Q/A Microwave

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BBorhan
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Year 3 Term 2

Solutions:

Microwave is a line-of-sight wireless communication technology that uses high frequency beams of radio waves to provide high speed wireless connection that can send and receive voice, video and data information.

Microwaves are called transverse electromagnetic waves because the electric and magnetic fields that make up the wave oscillate perpendicular to each other and to the direction the wave travels

Wavelength : as long as 1 meter as short as 1 millimeter

Frequency: 300MHz to 300 GHz

Microwave frequency bands are designated by specific letters

LetterGHz
L1-2
S2-4
C4-8
X8-12
Ku12-18
K18-26.5
Ka26.5-40
Q30-50
U40-60
V50-75
E60-90
W75-110
F90-140
D110-170

Solution:


An Antenna is a transducer which converts electrical power into electromagnet waves and vice versa.

An antenna is called a transducer because it converts electrical energy into electromagnetic (EM) waves and vice versa.

Antenna Parameters:

Directivity: The ratio of a maximum radiation intensity of the subject antenna to the radiation intensity of an isotropic antenna, radiating the same total power is called directivity.

The ratio of radiation intensity in a given direction from an antenna to the radiation intensity average overall direction is called directivity.

Directivity : D=maximum radiaition intensity of subject antennaRadiation intensity of an isotropic antenna=ϕ(θ,ϕ)max(subject antenna)ϕ0(isotropic antenna)D = \frac{\text{maximum radiaition intensity of subject antenna}}{\text{Radiation intensity of an isotropic antenna}} = \frac{\phi(\theta, \phi)_{max} \text{(subject antenna)}}{\phi_0 \text{(isotropic antenna)}}

Gain: Gain describes how much power is transmitted in the direction of peak radiation to that of an isotropic source.

Antenna gain is calculated by multiplying antenna efficiency with directivity of antenna.

G=ηeD=PradPinputϕ(θ,ϕ)maxϕ0G = \eta_e D = \frac{P_{rad}}{P_{input}} \cdot \frac{\phi(\theta, \phi)_{max}}{\phi_0}

An antenna that radiates equally in all directions would have effectively zero directionality, and the directivity of this type of antenna would be 1 (or 0 dB).

An ideal isotropic antenna with 0dB or 1(normal) gain, radiates signal equally in all directions with zero losses .

Aperture efficiencу: Aperture Efficiency is a term used to describe the effectiveness of an antenna in converting electrical energy to it into electromagnetic radiation.

It is the ratio of the effective radiating area to the physical are of the aperture.

ϵa=AeffAp=Effective areaPhysical area\epsilon_a = \frac{A_{eff}}{A_p} = \frac{\text{Effective area}}{\text{Physical area}}

Effective aperture (effective area) : The effective aperture parameter describes how much power is captured from a given plane wave. 

Let p be the power density of the plane wave (in W/m^2). If P_t represents the power (in Watts) at the antennas terminals available to the antenna's receiver, then:
Pt=pAeP_t = p A_e

Ae=λ24πGA_e = \frac{\lambda^2}{4\pi}G

Antenna Efficiency: It is the ratio of the radiated power of the antenna to the input to the input power by the antenna.

ηe=PradPin\eta_e = \frac{P_{rad}}{P_{in}}

VSWR: VSWR stands for Voltage Standing Wave Ratio, and is also referred to as Standing Wave Ratio (SWR).

VSWR is the ratio of the peak amplitude of a standing wave to the minimum amplitude of a standing wave.

S=VmaxVminS = |\frac{V_{max}}{V_{min}}|, VSWR=1+τ1τ\text{VSWR} = \frac{1 + |\tau| }{1 - |\tau| }

A transmission line having 50 impedance is terminated in a load of (40+j30) . Calculate VSWR.

Reflection Coefficient, τ=ZLZ0ZL+Z0=40+j305040+j30+50\tau = \frac{Z_L - Z_0}{Z_L + Z_0} = \frac{40+j30-50}{40+j30+50}

τ=1090|\tau| = \sqrt{\frac{10}{90}}

VSWR=1+τ1τ=2VSWR = \frac{1 + |\tau| }{1 - |\tau|} = 2

Beam width

Beam width is the aperture angle from where most of the power is radiated.

"Beam width is the aperture angle from where most of the power is radiated"-Explain.

