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Space Object Identification by In Situ Measurements of Orbit-Driven Waves (SOIMOW)

POSTER

Abstract

SOIMOW measures in situ electromagnetic plasma waves excited by satellites and space debris moving through the earth’s plasma in low earth orbit. Space debris detection is traditionally accomplished with satellite sensors employing optics and ranging radars. SOIMOW uses in situ conjunctions to measures low frequency plasma modes with electric and magnetic field receivers on host satellites. Satellites moving through the near-earth ionosphere between 200 and 1000 km altitude become electrically charged by both electron collection and photo emission in sunlight. These hypersonic charged objects pass through the ionosphere setting up electric currents and electric potentials that can produce a wide range of plasma waves. The SOIMOW technique may measure electromagnetic plasma waves launched by satellite motion out to ranges of tens of kilometers. The SOIMOW concept has been successfully demonstrated using the Radio Receiver Instrument (RRI) on the SWARM-E satellite with detection of micro-satellites and space debris in low earth orbit (LEO). Besides space object detection, the observations show how space-plasma waves affect the thermosphere and ionosphere.

Publication: Bernhardt, P.A., et al. (2020), Satellite Observations of Strong Plasma Wave Emissions with Frequency Shifts Induced by an Engine Burn from the Cygnus Spacecraft, Radio Science, 56, e2020RS007143. https://doi.org/10.1029/2020RS007143. <br>Bernhardt, P.A., et al. (2020), Strong Amplification of ELF/VLF Signals in Space Using Neutral Gas Injections from a Satellite Rocket Engine, Radio Science, 2021. https://doi.org/10.1029/2020RS007207 <br>Bernhardt, P.A., The Whistler Traveling Wave Parametric Amplifier (WTWPA) Driven by an Ion Ring-Beam Distribution from a Neutral Gas Injection in Space Plasmas, IEEE Trans. on Plasma Science. 49, 6, 1983-1996, DOI: 10.1109/TPS.2021.3079130, June 2021. <br>Hua, M., Bortnik, J., Ma, Q., and Bernhardt, P. A. (2022). Radiation belt electron acceleration driven by Very Low-Frequency transmitter waves in near-Earth space. Geophysical Research Letters, 49, e2022GL099258. https://doi.org/10.1029/2022GL099258<br>Bernhardt, P. A., et al. (2022). Active precipitation of radiation belt electrons using rocket exhaust driven amplification (REDA) of man‐made whistlers. Journal of Geophysical Research: Space Physics, 127, e2022JA030358. https://doi.org/10.1029/2022JA030358

Presenters

  • Paul A Bernhardt

    University of Alaska, Geophysical Institute, University of Alaska

Authors

  • Paul A Bernhardt

    University of Alaska, Geophysical Institute, University of Alaska

  • Lauchie Scott

    DRDC Ottawa Research Centre

  • Andrew Howarth

    University of Calgary