467 results found Selected 0 items No itemsClear selection Select / deselect all results (all pages, 467 total) Estimation of proton induced single event rate in very deep submicron technologies More and more space applications and missions are considering the use of deep submicron technologies. Digital CMOS technologies below 65nm are sensitive to proton induced Single Event Effects (SEE) by direct ionisation mechanism. The consequence is a significant increase of SEE rates in flight (up to several orders of magnitude). This effect will be the dominant cause of SEE in orbit for these technologies. This poses a very significant challenge to SEE mitigation methods used in spacecraft electronics. France TDE T723-605QE ALTER TECHNOLOGY TUV NORD FRANCE SAS 2020 - 2023 Estimation of proton induced single event rate in very deep submicron technologies Estimation of proton induced single event rate in very deep submicron technologies More and more space applications and missions are considering the use of deep submicron technologies. Digital CMOS technologies below 65nm are sensitive to proton induced Single Event Effects (SEE) by direct ionisation mechanism. The consequence is a significant increase of SEE rates in flight (up to several orders of magnitude). This effect will be the dominant cause of SEE in orbit for these technologies. This poses a very significant challenge to SEE mitigation methods used in spacecraft electronics. France TDE T723-605QE IROC TECHNOLOGIES SA 2020 - 2023 Estimation of proton induced single event rate in very deep submicron technologies Materials Selection for Surface EVA Suit development This work begins the material selection process for EVA suits based on initial inputs from the EAC team that is developing an ergonomic prototype space suit. France TDE T324-504QT COMEX 2018 - 2023 Materials Selection for Surface EVA Suit development Dust removal and cleaning of optical surfaces and seals in lunar environments The lunar environment has a challenging dust environment. The dust is highly abrasive and therefore can cause considerable damage in short time. For astronauts, the dust effects range from highly irritating to toxic. Many sample processing and sample analysis systems need reliable seals; spaceflight hardware must work reliably in the presence of dust. France TDE T314-602MM COMAT 2020 - 2023 Dust removal and cleaning of optical surfaces and seals in lunar environments Test methodology investigations and parameters influencing Passive InterModulation (PIM) interference Passive intermodulation is a real threat to all types of payloads. In some cases, it could even lead to total lost of the spaceship. Despite of this, there is very weak understanding of the parameters that generate this unwanted interference as well as their influence in the amplitude of the interfering signal. In addition, there is a total lack of agreed testing techniques, procedures and methodologies as well as justified test margins, as has already been recently stated by the European community (National Delegations, satellite operators and Eurospace). Germany TDE T706-502ET Airbus Defence and Space GmbH 2018 - 2023 Test methodology investigations and parameters influencing Passive InterModulation (PIM) interference GaN based PCDU for EO missions based on recurrent platforms Gan technology for power applications is becoming mature these days. Gan switches can operate at higher frequencies and with the same level of efficiency as Si ones, with overall mass and volume PCDU benefits. Belgium TDE T103-601EP THALES ALENIA SPACE BELGIUM 2019 - 2023 GaN based PCDU for EO missions based on recurrent platforms Characterization of MLI materials and definition of MLI blanket for aerobraking environment Aerobraking phase of ENVISION is critical in terms of duration and required operations. One limitation during aerobraking is the temperature reached on Multi Layer Insulation (MLI) due to the aerothermal heat flux.MLIs can withstand during short durations (intermittent exposure) higher temperatures than their steady state qualification temperature. Austria TDE T221-021MT RUAG SPACE GMBH 2021 - 2023 Characterization of MLI materials and definition of MLI blanket for aerobraking environment Fundamental techniques, models and algorithms for a Lunar Radio Navigation system The interest of having in the near future an available Position, Navigation and Timing (PNT) service supporting future missions to and at the Moon is currently supported by both institutional and commercial initiatives. On the commercial side, multiple companies are developing business solutions targeting the Moon and several major European companies are proposing to team up to build a communications network on the Moon compatible to terrestrial standards. In parallel, NASA has recently announced its plans to a ?Return to the moon? Italy TDE T606-701ES THALES ALENIA SPACE ITALIA SPA 2021 - 2023 Fundamental techniques, models and algorithms for a Lunar Radio Navigation system High-pressure auxiliary thruster for future all-electric propulsion navigation satellites. All satellites must have the ability to correct for the high rotational tip-off rates after initial release from the launch vehicle. On current navigation satellites, de-tumbling is usually achieved in short duration using the onboard chemical propulsion thrusters. With future Navigation satellites looking at using all-electric propulsion satellites, these manouevres are to be performed by xenon-fed auxiliary thrusters. COTS (xenon cold gas) auxiliary thrusters are limited in the max thrust level provided and the de-tumbling duration, in the absence of chemical thrusters, is a concern. Germany TDE T619-701MP AST ADVANCED SPACE TECHNOLOGIES GMBH 2023 - 2023 High-pressure auxiliary thruster for future all-electric propulsion navigation satellites. Characterization of W-band propagation channel through ground-based observations The use of higher frequencies is becoming necessary for supporting feeder links of High Throughput Telecom Satellites due to the larger bandwidths available. Q and V bands are now being considered as a baseline for next generation systems. The next step will be to look at W band. In order to understand the system sizing, it is necessary to have a good modelling of the propagation channel. So far no measurement campaign has been done, therefore it is needed to start characterizing the channel. 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