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By: Agrima Kothari
1
Content
 Introduction
 Laser
 Why laser?
 Objectives
 Flight payload
 Flight Optical Communications Module
 Flight modem
 DPSK
 PPM
 High speed electronics
 LCRD ground station
 LCRD ground station1
 LCRD ground station2
 LMOC
 Advantages
 Application
 Conclusion
2
Introduction
 LCRD is a joint project between
 NASA/GSFC (Goddard space flight center)
 MIT/LL (Massachusetts Institute of Technology / Lincoln Laboratory)
 Demonstrating how optical communications can meet NASA’s
growing need for higher data rates
 Provide two years of continuous high data rate
 Lower power, lower mass communications systems on
spacecraft.
3
Laser
 Light Amplification by
Stimulated Emission of
Radiation
 Output is narrow beam
 The beam is:
 Highly coherent
 Monochromatic
 Directional
4
Why laser?
 Used in optical communication.
 Basic idea was
 Establish a communication link between earth and satellite
 to increase the data rates
 For same mass, power, and volume higher data rates
achieved.
 For same data rate will require less mass, power, and
volume.
5
Objectives
 Near Earth applications
 Following were demonstrated:
 High rate bi-directional communications between Earth and
GEO.
 Real-time optical relay between 2 Ground Stations.
 Pulse Position Modulations.
 DPSK Modulations.
 Performance testing.
6
Flight Payload
 Optical communications terminal
 An optical module
 A modem
 An optical module controller
 High speed electronics
 To interconnect the two optical modules.
 Perform network and data processing.
 To interface to the host spacecraft.
7
Flight Optical Module construction
 Two optical communication
terminals
 Each optical module is a 4-inch
reflective telescope
 It houses a spatial acquisition
detector
 Telescope mounted on a 2 axis
stand & stabilized by MIRU
 Optical fibers couple the
optical module to the modems
 Each optical module is held and
protected during launch with a
cover and one time launch
latch.
8
Flight Optical Module working
 Transmit and receive optical signals.
 When transmitting
 To efficiently generate optical power
 Encode, format, and interleave incoming electronic data
 Modulate the optical beam
 Amplify and transmit
 Aim the very narrow beam at the ground station
 When receiving
 Large collector
 Couple light onto low noise efficient detectors
 Synchronization, demodulation and decoding
9
Flight modem
 Two types of mission
 Deep space mission
 Near earth mission
 Differ in range and data rates
 Different modulation techniques are used
 LCRD will demonstrate both techniques
10
DPSK
 Used for near earth mission
 A bit is encoded in the phase difference between
consecutive pulses
 2.88 GHz Clock rate
 Data rate from 72 Mbps to 2.88 Gbps.
 In future data rates beyond 10 Gbps.
11
PPM
 Used in deep space mission
 2.88 GHz clock rate
 Downlinks up to 100 Mbps
 Uplinks up to 1Gbps
 Maximum data rate is 360 Gbps
12
High Speed Electronics
 Objective is to demonstrate advanced relay operations
 Challenge is the susceptibility to cloud cover.
 Significant amount of data storage in order to demonstrate
store and forward relay services.
 HSE will support delay tolerant network (DTN) protocols.
 Implement required decoding and de-interleaving so the
payload can process and route the data.
13
LCRD ground segment
 LCRD mission operation
center (LMOC )
 Two ground stations
 LCRD Ground Station 1
 LCRD Ground Station 2
14
LMOC
 LCRD Mission Operations Center
 LMOC coordinates all optical communications activities
 LMOC communicates with all segments:
 Two ground stations
 Space segment
 The LMOC will provide services such as:
 Planning and scheduling
 Control
 Status Monitoring
 Reporting and Accountability
15
LCRD Ground Station 1
 OCTL is located in the San
Gabriel Mountains of southern
California
 The large aperture readily supports
the high data rate
 Required to operate 24/7 in the
presence of winds
 OCTL telescope enclosed in a
temperature controlled dome
 The Laser Safety System at the
OCTL will ensure safe laser beam
transmission
16
LCRD Ground Station 2
 MIT Lincoln Laboratory
designed the Lunar
Lasercom Ground
Terminal (LLGT) in
Hawaii
 The LLGT is an array of
 Four 40-cm receive
reflective telescopes
 Four 15-cm transmit
refractive telescopes
17
Advantages
 Relatively simple, yet
highly reliable.
 Six times faster in
delivering data.
 Increase in bandwidth of
five to six orders of
magnitude.
 Mass, weight and power
are reduced.
18
Application
 High resolution images of
interstitial objects
 Able to stream high
definition video
 Telepresence
 Carry more fuel or other
equipments
 Military operations
19
Conclusion
 In time, space communication will extend humanities
reach into space.
