activity
20002026
most citedA 3D Babcock-Leighton Solar Dynamo Model

82 citations · 651 across the 38 of their papers we have counts for

collaborators
Showing 2011Show all

7 papers · 1 filter

astro-ph.SR2011★ 12 cited

Theory of Solar Meridional Circulation at High Latitudes

Mausumi Dikpati, Peter A. Gilman

We build a hydrodynamical model for computing and understanding the Sun's large-scale high latitude flows, including Coriolis forces, turbulent diffusion of momentum and gyroscopic…

astro-ph.SR2011★ 73 cited

Nonlinear Evolution of Global Hydrodynamic Shallow-Water Instability in Solar Tachocline

Mausumi Dikpati

We present a fully nonlinear hydrodynamic 'shallow water' model of the solar tachocline. The model consists of a global spherical shell of differentially rotating fluid, which has…

astro-ph.SR2011

Magnetic feature tracking, what determines the speed?

G. Guerrero, M. Rheinhardt, M. Dikpati

Recent observations revealed that small magnetic elements abundant at the solar surface move poleward with a velocity which seems to be lower than the plasma velocity . Guerre…

astro-ph.SR2011★ 5 cited

Plasma flow vs. magnetic feature-tracking speeds in the Sun

G. Guerrero, M. Rheinhardt, A. Brandenburg +1

We simulate the magnetic feature tracking (MFT) speed using advective-diffusive transport models in both one and two dimensions. By depositing magnetic bipolar regions at different…

astro-ph.SR2011★ 6 cited

Resonance in Forced Flux Transport Dynamos

Peter A. Gilman, Mausumi Dikpati

We show that simple 2 and 3-layer flux-transport dynamos, when forced at the top by a poloidal source term, can produce a widely varying amplitude of toroidal field at the bottom,…

astro-ph.SR2011★ 4 cited

Analysis of 3D MHD Instability of Antisolar Latitudinal Differential Rotation in F, G and K stars

Mausumi Dikpati, Paul S. Cally

Motivated by observations that only a very few stars have been found to have antisolar differential rotation, much weaker in amplitude than that of the Sun, we analyze the stabilit…