Introduction Room: 6/2-024 - BE Auditorium Meyrin Ruben Garcia Alia, Paul Leroux and Sonia Allegretti will give the welcome to the RADSAGA Initial Workshop

Communicating to general public Room: 6/2-024 - BE Auditorium Meyrin Speaker: Dominique Bertola (CERN Visitors and Local Engagement) D. Bertola has worked as IT specialist in data acquisition systems for CERN experiments. He joined in 1992 the outreach and communication group to make the first permanent exhibition of CERN. Nowadays he works for the CERN Visits Service where he leads the CERN guides training. The course objectives: o Understanding communicating basics o Speaking to a general public o Developing self-knowledge o Learn to know the others and their role in RADSAGA Consortium RESTRICTED TO RADSAGA ESRs

Communicating to general public workshop- Role playing session Room: 6/2-024 - BE Auditorium Meyrin Speaker: D. Bertola (CERN Visitors and Local Engagement) Course objectives: o Learn to manage difficult situations o Learn to know the others and their role in RADSAGA Consortium. RESTRICTED TO RADSAGA ESRs

Social Media Workshop Room: 6/2-024 - BE Auditorium Meyrin Speaker: Julie Haffner (CERN social Media) After her studies in communications and public relations, Julie started working in the CERN Press Office in 2012 and in 2016 she joined the CERN Social Media Team. Nowadays, as CERN social media manager, Julie works closely with writers and the audiovisual production team to produce content to engage CERN’s social media audiences. Abstract We are living in a connected age, and this is providing us with new opportunities and ways to do outreach. In this presentation, we will show you how social media can be a useful tool for you to share your knowledge and passion about science. We will showcase a few best practices and case studies, and get you thinking about ways to use social media to act as ambassadors for science, do outreach and build connections.

Building Interactive Applications for Science Communication Room: 6/2-024 - BE Auditorium Meyrin Speaker: Joao Pequenao (CERN Media lab) Interactive applications are a powerful way to engage audiences and accelerate the learning of specific topics. They can be used in Science Centres, Classrooms and Special Events to complement more traditional Outreach techniques. At CERN we conceive interactive installations which explore the educational possibilities of this approach. In this presentation we will have a peek into the principles, the technology developed, the projects, the context and scope, and hint about what will come in the future.

Communicating with the media: Why and How? Room: 6/2-024 - BE Auditorium Meyrin RESTRICTED TO RADSAGA ESRs Speaker: Ana Godinho (CERN Communication Group) and Arnaud Marsollier (CERN Press Release office) Topics to be addressed: - What is news? - How does the media work? - The scientific paper versus the news story - How to write a press release

Visit to CERN Synchrocyclotron (SC) Room: 6/2-024 - BE Auditorium Meyrin The 600 MeV Synchrocyclotron (SC), built in 1957, was CERN’s first accelerator. It provided beams for CERN’s first experiments in particle and nuclear physics. In 1964, this machine started to concentrate on nuclear physics alone, leaving particle physics to the newer and much more powerful Proton Synchrotron (PS). The SC became a remarkably long-lived machine. In 1967, it started supplying beams for a dedicated unstable-ion facility called ISOLDE, which carries out research ranging from pure nuclear physics to astrophysics and medical physics. In 1990, ISOLDE was transferred to a different accelerator, and the SC closed down after 33 years of service.

Social dinner RESTRICTED TO RADSAGA ESRs Venue: Restaurant 1

Introduction to Knowledge Transfer, IP and Information databases

• Giovanni Anelli (CERN)

Room: 6/2-024 - BE Auditorium Meyrin Speakers: Myriam Ayass, Amy Bilton and Giovanni Anelli from the CERN Knowledge Transfer Group. Professional and academic skills of Amy, Myriam and Giovanni are resumed in the KT Team presentation (https://kt.cern/team/). Each ESR to come up with 2 - 3 topics in which they are interested. This has to be as specific as possible, preferably directly linked to the topic of their research project. Each attendee is requested to come to the course with his/her own laptop with internet access enabled. This is essential since part of the training will be through hands-on exercises.

Fundamentals of IP & patents

• Myriam Ayass (CERN)

Room: 6/2-024 - BE Auditorium Meyrin

Patent application procedure (and costs)

• Amy Bilton (CERN)

Room: 6/2-024 - BE Auditorium Meyrin

Anatomy of a patent vs Scientific publication anatomy

• Amy Bilton (CERN)

Room: 6/2-024 - BE Auditorium Meyrin

Walk through with whole group using one ESR's example

• Amy Bilton (CERN)

Room: 6/2-024 - BE Auditorium Meyrin

Practice: Using public patent information databases.

• Amy Bilton (CERN)

Room: 6/2-024 - BE Auditorium Meyrin

Patent classification & Data Analysis on patent information and Technology landscapes

• Amy Bilton (CERN)

Room: 6/2-024 - BE Auditorium Meyrin

Wrap up, Q & A

• Amy Bilton (CERN)
• Myriam Ayass (CERN)

Room: 6/2-024 - BE Auditorium Meyrin

Introduction Room: 6/2-024 - BE Auditorium Meyrin Ruben Garcia and P. Leroux

Guidelines and standards for micro-electronic component reliability Room: 6/2-024 - BE Auditorium Meyrin Speakers: Pipponzi Mauro ‎and Petrucci Stefano (INTEL inc.) Mauro Pipponzi graduated in Electronic Engineering at Politecnico di Milano, over the years held a number of positions in engineering and engineering management in both EDA and ASIC/SoC Design . Today he is the responsible for Functional Safety methodology and automation strategy in Intel. Previously functional safety automation manager, responsible for managing the development of the functional safety automation tool suite. Stefano Petrucci is responsible for Functional Safety methodology and automation execution in Intel. Previously CERN account manager for CAEN company for 18 years, responsible to support CAEN Power Supply system and readout electronic in LHC Experiments CMS, ATLAS, Alice and Lhcb. Graduated in Electronic Engineering at Università di Pisa. Fellowship at CERN in Atlas on associative memory system in 2014 The presentation will cover the main topics of functional safety with particular regards to standard developed for the automotive and industrial markets. We will cover the different factor affecting safety, including the reliability of the underlying technology fabric, the design implementation and the application. Techniques to analyze and mitigate the causes of failures will be presented as well as the most common tools used in this process.