Beam width is the angular range (aperture angle) over which the majority of an antenna's power is radiated. It is usually measured between the points where the power drops to half (−3 dB) of its maximum value. This defines the main lobe of the radiation pattern, indicating the direction in which the antenna transmits or receives most effectively.

Half Power Beam Width (HPBW): Half power beam width is the angle in which relative power is more than 50% of the peak power, in the effective radiated field of the antenna. BW=70λD\text{BW} = \frac{70\lambda}{D}

First Null Beam Width: The angular span between the first pattern nulls adjacent to the main lobe, is called as the First Null Beam Width (FNBW). FNBW=2HPBW=140λDradian\text{FNBW} = 2 \text{HPBW} = \frac{140 \lambda}{D} \text{radian}

Relationship between length, frequency, wavelength

The length of the antenna is inversely proportional to the frequency and directly proportional to the wavelength. The higher the frequency and the shorter the wavelength, the shorter the antenna can be made.

Equivalent Isotropic Radiated Power: The amount of power that an isotropic antenna radiates to produce the peak power density observed in the direction of maximum antenna gain, is called as Equivalent Isotropic Radiated Power.

Effective Radiated Power

If the radiated power is calculated by taking half-wave dipole as the reference, rather than an isotropic antenna, then it can be termed as ERP (Effective Radiated Power).

ERP(dBW)=EIRP(dBW)−2.15dBi

Solution:

λ=cf=3×108106=300 meter\lambda = \frac{c}{f} = \frac{3 \times 10^8}{10^6} = 300 \text{ meter}

Antenna TypeFormulaSize at 1 MHz
Monopoleλ/4300/4=75
Dipoleλ/2300/2=150
Full Wavelengthλ300

Solution:

A dipole antenna is defined as a symmetrical antenna in which the two ends are at equal potential relative to midpoint.

A half wave dipole antenna is the fundamental radio antenna of metal rod thin wire, it has a physical length of half wavelength in free space of the frequency of operation.

Half-wave dipole antenna (Hertz antenna. is the most widely used antenna because of its advantages.

Features of Half wave dipole antenna:

  1. The half-wave dipole antenna is a special case of the dipole antenna, with a length equal to half the wavelength (λ/2) of the operating frequency.
  1. The electric current distribution is maximum at the center and zero at the ends.
  1. It is a center-fed antenna.
  1. The typical input impedance of a standard half-wave dipole is approximately Zin = 73 + j42.5 Ohms.
  1. By slightly shortening the dipole to about 0.48λ, the antenna becomes resonant, and the impedance becomes purely real: Zin ≈ 70 Ohms, making it well-matched to transmitters or receivers.
  1. The directivity of the half-wave dipole is 1.64 (which is equivalent to 2.15 dB).
  1. The Half Power Beamwidth (HPBW) of the radiation pattern is approximately 78 degrees.
  1. 3KHz to 300 GHz

L=12kλ=143f meter=468f feet,f=MHzL = \frac{1}{2} k \lambda = \frac{143}{f} \text{ meter} = \frac{468}{f} \text{ feet}, f=MHz

Ptotal=12I02RradiationP_{total} = \frac{1}{2}I_0^2 R_{radiation}

Rradiation73.1ΩR_{radiation} \approx 73.1 \Omega (73 Ω resistance and +43 Ω reactance, )


Advantages

Disadvantages

A Yagi-Uda antenna is constructed with a central boom supporting multiple parallel conductive elements: a driven element (usually a half-wave dipole), a reflector (slightly longer), and one or more directors (slightly shorter)

To construct a Yagi-Uda antenna, se­veral components come toge­ther to create an e­fficient and directional antenna for transmitting or re­ceiving electromagne­tic signals. The central ele­ment is called the "boom," which se­rves as the framework for mounting all othe­r parts. Connected to the transmission line­ is the primary eleme­nt, known as the "driven ele­ment," responsible for signal transmission or re­ception. At the far end of the antenna is the "reflector," a longer element that reflects energy towards the antenna's radiation pattern. In front of the driven element, there are multiple strategically placed "directors" with specific lengths and spacings. These directors assist in directing the antenna's radiation pattern for optimal performance.

Solution:

A parabolic antenna is a high-gain reflector antenna used for radio, television and data communications, and also for radio location (radar) on the UHF and SHF parts of the electromagnetic spectrum .

