Image de couverture de livre

Forward modeling solar spectra onto Doppler images of λ And

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Adebali, Ö., Pietrow, A. G. M.
Format:	Preprint
Publié:	2026
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

First Doppler image and starspot-corrected orbit for $λ$ Andromedae: A multifaceted activity analysis
par: Adebali, Ö., et autres
Publié: (2025)

HelioSpectrotron 5000: An interactive multi-resolution solar spectral atlas
par: Pietrow, A. G. M.
Publié: (2026)

Spectral variations within solar flare ribbons
par: Pietrow, A. G. M., et autres
Publié: (2024)

Surface image and activity-corrected orbit of the RS CVn binary HR 7275: Disentangling activity tracers
par: Adebali, Ö., et autres
Publié: (2025)

Does the solar oxygen abundance change over the solar cycle? An investigation into activity-induced variations of the O I infrared triplet
par: Pietrow, A. G. M., et autres
Publié: (2026)

Synthesizing Sun-as-a-star flare spectra from high-resolution solar observations
par: De Wilde, M., et autres
Publié: (2025)

The spectra of solar magnetic energy and helicity
par: Kishore, G., et autres
Publié: (2025)

Automatic detection of Ellerman bombs in the H$α$ line
par: Faryad, A., et autres
Publié: (2025)

Multi-wavelength observations of substructures in solar flare ribbons
par: Singh, Vishal, et autres
Publié: (2025)

Differential rotation of solar α sunspots and implications for stellar light curves
par: Lößnitz, Emily Joe, et autres
Publié: (2025)

An Atlas of Spectroheliograms from 3641 to 6600 Å
par: Nagy, P. Váradi, et autres
Publié: (2025)

The calm before the storm: High spatial resolution mosaic of active region NOAA 14274 at the onset of an X1.2 flare
par: Denker, Carsten, et autres
Publié: (2025)

A comparative study of two X2.2 and X9.3 solar flares observed with HARPS-N: Reconciling Sun-as-a-star spectroscopy and high-spatial resolution solar observations in the context of the solar-stellar connection
par: Pietrow, A. G. M., et autres
Publié: (2023)

Spectral Characteristics of a Rotating Solar Prominence in Multiple Wavelengths
par: Pietrow, A. G. M., et autres
Publié: (2024)

Spectral resolution effects on the information content in solar spectra
par: Baso, C. J. Díaz, et autres
Publié: (2024)

Solar active region evolution and imminent flaring activity through a color-coded visualization of photospheric vector magnetograms
par: Kontogiannis, I., et autres
Publié: (2024)

Chromospheric and photospheric properties of sunspots as inferred from Stokes inversions under magneto-hydrostatic and non-local-thermodynamic equilibrium
par: Arevalo, A. Vicente, et autres
Publié: (2026)

Doppler imaging of a southern ApSi star HD 152564
par: Potravnov, I., et autres
Publié: (2023)

Prominence signatures in the Fraunhofer G-band; Testing ionization memory with multi-line prominence diagnostics
par: Pietrow, A. G. M., et autres
Publié: (2026)

Correlation between active regions' spectra at high radio frequencies and solar flare occurrences
par: Mulas, Sara, et autres
Publié: (2026)

Center-to-limb variation of spectral lines and their effect on full-disk observations
par: Pietrow, Alexander G. M., et autres
Publié: (2023)

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 theoretical pulsation spectra of hot B subdwarfs. Static and evolutionary STELUM models
par: Guyot, N., et autres
Publié: (2025)

Relationship between TIGRE solar S-index and USET Ca II K full disk images
par: Broeck, G. Vanden, et autres
Publié: (2024)

Precise and efficient modeling of stellar-activity-affected solar spectra using SOAP-GPU
par: Zhao, Yinan, et autres
Publié: (2024)

The solar beryllium abundance revisited with 3D non-LTE models
par: Amarsi, A. M., et autres
Publié: (2024)

Modeling spectra of MN112
par: Kostenkov, A., et autres
Publié: (2020)

Zeeman Doppler mapping deconstructed
par: Stift, M. J., et autres
Publié: (2025)

Towards a self-consistent hydrodynamical model of the solar tachocline
par: Garaud, P., et autres
Publié: (2025)

Testing a non-local 1-equation turbulent convection model: A solar model
par: Braun, T. A. M., et autres
Publié: (2024)

Probing solar modulation analytic models with cosmic ray periodic spectra
par: Long, Wei-Cheng, et autres
Publié: (2024)

The solar sulphur abundance in view of large-scale atomic structure calculations and 3D non-LTE models
par: Amarsi, A. M., et autres
Publié: (2025)

Diagnostics for the solar chromosphere using neutral carbon Rydberg lines
par: Dufresne, R. P., et autres
Publié: (2026)

In-depth analysis of solar models with high-metallicity abundances and updated opacity tables
par: Buldgen, G., et autres
Publié: (2024)

Why do solar wind models get it wrong: understanding the capabilities of time-dependent solar wind simulations
par: Samara, Evangelia, et autres
Publié: (2025)

Doppler Dimming and Brightening Effects in Solar Prominences
par: Peat, Aaron W., et autres
Publié: (2024)

Study of solar brightness profiles in the 18-26 GHz frequency range with INAF radio telescopes I: solar radius
par: Marongiu, M., et autres
Publié: (2024)

Observations of Flare Induced Doppler Shifts in the Si~\textsc{iii} $1206\,\textrm{Å}$ line
par: Majury, Luke H., et autres
Publié: (2025)

Why every observatory needs a disco ball
par: Cumming, Robert J., et autres
Publié: (2023)

Tracking the motion of a shock along a channel in the low solar corona
par: Rigney, J., et autres
Publié: (2024)