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Solar-blind photoelectric detection systems for satellite applications.

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    Magnetic Electron Multipliers (MEM) are crucial for satellite detection systems. Studies reveal afterpulses limit their linear range, necessitating advanced electronics for accurate performance analysis.

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    Area of Science:

    • Space instrumentation
    • Particle detection physics

    Background:

    • Open Magnetic Electron Multipliers (MEM) are utilized in satellite-borne detection systems.
    • Continuous dynode and field strip designs are key features of these detectors.

    Purpose of the Study:

    • To discuss the characteristics of open MEMs for space applications.
    • To emphasize selection, thermal stabilization, calibration, and long-time performance of extreme ultraviolet (EUV) detectors.
    • To describe practical design aspects for satellite systems, including monitoring, charged particle immunity, and electrical breakdown.

    Main Methods:

    • Laboratory studies using fast electronics to analyze MEM performance.
    • Statistical analysis of afterpulses.
    • Investigation of detector selection, thermal stabilization, and calibration procedures.

    Main Results:

    • The useful linear range of MEMs is restricted by afterpulses.
    • Slow electronics in previous studies masked the impact of afterpulses on MEM characteristics.
    • Fast electronics are essential for accurately resolving afterpulses and understanding MEM performance.

    Conclusions:

    • Afterpulses significantly impact the linear range of MEM detectors.
    • Accurate characterization of MEMs, especially for EUV detection in space, requires fast electronics capable of resolving afterpulses.
    • Further research into the generation mechanisms of afterpulses is needed for improved detector design.