Three-dimensional mapping of coronal magnetic field and plasma parameters in a solar flare
Fuente:
arXiv
Guardado en:
| Autores principales: | Kaltman, Tatyana, Yu, Sijie, Fleishman, Gregory D., Ryan, Daniel F. |
|---|---|
| Formato: | Preprint |
| Publicado: |
2026
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Dynamics of the coronal magnetic field in the 2022-10-02 X-class flare
por: Fleishman, Gregory D., et al.
Publicado: (2026)
por: Fleishman, Gregory D., et al.
Publicado: (2026)
Energy budget in the 2017-09-07 "cold" solar flare
por: Fleishman, Gregory D., et al.
Publicado: (2025)
por: Fleishman, Gregory D., et al.
Publicado: (2025)
Giant post-flare loops in active regions with extremely strong coronal magnetic fields
por: Alissandrakis, Costas E., et al.
Publicado: (2024)
por: Alissandrakis, Costas E., 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)
Unipolarity of the solar magnetic field in equatorial coronal holes
por: Katuwal, Khagendra, et al.
Publicado: (2026)
por: Katuwal, Khagendra, et al.
Publicado: (2026)
Coupling between magnetic reconnection, energy release, and particle acceleration in the X17.2 2003 October 28 solar flare
por: Kurt, Victoria G., et al.
Publicado: (2024)
por: Kurt, Victoria G., et al.
Publicado: (2024)
On the possibility of using decayless kink oscillations of coronal loops to forecast powerful solar flares and coronal mass ejections
por: Nechaeva, A. B., et al.
Publicado: (2025)
por: Nechaeva, A. B., et al.
Publicado: (2025)
Measurements of the solar coronal magnetic field based on coronal seismology with propagating Alfvenic waves: forward modeling
por: Gao, Yuhang, et al.
Publicado: (2024)
por: Gao, Yuhang, et al.
Publicado: (2024)
Three types of solar coronal rain during magnetic reconnection between open and closed magnetic structures
por: Qiao, Fangfang, et al.
Publicado: (2024)
por: Qiao, Fangfang, et al.
Publicado: (2024)
Three-dimensional kink modes in solar coronal slabs: group velocities and their implications for impulsively excited waves
por: Liu, Jing, et al.
Publicado: (2026)
por: Liu, Jing, et al.
Publicado: (2026)
Episodic energy release during the main- and post-impulsive phase of a solar flare
por: Wei, Yuqian, et al.
Publicado: (2024)
por: Wei, Yuqian, 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)
Spectroscopic investigations of a filament reconnecting with coronal loops during a two-ribbon solar flare
por: Joshi, Reetika, et al.
Publicado: (2025)
por: Joshi, Reetika, et al.
Publicado: (2025)
Three-dimensional properties of a coronal shock and the longitudinal distribution of its related solar energetic particles
por: Zhou, Yue, et al.
Publicado: (2026)
por: Zhou, Yue, et al.
Publicado: (2026)
Three-part structure of solar coronal mass ejection observed in low coronal signatures of Solar Orbiter
por: Podladchikova, Tatiana, et al.
Publicado: (2024)
por: Podladchikova, Tatiana, et al.
Publicado: (2024)
Understanding the thermal and magnetic properties of a X-class flare in the low solar atmosphere
por: Ferrente, F., et al.
Publicado: (2024)
por: Ferrente, F., et al.
Publicado: (2024)
Anomalous cross-field motions of solar coronal loops
por: Mandal, Sudip, et al.
Publicado: (2025)
por: Mandal, Sudip, 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)
Sun-as-a-star analysis of simulated solar flares
por: Yu, H. C., et al.
Publicado: (2025)
por: Yu, H. C., et al.
Publicado: (2025)
Nonthermal electron acceleration in turbulent post-flare coronal loops
por: Mora, Clarissa, et al.
Publicado: (2025)
por: Mora, Clarissa, 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)
Dynamic modeling of coronal abundances during flares on M-dwarf stars
por: Brooks, David H., et al.
Publicado: (2026)
por: Brooks, David H., et al.
Publicado: (2026)
Steady-State Heating of Diffuse Coronal Plasma in a Solar Active Region
por: Fleishman, Gregory D., et al.
