Results 101 to 110 of about 1,537 (202)
Turbulent convection as a significant hidden provider of magnetic helicity in solar eruptions. [PDF]
Toriumi S, Hotta H, Kusano K.
europepmc +1 more source
The Privileged Life of a Theoretical Observer. [PDF]
Gough D.
europepmc +1 more source
Full Waveform Inversion for Time-Distance Helioseismology
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
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
Solar Flare 1/f Fluctuations from Amplitude-Modulated Five-Minute Oscillation. [PDF]
Morikawa M, Nakamichi A.
europepmc +1 more source
The Shape of the Solar Tachocline
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
Towards passive non-line-of-sight acoustic localization around corners using uncontrolled random noise sources. [PDF]
Boger-Lombard J, Slobodkin Y, Katz O.
europepmc +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
Juno spacecraft gravity measurements provide evidence for normal modes of Jupiter. [PDF]
Durante D +14 more
europepmc +1 more source
Time-Distance Helioseismology With The Mdi Instrument: Initial Results
. 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
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