Results 101 to 110 of about 1,537 (202)

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
Tromp, J.   +3 more
core   +1 more source

Anisotropic Magnetized Asteroseismic Waves

open access: yesThe Astrophysical Journal
We solve for waves in a polytropic, stratified plasma with a spatially varying background magnetic field that points along the horizontal x -direction, and with gravity that is directed along the vertical z -direction.
B. Tripathi, Dhrubaditya Mitra
doaj   +1 more source

The Shape of the Solar Tachocline

open access: yesThe Astrophysical Journal
Early helioseismic results have shown that the tachocline has a prolate shape. However, the models used in those studies constrained the tachocline to be either prolate or oblate.
Sarbani Basu, Sylvain G. Korzennik
doaj   +1 more source

Characterizing the Observational Properties of the Sun’s High-latitude m = 1 Inertial Mode

open access: yesThe Astrophysical Journal
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

Juno spacecraft gravity measurements provide evidence for normal modes of Jupiter. [PDF]

open access: yesNat Commun, 2022
Durante D   +14 more
europepmc   +1 more source

Time-Distance Helioseismology With The Mdi Instrument: Initial Results

open access: yes, 2007
. In time-distance helioseismology, the travel time of acoustic waves is measured between various points on the solar surface. To some approximation, the waves can be considered to follow ray paths that depend only on a mean solar model, with the ...
T. D. Tarbell   +12 more
core  

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