Near-field optical model for directed energy-propelled spacecrafts

Amber Sucich; Tomas Snyder; Gary B. Hughes; Prashant Srinivasan; Philip Lubin; Qicheng Zhang; Alexander Cohen; Jonathan Madajian; Travis Brashears; Nic Rupert

doi:10.1117/12.2274692

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5 September 2017 Near-field optical model for directed energy-propelled spacecrafts

Amber Sucich; Tomas Snyder; Gary B. Hughes; Prashant Srinivasan; Philip Lubin; Qicheng Zhang; Alexander Cohen; Jonathan Madajian; Travis Brashears; Nic Rupert

Author Affiliations +

Proceedings Volume 10401, Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems; 1040107 (2017) https://doi.org/10.1117/12.2274692
Event: SPIE Optical Engineering + Applications, 2017, San Diego, California, United States

Abstract

Directed energy is envisioned to drive wafer-scale spacecraft to relativistic speeds. Spacecraft propulsion is provided by a large array of lasers, either in Earth orbit or stationed on the ground. The directed-energy beam is focused on the spacecraft sail, and momentum from photons in the laser beam is transferred to the spacecraft as the beam reflects off of the sail. In order for the beam to be concentrated on the spacecraft, precise phase control of all the elements across the laser array will be required. Any phase misalignments within the array will give rise to pointing fluctuations and flux asymmetry in the beam, necessitating creative approaches to spacecraft stability and beam following. In order to simulate spacecraft acceleration using an array of phase-locked lasers, a near field intensity model of the laser array is required. This paper describes a light propagation model that can be used to calculate intensity patterns for the near-field diffraction of a phased array. The model is based on the combination of complex frequencies from an array of emitters as the beams from each emitter strike a target surface. Ray-tracing geometry is used to determine the distance from each point on an emitter optical surface to each point on the target surface, and the distance is used to determine the phase contribution. Simulations are presented that explore the effects of fixed and time-varying phase mis-alignments on beam pointing, beam intensity and focusing characteristics.

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Amber Sucich, Tomas Snyder, Gary B. Hughes, Prashant Srinivasan, Philip Lubin, Qicheng Zhang, Alexander Cohen, Jonathan Madajian, Travis Brashears, and Nic Rupert "Near-field optical model for directed energy-propelled spacecrafts", Proc. SPIE 10401, Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems, 1040107 (5 September 2017); https://doi.org/10.1117/12.2274692

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