Guidelines and standards for micro-electronic component reliability - Part 2 Room: 6/2-024 - BE Auditorium Meyrin Speakers: Pipponzi Mauro ‎and Petrucci Stefano (INTEL inc.)

Introduction to Radiation Protection Room: 6/2-024 - BE Auditorium Meyrin Pierre Carbonez (CERN) Course Content • Introduction, Installations at CERN • Radioactivity and radiation, radiation types • Activation and stray radiation • Biological effects of ionizing radiation, understanding dose rate values compared to natural and medical radiation • Radiation protection principles, methods, and legislation • Measurements, external exposure • Contamination

Coffee Break and CERN Laboratory Visit VESPER and CHAM facilities

ESRs Individual Presentation Room: 6/2-024 - BE Auditorium Meyrin Each RADSAGA ESR will have a short presentation resuming the progress and outlook his/her work. ESRs that have just joined the RADSAGA ITN will present their background and a prospective view of their role and activities in the RADSAGA collaboration.

Radiation Test Standards for Space - part 1 Room: 6/2-024 - BE Auditorium Meyrin Francoise Bezerra (CNES) Course description First of all, we will start by an overview of the effects that can be induced in electronic components by radiation. For each effect, we will introduce how to characterize it and define the applicable terms and units. Then, applicable test methods and standards will be presented and compared and we will conclude our theoretical approach of radiation tests by standard radiation test plan examples. In a second time, back to “real-life”: Examples of radiation facilities used by CNES to perform radiation characterization of electronic devices will be presented. We will introduce the fact that many details may either complicate the test preparation or interfere with its execution and the final data analysis.

Radiation Test Standards for Space - Part 2 Room: 6/2-024 - BE Auditorium Meyrin Francoise Bezerra (CNES) Course description: The second part of this course, will start by a short exam (QMC) followed by its correction illustrated by real situations. This will give a chance to open discussion with Q/A.

Panel Discussion on "Qualification challenges for emerging technologies and effects, novel applications and system-level testing" Room: 6/2-024 - BE Auditorium Meyrin Participants from Industry and Academia

CERN Laboratory Visit Room: 6/2-024 - BE Auditorium Meyrin Visit to North Area and SM18

Industrial Experience in Radiation Engineering - Part1 Room: 6/2-024 - BE Auditorium Meyrin Speaker: Aminata CARVALHO, Radiation Engineer, Airbus Defence & Space

Space Weather and the variable radiation environment in space Room: 6/2-024 - BE Auditorium Meyrin Speaker: Dr. Gerhard Drolshagen, Space Environment Studies, Carl von Ossietzky University Oldenburg The radiation environment in space is not constant but shows variations on different time scales. The trapped radiation belts, the flux of cosmic rays and the normal solar wind are always present and relatively stable over periods of years or longer. Protons can have lifetimes in the trapped radiation belt exceeding 10s of years. These components of the radiation form a sort of ´radiation climate´. But even these types of radiation vary: the solar wind can become more energetic at certain times, electrons in the van Allen belt have typical lifetimes of only days to weeks before they are lost and replaced by new electrons. The populations and positions of the trapped radiation belts can vary and even the formation of temporary extra belts was observed. In addition, there is a secular change of the Earth magnetic field which is weakening by several percent over some decades and which effects the trapped radiation belts. Cosmic ray fluxes are modulated by the solar cycle. A higher solar activity leads to more magnetic shielding and reduced cosmic ray fluxes. On shorter time scales of days to hours there is even more variation in radiation components. These ´Space Weather´ effects include flares of energetic electromagnetic radiation (x-ray flares) and solar outbursts of energetic particles, mainly protons, at energies of 100s of MeV. The most energetic particles from such solar events can reach Earth within hours. Coronal mass ejections of energetic plasma take typically a few days to reach Earth. The plasma disturbs the geomagnetic field of Earth and can have a large range of effects from modifications of the radiation belts, interference with radio communication and navigation signals to the induction of ground currents. This lecture will address the variability of the space radiation environment near Earth and its connection with the so-called Space Weather.

Industrial Experience in Radiation Engineering - Part 2 Room: 6/2-024 - BE Auditorium Meyrin Speaker: Aminata CARVALHO, Radiation Engineer, Airbus Defence & Space

Guidelines in preparation for RADSAGA Mid -Term- Review Meeting Room: 6/2-024 - BE Auditorium Meyrin RADSAGA ESRs ONLY

CROC Competition- Ideas Selection over a coffee Room: 6/2-024 - BE Auditorium Meyrin RADSAGA ESRs ONLY The ESRs or Teams will present their idea (5 min presentation) A special prize will be assigned by the Jury to the most creative "CROC".

Closing of the workshop Room: 6/2-024 - BE Auditorium Meyrin P. Leroux and R. Garcia Alia