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Massive MIMO Self-Calibration: Optimal Interconnection for Full Calibration

机译:大规模MIMO自校准:全面校准的最佳互连

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摘要

In time-division duplexing (TDD) massive multiple-input multiple-output (MIMO) systems, the reciprocity between the downlink (DL) and the uplink (UL) channels can be utilized to infer the DL channel state information (CSI) with the acquired uplink (UL) CSI. However, the end-to-end UL and DL channel reciprocity are broken when there are mismatches in the radio frequency (RF) analog circuits among different antennas at the base station (BS). Without accurate calibration, there will be severe system performance degradation. This paper studies the internal self-calibration scheme to recover all the unknown full calibration coefficients when different BS antennas are interconnected via hardware transmission lines. On the one hand, we derive the calibration performance for an arbitrary interconnection network in closed-form and obtain closed-form Cramer-Rao lower bound (CRLB) expressions when (M - 1) transmission lines are consumed and M denotes the total number of BS antennas. On the other hand, we prove that the star interconnection network is optimal for internal full self-calibration due to its lowest CRLB. Numerical simulation are carried out to verify our theoretical analyses and results.
机译:在时分双工(TDD)大规模多输入多输出(MIMO)系统中,下行链路(DL)和上行链路(UL)信道之间的互易性可用于推断DL信道状态信息(CSI)与获得的上行链路(UL)CSI。但是,当基站(BS)上不同天线之间的射频(RF)模拟电路不匹配时,端到端UL和DL信道互易性将被破坏。没有精确的校准,将严重降低系统性能。本文研究了内部自校准方案,以在通过硬件传输线互连不同的BS天线时恢复所有未知的完整校准系数。一方面,我们推导了任意互连网络在封闭形式下的校准性能,并在消耗(M-1)条传输线并且M表示传输总数时获得封闭形式的Cramer-Rao下界(CRLB)表达式。 BS天线。另一方面,我们证明了星形互连网络的CRLB最低,因此是内部完全自校准的最佳选择。进行了数值模拟,以验证我们的理论分析和结果。

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