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Challenges in Scientific Data Communication from Low-mass Interstellar Probes

  • Authors: David G. Messerschmitt, Philip Lubin, and Ian Morrison

2020 The Astrophysical Journal Supplement Series 249 36.

  • Provider: AAS Journals

Caption: Figure 2.

The receive optical collector is composed as an NS-way replication (called scaling out) of the aperture. An individual aperture focuses on achieving the maximum and uniform sensitivity to the signals from all probes in a swarm across a coverage solid angle ΩA and has effective area ﹩{A}_{e}^{S}﹩. It is also responsible for achieving a sufficiently large SBR to achieve the target BPP, and it may also be responsible for separating the signals from different probes. The NS apertures independently capture and log photon detection events, with their only coordination a common clock for time stamps. The resulting incoherent accumulation of the incident optical power across the entire collector achieves a sufficient average photon detection rate ﹩{{\rm{\Lambda }}}_{A}^{R}﹩ to recover the scientific data at rate ﹩{ \mathcal R }﹩, while influencing neither the coverage nor SBR.

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