SuNeRF: 3D Reconstruction of the Solar EUV Corona Using Neural Radiance Fields

SuNeRF: 3D Reconstruction of the Solar EUV Corona Using Neural Radiance Fields

To understand its evolution and the effects of its eruptive events, the Sun is permanently monitored by multiple satellite missions. The optically thin emission of the solar plasma and the limited number of viewpoints make it challenging to reconstruct the geometry and structure of the solar atmosph...

Disgrifiad llawn

Manylion Llyfryddiaeth
Prif Awduron:	Robert Jarolim, Benoit Tremblay, Andrés Muñoz-Jaramillo, Kyriaki-Margarita Bintsi, Anna Jungbluth, Miraflor Santos, Angelos Vourlidas, James P. Mason, Sairam Sundaresan, Cooper Downs, Ronald M. Caplan
Fformat:	Erthygl
Iaith:	English
Cyhoeddwyd:	IOP Publishing 2024-01-01
Cyfres:	The Astrophysical Journal Letters
Pynciau:	Solar corona Active solar corona Neural networks Solar filament eruptions Solar coronal holes
Mynediad Ar-lein:	https://doi.org/10.3847/2041-8213/ad12d2

Eitemau Tebyg

Multistage Reconnection Powering a Solar Coronal Jet
gan: David M. Long, et al.
Cyhoeddwyd: (2023-01-01)

Analysis of Solar Eruptions Deflecting in the Low Corona: Influence of the Magnetic Environment
gan: Abril Sahade, et al.
Cyhoeddwyd: (2024-01-01)

Investigating Coronal Holes and CMEs as Sources of Brightness Depletion Detected in PSP/WISPR Images
gan: Guillermo Stenborg, et al.
Cyhoeddwyd: (2023-01-01)

Structure of the Plasma near the Heliospheric Current Sheet as Seen by WISPR/Parker Solar Probe from inside the Streamer Belt
gan: Paulett C. Liewer, et al.
Cyhoeddwyd: (2023-01-01)

Evidence of Continuous Reconnection along a Helmet Streamer Current Sheet Observed by WISPR on Parker Solar Probe
gan: Paulett C. Liewer, et al.
Cyhoeddwyd: (2024-01-01)

The Equilibrium of Coronal Loops Near Separatrices
gan: Emily I Mason, et al.
Cyhoeddwyd: (2023-01-01)

Dominance of Bursty over Steady Heating of the 4–8 MK Coronal Plasma in a Solar Active Region: Quantification Using Maps of Minimum, Maximum, and Average Brightness
gan: Sanjiv K. Tiwari, et al.
Cyhoeddwyd: (2022-01-01)

First Infrared Coronal Spectra from DKIST/Cryo-NIRSP: Comparisons with Global MHD Models
gan: Thomas A. Schad, et al.
Cyhoeddwyd: (2023-01-01)

Coronagraphic Observations of Si x 1430 nm Acquired by DKIST/Cryo-NIRSP with Methods for Telluric Absorption Correction
gan: Thomas A. Schad, et al.
Cyhoeddwyd: (2024-01-01)

Multifrequency Microwave Imaging of Weak Transients from the Quiet Solar Corona
gan: Surajit Mondal, et al.
Cyhoeddwyd: (2023-01-01)

Reconnection-generated Plasma Flows in the Quasi-separatrix Layer in Localized Solar Corona
gan: Sripan Mondal, et al.
Cyhoeddwyd: (2023-01-01)

First Determination in the Extended Corona of the 2D Thermal Evolution of a Current Sheet after a Solar Eruption
gan: Alessandro Bemporad, et al.
Cyhoeddwyd: (2024-01-01)

A Community Data Set for Comparing Automated Coronal Hole Detection Schemes
gan: Martin A. Reiss, et al.
Cyhoeddwyd: (2024-01-01)

Are Nonthermal Velocities in Active Region Coronal Loops Anisotropic?
gan: Michael Hahn, et al.
Cyhoeddwyd: (2023-01-01)

Challenges in Forecasting the Evolution of a Distorted CME Observed During the First Close Solar Orbiter Perihelion
gan: Alessandro Liberatore, et al.
Cyhoeddwyd: (2024-01-01)

Ion Kinetics of Plasma Interchange Reconnection in the Lower Solar Corona
gan: Vladimir Krasnoselskikh, et al.
Cyhoeddwyd: (2023-01-01)