Why is it used?
At higher microwave frequencies the physical size of the antenna becomes much smaller which in turn reduces the gain and directivity of the antenna.
The desired directivity can be achieved using suitably shaped parabolic reflector behind the main antenna which is known as primary antenna or feed .

Principle Operation

Application of parabolic Reflector:

  1. Telecommunication
  1. Optics
  1. Acoustics
  1. Scientific Research


Types of paraboloid/reflector

TypeDescriptionBeam CharacteristicsApplications
Truncated Paraboloid
- Horizontal TruncationParabolic in horizontal plane, truncated vertically.Narrow horizontal beam, spreads vertically.Surface search radar, detects aircraft at varying altitudes.
- Vertical TruncationParabolic in vertical plane, truncated horizontally.Narrow vertical beam, spreads horizontally.Height-finding systems for precise elevation.
Orange-Peel ParaboloidSegment of circular paraboloid, narrow horizontally, wide vertically.Wide horizontal beam, narrow vertically.Height-finding radar equipment.
Cylindrical ParaboloidCurved in one dimension, flat in other; focuses along a line using line source.Fan-shaped beam, narrow in curved dimension, wide in flat dimension.Radar systems requiring fan-shaped beams.
Corner ReflectorTwo flat conductive sheets forming a corner; driven by half-wave radiator.Simple reflected beam.Radar and communication systems for wave reflection.

G=4πAλ2,A=πd24,Beamwidth α=115λdG = \frac{4\pi A}{\lambda^2}, A=\frac{\pi d^2}{4}, \text{Beamwidth } \alpha = \frac{115\lambda}{d}

Types of Microwave feeder/Driven Element

TypeDescriptionAdvantagesDisadvantages
Axial FeedFeed antenna is placed at the focus, directly in front of the dish, pointing back.Simple and common design.Feed and supports block the beam (efficiency 55–60%).
Off-Axis / Offset FeedFeed is placed to the side of the dish (asymmetrical paraboloid).No blockage of the beam, better signal reception.More complex geometry.
CassegrainFeed located on or behind the dish; uses a convex hyperboloidal secondary reflector to reflect waves back to main dish.Suitable for bulky or complex feeds; efficiency ~65–70%.Slightly complex design and alignment.
GregorianSimilar to Cassegrain, but uses a concave (ellipsoidal) secondary reflector.Very high aperture efficiency (>70%).Most complex among these; higher cost.

A parabolic reflector is 9 cm deep and its diameter is 24 cm. How far is its focus from the vertex?

Let the equation of the parabolic shape of the reflector be y² = 4ax. ....(i)
As given, we have OM = 9 cm and AB = 24 cm
⇒ OM = 9 cm and AM = ½ AB = 12 cm.
∴ the coordinates of A are (9, 12).
Since A lies on equation (i), we have:
12² = 4 × a × 9
⇒ a = 4.
∴ the equation of the parabola is y² = 16x.
Its focus is F(a, 0), i.e., F(4, 0).
Hence, the focus is at a distance of 4 cm from the vertex.

Solution

Radiation Patterns are diagrammatical representations of the distribution of radiated energy into space, as a function of direction.

Radiation Pattern TypeShape (2D / 3D View)Description
Omni-directional Pattern3D: Doughnut shape
2D: Figure-of-eight
Radiates equally in all horizontal directions; non-directional.
Pencil-beam PatternPencil-shaped, narrow and highly directionalFocused beam in a specific direction; used for long-distance targeting.
Fan-beam PatternFan-shaped (broad in one direction, narrow in the other)Covers a wide area in one plane, narrow in the perpendicular plane.
Shaped Beam PatternIrregular, custom shapeBeam is tailored for specific coverage; no fixed pattern shape.

Simplest antenna design procedure:

  1. Choose Frequency (f): Decide the operating frequency (e.g., 100 MHz).
  1. Calculate Wavelength (λ)
  1. Find Antenna Length (L):
    • For half-wave dipole: L=λ/2
    • For quarter-wave monopole: L=λ/4
  1. Select Material: Use good conductor (e.g., copper).
  1. Feed at Center: For dipole, feed in the middle using coaxial cable.
  1. Test and Adjust: Use antenna analyzer or trim for better signal.

Solution

The Hertzian dipole is a theoretical dipole antenna that consists of an infinitesimally small current source acting in free-space.

