Satellite Theory & Signal Transmission Flashcards

In TDMA (Time Division Multiple Access) satellite systems, all earth stations must be precisely synchronized. What is the primary challenge this creates?

Answer: Propagation delay variations require burst timing adjustments to prevent overlap at the satellite

Because different earth stations are at different distances from the satellite, their bursts arrive at different times; stations must pre-correct their transmit timing so bursts arrive in assigned slots without colliding.

What is satellite look angle, and which two angles define it?

Answer: The direction from an earth station to a satellite, defined by azimuth and elevation

Look angle describes where an earth station must point its antenna, specified by azimuth (compass bearing) and elevation (angle above the horizon).

Which modulation format is specifically designed to maintain a constant envelope (constant amplitude) and is therefore preferred when a transponder amplifier must operate near saturation?

Answer: QPSK (Quadrature Phase Shift Keying)

QPSK carries information only in phase (not amplitude), making it constant-envelope and resilient to nonlinear amplification; QAM and OFDM vary in amplitude and suffer distortion near saturation.

Tropospheric scintillation primarily affects satellite signals in which conditions?

Answer: Hot and humid climates at low elevation angles

Tropospheric scintillation is caused by irregular refractive index variations in the lower atmosphere, most severe in hot, humid conditions and at low elevation angles where signals traverse more atmosphere.

What is a traveling wave tube amplifier (TWTA), and why is it commonly used in satellite transponders?

Answer: A broadband high-power amplifier using electron beam interaction with a slow-wave structure, preferred for its high power and efficiency over wide bandwidths

TWTAs use an electron beam traveling alongside a helical slow-wave structure to amplify RF signals across wide bandwidths at high power levels, making them ideal for satellite transponder output stages.

When a geostationary satellite experiences eclipse, what happens and how long can it last?

Answer: Earth's shadow blocks sunlight from the solar panels; eclipses can last up to about 72 minutes per day near equinoxes

Around the spring and fall equinoxes, GEO satellites pass through Earth's shadow for up to ~72 minutes per orbit; satellites operate on batteries during this period.

In a satellite system using frequency reuse with dual linear polarization, what is the minimum recommended cross-polarization isolation to prevent significant co-channel interference?

Answer: Approximately 30 dB

A minimum of ~30 dB cross-polarization isolation is typically required to ensure co-channel interference on the orthogonally polarized frequency is low enough to maintain acceptable signal quality.