Results 101 to 110 of about 6,507 (247)

A Linear Model for Inertial Modes in a Differentially Rotating Sun

open access: yesThe Astrophysical Journal
Inertial wave modes in the Sun are of interest owing to their potential to reveal new insight into the solar interior. These predominantly retrograde-propagating modes in the solar subsurface appear to deviate from the thin-shell Rossby–Haurwitz model at
Jishnu Bhattacharya   +3 more
doaj   +1 more source

Dynamics of Large-Scale Solar Flows. [PDF]

open access: yesSpace Sci Rev, 2023
Hotta H   +4 more
europepmc   +1 more source

Sensitivity of helioseismic travel-times to the imposition of a Lorentz force limiter in computational helioseismology

open access: yes, 2014
The rapid exponential increase in the Alfv\'en wave speed with height above the solar surface presents a serious challenge to physical modelling of the effects of magnetic fields on solar oscillations, as it introduces a significant CFL time-step ...
Cally, Paul S., Moradi, Hamed
core   +1 more source

Predicting Solar Magnetic Activity from Sph and Seismic Parameters Using Random Forest Regression

open access: yesThe Astrophysical Journal
We investigate the potential of using the photometric magnetic proxy S _ph and seismic parameters, such as the frequency of maximum power ( ${\nu }_{{\rm{\max }}}$ ) and the large frequency separation (Δ ν ), derived from Solar and Heliospheric ...
Ki-Beom Kim, Heon-Young Chang
doaj   +1 more source

Differential rotation and radiative equilibrium in the Sun: is the tachocline spreading?

open access: yes, 2015
It is well known that the combination of barotropic rotation and radiative equilibrium are mutually incompatible in stars. The Sun's internal rotation is far from barotropic, however, which allows at least the theoretical possibility that the Sun's ...
Balbus, Steven   +2 more
core   +1 more source

Full Waveform Inversion for Time-Distance Helioseismology

open access: yes, 2014
Inferring interior properties of the Sun from photospheric measurements of the seismic wavefield constitutes the helioseismic inverse problem. Deviations in seismic measurements (such as wave travel times) from their fiducial values estimated for a given
Hanasoge, Shravan, Tromp, Jeroen
core   +1 more source

Travel Time Shifts due to Amplitude Modulation in Time-Distance Helioseismology

open access: yes, 2009
Correct interpretation of acoustic travel times measured by time-distance helioseismology is essential to get an accurate understanding of the solar properties that are inferred from them. It has long been observed that sunspots suppress p-mode amplitude,
A. G. Kosovichev   +9 more
core   +1 more source

Constraining Solar Abundances Using Helioseismology

open access: yesThe Astrophysical Journal, 2004
To appear in ApJ Letters. 12 pages (that include 4 figures)
Basu, Sarbani, Antia, H. M.
openaire   +2 more sources

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