activity
20232025
most citedInflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution

5 citations · 13 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2025★ 5 cited

Inflated hot Jupiters: Inferring average atmospheric velocity via Ohmic models coupled with internal dynamo evolution

Daniele Viganò, Soumya Sengupta, Clàudia Soriano-Guerrero +4

The inflated radii observed in hundreds of hot Jupiters (HJ) represent a long-standing open issue. In this study, we quantitatively investigate this phenomenon within the framework…

astro-ph.EP2025

Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters

Albert Elias-López, Matteo Cantiello, Daniele Viganò +3

Hot Jupiters (HJs) are commonly thought to host the strongest dynamo-generated magnetic fields among exoplanets, up to one order of magnitude larger than Jupiter. Thus, they have o…

astro-ph.GA2024★ 3 cited

Vorticity and magnetic dynamo from subsonic expansion waves II: Dependence on magnetic Prandtl number, forcing scale, cooling time

Albert Elias-López, Fabio del Sordo, Daniele Viganò

The amplification of astrophysical magnetic fields takes place via dynamo instability in turbulent environments. The presence of vorticity is crucial for the dynamo to happen. Howe…

astro-ph.EP2024

The role of Ohmic dissipation of internal currents on Hot Jupiter radii

Taner Akgün, Clàudia Soriano-Guerrero, Albert Elias-López +3

The inflated radii observed in hundreds of Hot Jupiters represent a long-standing open issue. The observed correlation between radii and irradiation strength, and the occasional ex…

astro-ph.GA2023★ 5 cited

Vorticity and magnetic dynamo from subsonic expansion waves

Albert Elias-López, Fabio Del Sordo, Daniele Viganò

This work concentrates on the effect of an irrotational forcing on a magnetized flow in the presence of rotation, baroclinicity, shear, or a combination of them. By including magne…