Prerequisites & Notation

Before You Begin

Part V of this book turns from hardware and standards to the extreme deployment frontier: the sky. Low-Earth-orbit satellite constellations β€” Starlink, OneWeb, Kuiper, and the coming 6G NTN proposals β€” promise broadband coverage to the entire globe, including oceans, deserts, and regions where terrestrial cells will never exist. Delivering that promise requires re-doing massive-MIMO system design under two physical constraints that no terrestrial cell ever faces. First, LEO satellites orbit at β‰ˆ7.5\approx 7.5 km/s relative to the ground, generating Doppler shifts of 66–4040 kHz at Ka band β€” two to three orders of magnitude larger than any terrestrial mobility scenario. Second, the one-way propagation delay is 55–2020 ms, large enough that closed-loop schemes honed for ΞΌ\mus-scale terrestrial feedback must be rethought. This chapter adapts the cell-free and user-centric ideas of Part III to the orbital regime, with macro- diversity across simultaneously visible satellites as the central design lever and the choice of waveform (OFDM vs OTFS) as the secondary one. We assume familiarity with the following prior material.

  • Massive MIMO fundamentals, channel hardening and favorable propagation(Review ch01)

    Self-check: Can you state why 1NtHkHHkβ†’1\frac{1}{N_t} \mathbf{H}_{k}^{H} \mathbf{H}_{k} \to 1 as Ntβ†’βˆžN_t \to \infty and what it implies for linear precoding?

  • Cell-free and user-centric massive MIMO β€” APs without cells(Review ch11)

    Self-check: Can you state the difference between centralized cell-free and user-centric cluster operation, and name the serving-set selection rule?

  • Linear precoding β€” MRT, ZF, MMSE β€” in the multiuser downlink(Review ch06)

    Self-check: Can you write the ZF precoder W=HH(HHH)βˆ’1\mathbf{W} = \mathbf{H}^{H} (\mathbf{H} \mathbf{H}^{H})^{-1} and explain when it leaves residual interference?

  • Distributed processing: local vs centralized combining, LSFD, fronthaul(Review ch13)

    Self-check: Can you sketch level 1, 2, 3, 4 cooperation and state what each level sends over the fronthaul?

  • OFDM wideband signal model, CP length, subcarrier spacing, ICI(Review ch10)

    Self-check: Can you state the condition on the CP length that eliminates inter-symbol interference in OFDM, and the condition on fD/Ξ”ff_D / \Delta f that bounds inter-carrier interference?

  • Friis free-space path loss, link budget, noise power from bandwidth and G/TG/T(Review ch15)

    Self-check: Can you write Ξ²FSPL=(4Ο€d/Ξ»)2\beta_{\text{FSPL}} = (4\pi d / \lambda)^2 and the receive SNR in terms of PtP_t, antenna gains, and noise temperature?

  • Doppler shift for a moving terminal, coherence time Tc∼1/fDT_c \sim 1/f_D(Review ch18)

    Self-check: Can you derive fD=vf0/cf_D = v f_0 / c and explain why the LEO case breaks the usual 'slow time variation' assumption?

Notation for This Chapter

Symbols specific to this chapter. The altitude hh, the elevation angle ΞΈel\theta_{\text{el}}, the satellite velocity vsatv_{\text{sat}}, and the number of simultaneously visible satellites MM are chapter-local and are not global \ntn\ntn{} tokens; they are defined here. See NGlobal Notation Table for the master table.

SymbolMeaningIntroduced
hhSatellite altitude above the Earth's surface (km). LEO: 500500–20002000; MEO: β‰ˆ8000\approx 8000–2000020000; GEO: β‰ˆ35786\approx 35786s01
RER_EEarth radius (β‰ˆ6371\approx 6371 km)s01
ΞΈel\theta_{\text{el}}Elevation angle of the satellite from the user terminal (rad or deg)s01
vsatv_{\text{sat}}Satellite orbital velocity, vsat=GME/(RE+h)v_{\text{sat}} = \sqrt{G M_E / (R_E + h)} (β‰ˆ7.5\approx 7.5 km/s for LEO)s01
dslantd_{\text{slant}}Slant range from terminal to satellite as a function of hh and ΞΈel\theta_{\text{el}}s01
Ο„prop\tau_{\text{prop}}One-way propagation delay, Ο„prop=dslant/c\tau_{\text{prop}} = d_{\text{slant}} / c (ms)s01
MMNumber of satellites simultaneously visible to a terminal under the macro-diversity architectures03
Hm\mathbf{H}_{m}Downlink channel vector from satellite mm to the user; Hm∈CNt\mathbf{H}_{m} \in \mathbb{C}^{N_t} where NtN_t is the satellite array sizes03
fDf_DPeak one-way Doppler shift, fD=vsatf0/cf_D = v_{\text{sat}} f_0 / c at zenith overhead passs02
Ξ”fD(ΞΈel)\Delta f_D(\theta_{\text{el}})Instantaneous Doppler shift as a function of elevation; varies from +fD+f_D at horizon-approach to βˆ’fD-f_D at horizon-departures02
G/TG/TReceiver figure of merit: antenna gain divided by system noise temperature (dB/K)s02
LrainL_{\text{rain}}Rain fade attenuation (dB), dominant excess loss at Ka bands02
TvisibleT_{\text{visible}}Duration a given LEO satellite remains above the minimum elevation for a fixed terminals01
THOT_{\text{HO}}Handover interval β€” how often a terminal must switch its master satellites05
TcT_cChannel coherence time β‰ˆ1/fD\approx 1 / f_D; for LEO Ka band this is sub-milliseconds02