Exercises
ex-otfs-ch18-01
EasyCompute the LEO Doppler at 28 GHz for a satellite at 500 km altitude, approaching the UE at 10° elevation.
.
Orbital velocity
km/s at 500 km.
Radial velocity
At : m/s.
Doppler
kHz.
ex-otfs-ch18-02
EasyWhy does 5G NR OFDM fail at LEO velocities? What SINR does it achieve for 690 kHz Doppler and kHz?
.
Failure reason
OFDM ICI grows as . At LEO Doppler, . ICI overwhelms signal.
SINR calculation
SINR = dB. Negative. Unusable.
Interpretation
OFDM at LEO cannot function. OTFS achieves 20 dB SINR at same conditions.
ex-otfs-ch18-03
EasyDescribe the satellite pass geometry: how does Doppler change as satellite moves from approach horizon to zenith to recede horizon?
Doppler depends on radial velocity component.
Approach
Satellite moving toward UE at horizon: max Doppler kHz.
Zenith
Satellite directly overhead: radial velocity = 0. Doppler = 0.
Recede
Satellite moving away at horizon: Doppler kHz.
Sweep rate
Doppler sweeps MHz over 10-minute pass. Rate: kHz per second.
ex-otfs-ch18-04
MediumDerive the LEO link budget at 28 GHz, 500 km, 45° elevation. Assume Tx power 5 W, Tx antenna gain 45 dBi, Rx antenna gain 10 dBi, bandwidth 100 MHz.
, .
Slant range
km.
Path loss
= 179 dB.
Received signal
dBW = dBm.
SNR
Noise: dBm. SNR = 1 dB. Very low. Need longer frame, larger array, or lower band for usable SNR.
ex-otfs-ch18-05
MediumFor an OTFS frame at LEO with MHz, ms, what is the required frame size to accommodate kHz Doppler?
where .
Doppler resolution
Hz.
Doppler bins
bins.
Delay bins
? Wait: and relate via , so . Delay resolution: ns. 14 delay bins cover 700 ns — enough for LEO LOS (no significant multipath).
Frame size
. Feasible.
ex-otfs-ch18-06
MediumA UE has simultaneously-visible LEO satellites, each with per-satellite outage probability 5%. Compute the multi-sat aggregate outage.
Independent outages: .
Independent outage
.
Availability
1 - = 99.99997% — "5 nines".
GEO comparison
GEO single-sat: 99.5% (rain fades at Ka-band). LEO multi-sat OTFS: 99.9999%. better.
Interpretation
Macro-diversity delivers dramatic reliability improvements. Core advantage of LEO constellations over GEO.
ex-otfs-ch18-07
MediumExplain soft handover in LEO-OTFS. How does it avoid the service interruption of hard handover?
Multiple satellites always serving; gradual transition.
Hard handover
Old satellite hand off → UE pauses → connects to new satellite. Pause: 0.1-1 second. Rate drop during pause.
Soft handover
UE maintains multiple concurrent satellite links. As one sets, its contribution diminishes gradually; as new rises, its contribution grows. Seamless.
Cell-free mechanism
Ground station coordinates which satellites serve which UE. As satellites change visibility, cluster updates. No UE- triggered handover.
Result
Zero handover overhead. Continuous rate. Critical for URLLC and mobile applications.
ex-otfs-ch18-08
MediumCalculate the Starlink constellation global coverage: what fraction of Earth's population can be served with simultaneously-visible satellites?
6000 satellites, 550 km altitude.
Per-sat footprint
Effective coverage area per LEO satellite (above 10° elevation): km² effective footprint.
Total coverage
Total potential coverage: 6000 5000 km² = km². Earth land surface: km². Ratio: 20% simultaneously in coverage of any satellite.
S ≥ 3
Per-location probability of : depends on density. For Starlink: 80% of populated Earth has (concentrating toward lower latitudes).
Population
80% of 8 billion = 6.4 billion people potentially served by LEO-OTFS at . Including oceans/deserts: similar fraction of surface covered.
ex-otfs-ch18-09
HardDerive the SINR scaling as for LEO-OTFS cell-free combining.
Coherent combining at UE; law of large numbers.
Per-sat signal
Per-satellite SNR: . Assumes fixed per-sat SNR for simplicity (in practice varies with elevation).
Coherent sum
Signal: . Noise: (sum of uncorrelated Gaussians). Signal magnitude: (coherent). Noise std: .
Aggregate SINR
= per-sat SNR. No gain if per-sat SNR is fixed!
Effective gain
The gain is in outage probability, not SNR: reliability improves as . Rate: constant, but at probability of availability.
With path-loss diversity
If satellites have different path losses: best-AP SNR dominates. Effective SNR gain: for diverse paths.
ex-otfs-ch18-10
HardCompare LEO-OTFS rate to GEO single-satellite rate for the same UE power budget.
GEO: longer range, higher path loss.
GEO path loss
km. at 28 GHz: = 218 dB.
LEO path loss
km (45° elevation): dB. 39 dB less than GEO.
