TEC-EPS Final Presentation Days - June 2021

16 Jun 2021, 09:00 → 17 Jun 2021, 17:00 Europe/Amsterdam

Online

The TEC-EPS Final Presentation Days, organised by ESA's Space Environments and Effects section, will take place on June 16 and 17, 2021 virtually. The two days will cover recent results from ESA's Space Environment R&D activities on space environment monitor developments and space environment modelling, analysis and simulation tools.

 

For more information on the activities of TEC-EPS, please visit the section website at http://space-env.esa.int/

Wednesday, 16 June

09:30 → 09:45 Welcome Talk

09:45 → 10:45 Modelling of the Electrostatic Environment of Ions Emitting Spacecraft (SPIS-ASPOC)

10:45 → 11:00 Coffee Break

11:00 → 12:00 Development and validation of a contamination package in SPIS for liquid based electric propulsion subsystems for LISA (SPIS-LISA)

12:00 → 13:00 Lunch Break

13:00 → 14:00 ROSSINI 3

14:00 → 14:30 Open Discussion

14:30 → 15:30 ATHENA Radiation Environment Models and X-ray Background Effects Simulators (AREMBES)

Speaker: Claudio Macculi (Istituto Nazionale Di Astrofisica (INAF))

Thursday, 17 June

09:30 → 09:35 Refresher Welcome Talk

09:35 → 10:35 Solar Particle Radiation Advanced Warning System (SAWS) - ASPECS (Advanced Solar Particle Events Casting System)

Speakers: Dr Anastasios Anastasiadis (National Observatory of Athens: Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing), Athanasios Papaioannou

10:35 → 10:55 SpacePix2 / SXRM Miniaturized Spacepix radiation monitor

10:55 → 11:10 Coffee Break

11:10 → 11:30 RadMag D3S: Radiation monitor development for ESA’s D3S hosted payload missions

11:30 → 11:50 DPE: Data Processing Engine

11:50 → 12:15 MIRAM Miniaturised Radiation Monitor

12:15 → 12:45 ARTES EOR Radiation Environment and Solar Array Degradation

Speakers: Athina Varotsou (TRAD) & Angélica Sicard (ONERA)
In the frame of this ARTES Project a new proton radiation environment model has been developed and a Solar Array Degradation Calculator (SADC) is being developed to allow for more precise calculation of solar array degradation specific to EOR orbits. During this presentation both developments will be presented with a special emphasis on the proton model developed by ONERA. This model is a global statistical model dedicated to EOR orbit environment specification. OMEP-EOR (ONERA Middle Energy Proton) provides the proton fluxes everywhere in the radiation belts between 30keV and 20MeV. The temporal dynamics of the radiation belt is accounted for at the scale of EOR missions, using a Gaussian Process model.

12:45 → 13:45 Lunch Break

13:45 → 14:15 MIRAD – Micro-Particle Impact Related Attitude Disturbance

Speaker: Patrik Kärräng (Hyperschall Technologie Göttingen)

14:15 → 15:00 Micrometeoroid Risk Assessment Tool for Missions Leaving Earth Orbits

Speaker: Jens Rodman (Etamax Space GmbH)

15:00 → 15:15 Focussing of Micrometeoroids in xray optics

Speaker: Yanwei Li (University of Stuttgart)

15:15 → 15:30 Open Discussion

15:30 → 15:40 Conclude and Thanks