Signs of Sulphur fractionation under high magnetic field strength
Fuente:
arXiv
Guardado en:
| Autores principales: | Orlovskij, Dominik, To, Andy S. H., Long, David M. |
|---|---|
| Formato: | Preprint |
| Publicado: |
2026
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Testing the reliability of magnetic field strength measurements for M dwarfs
por: Amateis, I., et al.
Publicado: (2026)
por: Amateis, I., et al.
Publicado: (2026)
Sulfur fractionation in coronal plumes as observed by Solar Orbiter/SPICE
por: Mzerguat, Slimane, et al.
Publicado: (2026)
por: Mzerguat, Slimane, et al.
Publicado: (2026)
Radiative hydrodynamic simulations of FIP fractionation in solar flares
por: Reep, Jeffrey W., et al.
Publicado: (2025)
por: Reep, Jeffrey W., et al.
Publicado: (2025)
Asteroseismology reveals the near-core magnetic field strength in the early-B star HD 43317
por: Bowman, D. M., et al.
Publicado: (2022)
por: Bowman, D. M., et al.
Publicado: (2022)
Comparing First Ionisation Potential bias diagnostics in the solar atmosphere
por: Spruksta, Kristena D., et al.
Publicado: (2026)
por: Spruksta, Kristena D., et al.
Publicado: (2026)
Identifying plasma fractionation processes in the chromosphere using IRIS
por: Long, David M., et al.
Publicado: (2024)
por: Long, David M., et al.
Publicado: (2024)
Statistical relations between spectropolarimetric observables and the polar strength of the stellar dipolar magnetic field
por: Kochukhov, O.
Publicado: (2024)
por: Kochukhov, O.
Publicado: (2024)
Variations in the magnetic field strength of pre-main-sequence stars, solar-type main-sequence stars, and the Sun
por: Yamashita, Mai, et al.
Publicado: (2025)
por: Yamashita, Mai, et al.
Publicado: (2025)
Evolution of solar and stellar coronal abundances due to magnetic activity
por: Brooks, David H., et al.
Publicado: (2025)
por: Brooks, David H., et al.
Publicado: (2025)
A fast method for deriving relative small-scale magnetic field variations from high-resolution spectroscopy
por: Cristofari, Paul I., et al.
Publicado: (2026)
por: Cristofari, Paul I., et al.
Publicado: (2026)
A conclusive non-detection of magnetic field in the Am star o Peg with high-precision near-infrared spectroscopy
por: Kochukhov, O., et al.
Publicado: (2024)
por: Kochukhov, O., et al.
Publicado: (2024)
Oscillations of the solar photospheric magnetic field caused by the m = 1 high-latitude inertial mode
por: Heinemann, Stephan G., et al.
Publicado: (2025)
por: Heinemann, Stephan G., et al.
Publicado: (2025)
The dynamics of small-scale magnetic fields modulated by the solar cycle
por: Stangalini, M., et al.
Publicado: (2025)
por: Stangalini, M., et al.
Publicado: (2025)
Morphological variations of solar granules in the presence of magnetic fields
por: Rozo, J. I. Campos, et al.
Publicado: (2026)
por: Rozo, J. I. Campos, et al.
Publicado: (2026)
A search for chemical stratification and magnetic fields in eight field blue horizontal-branch stars
por: Kafando, Issouf, et al.
Publicado: (2025)
por: Kafando, Issouf, et al.
Publicado: (2025)
The magnetic fields in Be stars are stronger than previously suggested
por: Hubrig, S., et al.
Publicado: (2026)
por: Hubrig, S., et al.
Publicado: (2026)
SiO maser polarization and magnetic field in evolved cool stars
por: Marinho, L., et al.
Publicado: (2024)
por: Marinho, L., et al.
Publicado: (2024)
Near-critical magnetic fields in Kepler red giants
por: Deheuvels, S., et al.
Publicado: (2026)
por: Deheuvels, S., et al.
Publicado: (2026)
Exploring spectropolarimetric inversions using neural fields. Solar chromospheric magnetic field under the weak-field approximation
por: Baso, C. J. Díaz, et al.
Publicado: (2024)
por: Baso, C. J. Díaz, et al.
Publicado: (2024)
Generation and annihilation of three dimensional magnetic nulls in extrapolated solar coronal magnetic field: Data-based Implicit Large Eddy Simulation
por: Maurya, Yogesh Kumar, et al.
Publicado: (2024)
por: Maurya, Yogesh Kumar, et al.
Publicado: (2024)
Fine-scale opposite-polarity magnetic fields in a solar plage revealed by integral field spectropolarimetry
por: Liu, G., et al.