Rrad=2I02Ptotal=2πμ0c03(d/λ)2=2π3z0(d/λ)2,Z0=377ohmR_{rad} = \frac{2}{I_0^2} P_{total} = \frac{2 \pi \mu_0 c_0}{3} (d/\lambda)^2 = \frac{2 \pi}{3} z_0 (d/\lambda)^2, Z_0 = 377 \text{ohm}

Rrad=80π2(0.1λλ)2=7.88R_{rad} = 80 \pi^2 (\frac{0.1\lambda }{\lambda})^2 = 7.88 ohm

Solution

A Horn antenna may be considered as a flared out wave guide. To improve the radiation efficiency and directivity of the beam, the waveguide should be provided with an extended aperture to make the abrupt discontinuity of the wave into a gradual transformation.

Operational frequencies 300MHz to 30GHz.

Type of Horn AntennaStructure / ShapeFlaring DirectionKey Features / Applications
Pyramidal HornTruncated pyramid; flaring on both E-plane and H-plane walls of a rectangular waveguideBoth E & H planesMost common type; used in rectangular waveguides
Sectoral E-plane HornFlaring in one direction only (Electric field direction)E-plane onlyNarrow beam in E-plane; wider in H-plane
Sectoral H-plane HornFlaring in one direction only (Magnetic field direction)H-plane onlyNarrow beam in H-plane; wider in E-plane
Conical HornCircular flare from a circular waveguideAll around (circularly symmetric)Used with circular waveguides; good for symmetric beam patterns
Exponential HornCurved sides; flare increases exponentially with lengthSmooth exponential flareMinimum reflection, wide bandwidth; used in satellite antennas and radio telescopes

A=125100=0.0125m2A= 125*100 = 0.0125 m^2

G=4π×0.01250.032=...G= \frac{4\pi \times 0.0125}{0.03^2} = ...

GdB=10log10G=...G_{dB} = 10 \log _{10} \text{G} = ...


Transmission Line

WaveguideTransmission Line
The waveguide is a hollow metallic structure through which electric and magnetic fields are transmitted.The transmission line is a conductor which is used to carry electrical signal over a long range.
It has simple to manufactured.It has complex to manufactured.
In waveguide the power handling is high as compared to transmission line.In transmission line the power handling is low as compared to waveguide.
The Operating modes are TE or TM mode.The operating mode are TEM or quasi TEM mode.
In waveguide high power is transmitted.In transmission line low power is transmitted.
In waveguide the electromagnetic signal is transmitted.In transmission line the electrical signal is transmitted.
The operating frequency is 3 GHZ to 100 GHZ in waveguide.The operating frequency is up to 18 GHz.

βl=2πλλ4=π2\beta l = \frac{2\pi}{\lambda} \frac{\lambda}{4} = \frac{\pi}{2}

Zsc=jZ0tanβl=Z_{sc} = jZ_0 \tan \beta l = \infin

VSWR is the ratio of the peak amplitude of a standing wave to the minimum amplitude of a standing wave.

S=VmaxVminS = |\frac{V_{max}}{V_{min}}|, VSWR=1+τ1τ\text{VSWR} = \frac{1 + |\tau| }{1 - |\tau| }

A transmission line having 50 impedance is terminated in a load of (40+j30) . Calculate VSWR.

Reflection Coefficient, τ=ZLZ0ZL+Z0=40+j305040+j30+50\tau = \frac{Z_L - Z_0}{Z_L + Z_0} = \frac{40+j30-50}{40+j30+50}

τ=19|\tau| = \sqrt{\frac{1}{9}}

VSWR=1+τ1τ=2VSWR = \frac{1 + |\tau| }{1 - |\tau|} = 2

β=2πfv\beta = \frac{2\pi f}{v}, f in hertz

Z0=LCZ_0 = \sqrt{\frac{L}{C}}

Z0=ZsZL=30075=22500=150ΩZ_0 = \sqrt{Z_s \cdot Z_L} = \sqrt{300 \cdot 75} = \sqrt{22500} = 150 \, \Omega

λ=3×10850×106=6m\lambda = \frac{3 \times 10^8}{50 \times 10^6} = 6 \, \text{m}, l=λ4=64=1.5ml = \frac{\lambda}{4} = \frac{6}{4} = 1.5 \, \text{m}

Zin=Z02ZL=150275=300ΩZ_\text{in} = \frac{Z_0^2}{Z_L} = \frac{150^2}{75} = 300Ω

Now, since quarter-wave transformers are symmetric, impedance matching is still achieved even when source and load are swapped.