Rate
For same Tx power: 39 dB better SNR for LEO. Rate: vs . At 20 dB LEO SNR: 7 bits/s/Hz. At -19 dB GEO SNR: essentially 0.
Macro-diversity
LEO can add dB via combining. GEO: no diversity. Total advantage: 40+ dB in effective SNR, 6-7 bits/s/Hz.
ex-otfs-ch18-11
HardModel the time-variation of Doppler across a LEO pass. How many Hz/s does Doppler change for a typical 500 km orbit at zenith?
Doppler sweeps linearly through zenith.
Doppler sweep equation
where .
At zenith
. . . at zenith: maximum.
Rate of change
Over a 10-minute pass ( rad): kHz/s.
Compensation
2.3 kHz/s Doppler drift is easily tracked by OTFS DD processing. Per-frame Doppler shift: 23 Hz (at 10 ms frame). Well within Hz per-bin resolution.
ex-otfs-ch18-12
HardFor a polar UE (e.g., Antarctica), Starlink coverage is reduced. Estimate the number of visible satellites and throughput.
Starlink orbital inclination: 53°.
Orbital coverage
Starlink orbits have inclination 53°. Satellites spend most time in middle latitudes. Polar coverage: few satellites simultaneously, quick transits.
Visibility count
At Antarctica (80°S): - satellites on average. Polar orbit (90° inclination) would be needed for high-lat coverage — Iridium Next has this.
Throughput
: aggregate SNR single-sat + 3 dB diversity. Rate Mbps (vs 60-80 Mbps equatorial). Still dramatically better than GEO (where polar is zero coverage above 82°).
Compared to GEO
Antarctic research stations: LEO-OTFS is the only broadband option. Starlink + Iridium NEXT combined coverage.
ex-otfs-ch18-13
HardCompute the 6G NTN aggregate capacity for a 10,000-satellite constellation serving 1 billion devices.
Total bandwidth × spatial reuse × devices.
Per-satellite capacity
Per-satellite: 100 Mbps → bps. Aggregate 10,000 sats: bps = 1 Tbps.
Spatial reuse
Each satellite's beam covers ~5000 km² with 50 UEs. Spatial reuse: 50 UEs/beam × 1000 beams/sat = 50,000 UEs/sat.
Aggregate
10,000 sats × 50,000 UEs/sat = served UEs. Half a billion users.
Per-user rate
1 Tbps / 500M users = 2 Mbps average. Modest but sufficient for basic services.
Scaling up
For 1B users at 50 Mbps average: need 50 Tbps aggregate, = 500,000 satellites. Not feasible with today's launches but within 2035+ horizon.
ex-otfs-ch18-14
HardDerive the minimum satellite count for a given coverage target. What gives 99.99% availability globally?
Visibility fraction + desired for diversity.
Per-sat visibility
A LEO satellite at 550 km: visibility from any ground location for 5-10 minutes per ~95-minute orbit. of time.
Required $S$
For 99.99% availability with 95% per-sat: .
Concurrent $S$
Need satellites simultaneously visible. Given per-sat 5% visibility: total satellites (at any given time). Over full sky: sats needed.
Current
Starlink: 6000 satellites. Matches the minimum for 99.99% global availability. Not coincidentally the deployed scale.
ex-otfs-ch18-15
HardDescribe the 3GPP NTN timeline: when will OTFS become standard for LEO? What are the key milestones?
Rel. 17 → Rel. 22+
Current (Rel. 17, 2022)
Initial NTN support for OFDM. Starlink Direct-to-Cell. Doppler pre-compensation.
Rel. 18 (2024)
Enhanced NTN. Better pre-comp. OFDM still dominant.
Rel. 19 (2026)
LEO-specific optimizations. Cell reconfiguration.
Rel. 20 (2028) — OTFS Study Item
3GPP evaluates OTFS for NTN. Performance comparisons. Standards work begins.
Rel. 21 (2030) — OTFS Standard
OTFS becomes standard for LEO-NTN. First OTFS-capable satellites launched.
Rel. 22+ (2032+)
Full 6G deployment. OTFS universal.
Migration
UE software-upgradable from OFDM to OTFS (hardware supports both). Satellites launch OTFS-enabled from 2028.
ex-otfs-ch18-16
HardPropose a mitigation for the "all satellites in same orbital plane" problem: what if a plane passes over a UE without any satellites?
Multi-plane constellations.
Problem
Single-plane constellation: satellites uniformly spread along orbit. Between satellites: coverage gap.
Multi-plane
Multiple orbital planes, each with satellites. Multiple planes simultaneously overhead. Starlink: 72 planes × 22 sats/plane.
Coverage
At any given ground location: always multiple planes visible. No single-plane gap.
Inter-plane handover
Handover between planes is hard (satellites in different orbits). But within each plane: soft handover (§3).
Design principle
For 99.99% global coverage: 3+ orbital planes per latitude band. Starlink, Kuiper: several planes. Iridium Next: 6 planes for polar coverage.