lec8

23
CE-462 FALL 2010 SATELLITE COMMUNICATIONS Lecture 8 Link Design (Part 4)

Upload: samsim1232

Post on 30-Sep-2015

214 views

Category:

Documents


0 download

DESCRIPTION

Satellite

TRANSCRIPT

  • CE-462 FALL 2010SATELLITE COMMUNICATIONSLecture 8Link Design (Part 4)

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Downlink Design

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 1 (1):Noise Temperature

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 1 (2):Noise Temperature

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 1 (3):Noise Temperature

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 2 (1):Lossy Elements

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 2 (2):Lossy Elements

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 2 (3):Lossy Elements

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 2 (4):Lossy Elements

    Institute of Space Technology

  • 04-Nov-2010Institute of Space Technology*Note:When system noise temperature is low, each 0.1 dB of attenuation ahead of RF amplifier will add approx. 6.6 K (290(1-1/100.01))

    Institute of Space Technology

  • Carrier power to noise power spectral density ratio at Rx input04-Nov-2010Institute of Space Technology*Carrier power: C = PRNoise power spectral density: No = kT

    or,C/No = (transmitter EIRP) (1/path loss) x (composite receiving gain/noise temperature) x (1/k)C/No = (EIRP)(1/L)(G/T)(1/k)

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 3: (1)Link Budget: DBS-TV

    Institute of Space Technology

  • Numerical Example 3: (2)Link Budget: DBS-TVIF filter designed to approximate root raised cosine (RRC) transfer function Noise BW of all RRC filters is always equal to the symbol rate of the digital txn.In DBS-TV system, QPSK signal with symbol rate = 20 Msps is assumedAntenna noise temperature = 35KLNA noise temp = 110K04-Nov-2010Institute of Space Technology*

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 3: (3)Link Budget: DBS-TV

    Institute of Space Technology

  • Selection of C/N marginsC/N margins used in DBS-TV systems are usually quiet small to avoid the need for large receiving antennaThe selection of C/N margins is a design tradeoff between:the outage level that customers can be expected to tolerate, the max allowable diameter for a receiving dish antenna, and the power o/p from the satellite transponders04-Nov-2010Institute of Space Technology*

    Institute of Space Technology

  • Reduction in C/N due to increase in sky noise temperatureTotal path attenuation:

    Sky noise temperature:

    Coupling coefficient, of 90 to 95% is usedAntenna noise temperature:

    System noise temp:

    04-Nov-2010Institute of Space Technology*

    Institute of Space Technology

  • Increase in noise power:

    Received power reduced by attenuation:

    Resulting downlink (C/N) in rain:

    04-Nov-2010Institute of Space Technology*

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 4: (1)Intelsat IV A Downlink Antenna Beams

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 4: (2)Intelsat IV A Downlink

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 4: (3)Intelsat IV A Downlink

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 4: (4)Intelsat IV A Downlink

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Numerical Example 4: (5)Intelsat IV A Downlink

    Institute of Space Technology

  • 9/16/2009Institute of Space Technology*Note: Link Budgets and Multiple Access

    Institute of Space Technology

    *