111 results found Selected 0 items No itemsClear selection Select / deselect all results (all pages, 111 total) Differential radiating front-end for DRA telecom applications in K-band. Direct Radiating Antenna arrays (DRAs) are an emerging solution to offer multiple beam, cellular-like coverage to satellite communication services, evolving to meet the demands for high data-rates, capacity and availability over a flexible area. A DRA array provides several advantages to the satellite: for downlink, an improved Equivalent Isotropically Radiated Power (EIRP), due to the smaller size of the beam; for uplink, an improved Gain-to-noise-Temperature (G/T). Netherlands TDE T506-701EF TNO, Netherlands Organisation for Applied Scientific Research 2022 - 2025 Differential radiating front-end for DRA telecom applications in K-band. Impact of storage conditions and aging effect on RF breakdown and electrical performance in flight hardware The activity shall investigate the change in SEY (Secondary Emission Yield) properties due to storage conditions prior integration in the satellite. This parameter has a direct impact in the power handling (Multipactor threshold) of the RF component. The activity shall cover the changes in the threshold over time at typical storage conditions. To achieve successful results, the activity shall commence with a review of the Hatch-Williams curves with new test samples. These samples shall be used for the whole duration of the activity to study the aging process. France TDE T706-402ET ONERA 2016 - 2025 Impact of storage conditions and aging effect on RF breakdown and electrical performance in flight hardware L-band antenna for next generation SMOS missions ESA?s Soil Moisture and Ocean Salinity (SMOS) mission launched in 2009 is based on an L-band interferometric radiometer providing images of the entire earth globe every three days. Several studies have been conducted in the past few years to define a different antenna configuration which could allow to improve the image quality and simultaneously reduce the imaging time. Spain TDE T107-701EF AIRBUS DEFENCE AND SPACE S.A.U. 2021 - 2025 L-band antenna for next generation SMOS missions High Performance MEMS Reference Oscillator Today, reference oscillators are based on a quartz resonator which is carefully sheltered in order to provide a very stable environment to this key component which in turn provides a very stable and low phase noise reference. This type of oscillator also called Oven Controlled Oscillator (OCXO) is the core technology in most space products requiring either stable frequency or low phase noise or both. Though far more recent on the market, MEMS oscillators are already as good as TCXO while being much smaller (hybrid assembly as compared to single chip solution). France TDE T706-501ET SYRLINKS 2019 - 2025 High Performance MEMS Reference Oscillator Architectures for wide-band meta-signal processing in low cost devices The exploitation of the wide bandwidth signals in the lower GNSS L-band is expected to be of interest for mass-market user equipment (UE) in order to improve significantly code-based position accuracy in location-based services. Austria TDE T606-704ES JOANNEUM RESEARCH FORSCHUNGSGESELLSCHAFT 2022 - 2025 Architectures for wide-band meta-signal processing in low cost devices Hybrid, grating-MOT + magnetic chip trap, approach to compact high frequency BEC production in space Quantum degenerate gases such as Bose-Einstein Condensates (BECs) are key tools for ultimate precision quantum technologies in space. On earth, gravity prevents long measurement times except in experiments with prohibitively large footprints (10m), however in orbit or in deep space the chilliest terrestrial atomic clouds would take minutes to expand to a radius of 1cm which corresponds to 100km of ballistic free-fall. Germany TDE T717-504MM Leibniz Universit?t Hannover 2018 - 2024 Hybrid, grating-MOT + magnetic chip trap, approach to compact high frequency BEC production in space High Accuracy Coherent Antenna Testing over Temperature The increased need for accurate knowledge of amplitude and phase antenna patterns for a very broad frequency range and over a large thermal range is a reality for a multitude of space applications. Among them are the high accuracy Radio Science Experiments for ranging and radio occultation that require accurate knowledge of the phase information. This enable the characterisation of the thermo-elastic effects provided that test techniques are developed in a temperature range down to -140C. Italy TDE T707-503EE MICROWAVE VISION ITALY SRL 2018 - 2024 High Accuracy Coherent Antenna Testing over Temperature Characterisation of contamination induced straylight With state-of-the-art polishing techniques straylight from surface roughness is decreased and straylight induced by contamination is becoming one of the main contributors to the straylight performance. It is then important to rely on representative models for contamination induced straylight. Typically, industry is using models coming from literature, which can lead to very different results. The activity shall include the following tasks : - A critical review of the existing models shall be performed. Germany TDE T116-501MM Fraunhofer Gesellschaft 2019 - 2024 Characterisation of contamination induced straylight Straylight LIDAR OGSE verification tool, hardware pre-development. Background and context: The aim of this activity is to breadboard the Straylight LIDAR instrument concept and to verify its performance experimentally. This activity aims to raise the TRL to 4 and follows the TDE activity (T216-104MM Verification of straylight rejection of optical science payloads using a pulsed laser source). The aim of this smooth follow-on is to verify the concept experimentally using an available flight spare space telescope baffle as a representative test object.Description of the concept: The technique is called ?straylight LIDAR? Switzerland TDE T208-022MM CSEM SA. Centre Suisse dElectronique et de Microtechnique SA 2021 - 2024 Straylight LIDAR OGSE verification tool, hardware pre-development. Low Noise Amplifier (LNA) at 600 Gigahertz (GHz) Advancements in semiconductor technologies like INP and MHEMT have made low-noise amplifiers (LNA) possible for increasingly higher frequencies. Currently efforts are taken to reach frequencies close to 1 THz. Aggressive reduction of the gate length has been essential in this progress, but is becoming less effective with gate lengths approaching 30 nm scale. New technological approaches are needed to reach thz frequencies. New material systems are being investigated, especially those based on antimonides. 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