activity
20022019
most citedSolar Multi-Scale Convection and Rotation Gradients Studied in Shallow Spherical Shells

42 citations · 148 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2019★ 11 cited

The Solar Benchmark: Rotational Modulation of the Sun Reconstructed from Archival Sunspot Records

Brett M. Morris, James R. A. Davenport, Helen A. C. Giles +5

We use archival daily spot coverage measurements from Howard et al. (1984) to study the rotational modulation of the Sun as though it were a distant star. A quasi-periodic Gaussian…

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★ 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.SR2010★ 25 cited

Physical Origin of Differences among various Measures of Solar Meridional Circulation

Mausumi Dikpati, Peter A. Gilman, Roger K. Ulrich

We show that systematic differences between surface Doppler and magnetic element tracking measures of solar meridional flow can be explained by the effects of surface turbulent mag…

astro-ph2005★ 30 cited

Recovering Solar Toroidal Field Dynamics From Sunspot Location Patterns

Aimee A. Norton, Peter A. Gilman

We analyze both Kitt Peak magnetogram data and MDI continuum intensity sunspot data to search for the following solar toroidal band properties: width in latitude and the existence…

astro-ph2005★ 22 cited

Concentration of toroidal magnetic field in the solar tachocline by eta-quenching

Peter A. Gilman, Matthias Rempel

We show that if the turbulent magnetic diffusivity used in solar dynamos is assumed to be 'quenched' by increasing toroidal fields, much larger amplitude and more concentrated toro…