Impedance matching in transmission lines is the practice of ensuring the source, transmission line, and load impedances are equal to minimize signal reflections and maximize power transfer

The transmission line, if not terminated with a matched load, occurs in losses. These losses are many types such as attenuation loss, reflection loss, transmission loss, return loss, insertion loss, etc

I0+=V0+Z0=100100=1AI_0^+ = \frac{V_0^+}{Z_0} = \frac{100}{100} = 1 \, \text{A}

Iref=ΓLIinc=0.143 A I_{\text{ref}} = |\Gamma_L| \cdot I_{\text{inc}} = 0.143 \text{ A}

vf=1k=vcv_f = \frac{1}{\sqrt{k}}=\frac{v}{c}

v=vf×c=2.47×106 m/s\rightarrow v = v_f \times c = 2.47 \times 10^6 \text{ m/s}

The speed of energy transfer in the twin lead is approximately 82% of the speed of light in a vacuum.

Impedance matching in transmission lines is the practice of ensuring the source, transmission line, and load impedances are equal to minimize signal reflections and maximize power transfer

Impedance matching is necessary to maximize power transfer and minimize signal reflections in electrical circuits

Scattering Matrix

It is a square matrix which gives all the combinations of power relationships between the various input and output ports of a Microwave junction. The elements of this matrix are called "Scattering Coefficients" or "Scattering (S) Parameters".

AspectE-PlaneH-PlaneMagic Tee
DefinitionPlane of electric fieldPlane of magnetic fieldHybrid junction of E- and H-planes
Field OrientationElectric fieldMagnetic fieldCombines both fields
StructurePart of waveguide/antennaPart of waveguide/antennaFour-port device
Radiation PatternVertical (E-field direction)Horizontal (H-field direction)N/A (device, not pattern)
IsolationNo inherent isolationNo inherent isolationYes, between specific ports
Power DivisionNot applicableNot applicableEqual or controlled split
ApplicationsAntenna pattern analysisAntenna pattern analysisPower splitting, mixing
Phase BehaviorDepends on antenna designDepends on antenna design180° phase difference possible

An H-Plane Tee junction is formed by attaching a simple waveguide to a rectangular waveguide which already has two ports. The arms of rectangular waveguides make two ports called collinear ports i.e., Port1 and Port2, while the new one, Port3 is called as Side arm or H-arm. This H-plane Tee is also called as Shunt Tee.

The H-plane (Magnetic plane) is the plane containing the magnetic field vector (H-field) and the direction of propagation.

Directional coupler is a four-port device where Port 1 is the incident port, Port 2 is the through port (because it connects via a straight line). Port 4 is the coupled port, and Port 3 is the isolated port.

Properties:

TravelsCouplednot coupled
1 → 243
2 → 134
Incident through port 321
Incident through port 412

FeatureIsolatorCirculatorPhase Shifter
DefinitionAllows signal in one direction only, blocks reverseRoutes signal from one port to the next port in a circleShifts the phase of signal without changing its magnitude
Type of DeviceNon-reciprocal 2-port deviceNon-reciprocal 3 or 4-port deviceReciprocal 2-port device
Main PurposeProtects devices from reflected signalsRoutes signals between ports in a defined sequenceChanges the phase angle of a signal
Working PrincipleUses Faraday rotationUses Y-junction with magnetized ferriteUses delay lines or varactors
Signal FlowPort A → Port B only (blocks B → A)Port 1 → 2, 2 → 3, 3 → 1 (or circular path)Same signal goes through, but with phase shifted
Ports2 (3rd port used for termination)Typically 3 or 42
Insertion Loss~2 dB~0.5 – 1.5 dBIdeally low in all phase states
Key PropertyBlocks unwanted reflectionsAllows directional signal routingProvides variable or fixed phase shift
Reciprocal?NoNoYes
Common UseBetween source and load to block reflected powerIn radar or duplex communication systemsIn phased arrays, beam steering, RF control systems

Radar

Radar stands for Radio Detection and Ranging System. It detects location and distance of objects using electromagnetic energy. It is basically an electromagnetic system used to detect the location and distance of an object from the point where the RADAR is placed.

Operating range: UHF and microwave frequencies (400 MHz to 40 GHz).

