
- Select a language for the TTS:
- UK English Female
- UK English Male
- US English Female
- US English Male
- Australian Female
- Australian Male
- Language selected: (auto detect) - EN
Play all audios:
ABSTRACT The atmosphere of Jupiter has a complex circulation which, until recently, has been observable only at the cloud tops1,2; the mechanisms driving the winds, and the nature of the
interior circulation, remained unknown3. Recent analyses4,5,6 of the radio signal from the Galileo probe, obtained during its descent into the jovian atmosphere, have suggested a vigorous
interior circulation below the 4-bar level. Here we report an independent measurement of the winds below the cloud tops, making use of the data obtained by the two accelerometers on the
descending probe. We find evidence for two distinct wind regimes, in general agreement with the Doppler radio measurements: a region of wind shear between 1 and 4 bar, where the wind speed
increases dramatically with depth; and then a region of constant high-velocity winds down to at least the 17-bar level. Access through your institution Buy or subscribe This is a preview of
subscription content, access via your institution ACCESS OPTIONS Access through your institution Subscribe to this journal Receive 51 print issues and online access $199.00 per year only
$3.90 per issue Learn more Buy this article * Purchase on SpringerLink * Instant access to full article PDF Buy now Prices may be subject to local taxes which are calculated during checkout
ADDITIONAL ACCESS OPTIONS: * Log in * Learn about institutional subscriptions * Read our FAQs * Contact customer support SIMILAR CONTENT BEING VIEWED BY OTHERS VARIATIONS IN THE EARTH’S
ROTATION RATE MEASURED WITH A RING LASER INTERFEROMETER Article 18 September 2023 DISCOVERY OF HIGH-FREQUENCY RETROGRADE VORTICITY WAVES IN THE SUN Article 24 March 2022 TETHERED
BALLOON-BORNE TURBULENCE MEASUREMENTS IN WINTER AND SPRING DURING THE MOSAIC EXPEDITION Article Open access 19 October 2023 REFERENCES * Limaye, S. et al. Jovian winds from Voyager 2, Part
I: zonal mean circulation. _J. Atmos. Sci._ 39, 1413–1432 (1982). Google Scholar * Beebe, R. F., Simon, A. A. & Huber, L. F. Comparison of Galileo Probe and Earth-based translation
rates of Jupiter's equatorial clouds. _Science_ 272, 841 (1996). Google Scholar * Pollack, J. B., Atkinson, D. H., Seiff, A. & Anderson, J. D. Retrieval of a wind profile from the
Galileo Probe telemetry signal. _Space Sci. Rev._ 60, 143–178 (1992). Google Scholar * Atkinson, D. P., Pollack, J. B. & Seiff, A. Galileo Doppler measurements of the deep zonal winds
at Jupiter. _Science_ 272, 842–843 (1996). Google Scholar * Atkinson, D. H., Ingersoll, A. P. & Seiff, A. Deep winds on Jupiter as measured by the Galileo probe. _Nature_ 388, 649–650
(1997). Google Scholar * Folkner, W. M. Earth-based radio tracking of the Galileo Probe for Jupiter wind estimation. _Science_ 275, 844–845 (1997). Google Scholar * Seiff, A. & Knight,
T. C. D. K. The Galileo Probe atmosphere structure instrument. _Space Sci. Rev._ 60, 203–232 (1992). Google Scholar * Seiff, A. et al. Structure of the atmosphere of Jupiter: Galileo Probe
measurements. _Science_ 272, 844–845 (1996). Google Scholar * Ingersoll, A. P. & Cuzzi, J. N. Dynamics of Jupiter's cloud bands. _J. Atmos. Sci._ 26, 981–985 (1969). Google
Scholar * Anderson, J. D. in _Jupiter_ (ed. Gehrels, J.) 113–121 (Univ. Arizona Press, Tucson, 1976). Google Scholar Download references ACKNOWLEDGEMENTS We thank the Galileo Project and
NASA's Planetary Atmospheres Program. This work was supported by NASA. AUTHOR INFORMATION AUTHORS AND AFFILIATIONS * NASA-Ames Research Centre, Moffett Field, 94035, California, USA A.
Seiff, J. D. Mihalov & R. E. Young * Department of Meteorology, San Jose State University, San Jose, California, USA A. Seiff * NASA Langley Field, MS-107, Hampton, 23665, Virginia, USA
R. C. Blanchard * Department of Earth, Space Science, UCL, Los Angles, 90024, California, USA G. Schubert * Department of Electrical Engineering, University of Idaho, Moscow, 83844, Idaho,
USA D. Atkinson * Retired, T. C. D. Knight & D. B. Kirk Authors * A. Seiff View author publications You can also search for this author inPubMed Google Scholar * R. C. Blanchard View
author publications You can also search for this author inPubMed Google Scholar * T. C. D. Knight View author publications You can also search for this author inPubMed Google Scholar * G.
Schubert View author publications You can also search for this author inPubMed Google Scholar * D. B. Kirk View author publications You can also search for this author inPubMed Google
Scholar * D. Atkinson View author publications You can also search for this author inPubMed Google Scholar * J. D. Mihalov View author publications You can also search for this author
inPubMed Google Scholar * R. E. Young View author publications You can also search for this author inPubMed Google Scholar CORRESPONDING AUTHOR Correspondence to A. Seiff. RIGHTS AND
PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE Seiff, A., Blanchard, R., Knight, T. _et al._ Wind speeds measured in the deep jovian atmosphere by the Galileo
probe accelerometers. _Nature_ 388, 650–652 (1997). https://doi.org/10.1038/41721 Download citation * Received: 10 March 1997 * Accepted: 25 June 1997 * Issue Date: 14 August 1997 * DOI:
https://doi.org/10.1038/41721 SHARE THIS ARTICLE Anyone you share the following link with will be able to read this content: Get shareable link Sorry, a shareable link is not currently
available for this article. Copy to clipboard Provided by the Springer Nature SharedIt content-sharing initiative