Presentation + Paper
15 March 2023 High-rate 256+ Gbit/s laser communications for enhanced high-resolution imaging using space-based very long baseline interferometry (VLBI)
Jade P. Wang, Bryan Bilyeu, Don Boroson, David Caplan, Bryan Robinson, Curt Schieler, Michael Johnson, Lindy Blackburn, Sheperd Doeleman, Kari Haworth
Author Affiliations +
Proceedings Volume 12413, Free-Space Laser Communications XXXV; 1241308 (2023) https://doi.org/10.1117/12.2651471
Event: SPIE LASE, 2023, San Francisco, California, United States
Abstract
Space-based VLBI imaging can dramatically improve state-of-the-art astronomical radio-imaging resolution by enabling significantly longer baseline distances and eliminating atmospheric-attenuation constraints on RF carrier imaging wavelength. However, smaller space-based apertures and sensitivity constraints impose challenging recorded-data downlink-rate requirements, potentially to 256 Gbit/s. Laser communications is a promising option for realizing such highrate long-distance downlinks with modest power and aperture demands. Here, we present a scalable lasercom architecture that can enable high-rate long-distance downlinks needed for enhanced space-based VLBI imaging from geosynchronous orbit (GEO).
Conference Presentation
© (2023) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jade P. Wang, Bryan Bilyeu, Don Boroson, David Caplan, Bryan Robinson, Curt Schieler, Michael Johnson, Lindy Blackburn, Sheperd Doeleman, and Kari Haworth "High-rate 256+ Gbit/s laser communications for enhanced high-resolution imaging using space-based very long baseline interferometry (VLBI)", Proc. SPIE 12413, Free-Space Laser Communications XXXV, 1241308 (15 March 2023); https://doi.org/10.1117/12.2651471
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Automatic repeat request

Receivers

Telecommunications

Optical communications

Data communications

Wavelength division multiplexing

Back to Top