Image de couverture de livre

Transport of the magnetic flux away from a decaying sunspot via convective motions

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Zheng, Chenxi, Roudier, Thierry, Schmieder, Brigitte, Ruan, Guiping, Malherbe, Jean-Marie, Liu, Yang, Chen, Yao, Cao, Wenda
Format:	Preprint
Publié:	2024
Sujets:	Solar and Stellar Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

The role of Trees of Fragmenting Granules (TFG) in the formation of the solar supergranular pattern from Hinode observations
par: Malherbe, Jean-Marie, et autres
Publié: (2025)

Hidden magnetic fields of the quiet Sun derived from Hanle depolarization of lines of the "second solar spectrum" at the limb from Pic du Midi observations
par: Malherbe, Jean-Marie
Publié: (2025)

Structure of proper motions in a sunspot penumbra
par: Hamedivafa, Hashem
Publié: (2024)

Apparent motion of penumbral grains in a sunspot simulation
par: Sobotka, Michal, et autres
Publié: (2025)

The quadruple spectroheliograph of Meudon observatory (1909-1959)
par: Malherbe, Jean-Marie
Publié: (2024)

The Paris Meudon ground based support to the NASA Solar Maximum Mission in the eighties
par: Malherbe, Jean-Marie
Publié: (2025)

Polarized lines of the second solar spectrum (SrI, SrII, CaI, BaII) observed at the Pic du Midi Turret Dome spectropolarimeter with the slit orthogonal to the limb
par: Malherbe, Jean-Marie
Publié: (2026)

A compilation of solar atlases (from Delbouille, Kurucz, Gandorfer, Stenflo) at disk centre and at limb from $λ$ 3000 Å to $λ$ 8800 Å
par: Malherbe, Jean-Marie
Publié: (2024)

The golden age of solar magnetography at Paris-Meudon observatory in the second half of the twentieth century
par: Malherbe, Jean-Marie
Publié: (2025)

150 years of ground-based solar instrumentation at Meudon observatory (1876-2026)
par: Malherbe, Jean-Marie
Publié: (2026)

In pursuit of the Sun, from Jules Janssen to the present day
par: Malherbe, Jean-Marie
Publié: (2024)

Weak polarized lines of the second solar spectrum (Na, Al, H, He, Ti, Li, Sc, C2 and MgH) observed at the Pic du Midi turret dome
par: Malherbe, Jean-Marie
Publié: (2026)

High resolution spectra of the [6297-6303] and [6361-6367] Angstr{ö}m domains (including forbidden OI lines) of the Sun and brightest stars
par: Malherbe, Jean-Marie
Publié: (2025)

High polarization lines of the second solar spectrum of the Solar limb
par: Malherbe, Jean-Marie
Publié: (2025)

70 years of spectroscopy of the photosphere and the solar chromosphere at the Pic du Midi Observatory (1956-2026)
par: Malherbe, Jean-Marie
Publié: (2026)

The Haute Provence monochromatic heliograph (1958-1994)
par: Malherbe, Jean-Marie
Publié: (2024)

Datacubes of H$α$, CaII K, CaII H and H$ε$ line profiles of the full solar disk recorded daily at Meudon observatory since 2017 and some typical profiles of solar features
par: Malherbe, Jean-Marie
Publié: (2026)

Rotation of flux ropes in the low corona
par: Schmieder, Brigitte, et autres
Publié: (2025)

The magnetic origin of the outer boundaries of sunspots
par: Schmassmann, Markus, et autres
Publié: (2025)

Recent advances in solar data-driven MHD simulations of the formation and evolution of CME flux ropes
par: Schmieder, Brigitte, et autres
Publié: (2024)

The dependence of the magnetism of a near-limb sunspot on height
par: Benko, M., et autres
Publié: (2024)

Automated detection of exploding granules with SDO/HMI data
par: Ballot, J., et autres
Publié: (2024)

Magnetic properties of the umbral boundary during sunspot decay. Comparative study of multiple datasets
par: García-Rivas, M., et autres
Publié: (2024)

Eruption of a million-Kelvin warm magnetic flux rope on the Sun
par: Li, Leping, et autres
Publié: (2024)

Bistability in the sunspot cycle
par: Vashishtha, Sumit, et autres
Publié: (2024)

Deflection of a Filament Eruption with Three Parallel Flare Ribbons via Reconnection at an X-Point
par: Zhang, Xiaomeng, et autres
Publié: (2026)

The latitudinal migration of the sunspot groups
par: Takalo, Jouni J.
Publié: (2024)

Discovery of a relation between the decay rate of the Sun's magnetic dipole and the growth rate of the following sunspot cycle: a new precursor for solar cycle prediction
par: Jaswal, Priyansh, et autres
Publié: (2023)

Improved reconstruction of the century-long solar magnetic field by incorporating morphological asymmetry in sunspots
par: Pal, Subhadip, et autres
Publié: (2025)

Solar prominence diagnostics and their associated estimated errors from 1D NLTE Mg II h&k modelling
par: Peat, Aaron W., et autres
Publié: (2024)

The role of the Lorentz force in sunspot equilibrium
par: Borrero, J. M., et autres
Publié: (2025)

Do the planets cause the sunspot cycles?
par: Jetsu, Lauri
Publié: (2023)

MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT
par: Wang, Haopeng, et autres
Publié: (2026)

Spectroscopic investigations of a filament reconnecting with coronal loops during a two-ribbon solar flare
par: Joshi, Reetika, et autres
Publié: (2025)

Observations of umbral flashes in the resonant sunspot chromosphere
par: Felipe, T., et autres
Publié: (2024)

Statistical analysis of the total magnetic flux decay rate in solar active regions
par: Plotnikov, Andrei A., et autres
Publié: (2023)

Empirical flare energy limits for the largest historical sunspots
par: Krivova, N. A., et autres
Publié: (2026)

Variation of sunspot groups' polarity separation during their evolution
par: Muraközy, Judit
Publié: (2024)

EUV Wave and Coronal Seismology
par: Devi, Pooja, et autres
Publié: (2025)

Prediction of the amplitude of solar cycle 25 from the ratio of sunspot number to sunspot-group area, low latitude activity, and 130-year solar cycle
par: Javaraiah, J.
Publié: (2024)