Results 121 to 130 of about 6,507 (247)
The Shape of the Solar Tachocline
The Astrophysical JournalEarly 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
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Latitude-dependent Time Variations of the Solar Tachocline
The Astrophysical JournalWe have examined how the characteristics of the tachocline—i.e., the change in rotation rate δ Ω, or the “jump,” the position of the midpoint of the tachocline, r _d , and the width of the tachocline, w _d —change as a function of time at different ...
Sarbani Basu +2 more
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The Privileged Life of a Theoretical Observer. [PDF]
Sol Phys, 2022 Gough D.
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Helioseismology: a fantastic tool to probe the interior of the Sun
, 2012 Helioseismology, the study of global solar oscillations, has proved to be an extremely powerful tool for the investigation of the internal structure and dynamics of the Sun.
Di Mauro, M. P.
core
VALIDATING TIME-DISTANCE HELIOSEISMOLOGY WITH REALISTIC QUIET-SUN SIMULATIONS [PDF]
, 2014 K. DeGrave, Jason Jackiewicz, M. Rempel
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Anisotropic Magnetized Asteroseismic Waves
The Astrophysical JournalWe 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
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Juno spacecraft gravity measurements provide evidence for normal modes of Jupiter. [PDF]
Nat Commun, 2022 Durante D +14 more
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AN UPPER BOUND FROM HELIOSEISMOLOGY ON THE STOCHASTIC BACKGROUND OF GRAVITATIONAL WAVES [PDF]
, 2014 Daniel M. Siegel, M. Roth
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Solar Flare 1/f Fluctuations from Amplitude-Modulated Five-Minute Oscillation. [PDF]
Entropy (Basel), 2023 Morikawa M, Nakamichi A.
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