Data Set Overview
  =================
    From [SEIFFETAL1996]:
 
    The Galileo Probe Atmospheric Structure Instrument (ASI) measured
    state properties of Jupiter's atmosphere from nanobar pressure
    levels to a final pressure of ~24 bars.  The depth reached in the
    probe's parachute descent, calculated from measured temperatures
    and pressures assuming hydrostatic equilibrium, was ~160 km or
    0.22% of the radius of Jupiter.  Velocities during descent
    decreased from ~400 m/s at parachute deployment to 156 m/s in the
    first 100 s, to ~48 m/s at the 3-bar level, and to ~30 m/s at
    loss of signal.
 
    Temperatures measured in parachute descent had an accuracy of ~1
    K and a dispersion on the order of the digital resolution (0.12
    K).  Comparison with the Orton model indicates that the
    atmosphere is close to a dry adiabat over this pressure range.
    Water condensation, expected above the 5-bar level if the oxygen
    mole fraction is solar (0.0017) and above the 4-bar level for the
    low water abundance detected by the neutral mass spectrometer
    (~0.2 of the solar abundance value), has major effects on the
    temperature variation.  Temperatures following the dry adiabat at
    these levels confirm the low water abundance and are consistent
    with the absence of a detectable water cloud.  Deviations from
    the adiabat between 1 and 3 bars, which were initially
    interpreted as a stable layer in the tenuous cloud above 1.6 bars
    and an unstable layer below the cloud, now are believed to
    reflect departures from preflight pressure sensor calibrations
    resulting from unanticipated variations in the probe's internal
    temperature.

Confidence Level Overview
  =========================
    Details can be found in [SEIFFETAL1996].