Results 111 to 120 of about 1,264 (214)

Computational aspects of Green's kernels in local helioseismology. [PDF]

International audienceHelioseismology infers the interior of the Sun from oscillations which are continuously excited by near-surface turbulent convection and observed in the photosphere.
Gizon, Laurent,, Pham, Ha, Barucq, Hélène, Fournier, Damien, Faucher, Florian   +4 more
core   +2 more sources

Structural Tilting and Depth-dependent Behavior of Equatorial Rossby Waves

The Astrophysical Journal
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

Dynamics of the Tachocline. [PDF]

Space Sci Rev, 2023
Strugarek A, Belucz B, Brun AS, Dikpati M, Guerrero G.   +4 more
europepmc   +1 more source

The Iris Network For Whole Disc Helioseismology: Recent Results [PDF]

, 2007
IRIS(International Research on the Interior of the sun) is the name of a worldwide network of 6 stations for whole disc Doppler shift measurements. The network has been operating since 1987 and by now a few series of a hundred days long unbroken (by day ...
Sh Ehgamberdiev
core  

Anisotropic Magnetized Asteroseismic Waves

The 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

Turbulent convection as a significant hidden provider of magnetic helicity in solar eruptions. [PDF]

Sci Rep, 2023
Toriumi S, Hotta H, Kusano K.
europepmc   +1 more source

It Takes a Village. [PDF]

Sol Phys, 2022
Canfield RC.
europepmc   +1 more source

The Privileged Life of a Theoretical Observer. [PDF]

Sol Phys, 2022
Gough D.
europepmc   +1 more source

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

The 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, Junwei Zhao, Ruizhu Chen, Matthias Waidele, Sushant S. Mahajan, Oana Vesa   +5 more
doaj   +1 more source

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

Nat Commun, 2022
Durante D, Guillot T, Iess L, Stevenson DJ, Mankovich CR, Markham S, Galanti E, Kaspi Y, Zannoni M, Gomez Casajus L, Lari G, Parisi M, Buccino DR, Park RS, Bolton SJ.   +14 more
europepmc   +1 more source