Santiago Andrés TrianaJul 28, 2023

Do you work on #fluiddynamics of #planetaryCores /moons/atmospheres or #stars? submit your abstract to our #interdisciplinary session for this year's AGU meeting in San Francisco!

https://agu.confex.com/agu/fm23/prelim.cgi/Session/185760

#AGU23 #InertialWaves #GravityWaves #Asteroseismology #Helioseismology #PlanetaryScience
#IcyMoons #GasGiants

<i>Oscillations in internal fluid layers of planets, moons and stars</i>

Oscillations in internal fluid layers play an important role in the dynamics and evolution of planets, moons and stars. In these objects, the Coriolis force supports the existence of inertial waves, while buoyancy gives rise to internal gravity waves. When a magnetic field is present, magnetic Alfvén waves can also exist. In realistic situations, all these types of motion combine to produce complex oscillations.  While inertial (Rossby) and internal gravity waves were initially described in the context of atmospheric and oceanic science, they are also a long-standing subject of study in the Earth’s liquid core and in the subsurface oceans of icy moons. Inertial waves have also been recently identified in Sun's convective envelope and are cited as an important ingredient in gas giants' dynamics.  This interdisciplinary session aims to bring together scientists from the Earth, Solar, and planetary communities to synergistically consolidate our collective knowledge of these phenomena.

AGU - AGU23
Santiago Andrés TrianaJul 28, 2023

Do you work on #fluiddynamics of #planetaryCores /moons/atmospheres or #stars? submit your abstract to our #interdisciplinary session for this year's AGU meeting in San Francisco!

https://agu.confex.com/agu/fm23/prelim.cgi/Session/185760

#AGU23 #InertialWaves #GravityWaves #Asteroseismology #Helioseismology #PlanetaryScience
#IcyMoons #GasGiants

<i>Oscillations in internal fluid layers of planets, moons and stars</i>

Oscillations in internal fluid layers play an important role in the dynamics and evolution of planets, moons and stars. In these objects, the Coriolis force supports the existence of inertial waves, while buoyancy gives rise to internal gravity waves. When a magnetic field is present, magnetic Alfvén waves can also exist. In realistic situations, all these types of motion combine to produce complex oscillations.  While inertial (Rossby) and internal gravity waves were initially described in the context of atmospheric and oceanic science, they are also a long-standing subject of study in the Earth’s liquid core and in the subsurface oceans of icy moons. Inertial waves have also been recently identified in Sun's convective envelope and are cited as an important ingredient in gas giants' dynamics.  This interdisciplinary session aims to bring together scientists from the Earth, Solar, and planetary communities to synergistically consolidate our collective knowledge of these phenomena.

AGU - AGU23