activity
20092024
most citedA magnetic field evolution scenario for brown dwarfs and giant planets

166 citations · 308 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2024

The Effects of a Stably Stratified Region with radially varying Electrical Conductivity on the Formation of Zonal Winds on Gas Planets

Paula N. Wulff, Ulrich R. Christensen, Wieland Dietrich +1

The outer areas of Jupiter and Saturn have multiple zonal winds, reaching the high latitudes, that penetrate deep into the planets' interiors, as suggested by gravity measurements.…

astro-ph.SR2013

Bridging planets and stars using scaling laws in anelastic spherical shell dynamos

Rakesh K. Yadav, Thomas Gastine, Ulrich R. Christensen +1

Dynamos operating in the interiors of rapidly rotating planets and low-mass stars might belong to a similar category where rotation plays a vital role. We quantify this similarity…

astro-ph.SR2013

What controls the large-scale magnetic fields of M dwarfs?

T. Gastine, J. Morin, L. Duarte +3

Observations of active M dwarfs show a broad variety of large-scale magnetic fields encompassing dipole-dominated and multipolar geometries. We detail the analogy between some anel…

astro-ph.SR2012★ 97 cited

What controls the magnetic geometry of M dwarfs?

T. Gastine, J. Morin, L. Duarte +3

Context: observations of rapidly rotating M dwarfs show a broad variety of large-scale magnetic fields encompassing dipole-dominated and multipolar geometries. In dynamo models, th…

astro-ph.EP2010★ 166 cited

A magnetic field evolution scenario for brown dwarfs and giant planets

Ansgar Reiners, Ulrich R. Christensen

Very little is known about magnetic fields of extrasolar planets and brown dwarfs. We use the energy flux scaling law presented by Christensen et al. (2009) to calculate the evolut…

astro-ph.SR2009★ 45 cited

Surprisingly Weak Magnetism on Young Accreting Brown Dwarfs

Ansgar Reiners, Gibor Basri, Ulrich R. Christensen

We have measured the surface magnetic flux on four accreting young brown dwarfs and one non-accreting young very low-mass star utilizing high resolution spectra of absorption lines…