scientifico Michelangelo
Liceo Classico e Scientifico Euclide
Catanzaro IIS E. Fermi
Carcare (SV)  (installation to be completed) Liceo Statale San Giuseppe Calasanzio
Cariati (CS) Liceo Scientifico Stefano Patrizi
Cosenza Liceo Scientifico G.B. Scorza
Frascati (RM) Istituto Tecnico E. Fermi
Istituto Salesiano Villa Sora
Grosseto Rete Scuole della Cittadella dello Studente - IIS A.Manetti 
Grottaferrata (RM) Liceo Scientifico B. Touschek
Lampedusa (AG) (installation to be completed) Istituto Omnicomprensivo Luigi Pirandello
L'Aquila Liceo Scientifico A. Bafile
ITIS A. D'Aosta
Lecce Liceo Scientifico G.Banzi Bazoli
Liceo Classico Palmieri
Lodi Liceo Scientifico G. Gandini
IIS Volta
Parma Liceo Scientifico G. Marconi
Paternò (CT) Liceo Scientifico E. Fermi
Quartu Sant'Elena (CA) IISS Primo Levi
Reggio Calabria Liceo Scientifico A.Volta
Reggio Emilia IIS L. Nobili
Roma ITIS H. Hertz (sede IIS Enzo Ferrari)
Liceo Classico P. Albertelli
Salerno Liceo Scientifico G. Da Procida
Liceo Statale Regina Margherita
Savona Liceo Chiabrera - Martini
Siena IIS Sarrocchi
Liceo Scientifico Galilei
Teramo IIS Alessandrini - Marino - Forti
Torino Liceo Scientifico G. Ferraris
Trapani Liceo Scientifico V.Fardella
Treviso Liceo Duca degli Abruzzi
Trinitapoli (BAT) IISS M. Dell'Aquila-S. Staffa
Viareggio (LU) IIS Galilei - Artiglio
Liceo Scientifico Barsanti e Matteucci
Vicenza (ITIS Rossi installation to be completed) Liceo Scientifico Quadri
ITIS Alessandro Rossi

 

  

Schools (without telescope) partecipating in EEE project:

CITY; SCHOOL
Altamura (BA) Liceo Scientifico Federico II di Svevia
Ancona Liceo Scientifico Galilei
Avellino Liceo Scientifico P.S. Mancini
Bagheria IIS D'Alessandro
Bari IIS Gorjuk-Tridente-Vivante
ITT Panetti Pitagora
Bitetto (BA) Liceo Statale E.Amaldi
Bolzano Liceo Scientifico E. Torricelli
Caltanissetta Liceo Scientifico Volta
Ciampino Liceo Scientifico Statale Vito Volterra
Cinisello Balsamo (MI) IIS Giulio Casiraghi
Fabriano (AN) Liceo Scientifico Vito Volterra
Gardone V.T. (BS) IIS Carlo Beretta
Giaveno (TO) IISS Blaise Pascal
Iseo (BS) IIS Giacomo Antonietti
Milano Liceo Scientifico Vittorio Veneto
Montesilvano (PE) Liceo Scientifico Statale C. D'Ascanio
Passo Corese-Frazione di Fara in Sabina (Ri) Liceo Scientifico Rocci
Piacenza Liceo Scientifico Lorenzo Respighi
Pisa Liceo Statale Filippo Buonarroti
Pomezia (RM) IIS Blaise Pascal
Pontedera (PI) ITIS G. Marconi
Reggio Emilia IIS B. Pascal
Roma Liceo Scientifico Cavour
Liceo Vittoria Colonna
Liceo Scientifico Righi
IIS Charles Darwin
Sant'Anastasia (NA)
IISS Luca Pacioli
Senigallia (AN) Liceo Statale Enrico Medi
Trento Liceo Scientifico Leonardo da Vinci 
Verona IIS Copernico-Pasoli 
Vicenza Itis Rossi 
Villafranca di Verona IIS Carlo Anti 

 

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