Structural Tilting and Depth-dependent Behavior of Equatorial Rossby Waves
Over the past decade, solar equatorial Rossby waves have been unambiguously identified and are considered potential diagnostics of solar interior dynamics.
Oana Vesa, Junwei Zhao, Ruizhu Chen
doaj +1 more source
Propagating Linear Waves in Convectively Unstable Stellar Models: a Perturbative Approach
Linear time-domain simulations of acoustic oscillations are unstable in the stellar convection zone. To overcome this problem it is customary to compute the oscillations of a stabilized background stellar model.
Birch, Aaron C. +2 more
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We use rotation splittings derived from very long and long time series, namely 25.2, 12.6, and 6.3 yr long, computed by S. G. Korzennik independent methodology to characterize the solar tachocline and its variation with latitude and time.
Sylvain G. Korzennik +1 more
doaj +1 more source
SPECTROPOLARIMETRICALLY ACCURATE MAGNETOHYDROSTATIC SUNSPOT MODEL FOR FORWARD MODELING IN HELIOSEISMOLOGY [PDF]
Damien Przybylski +2 more
openalex +1 more source
Characterizing the Observational Properties of the Sun’s High-latitude m = 1 Inertial Mode
Low- m inertial modes have been recently discovered in the Sun’s high-latitude regions. In this study, we characterize the observational properties of the m = 1 mode by analyzing time–distance subsurface flow maps.
Boyang Ding +5 more
doaj +1 more source
The Sun’s Dark Core: Helioseismic and Neutrino Flux Constraints on a Compact Solar Center
As dark matter appears to comprise most of the Galactic mass, some of it may accumulate in the cores of stars, thereby making the Sun a laboratory for constraining various dark matter theories.
Earl P. Bellinger, Matt E. Caplan
doaj +1 more source
Turbulent convection as a significant hidden provider of magnetic helicity in solar eruptions. [PDF]
Toriumi S, Hotta H, Kusano K.
europepmc +1 more source
Implementation and Comparison of Acoustic Travel-Time Measurement Procedures for the Solar Dynamics Observatory/Helioseismic and Magnetic Imager Time – Distance Helioseismology Pipeline [PDF]
S. Couvidat +6 more
openalex +1 more source

