Publication Abstracts
Allison and Atkinson 2001
, and D.H. Atkinson, 2001: Galileo Probe Doppler residuals as the wave-dynamical signature of weakly stable, downward-increasing stratification in Jupiter's deep wind layer. Geophys. Res. Lett., 28, 2747-2750, doi:10.1029/2001GL012927.
Doppler radio tracking of the Galileo probe-to-orbiter relay, previously analyzed for its in situ measure of Jupiter's zonal wind at the equatorial entry site, also show a record of significant residual fluctuations apparently indicative of varying vertical motions. Regular oscillations over pressure depth in the residual Doppler measurements of roughly 1-8 Hz (increasing upward), as filtered over a 134 sec window, are most plausibly interpreted as gravity waves, and imply a weak, but downward increasing static stability within the 5-20 bar region of Jupiter's atmosphere. A matched extension to deeper levels of an independent inertial stability constraint from the measured vertical wind shear at 1-4 bars is roughly consistent with a static stability of ∼0.5 K/km near the 20 bar level, as independently detected by the probe Atmospheric Structure Instrument.
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BibTeX Citation
@article{al08000d, author={Allison, M. and Atkinson, D. H.}, title={Galileo Probe Doppler residuals as the wave-dynamical signature of weakly stable, downward-increasing stratification in Jupiter's deep wind layer}, year={2001}, journal={Geophysical Research Letters}, volume={28}, pages={2747--2750}, doi={10.1029/2001GL012927}, }
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RIS Citation
TY - JOUR ID - al08000d AU - Allison, M. AU - Atkinson, D. H. PY - 2001 TI - Galileo Probe Doppler residuals as the wave-dynamical signature of weakly stable, downward-increasing stratification in Jupiter's deep wind layer JA - Geophys. Res. Lett. JO - Geophysical Research Letters VL - 28 SP - 2747 EP - 2750 DO - 10.1029/2001GL012927 ER -
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