78 citations · 96 across the 6 of their papers we have counts for
6 papers
Dwindling Surface Cooling of a Rotating Jovian Planet Leads to a Convection Zone that Grows to a Finite Depth
Bradley W. Hindman, J. R. Fuentes
Recent measurements of Jupiter's gravitational field (by Juno) and seismology of Saturn's rings (by Cassini) strongly suggest that both planets have a stably-stratified core that s…
Latitudinal Propagation of Thermal Rossby Waves in Stellar Convection Zones
Rekha Jain, Bradley W. Hindman
Using an analytic model, we derive the eigenfrequencies for thermal Rossby waves that are trapped radially and latitudinally in an isentropically stratified atmosphere. We ignore t…
The Puzzling Structure of Solar Convection: Window into the Dynamo
Nicholas A. Featherstone, Kyle C. Augustson, Jonathan M. Aurnou +25
The operation of the solar dynamo, with all of its remarkable spatio-temporal ordering, remains an outstanding problem of modern solar physics. A number of mechanisms that might pl…
Overstable Convective Modes in a Polytropic Stellar Atmosphere
Bradley W. Hindman, Rekha Jain
Within the convection zone of a rotating star, the presence of the Coriolis force stabilizes long-wavelength convective modes. These modes, which would have been unstable if the st…
The Emergence of Solar Supergranulation as a Natural Consequence of Rotationally-Constrained Interior Convection
Nicholas A. Featherstone, Bradley W. Hindman
We investigate how rotationally-constrained, deep convection might give rise to supergranulation, the largest distinct spatial scale of convection observed in the solar photosphere…
Five-minute oscillation power within magnetic elements in the solar atmosphere
Rekha Jain, Andrew Gascoyne, Bradley W. Hindman +1
It has long been known that magnetic plage and sunspots are regions in which the power of acoustic waves is reduced within the photospheric layers. Recent observations now suggest…