 Doing this demonstration will allow initial operational
capability (IOC) of an optical service on the first next
generation satellite.
20
Thank you !
21
Queries?
22

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Lc

  • 2. Content  Introduction  Laser  Why laser?  Objectives  Flight payload  Flight Optical Communications Module  Flight modem  DPSK  PPM  High speed electronics  LCRD ground station  LCRD ground station1  LCRD ground station2  LMOC  Advantages  Application  Conclusion 2
  • 3. Introduction  LCRD is a joint project between  NASA/GSFC (Goddard space flight center)  MIT/LL (Massachusetts Institute of Technology / Lincoln Laboratory)  Demonstrating how optical communications can meet NASA’s growing need for higher data rates  Provide two years of continuous high data rate  Lower power, lower mass communications systems on spacecraft. 3
  • 4. Laser  Light Amplification by Stimulated Emission of Radiation  Output is narrow beam  The beam is:  Highly coherent  Monochromatic  Directional 4
  • 5. Why laser?  Used in optical communication.  Basic idea was  Establish a communication link between earth and satellite  to increase the data rates  For same mass, power, and volume higher data rates achieved.  For same data rate will require less mass, power, and volume. 5
  • 6. Objectives  Near Earth applications  Following were demonstrated:  High rate bi-directional communications between Earth and GEO.  Real-time optical relay between 2 Ground Stations.  Pulse Position Modulations.  DPSK Modulations.  Performance testing. 6
  • 7. Flight Payload  Optical communications terminal  An optical module  A modem  An optical module controller  High speed electronics  To interconnect the two optical modules.  Perform network and data processing.  To interface to the host spacecraft. 7
  • 8. Flight Optical Module construction  Two optical communication terminals  Each optical module is a 4-inch reflective telescope  It houses a spatial acquisition detector  Telescope mounted on a 2 axis stand & stabilized by MIRU  Optical fibers couple the optical module to the modems  Each optical module is held and protected during launch with a cover and one time launch latch. 8
  • 9. Flight Optical Module working  Transmit and receive optical signals.  When transmitting  To efficiently generate optical power  Encode, format, and interleave incoming electronic data  Modulate the optical beam  Amplify and transmit  Aim the very narrow beam at the ground station  When receiving  Large collector  Couple light onto low noise efficient detectors  Synchronization, demodulation and decoding 9
  • 10. Flight modem  Two types of mission  Deep space mission  Near earth mission  Differ in range and data rates  Different modulation techniques are used  LCRD will demonstrate both techniques 10
  • 11. DPSK  Used for near earth mission  A bit is encoded in the phase difference between consecutive pulses  2.88 GHz Clock rate  Data rate from 72 Mbps to 2.88 Gbps.  In future data rates beyond 10 Gbps. 11
  • 12. PPM  Used in deep space mission  2.88 GHz clock rate  Downlinks up to 100 Mbps  Uplinks up to 1Gbps  Maximum data rate is 360 Gbps 12
  • 13. High Speed Electronics  Objective is to demonstrate advanced relay operations  Challenge is the susceptibility to cloud cover.  Significant amount of data storage in order to demonstrate store and forward relay services.  HSE will support delay tolerant network (DTN) protocols.  Implement required decoding and de-interleaving so the payload can process and route the data. 13
  • 14. LCRD ground segment  LCRD mission operation center (LMOC )  Two ground stations  LCRD Ground Station 1  LCRD Ground Station 2 14
  • 15. LMOC  LCRD Mission Operations Center  LMOC coordinates all optical communications activities  LMOC communicates with all segments:  Two ground stations  Space segment  The LMOC will provide services such as:  Planning and scheduling  Control  Status Monitoring  Reporting and Accountability 15
  • 16. LCRD Ground Station 1  OCTL is located in the San Gabriel Mountains of southern California  The large aperture readily supports the high data rate  Required to operate 24/7 in the presence of winds  OCTL telescope enclosed in a temperature controlled dome  The Laser Safety System at the OCTL will ensure safe laser beam transmission 16
  • 17. LCRD Ground Station 2  MIT Lincoln Laboratory designed the Lunar Lasercom Ground Terminal (LLGT) in Hawaii  The LLGT is an array of  Four 40-cm receive reflective telescopes  Four 15-cm transmit refractive telescopes 17
  • 18. Advantages  Relatively simple, yet highly reliable.  Six times faster in delivering data.  Increase in bandwidth of five to six orders of magnitude.  Mass, weight and power are reduced. 18
  • 19. Application  High resolution images of interstitial objects  Able to stream high definition video  Telepresence  Carry more fuel or other equipments  Military operations 19
  • 20. Conclusion  In time, space communication will extend humanities reach into space.  Doing this demonstration will allow initial operational capability (IOC) of an optical service on the first next generation satellite. 20