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Träfflista för sökning "WFRF:(Cecconi B.) srt2:(2015-2019)"

Sökning: WFRF:(Cecconi B.) > (2015-2019)

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  • Brown, P., et al. (författare)
  • Meeting the Magnetic Emc Challenges for the In-Situ Field Measurements on the Juice Mission
  • 2019
  • Ingår i: Proceedings of 2019 ESA Workshop on Aerospace EMC (Aerospace EMC). - : IEEE. - 9789082684780
  • Konferensbidrag (refereegranskat)abstract
    • The JUICE (JUpiter ICy moon Explorer) mission features instrument designs tailored to meet the specific challenges of the respective measuring environment, including EMC constraints. We describe the magnetic field science requirements for this mission and show how they drive the EMC requirements on the spacecraft and selected in-situ instrument configurations. We describe the results of two mutual interference campaigns and discuss the design mitigations employed in order to realise in-situ magnetic and electric field data in-flight with the accuracy required to meet very challenging mission science goals.
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  • Lamy, L., et al. (författare)
  • The low-frequency source of Saturn's kilometric radiation
  • 2018
  • Ingår i: Science. - : AMER ASSOC ADVANCEMENT SCIENCE. - 0036-8075 .- 1095-9203. ; 362:6410
  • Tidskriftsartikel (refereegranskat)abstract
    • Understanding how auroral radio emissions are produced by magnetized bodies requires in situ measurements within their source region. Saturn's kilometric radiation (SKR) has been widely used as a remote proxy of Saturn's magnetosphere. We present wave and plasma measurements from the Cassini spacecraft during its ring-grazing high-inclination orbits, which passed three times through the high-altitude SKR emission region. Northern dawn-side, narrow-banded radio sources were encountered at frequencies of 10 to 20 kilohertz, within regions of upward currents mapping to the ultraviolet auroral oval. The kilometric waves were produced on the extraordinary mode by the cyclotron maser instability from 6- to 12-kiloelectron volt electron beams and radiated quasi-perpendicularly to the auroral magnetic field lines. The SKR low-frequency sources appear to be strongly controlled by time-variable magnetospheric electron densities.
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