415 results found Selected 0 items No itemsClear selection Select / deselect all results (all pages, 415 total) Exploiting numerical modelling for the characterisation of collision break-ups All missions in Earth-bound orbits rely on space debris and meteoroid flux models. These models are used to assess the mission risk and design shielding concepts (for manned modules). The flux predictions have been found to have a remarkable sizing effect. Collision break-ups are the major source of debris >1mm and are poorly understood. This needs to be improved significantly. On Agency level, collision break-up modelling is decisive to define the Agency's position towards international agreements on space debris mitigation. Current models will be misleading. Italy TDE T711-603SD SPACEDYS S.R.L. SPACE DYNAMICS SERVICES S.R.L. 2020 - 2023 Exploiting numerical modelling for the characterisation of collision break-ups Novel In-Vacuum Alignment and Assembly Technologies for Optical Assemblies Many astronomical space missions observe at wavelengths which are absorbed by the atmosphere, as for example some infrared, ultraviolet or x-ray bands. Especially UV and x-ray optics have very stringent alignment tolerances due to the small wavelengths. Consequently, telescopes and instruments can only be tested at their operational wavelengths under vacuum conditions. Traditional methods for fixing optical elements and subassemblies (eg. Germany TDE T216-103MM Fraunhofer Gesellschaft 2017 - 2023 Novel In-Vacuum Alignment and Assembly Technologies for Optical Assemblies Metallic Glasses for High Performance Mechanism Applications on Long Term Missions Metallic Glasses (MG) are a class of alloys which retain an amorphous structure in the solid state, when cooled from the liquid state. Formation of a fully amorphous structure for large cross sections (up to > 1 cm) is now possible for several alloying systems referred to as Bulk Metallic Glasses (e.g. Fe-base, Ti-base, Al-base, Mg-base, Ca-base, Zr-base). Ireland TDE T524-503QT UNIVERSITY COLLEGE DUBLIN 2018 - 2023 Metallic Glasses for High Performance Mechanism Applications on Long Term Missions Metallic Glasses for High Performance Mechanism Applications on Long Term Missions Metallic Glasses (MG) are a class of alloys which retain an amorphous structure in the solid state, when cooled from the liquid state. Formation of a fully amorphous structure for large cross sections (up to > 1 cm) is now possible for several alloying systems referred to as Bulk Metallic Glasses (e.g. Fe-base, Ti-base, Al-base, Mg-base, Ca-base, Zr-base). Austria TDE T524-503QT RHP-TECHNOLOGY GMBH 2018 - 2023 Metallic Glasses for High Performance Mechanism Applications on Long Term Missions AOCS COTS hardware fostering AOCS architecture and functions innovation The use of equipment based on COTS for small/constellation/low-cost platforms is impacting the reliability, availability, performance and robustness of the commonly used AOCS [Attitude and Orbit Control System] equipment (e.g. Gyros, star trackers, GNSS receivers). This activity explores innovative solutions at AOCS functions and architecture level (incl. AOCS FDIR) to mitigate the changes introduced by the use of COTS hardware for AOCS equipment. Germany TDE T705-604SA Airbus Defence and Space GmbH 2020 - 2023 AOCS COTS hardware fostering AOCS architecture and functions innovation European Methods for Thermo-Elastic Verification Almost every Scientific and Earth Observation spacecraft has stringent thermo-elastic stability/alignment requirements for the spacecraft. During the reviews of almost all of these projects many discussions on verifyng these requirements. The criticality and the complexity to verify compliance has become evident from projects like Herschel telescope, GAIA, Bepi Colombo and Solar Orbiter. France TDE T708-601MS THALES ALENIA SPACE FRANCE 2020 - 2023 European Methods for Thermo-Elastic Verification Frequency stabilisation of a Quantum Cascade Laser for Supra-THz applications The supra-THz (>3 THz) bands have been recently proposed for low Earth orbit THz remote sounding missions such as LOCUS (Low-Cost Upper-atmosphere Sounder). In order to achieve coherent detection, heterodyne receivers at supra-THz frequencies are under development by integrating in a single waveguide cavity a Schottky based mixers fed by a Quantum Cascade Laser (QCL) as Local Oscillator (LO). Thanks to the QCL, enough LO power is available to drive the mixer. Germany TDE T107-505EE DLR - German Aerospace Center 2018 - 2023 Frequency stabilisation of a Quantum Cascade Laser for Supra-THz applications High pressure water electrolyser development for exploration surface missions Any manned exploration surface mission will rely on the availability of Oxygen for breathing, a power source that can operate independently of solar illumination and possibly, the ability to manufacture rocket propellant in-situ. All of these requirements can be met by the electrolysis of in-situ manufactured water. To achieve a highly reliable, light weight system, development of an electrolysis system that operates at high pressure is crucial. Norway TDE T322-602EP PROTOTECH A.S. 2019 - 2023 High pressure water electrolyser development for exploration surface missions High energy density solid-state batteries based on Li metal anode Conventional lithium ion batteries use organic highly flammable liquid electrolytes increasing the risk of catastrophic failure due to thermal runaways. In addition, the use of carbon anode in Li-ion batteries limit the maximum energy density. Based on scientific results, it is believed that the use of solid state electrolytes will significantly improve the electrochemical and thermal stability range of the battery cells. France TDE T703-606EP SAFT S.A.S 2020 - 2023 High energy density solid-state batteries based on Li metal anode High frequency millimetre-wave Voltage Controlled Oscillattor Local oscillators (LO) used in microwave and millimetre-wave radiometer receivers for Earth Observation (EO) are normally based on Dielectric Resonator Oscillators (DRO) that are limited to a typical frequency of about 30 GHz. The LO frequency in the millimetre-wave range (165.4 to 229 GHz) is then obtained by means of additional multiplier circuits and band-pass filters, thus increasing the complexity of the circuit, mass and power consumption, and reducing reliability. 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