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Upcoming Earth Exploration Satellite Services (EESS) missions, especially to monitor Brazilian diversified biomes, will require progressively higher data rates for downlink transmissions, besides the ability to share its frequency spectrum with cellular base stations. Both impact issues on spectral efficiency (in bps/Hz) and coexistence in frequency, time, location, etc. This paper proposes a technique suitable for LEO Earth Observation Satellites (EOS) by combining two strategies. We initially present the Cognitive Radio (CR) spectrum awareness and exploitation approaches to propose techniques for improving their uses. Next, we detail the Adaptive MODulation and CODing (MODCOD) techniques (ACM) based on DVB-S2X systems to increase RF power and spectral efficiencies. Finally, we evaluate our solution by monitoring the Signal to Interference plus Noise Ratio (SINR) and combining CR/MODCOD techniques. Two case studies are presented that demonstrate the proposed approach on Brazilian satellites developed by the National Institute for Space Research (INPE). A real in-situ characterization of the interfering scenarios was performed during the passes of the two EESS satellites that proves the effectiveness of spectral efficiency and coexistence.
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http://dx.doi.org/10.1590/0001-3765202420230487 | DOI Listing |
Background: Space exploration has progressed significantly, with increased human presence in orbit, the development of space stations, and the planning of increasingly prolonged missions. However, the space environment poses substantial physiological challenges, particularly for the cardiovascular system. According to NASA's Human Research Program, the five primary risks associated with human spaceflight are: (1) microgravity, (2) ionizing cosmic radiation, (3) isolation and confinement, (4) closed environmental systems, and (5) the great distance from Earth.
View Article and Find Full Text PDFNature
September 2025
Los Alamos National Laboratory, Los Alamos, NM, USA.
The Perseverance rover has explored and sampled igneous and sedimentary rocks within Jezero Crater to characterize early Martian geological processes and habitability and search for potential biosignatures. Upon entering Neretva Vallis, on Jezero Crater's western edge, Perseverance investigated distinctive mudstone and conglomerate outcrops of the Bright Angel formation. Here we report a detailed geological, petrographic and geochemical survey of these rocks and show that organic-carbon-bearing mudstones in the Bright Angel formation contain submillimetre-scale nodules and millimetre-scale reaction fronts enriched in ferrous iron phosphate and sulfide minerals, likely vivianite and greigite, respectively.
View Article and Find Full Text PDFNature
September 2025
Natural History Sciences, IIL, Hokkaido University, Sapporo, Japan.
Carbonaceous asteroids are the source of the most primitive meteorites and represent leftover planetesimals that formed from ice and dust in the outer Solar System and may have delivered volatiles to the terrestrial planets. Understanding the aqueous activity of asteroids is key to deciphering their thermal, chemical and orbital evolution, with implications for the origin of water on the terrestrial planets. Analyses of the objects, in particular pristine samples returned from asteroid Ryugu, have provided detailed information on fluid-rock interactions within a few million years after parent-body formation.
View Article and Find Full Text PDFBiomaterials
September 2025
Medical Research Institute, Department of Orthopedics, Guangdong Provincial People's Hospital (Guangdong Academy of Medical Sciences), Southern Medical University, Guangzhou, 510080, China. Electronic address:
Contrary to the traditional strengthening route by adding multiple & high-dosage alloying elements, we here explored extremely compositional and phase-constituent "simplification" in rare earth (RE) containing biodegradable magnesium alloys for better biocompatibility. An ultra-lean Mg-0.1Pr alloy with a multiscale microstructure has been developed through casting and extrusion, which showed well-balanced performances that match the commercial Mg-based orthopedic products.
View Article and Find Full Text PDFPhys Rev Lett
August 2025
National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing, 100101, Peoples Republic of China.
The Dark Energy Spectroscopic Instrument (DESI) is a massively parallel spectroscopic survey on the Mayall telescope at Kitt Peak, which has released measurements of baryon acoustic oscillations determined from over 14 million extragalactic targets. We combine DESI Data Release 2 with CMB datasets to search for evidence of matter conversion to dark energy (DE), focusing on a scenario mediated by stellar collapse to cosmologically coupled black holes (CCBHs). In this physical model, which has the same number of free parameters as ΛCDM, DE production is determined by the cosmic star formation rate density (SFRD), allowing for distinct early- and late-time cosmologies.
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