Search results for "Geocentric orbit"
showing 3 items of 3 documents
Risk Assessment of Electron Induced SEE during the JUICE Mission
2018
The SEE sensitivity of electronic devices to high energy electrons has been put in evidence experimentally. Several ground experiments have shown that electron induced SEE could occur in recent technologies. In the case of the JUICE mission, the expected electron environment is harsher than for Earth orbits. The impact of such electron fluxes on the embedded electronics was assessed in this work. The study focused on SRAM memories SEU sensitivity. Three different device references were tested under electrons, as well as under protons and heavy ions. The electron and the low energy proton direct ionization contributions to the total SEU rate have been studied in more detail.
GrailQuest: hunting for atoms of space and time hidden in the wrinkle of Space-Time: A swarm of nano/micro/small-satellites to probe the ultimate str…
2021
AbstractGrailQuest(Gamma Ray Astronomy International Laboratory for QUantum Exploration of Space-Time) is a mission concept based on a constellation (hundreds/thousands) of nano/micro/small-satellites in low (or near) Earth orbits. Each satellite hosts a non-collimated array of scintillator crystals coupled with Silicon Drift Detectors with broad energy band coverage (keV-MeV range) and excellent temporal resolution (≤ 100 nanoseconds) each with effective area$\sim 100 \text {cm}^{2}$∼100cm2. This simple and robust design allows for mass-production of the satellites of the fleet. This revolutionary approach implies a huge reduction of costs, flexibility in the segmented launching strategy, …
Background in low Earth orbits measured by LEGRI telescope – short and long term variability
1999
Abstract In this paper we present the first Low Energy Gamma Ray Imager (LEGRI) background measurements which were carried out in the earlier nominal operation activities of LEGRI Instrument on board MINISAT-01, after initial spacecraft and instrument check-up procedures. Short term (daily) and expected long term background variability is presented. A background model is also discussed in order to be used for celestial γ-ray emitters observations.