Image de couverture de livre

Testing volume integrals of travel-time sensitivity kernels for flows

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Svanda, Michal, Chmurny, Daniel
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

Average solar active region: I. Intensities, velocities, and the photospheric magnetic field
par: Švanda, M., et autres
Publié: (2025)

Habitability of exoplanets orbiting flaring stars
par: Szabó, Rebecca, et autres
Publié: (2025)

Predicting coronal mass ejection travel times using enhanced model-guided machine learning
par: Lampani, M., et autres
Publié: (2025)

Flare heating of the chromosphere: Observations of flare continuum from GREGOR and IRIS
par: García-Rivas, M., et autres
Publié: (2024)

The magnetic sensitivity of the Ca II H and K lines
par: Kriginsky, M., et autres
Publié: (2026)

The sensitivity and behaviour of the curvature in the échelle diagram of red-giant stars
par: Hekker, S., et autres
Publié: (2026)

The magnetic sensitivity of the Ca II resonance and subordinate lines in the solar atmosphere
par: Berasategi, I. Juanikorena, et autres
Publié: (2025)

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

Testing the wavelength dependence of oscillations and granulation in red giants using Kepler and TESS
par: Sreenivas, K. R., et autres
Publié: (2025)

The vertical shear instability in protoplanetary discs as an outwardly travelling wave. I. Linear theory
par: Ogilvie, Gordon I., et autres
Publié: (2025)

The polarization of the solar Ba II D1 line with partial frequency redistribution and its magnetic sensitivity
par: Ballester, E. Alsina, et autres
Publié: (2024)

Unveiling stellar aurorae: Simulating auroral emission lines in hot stars induced by high-energy irradiation
par: Kajan, Michal, et autres
Publié: (2024)

Testing Red Clump Models with the Asteroseismic Binary KIC 10841730
par: Schimak, Lea S., et autres
Publié: (2026)

Horizontal flows in the atmospheres of chemically peculiar stars
par: ud-Doula, A., et autres
Publié: (2025)

Frequency-time-resolved Imaging Spectroscopy of Fine Structures in a Solar Radio Noise Storm
par: Clarkson, Daniel L., et autres
Publié: (2026)

The connection between internetwork magnetic elements and supergranular flows
par: Suárez, D. Orozco, et autres
Publié: (2024)

A 500 pc volume-limited sample of hot subluminous stars II. Atmospheric parameters, mass distribution, and kinematics
par: Dawson, H., et autres
Publié: (2026)

Multi-height probing of horizontal flows in the solar photosphere
par: Kostić, Teodor, et autres
Publié: (2025)

Visualizing the mass transfer flow in direct-impact accretion
par: Frank, Juhan, et autres
Publié: (2025)

A sudden fine-scale bright kernel captured by Hi-C Flare in 11 MK emission during an M1.6-class solar flare's post-maximum phase
par: Tiwari, Sanjiv K., et autres
Publié: (2025)

Scale-dependent surface and volume density properties of filaments in molecular clouds
par: Zhang, Guo-Yin, et autres
Publié: (2026)

A new sample of massive B-type contact binary candidates from the OGLE survey of the Magellanic Clouds
par: Menon, Athira, et autres
Publié: (2024)

Testing the Rossby Paradigm: Weakened Magnetic Braking in early K-type Stars
par: Metcalfe, Travis S., et autres
Publié: (2025)

Detection of the solar internal flows with numerical simulation and machine learning
par: Masaki, Hiroyuki, et autres
Publié: (2024)

Magnetic flux in the Sun emerges unaffected by supergranular-scale surface flows
par: Mani, Prasad, et autres
Publié: (2024)

Inferring photospheric horizontal flows from multiple observations with SUVEL models
par: Xie, Quan, et autres
Publié: (2026)

Radial flow component of Sun's high frequency retrograde inertial waves
par: Hanson, Chris S., et autres
Publié: (2025)

A Study on Magnetic-sensitivity Wavelength Position of the Working Line Used by the Full-Disk Magnetograph onboard the Advanced Space based Solar Observatory (ASO-S/FMG)
par: Liu, S., et autres
Publié: (2024)

Quadruple system HD 135160 in a unique 2+2 configuration
par: Zummer, Michal, et autres
Publié: (2025)

Meridional flow in the solar polar caps revealed by magnetic field observation and simulation
par: Yang, Shuhong, et autres
Publié: (2024)

Energy and mass transport associated with impulsive spicular flows in solar coronal holes
par: Ni, Lei, et autres
Publié: (2026)

Testing the Breakdown of the Asteroseismic Scaling Relations in Luminous Red Giants
par: Ash, Amanda L., et autres
Publié: (2024)

Fundamental Tests of White Dwarf Cooling Physics with Wide Binaries
par: Barrientos, Manuel, et autres
Publié: (2024)

Testing the 3-equation Kuhfuss Convection Model using the Sun
par: Braun, T. A. M., et autres
Publié: (2026)

Testing the reliability of magnetic field strength measurements for M dwarfs
par: Amateis, I., et autres
Publié: (2026)

Connecting integrated RGB mass loss from asteroseismology and globular clusters
par: Brogaard, K., et autres
Publié: (2024)

Wave coupling in partially ionized plasmas with shear flows I. Fast-to-Alfvén transformation
par: Cantallops, Miquel, et autres
Publié: (2025)

Helical flows along coronal loops following the launch of a coronal mass ejection
par: Nedal, Mohamed, et autres
Publié: (2025)

Tests and calibrations of stellar models with two triply eclipsing triple systems
par: Valle, G., et autres
Publié: (2025)

Numerical experiments on granulation-generated two-fluid waves and flows in a solar magnetic carpet
par: Niedziela, R., et autres
Publié: (2024)