Jupiter atmospheric dynamics from ground-based Doppler imaging

François-Xavier X Schmider , Ivan Gonçalves (1) , Tristan Guillot , Jason Jackiewicz (2) , Thomas Underwood (2) , Patrick Gaulme (3) , David Voelz (2) , Thierry Appourchaux (4) , Patrick Boumier (4) , Raùl Morales-Juberias (5) , Masahiro Ikoma (6) , Bun'Ei Sato (7) , Hideyuki Izumiura (8)

1 LAGRANGE - Joseph Louis LAGRANGE
2 NMSU, Dept Astron, Las Cruces, NM USA
3 Max Planck Inst Sonnensyst Forsch, Gottingen, Germany
4 IAS - Institut d'astrophysique spatiale
5 NMT - New Mexico Institute of Mining and Technology [New Mexico Tech]
6 Tokyo University of Science [Tokyo]
7 TITECH - Tokyo Institute of Technology [Tokyo]
8 OAO - Okayama Astrophysical Observatory

We present velocity maps of Jupiter obtained from the ground with a dedicated Doppler imaging spectrograph. It demonstrates the potential of this method to study the motion in the atmosphere of gaseous planets. It proves to be complementary to cloud-tracking to understand the atmospheric dynamics

Domaines: Astrophysique [astro-ph]

François-Xavier X Schmider, Ivan Gonçalves, Tristan Guillot, Jason Jackiewicz, Thomas Underwood, et al.. Jupiter atmospheric dynamics from ground-based Doppler imaging. EPSC-DPS Joint Meeting 2019, Sep 2019, Genève, Switzerland. pp.EPSC-DPS2019-1613-2. ⟨hal-03007356⟩