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Nutation in Ulysses Third Orbit

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Analysis of the past nutation season and predictions for the upcoming season ... Nutation Control: Closed Loop CONSCAN. Onboard attitude control system ... – PowerPoint PPT presentation

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Title: Nutation in Ulysses Third Orbit


1
Nutation in Ulysses Third Orbit
  • Daniel Presti, Colin Goulding

2
Presentation Overview
  • The Ulysses mission
  • Ulysses nutation anomaly
  • Nutation in the third orbit
  • Analysis of the past nutation season and
    predictions for the upcoming season
  • Operations concepts

3
Mission Overview
  • 6 October 1990 Launch (Space Shuttle Discovery)
  • 1992 Jupiter flyby and injection into polar
    orbit
  • 1994-1995 First set of polar passes
  • 2000-2001 Second set of polar passes
  • 2006-2008 Third set of polar passes

4
The Ulysses Spacecraft
  • Spin-stabilised at 5 rpm
  • Thermally isolated
  • Two internal platforms
  • Power provided by RTG
  • Two 35 m wire booms
  • One axial boom
  • One radial boom
  • Attitude control provided by hydrazine thrusters
  • High-gain antenna (1.65 m) for X-Band downlink
    and S-Band uplink

5
Instruments and Investigations
6
The Nutation Anomaly
  • Caused by thermal distortions of the axial boom,
    when partially illuminated by the Sun
  • Occurs around perihelion
  • Spacecraft wobbles about its spin axis,
    coupling energy into wire booms
  • Can grow exponentially, if left uncontrolled

7
Nutation Forcing Function (NFF)
  • Quantifies the intensity of nutation (build-up
    rates)
  • Based only on solar aspect angle (SAA) and range
    (R)
  • SAA determines the fraction of the boom
    illuminated by the Sun
  • R determines the intensity of the incident
    radiation

8
Nutation Control Closed Loop CONSCAN
  • Onboard attitude control system
  • Requires a stable uplink from a ground station
    for closed-loop control
  • Estimates the Earth off-pointing (amplitude and
    phase) by measuring physical properties of the
    receivers AGC signal (conical scanning)
  • Fires thrusters to re-align the spin axis with
    the Earth
  • Reduces the Earth off-pointing
  • Damps the nutation (secondary effect)
  • Two pre-defined selectable deadbands (wide and
    narrow)

9
The Third Orbits Nutation Season
  • From February 2007 to February 2008
  • NFF comparable to second orbits season
  • Lower RTG power
  • Minimal power margin
  • Mutually-exclusive operations
  • Reduced DSN ground station coverage
  • Large gaps with uncontrolled nutation build-up

10
Analysis of Previous Nutation Season
  • Based on high-rate attitude data from the 2001
    season (instantaneous Earth off-pointing and
    nutation angle)
  • Empirical characterisation of the nutation
    build-up rates and CONSCANs nutation damping
    performance

11
MAGIC
  • Maximum Allowable Gaps In CONSCAN operations have
    been defined, based on predicted nutation
    build-up rates
  • As gaps in nutation control increase
  • Nutation increases above acceptable levels
    (science-defined)
  • Loss of downlink due to off-pointing
  • Severe increase in unwanted oscillations in wire
    booms
  • Loss of spacecraft?

12
Ground Station Coverage Requirements
  • Maximum acceptable nutation limit defined as 0.5
    half-cone (science-driven)
  • Resulting gaps in station coverage based on
    maximum gaps in CONSCAN, minus an operational
    overhead
  • Almost-continuous coverage required at the peak
    of the nutation season

13
Typical Nutation Operations Sequence
  • Two nutation-control CONSCAN session per pass
  • Uplink of commands during CONSCAN sessions
  • High-rate playback of recorded data in between
    CONSCAN sessions
  • Gap in coverage (lt MAGIC) with nutation build-up
    and data recording

14
DSN Visibility
  • DSN designed primarily for in-ecliptic spacecraft
  • Non-continuous visibility between March and July
    2007
  • DSN gap exceeds maximum allowable gap!

15
Use of Kourou
  • The ESA Kourou station can fill the gap almost
    entirely
  • Negotiations for the use of other stations for
    nutation control are currently taking place

16
Conclusions
  • The Ulysses extended mission operations are
    challenging due to the diminishing resources
  • The nutation anomaly increases the challenge
    significantly
  • Nutation control has to take place with reduced
    coverage and mutually-exclusive spacecraft
    operations
  • A detailed characterisation of the past nutation
    season took place, leading to
  • An improved understanding and quantification of
    the nutation phenomenon
  • A proven need for additional ground resources
    during critical phases
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