New Insights into Type-I Solar Noise Storms from High Angular Resolution Spectroscopic Imaging with the Upgraded Giant Metrewave Radio Telescope
gan: Surajit Mondal, et al.
Cyhoeddwyd: (2024-01-01)

Broad and Bidirectional Narrow Quasiperiodic Fast-propagating Wave Trains Associated with a Filament-driven Halo Coronal Mass Ejection on 2023 April 21
gan: Xinping Zhou, et al.
Cyhoeddwyd: (2024-01-01)

Density Enhancement Streams in The Solar Wind
gan: F. S. Mozer, et al.
Cyhoeddwyd: (2023-01-01)

On the Existence of Long-period Decayless Oscillations in Short Active Region Loops
gan: Arpit Kumar Shrivastav, et al.
Cyhoeddwyd: (2025-01-01)

Observations of the solar corona during the total solar eclipse on 21 August 2017
gan: Hui Tian, et al.
Cyhoeddwyd: (2017-08-01)

Solar signatures and eruption mechanism of the August 14, 2010 coronal mass ejection (CME)
gan: D’Huys Elke, et al.
Cyhoeddwyd: (2017-01-01)

A Near-half-century Simulation of the Solar Corona
gan: Valentin Aslanyan, et al.
Cyhoeddwyd: (2024-01-01)

The Solar Minimum Eclipse of 2019 July 2. III. Inferring the Coronal T e with a Radiative Differential Emission Measure Inversion
gan: Benjamin Boe, et al.
Cyhoeddwyd: (2023-01-01)

131 and 304 Å Emission Variability Increases Hours Prior to Solar Flare Onset
gan: Kara L. Kniezewski, et al.
Cyhoeddwyd: (2024-01-01)

Future high-resolution and high-cadence observations for unraveling small-scale explosive solar features
gan: Alphonse C. Sterling, et al.
Cyhoeddwyd: (2023-03-01)

First Direct Imaging of a Kelvin–Helmholtz Instability by PSP/WISPR
gan: Evangelos Paouris, et al.
Cyhoeddwyd: (2024-01-01)

Moreton waves and EUV waves in the solar atmosphere
gan: Pengfei Chen
Cyhoeddwyd: (2023-07-01)

Modeling of Condensations in Coronal Loops Produced by Impulsive Heating with Variable Frequencies and Locations
gan: Therese A. Kucera, et al.
Cyhoeddwyd: (2024-01-01)

The Stationary Point: A New Method for Solar Wind Speed Measurements from a Moving Vantage Point
gan: Samuel J. Van Kooten, et al.
Cyhoeddwyd: (2025-01-01)

A Precursor to Solar Prominence Eruptions: Detection and Analysis of EUV Prominence Oscillations
gan: William Beckwith-Chandler, et al.
Cyhoeddwyd: (2024-01-01)

The Error Estimation of Transverse Coronal Loop Oscillation Parameters Based on Least Chi-squares Fitting
gan: Hongbo Li, et al.
Cyhoeddwyd: (2025-01-01)

The Fine-scale Structure of Polar Coronal Holes
gan: R. J. Morton, et al.
Cyhoeddwyd: (2023-01-01)

Multiwavelength Sun-as-a-star Analysis of the M8.7 Flare on 2022 October 2 Using Hα and EUV Spectra Taken by SMART/SDDI and SDO/EVE
gan: Takato Otsu, et al.
Cyhoeddwyd: (2024-01-01)

Time-dependent Dynamics of the Corona
gan: Emily I. Mason, et al.
Cyhoeddwyd: (2023-01-01)

Is There a Dynamic Difference between Stealthy and Standard Coronal Mass Ejections?
gan: Beili Ying, et al.
Cyhoeddwyd: (2022-01-01)

Three-dimensional Velocity Fields of the Solar Filament Eruptions Detected by CHASE
gan: Ye Qiu, et al.
Cyhoeddwyd: (2024-01-01)

A Coronal Mass Ejection Impacting Parker Solar Probe at 14 Solar Radii
gan: Carlos R. Braga, et al.
Cyhoeddwyd: (2024-01-01)

Spectroscopic Observations of the Solar Corona during the 2017 August 21 Total Solar Eclipse: Comparison of Spectral Line Widths and Doppler Shifts between Open and Closed Magnetic Structures
gan: Yingjie Zhu, et al.
Cyhoeddwyd: (2024-01-01)

Simulation of Thermal Nonequilibrium Cycles in the Solar Wind
gan: Roger B. Scott, et al.
Cyhoeddwyd: (2024-01-01)