Publicado: (2025)
por: Liu, G., et al.
Publicado: (2025)
Average solar active region: I. Intensities, velocities, and the photospheric magnetic field
por: Švanda, M., et al.
Publicado: (2025)
por: Švanda, M., et al.
Publicado: (2025)
The H$α$ line as a probe of chromospheric magnetic fields
por: Mathur, Harsh, et al.
Publicado: (2025)
por: Mathur, Harsh, et al.
Publicado: (2025)
Mapping the Sun's coronal magnetic field using the Zeeman effect
por: Schad, Thomas A., et al.
Publicado: (2024)
por: Schad, Thomas A., et al.
Publicado: (2024)
How are the abnormally hot chromosphere and corona heated by the solar magnetic fields?
por: Li, K. J., et al.
Publicado: (2024)
por: Li, K. J., et al.
Publicado: (2024)
Gnevyshev gap in the large-scale magnetic field
por: Obridko, V. N., et al.
Publicado: (2024)
por: Obridko, V. N., et al.
Publicado: (2024)
Periodic change of polarity of photospheric magnetic field
por: Vernova, Elena, et al.
Publicado: (2025)
por: Vernova, Elena, et al.
Publicado: (2025)
Dependence of the intensity of the nonwave component of EUV waves on coronal magnetic field configuration
por: Li, Yuwei, et al.
Publicado: (2025)
por: Li, Yuwei, et al.
Publicado: (2025)
Effects of harmonic magnetic field boundary conditions in mean-field solar dynamo
por: Pipin, V. V.
Publicado: (2025)
por: Pipin, V. V.
Publicado: (2025)
Solar vortex detection methods in MHD simulations: impact of magnetic field and spatial resolution
por: Pistarini, M. Koll, et al.
Publicado: (2026)
por: Pistarini, M. Koll, et al.
Publicado: (2026)
Observation of Alfvén Wave Reflection in the Solar Chromosphere: Ponderomotive Force and First Ionization Potential Effect
por: Murabito, Mariarita, et al.
Publicado: (2024)
por: Murabito, Mariarita, et al.
Publicado: (2024)
Stability of the coronal magnetic field around large confined and eruptive solar flares
por: Gupta, Manu, et al.
Publicado: (2024)
por: Gupta, Manu, et al.
Publicado: (2024)
The first out-of-ecliptic observations of the polar magnetic field of the Sun
por: Calchetti, D., et al.
Publicado: (2025)
por: Calchetti, D., et al.
Publicado: (2025)
Searching for evidence of subchromospheric magnetic reconnection on the Sun
por: Baker, D., et al.
Publicado: (2024)
por: Baker, D., et al.
Publicado: (2024)
Unipolarity of the solar magnetic field in equatorial coronal holes
por: Katuwal, Khagendra, et al.
Publicado: (2026)
por: Katuwal, Khagendra, et al.
Publicado: (2026)
Seismology and diffusion of ultramassive white dwarf magnetic fields
por: Blatman, Daniel, et al.
Publicado: (2025)
por: Blatman, Daniel, et al.
Publicado: (2025)
Measuring the magnetic fields in the chromospheres of low-mass stars
por: Cang, Tianqi, et al.
Publicado: (2025)
por: Cang, Tianqi, et al.
Publicado: (2025)
Cyclic variations of the structure and energetics of solar magnetic fields
por: Obridko, V. N., et al.
Publicado: (2024)
por: Obridko, V. N., et al.
Publicado: (2024)
The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields
por: Schreiber, Matthias R., et al.
Publicado: (2025)
por: Schreiber, Matthias R., et al.
Publicado: (2025)
Reconstructing solar magnetic fields from historical observations X. Effect of magnetic field inclination and boundary structure on AIA 1600 Å emission
por: Tähtinen, Ismo, et al.
Publicado: (2024)
por: Tähtinen, Ismo, et al.
Publicado: (2024)
Ejemplares similares
-
Testing the reliability of magnetic field strength measurements for M dwarfs
por: Amateis, I., et al.
Publicado: (2026) -
Sulfur fractionation in coronal plumes as observed by Solar Orbiter/SPICE
por: Mzerguat, Slimane, et al.
Publicado: (2026) -
Radiative hydrodynamic simulations of FIP fractionation in solar flares
por: Reep, Jeffrey W., et al.
Publicado: (2025) -
Asteroseismology reveals the near-core magnetic field strength in the early-B star HD 43317
por: Bowman, D. M., et al.
Publicado: (2022) -
Comparing First Ionisation Potential bias diagnostics in the solar atmosphere
por: Spruksta, Kristena D., et al.
Publicado: (2026)