[ Extra : Radar, which is used to track the path of one or more targets is known as Tracking Radar.
The pencil beams of Radar Antenna perform tracking in angle. The axis of Radar Antenna is considered as the reference direction. If the direction of the target and reference direction is not same, then there will be angular error, which is nothing but the difference between the two directions. ]

  1. Sequential Lobing
    • Antenna beams are switched alternately between two directions (beam positions) to track a target.
    • Radar alternates beam between Position 1 and Position 2.
    • Compares received signal strength from both positions.
    • Difference in signal strength indicates direction and magnitude of angular error.
  1. Conical Scanning

Satellite

A communication satellite is an orbiting artificial earth satellite that receives a communications signal from a transmitting ground station, amplifies and possibly processes it, then transmits it back to the earth for reception by one or more receiving ground stations.

Eccentricity defines the shape of the satellite orbit. It is the ratio of the distance between the foci of the ellipse to the length of its major axis. For a perfect circle, eccentricity is zero.

The Vernal Equinox is the point where the Sun crosses the Earth’s equatorial plane moving from the southern to the northern hemisphere. It is used as a reference point in the celestial coordinate system.

Right Ascension of Ascending Node is the angle measured from the vernal equinox to the ascending node of the satellite orbit, measured in the equatorial plane.

The line of nodes is the line joining the ascending and descending nodes through the centre of Earth.

Look angle is the angle between the direction of the satellite from the Earth station and the local horizontal at the Earth station.

  • The angle between local horizontal plane and the plane passing through earth station, satellite and center of earth is called as azimuth angle.
  • The angle between vertical plane and line pointing to satellite is known as Elevation angle.

The sub-satellite point is the point on the Earth's surface directly beneath the satellite at any given time.

Apogee is the farthest point of the satellite from the Earth in its orbit.

Perigee is the closest point of the satellite to the Earth in its orbit.

A transponder is an electronic device that transmits and receives radio signals

AspectAOC SubsystemTTCM Subsystem
Full FormAttitude and Orbit ControlTelemetry, Tracking, Commanding, and Monitoring
Main FunctionControls the orientation (attitude) and orbit position of the satelliteHandles communication and control between satellite and Earth station
PurposeEnsures satellite points in correct direction (e.g., antennas towards Earth, solar panels to Sun)Ensures satellite’s health, position, and commands are transmitted, received, and monitored
Methods Used-Spin stabilization (rotating body)- Three-axis stabilization (using momentum wheels)- Telemetry (sends sensor data to Earth)- Tracking (finds satellite location)- Commanding (sends control signals)
Key Components- Spinning drum- De-spin mechanism- Momentum wheels for 3-axis control- Sensors and encoders- RF transmitters for telemetry- Antennas and command receivers
Satellite StabilityKeeps satellite stable and correctly oriented in orbitKeeps satellite communicating and under control from ground
Example of UseMaking antennas continuously face Earth despite satellite motionSending temperature, pressure data to Earth; commanding thrusters to adjust orbit
  1. The orbit of a satellite around the Earth is an ellipse, with the center of mass of the Earth located at one of the two foci of the ellipse.
  1. A line joining a satellite and the Earth sweeps out equal areas in the orbital plane in equal intervals of time.
  1. The square of the orbital period of a satellite is directly proportional to the cube of the semi-major axis of its orbit.

    T2=(4π2μ)a3T^2 = \left( \frac{4\pi^2}{\mu} \right) a^3; μ=3.986004×105km3/s2\mu = 3.986004 \times 10^5 \, \text{km}^3/\text{s}^2

Distinguish between Active and Passive satellite.

AspectPassive SatelliteActive Satellite
DefinitionA satellite that only reflects signals from Earth without amplification or modification.A satellite that receives, amplifies, and retransmits signals back to Earth using onboard electronics.
FunctionReflects incoming signals from Earth.Amplifies and retransmits received signals.
Power SupplyNo onboard power; relies entirely on external transmitted energy.Contains onboard power sources to operate internal electronics.
Earth Station RequirementNeeds high power transmitters and large tracking facilities.Needs lower power Earth stations due to onboard amplification.
Control from GroundCannot be controlled once in orbit.Can be actively controlled and monitored from ground.
Signal StrengthSignal weakens significantly (high attenuation) due to long travel path and no amplification.Signal strength is maintained or enhanced due to onboard amplification (low attenuation).
User AccessOpen to random usersControlled access
ExampleEcho-I (NASA, 1960)Most modern communication satellites
Tracking FacilityNeeds large tracking stationsCompact and efficient ground stations possible
AmplificationNo Amplifies the received signals
Power GenerationCannot generate or transmit powerCan generate and transmit power

The path a Satellite follows around a planet is defined as an orbit.

