mmWave Radio

A key feature of the COSMOS platform is the integration of fully-programmable, high-performance SDR nodes with mmWave phased arrays. While there has been significant industrial and academic research on silicon-based mmWave phased array RFICs dating back to 2004, it is only recently that we are seeing commercial-grade mmWave phased arrays suitable for deployment in testbeds. Leveraging our ongoing partnership with IBM, the COSMOS platform will include mmWave nodes operating at both 28 and 60 GHz. The IBM 28GHz phased-array antenna module (PAAM) features 4 tiled RFICs supporting 64 dual-polarized antennas, 8 beams enabling hybrid analog-digital beamforming and MIMO, 30 degrees steerable beamwidth, 43 dBm EIRP, and up to 3 GHz IF. Another key aspect of the IBM 28GHz PAAM is the orthogonal amplitude and phase control enabled by (i) a gain-invariant phase-shifter design and phase-invariant variable-gain amplifier, and (ii) a careful antenna-array-in-package design the eliminates gain and phase mismatches. The front-end will offer rich programmability, including full access to the beamforming control, and latency as low as 10s of ns for low latency MAC and hybrid beamforming.

COSMOS cloud architecture
(a) The die photograph of the 28GHz phased array IC implemented in 130nm SiGe BiCMOS technology co-developed by IBM and Ericsson, (b) the siliconbased 28GHz mmWave phased array antenna module (PAAM) mounted on a test board, and (c) top and bottom views of a fully assembled PAAM [1].

[1] B. Sadhu, Y. Tousi, J. Hallin, S. Sahl, S. Reynolds, O. Renstrom, K. Sjogren, O. Haapalahti, N. Mazor, B. Bokinge, G. Weibull, H. Bengtsson, A. Carlinger, E. Westesson, J. Thillberg, L. Rexberg, M. Yeck, X. Gu, M. Ferriss, D. Liu, D. Friedman, and A. Valdes-Garcia, “A 28-GHz 32-element TRX phased-array IC with concurrent dual-polarized operation and orthogonal phase and gain control for 5G communications.” IEEE Journal of Solid-State Circuits, vol. 52, no. 12, pp. 3373-3391, Dec. 2017.

28GHz Channel Measurements in the COSMOS Testbed Area

The operation of mmWave networks will require accurate channel models designed for specific deployment sites since mmWave radio signals experience high path loss. In collaboration with Nokia Bell Labs, we conducted and reported extensive 28 GHz channel measurements in the COSMOS testbed deployment area [2], which is a representative urban street canyon environment with both line-of-sight (LOS) and non-lightof-sight (NLOS) links. In particular, we consider 3 sites that emulate different deployment scenarios of a mmWave base station (BS): (i) a 15 m-high balcony at a 4-way street intersection (referred to as “Intersection Balcony [Int]”), (ii) a 6 m-high bridge over-crossing an avenue (referred to as “Bridge [Bri]”), and (iii) a 15 m-high balcony facing a park (referred to as “Open Balcony [Bal]”). Our measurement campaign includes over 1,500 link measurements (with over 24 million power measurements) collected along 13 sidewalks adjacent to the 3 considered measurement sites.

28ghz_meas_map
28ghz_meas_pathgain

(Left) Locations and example street views of the three measurement sites in the COSMOS testbed deployment area. The receiver (Rx) is placed at a fixed location in each site (marked by a circle), and the transmitter (Tx) is moved along the measurement sidewalks (marked by lines). Solid and dashed lines correspond to sidewalks (or part of the sidewalks) where the Tx and Rx are in line-of-sight (LOS) and non-line-of-sight (NLOS), respectively. (Right) Measured path gain values and the corresponding fitted lines for different sidewalk groups (Int-LOS, Int-NLOS, Bri, and Bal).

[2] T. Chen, M. Kohli, T. Dai, A. D. Estigarribia, D. Chizhik, J. Du, R. Feick, R. Valenzuela, and G. Zussman, “28GHz channel measurements in the COSMOS testbed deployment area,” in Proc. ACM MobiCom’19 Workshop on Millimeter-Wave Networks and Sensing Systems (mmNets) (to appear), 2019. [download]

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