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Steps towards the Standardization of a more efficient Uplink Protocol and Code

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Title: Steps towards the Standardization of a more efficient Uplink Protocol and Code


1
Steps towards the Standardization of a more
efficient Uplink Protocol and Code
  • Greg J. Kazz
  • Ed Greenberg
  • NASA/JPL

2
Problem Statement
  • Greater Demand It is anticipated that greater
    uplink data throughput is required for future
    lunar and deep space missions. These trends are
    driven by
  • Use of Selective repeat (ARQ) protocols ,e.g.,
    CFDP
  • Available Uplink margin while using ARQ
  • Standalone antenna replacement with arrays
  • On-board applications demand larger uplink
    volumes
  • Video applications drive data rates

CFDP CCSDS File Delivery Protocol
3
IOAG Requirement
  • Need for a standard approach Develop the
    functional and performance requirements for a
    CCSDS telecommand standard accommodating data
    rates up to 10 Mb/s by the year 2007.
  • CCSDS Working Group High Rate Uplink WG formed
    to provide an integrated solution across
  • RF Modulation
  • Channel Coding
  • Link Layer Protocols
  • IOAG is the Interagency Operations Advisory
    Group composed of ASI, CNES, DLR, ESA, JAXA,
    NASA.

4
ARQ Protocols are a potential Uplink Hog
  • How do ARQ protocols require more bandwidth?
  • Example
  • If downlink rate is 30 Mb/sec and file size is
    6Mb, then ground receives 5 files/second.
  • CFDP transfers 5 Finish Messages per second (file
    accepted by the ground) to the spacecraft
  • Each Finish message is 160 bits long.
  • 5 x 160 800 bits/sec
  • Assuming nominal 2000 bit/sec uplink, CFDP
    nominal traffic is 40 which is required
    throughout the pass
  • Worst case If retransmission necessary, more
    bandwidth needed

5
But ARQ can provide more Uplink Margin
  • Typical deep space mission operate with minimum 3
    dB uplink margin and require a minimum BER of
    10-5.
  • By operating at 10-4 BER, a factor of 10 more
    errors can occur, but selective or preemptive
    retransmission fills in the missing file elements
  • When sufficient RT light time permits use
    selective repeat (e.g., CFDP acknowledged mode)
  • Else use Preemptive Retransmission (send
    duplicates) for small subsets of critical data

6
Other Considerations
  • Standalone Antenna Replacement with Arrays
  • An array is efficient for supporting multiple
    spacecraft per aperture but is unproven for
    uplink.
  • Initial array operations will time share the
    uplink which result in shorter commanding times
    per mission
  • On-board Applications require larger volume
    Uplinks
  • Software radio reconfiguration (FPGAs)
  • Flight Software Uploads
  • Video applications require high rates for manned
    missions

7
Uplink Constraints Physical Layer
  • Current State of the Art (SDST) deep space
    transponders are data rate limited
  • Maximum uplink rate 4 Kb/sec
  • Receiver Symbol SNR requirements limit the use
    of high performance codes
  • Frequency bands and allocated bandwidths must
    meet SFCG guidelines
  • Cost of reducing receiver thermal noise is
    significant

8
Uplink Constraints Coding Layer
  • The chosen code must be relatively easy for the
    flight system to implement
  • Provide a mechanism to ensure extremely low
    undetected frame error rates
  • Coding gain increases with increasing block size
    increases and decreasing code rate
  • To benefit from the coding gain of state of the
    art coding, two things must be achieved in the
    receiver
  • More power must allocated to the data and less to
    the carrier. (Set the Mod index)
  • Receiver must be capable of operating at much
    lower Symbol Signal to Noise Ratios (SSNR)

9
Uplink Constraints Link Layer
  • Additional requirements for carrying voice and
    video along with data
  • Create a data system that provides varying
    Qualities of Service based upon the data type
    (Low latency voice vs low error tolerant video).
  • Potential need to multiplex IP and other types of
    data
  • CCSDS link layer provides a rich set of
    multiplexing capability
  • IP, SCPS, CCSDS Space packets, Encapsulation
    packets onto the same or different virtual
    channels
  • Maximum frame length limits for data latency
    considerations
  • Current max frame length is 16,384 bits
    (constrained by 1st header pointer)
  • Frame lengths could be extended but current
    proposed block code lengths do not exceed it
  • Use of Block Codes on the uplink requires a
    synchronous data link
  • Currently the CCSDS Telecommand standard is an
    asynchronous data link

10
Uplink Application Profiles
11
Acknowledgement
  • The authors also acknowledge the contribution of
    Ken Andrews, Dariush Divsalar, Sam Dollinar, Jon
    Hamkins, Bruce Moision and Fabrizio Pollara of
    JPLs Communications Architectures Research
    Section for the coding related aspects of this
    paper.

12
Conclusion
  • This paper summarizes the issues, constraints,
    and potential benefits associated with developing
    a standard higher rate uplink throughput to space
    missions.
  • CCSDS has embarked upon the creation of a High
    Rate Uplink Working Group
  • Charter is to develop an integrated RF and
    modulation, channel coding, and link layer
    solution to the high rate uplink needs expressed
    in this paper.
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