AspectNon-Geostationary Orbit (NGSO)Geostationary Orbit (GSO)
DefinitionSatellites that orbit the Earth at lower altitudes and do not remain fixed relative to a point on Earth.A circular orbit directly above the equator where the satellite appears stationary from Earth because it rotates at the same speed as Earth.
Orbit AltitudeLow Earth Orbit (LEO) or Medium Earth Orbit (MEO), generally below 35,786 kmFixed at 35,786 km above the equator
Tracking RequirementComplex tracking needed; satellite moves relative to EarthSimple tracking; satellite appears fixed in the sky
Signal HandoverRequires handover of signal between satellites due to motionNo handover needed; signal from a single satellite is continuous
Lifetime & ReplacementShorter satellite life, requires frequent replacementLonger life, fewer replacements needed
Transmission DelayLower delay due to shorter distanceHigher delay (~250 ms) due to long distance
Coverage AreaCan provide global or polar coverageNo coverage at poles; best suited for equatorial and mid-latitudes
Free Space LossLower, due to closer distance to EarthHigher, due to larger distance
AspectGEO (Geostationary Earth Orbit)MEO (Medium Earth Orbit)LEO (Low Earth Orbit)
DefinitionSatellite appears stationary from Earth; orbits at 36,000 km above equator.Satellite orbits Earth at 8,000–20,000 km altitude; slower movement than LEO.Satellite orbits at 500–2,000 km altitude; fast-moving with frequent Earth passes.
Orbit TypeCircular orbit above equator, 0° inclination.Can have varied inclinations; often circular.Inclined or polar orbits; moves across Earth quickly.
CoverageCovers 1/3 of Earth per satellite; 3 satellites cover almost entire Earth.Fewer satellites needed than LEO, but more than GEO.Needs many satellites for full Earth coverage (e.g., 50–200).
Latency (Delay)High (~250 ms); not ideal for real-time data or voice.Moderate latency; better than GEO but not as good as LEO.Low latency (~10 ms); ideal for data and voice communications.
FootprintVery large; allows wide area coverage.Medium footprint; good balance between coverage and resolution.Small footprint; allows for high frequency reuse like cellular networks.
Tracking RequirementMinimal; appears stationary, so simple ground tracking.Moderate tracking needed; satellites move slowly relative to Earth.High tracking required; fast movement requires continuous tracking and handovers.
LifetimeLong (up to 15 years or more).Moderate lifetime.Short (5–8 years); affected by atmospheric drag.
Use CasesTV, radio broadcast, weather, global telephone backbone.GPS, navigation, communication systems.Mobile communication, remote sensing, Earth observation, internet (e.g., Starlink).
Advantages- Constant view of same area - Ideal for broadcasting - Minimal Doppler shift- Fewer satellites than LEO - Good regional coverage - Less complex than LEO- Low delay - Good for mobile & polar regions - Better signal strength due to proximity


Pr=PtGtAer4πR2=PtGtGr(4πRλ)2=EIRP×GrPathlossP_r = \frac{P_t G_t A_{er}}{4\pi R ^2} = \frac{P_t G_t G_r}{(\frac{4\pi R}{ \lambda} )^2} = \frac{EIRP \times G_r}{Pathloss}

PrdB=10logEIRP+10logGr10loglp=(EIRP)dB+(Gr)dB20[log4π+logRlogλ]Pr_{dB} = 10\log \text{EIRP} + 10 \log G_r - 10\log l_p \\ = (EIRP)_{dB} + (G_r)_{dB} - 20[\log4\pi + \log R -\log \lambda]

EIRPdb=10logPt+GtdB=10log6+48.2=7.78+48.2=55.98EIRP_{db} = 10\log P_t + Gt_{dB} = 10 \log 6 + 48.2 = 7.78 + 48.2 = 55.98

v2=μRv^2 = \frac{\mu}{R}v=3.99×101242220×1000=307.42 m/sv = \sqrt \frac{3.99\times10^{12}}{42220 \times 1000} = 307.42 \text{ m/s}

(c)