Publicado: (2025)
por: Fleishman, Gregory D., et al.
Publicado: (2025)
Addressing the open flux problem with a non-spherical solar coronal magnetic field model
por: Wu, Ziqi, et al.
Publicado: (2026)
por: Wu, Ziqi, et al.
Publicado: (2026)
Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops
por: Li, Leping, et al.
Publicado: (2024)
por: Li, Leping, et al.
Publicado: (2024)
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)
Heating and cooling at a coronal magnetic null
por: Cargill, P. J., et al.
Publicado: (2025)
por: Cargill, P. J., et al.
Publicado: (2025)
Determination of the Height-Temperature Profile Above a Solar Active Region from Multi-Frequency Radio Observations
por: Kaltman, T. I., et al.
Publicado: (2026)
por: Kaltman, T. I., et al.
Publicado: (2026)
Stellar flares, superflares and coronal mass ejections -- entering the Big data era
por: Vida, Krisztián, et al.
Publicado: (2024)
por: Vida, Krisztián, et al.
Publicado: (2024)
Infrared spectropolarimetry of a C-class solar flare footpoint plasma -- I. Spectral features and forward modelling
por: Vashalomidze, Z., et al.
Publicado: (2026)
por: Vashalomidze, Z., et al.
Publicado: (2026)
MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT
por: Wang, Haopeng, et al.
Publicado: (2026)
por: Wang, Haopeng, et al.
Publicado: (2026)
Three-dimensional velocity fields of the solar filament eruptions detected by CHASE
por: Qiu, Ye, et al.
Publicado: (2024)
por: Qiu, Ye, et al.
Publicado: (2024)
Dreicer electric field definition and runaway electrons in solar flares
por: Tsap, Yu. T., et al.
Publicado: (2024)
por: Tsap, Yu. T., et al.
Publicado: (2024)
Thermodynamic and magnetic evolution of an eruptive C-class solar flare observed with SST/TRIPPEL-SP
por: Baso, C. J. Díaz, et al.
Publicado: (2025)
por: Baso, C. J. Díaz, et al.
Publicado: (2025)
The relationships among solar flare impulsiveness, energy release, and ribbon development
por: Tamburri, Cole A, et al.
Publicado: (2024)
por: Tamburri, Cole A, et al.
Publicado: (2024)
Solar Flare Hosts MeV-peaked Electrons in a Coronal Source
por: Fleishman, Gregory D., et al.
Publicado: (2026)
por: Fleishman, Gregory D., et al.
Publicado: (2026)
Ion acceleration in Fermi-LAT behind-the-limb solar flares: the role of coronal shock waves
por: Warmuth, Alexander, et al.
Publicado: (2025)
por: Warmuth, Alexander, et al.
Publicado: (2025)
Observing the evolution of the Sun's global coronal magnetic field over eight months
por: Yang, Zihao, et al.
Publicado: (2024)
por: Yang, Zihao, et al.
Publicado: (2024)
Simultaneous observations of a breakout current sheet and a flare current sheet in a coronal jet event
por: Yang, Liheng, et al.
Publicado: (2024)
por: Yang, Liheng, et al.
Publicado: (2024)
Properties of magnetic null points associated with X-class flares during solar cycle 24
por: Edgar, R. L., et al.
Publicado: (2024)
por: Edgar, R. L., et al.
Publicado: (2024)
Ejemplares similares
-
Dynamics of the coronal magnetic field in the 2022-10-02 X-class flare
por: Fleishman, Gregory D., et al.
Publicado: (2026) -
Energy budget in the 2017-09-07 "cold" solar flare
por: Fleishman, Gregory D., et al.
Publicado: (2025) -
Giant post-flare loops in active regions with extremely strong coronal magnetic fields
por: Alissandrakis, Costas E., et al.
Publicado: (2024) -
Stability of the coronal magnetic field around large confined and eruptive solar flares
por: Gupta, Manu, et al.
Publicado: (2024) -
Unipolarity of the solar magnetic field in equatorial coronal holes
por: Katuwal, Khagendra, et al.
Publicado: (2026)