Oscillations detected on the solar surface provide a unique opportunity for investigations of
the interior properties of a star. Through major observational efforts, including extensive …

We present estimates of the amplitudes of intrinsically stable stochastically excited radial
oscillations in stars near the main sequence. The amplitudes are determined by the balance …

In recent years, helioseismology has provided an unprecedented look at the dynamics of the
solar interior. These new insights have been accompanied by tremendous advances in high …

The physics of solar and stellar oscillations determines their observable properties:
frequencies, amplitudes, lifetimes, line asymmetries and phase relations. In the solar case …

We report on realistic simulations of solar surface convection that are essentially parameter-
free, but include detailed physics in the equation of state and radiative energy exchange …

Abstract The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will
revolutionize our ability to measure, understand, and model the basic physical processes …

We have searched helioseismic data collected by the Birmingham Solar Oscillations
Network (BiSON) for solar-cycle changes to those low-ℓ p-mode parameters that relate to the …

We use the ring-diagram technique of local helioseismology to study the amplitude and line
width of high-degree solar acoustic modes from 474 days of data from the Michelson …

We have used observations made by the Global Oscillations at Low Frequency (GOLF) and
the Variability of Irradiance and Gravity Oscillations Sun Photometer (VIRGO/SPM) …

We propose that solar acoustic oscillations are excited by localized cooling events and new
downflow-plume formation at the solar surface. The excitation process involves, in …