Jupiter's Temperate Belt/Zone Contrasts Revealed at Depth by Juno Microwave Observations-Reference-Cited by-同舟云学术

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Jupiter's Temperate Belt/Zone Contrasts Revealed at Depth by Juno Microwave Observations

Published:2021-05-14 Issue: Volume: Page:
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Author:

Fletcher Leigh N¹^ORCID,Oyafuso Fabiano A²,Allison Michael D³,Ingersoll Andrew⁴^ORCID,Li Liming⁵^ORCID,Kaspi Yohai⁶^ORCID,Galanti Eli⁶^ORCID,Wong Mike H⁷,Orton Glenn S⁸^ORCID,Duer Keren⁶,Zhang Zhimeng⁹^ORCID,Li Cheng¹⁰,Guillot Tristan¹¹^ORCID,Levin Steven M.²^ORCID,Bolton Scott J¹²^ORCID

Affiliation:

1. University of Leicester

2. Jet Propulsion Laboratory

3. Goddard Institute for Space Studies

4. Caltech

5. University of Houston

6. Weizmann Institute of Science

7. SETI Institute

8. Jet Propulsion Laboratory, California Institute of Technology

9. California Institute of Technology

10. University of Michigan

11. Observatoire de la Cote d'Azur

12. Southwest Research Institute

Funder

European Research Council

Publisher

Wiley

Reference101 articles.

1. Cassini CIRS retrievals of Ammonia in Jupiter’s Upper Troposphere;Achterberg R. K.;Icarus,2006

2. February). Planetary waves in Jupiter’s equatorial atmosphere;Allison M.;Icarus,1990

3. Galileo Probe Doppler residuals as the wave-dynamical signature of weakly stable, downward-increasing stratification in Jupiter’s deep wind layer;Allison M.;Geophys. Res. Lett.,2001

4. Sep). Jupiter’s Atmospheric Variability from Long-term Ground-based Observations at 5 µm;Antuñano A.;Astronomical Journal,2019

5. September). The GalileoJupiter Probe Doppler Wind Experiment;Atkinson D. H.;Solar System Research,2001

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