The Solar Dynamics Observatory (SDO)
2011/10/17 by W. Dean Pesnell, W. D. Pesnell, B. J. Thompson +2 · 3,476 citations
Physics and Astronomy · #Aerospace engineering #Astro and Planetary Science #Astronomy #Coronal mass ejection #Extreme ultraviolet #Geography #Geosynchronous orbit #Heliosphere #Meteorology #Observatory #Orbital mechanics #Physics #Planetary Science and Exploration #Plasma #Remote sensing #Satellite #Solar and Space Plasma Dynamics #Solar irradiance #Solar wind #Space weather #Spacecraft
paper · pdf · doi:10.1007/s11207-011-9841-3
published in Solar Physics 275(1-2), 3-15 (Springer Science+Business Media)
openalex publication_date 2011/10/17 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
Abstract
The Solar Dynamics Observatory (SDO) was launched on 11 February 2010 at 15:23 UT from Kennedy Space Center aboard an Atlas V 401 (AV-021) launch vehicle. A series of apogee-motor firings lifted SDO from an initial geosynchronous transfer orbit into a circular geosynchronous orbit inclined by 28° about the longitude of the SDO-dedicated ground station in New Mexico. SDO began returning science data on 1 May 2010. SDO is the first space-weather mission in NASA’s Living With a Star (LWS) Program. SDO’s main goal is to understand, driving toward a predictive capability, those solar variations that influence life on Earth and humanity’s technological systems. The SDO science investigations will determine how the Sun’s magnetic field is generated and structured, how this stored magnetic energy is released into the heliosphere and geospace as the solar wind, energetic particles, and variations in the solar irradiance. Insights gained from SDO investigations will also lead to an increased understanding of the role that solar variability plays in changes in Earth’s atmospheric chemistry and climate. The SDO mission includes three scientific investigations (the Atmospheric Imaging Assembly (AIA), Extreme Ultraviolet Variability Experiment (EVE), and Helioseismic and Magnetic Imager (HMI)), a spacecraft bus, and a dedicated ground station to handle the telemetry. The Goddard Space Flight Center built and will operate the spacecraft during its planned five-year mission life; this includes: commanding the spacecraft, receiving the science data, and forwarding that data to the science teams. The science investigations teams at Stanford University, Lockheed Martin Solar Astrophysics Laboratory (LMSAL), and University of Colorado Laboratory for Atmospheric and Space Physics (LASP) will process, analyze, distribute, and archive the science data. We will describe the building of SDO and the science that it will provide to NASA.
Citations
Cited by
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- Development of a Confined Circular-Cum-Parallel Ribbon Flare and Associated Pre-Flare Activity
- High-Resolution Observations of a Flux Rope with the Interface Region Imaging Spectrograph
- Magnetic Reconnection at a Hyperbolic Flux Tube Associated with a Confined Flare in NOAA Active Region 12268
- Recalibration of the Sunspot-Number: Status Report
- The Tests and Calibrations of the Hard X-ray Imager Aboard ASO-S
- Quasi-Separatrix Layers and Three-Dimensional Magnetic Reconnection: Theory and Observations of Solar Flares (Invited Review)
- TuMag: The Tunable Magnetograph for the Sunrise III Mission
- Invited Review: Short-term Variability with the Observations from the Helioseismic and Magnetic Imager (HMI) Onboard the Solar Dynamics Observatory (SDO): Insights into Flare Magnetism
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- Science Operation and Data Analysis Center of the Advanced Space-Based Solar Observatory (ASO-S) Mission
- First Observations of a Geomagnetic Superstorm With a Sub‐L1 Monitor
- Apparent Transverse Motion of Light Bridges Coupled to Coronal Loop Dynamics
- Solar Flare Ribbons Structured by Uncombed Chromospheric Loops
- Simulating the Solar Corona with Multiple Solar Photospheric Magnetic Maps during the 2024 April 8 Total Solar Eclipse
- Spectral and Spatial Graph Learning for Multispectral Solar Image Compression
- A coronal mass ejection encountered by four spacecraft within 1 au from the Sun: ensemble modelling of propagation and magnetic structure
- The M- and X-class White-light Flares in Super Active Region NOAA 13664/13697 Observed by ASO-S/LST/WST
- Tracking an eruptive intermediate prominence originating from the farside of the Sun
- Sunrise iii: Overview of Observatory and Instruments
- Data-Constrained Magnetohydrodynamics Simulation of a Confined X-class Flare in NOAA Active Region 11166
- On the Magnetic Reconnection and its Properties during a Flare Using a Magnetohydrodynamics Simulation
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- Thread Separation and Expansion Observed in Multi-Stranded Solar Coronal Loops
- Spatial and Dynamical Relations between Spicules and Network Bright Points
- Two-stage primary acceleration in filament initial eruption under a fan-spine magnetic configuration
- Driving mechanisms of solar active region geysers: The role of interacting magnetic flux
- 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
- The Formation of Solar Prominences: Plasma Origin and Mechanisms
- The Spontaneous Genesis of Solar Prominence Structures Driven by Supergranulation in Three-Dimensional Simulations
- The Atmospheric Response to Large Electron Beam Fluxes in Solar Flares III: Comprehensive Modeling of the Brightest Observed Near-Ultraviolet Continuum Source in an X9 Solar Flare
- Investigation on the Predictive Potentiality of Photospheric Magnetic Parameters for Distinguishing Confined from Eruptive Solar Flares
- Partial Null Point Reconnection of an Eruptive Filament
- Two-Stage Nature of a Solar Flare with Parallel and Semi-Circular Ribbons
- The He I D3 Line as a Proxy for Magnetic Activity using EXPRES Solar Observations
- When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps
- Observation and Modeling of Shear Evolution of Post-reconnection Flare Loops
- The Temperature-dependent Damping of Propagating Slow Magnetoacoustic Waves
- Solar orbiter: a short review of the mission and early science results
- The Behaviour of the EUV Corona Before Flares in Regions with High Free Magnetic Energy
- Solar flare forecasting with foundational transformer models across image, video, and time-series modalities
- Magnetic Field Configuration of a Quiescent Prominence Revealed by Large-amplitude Longitudinal Oscillations in End-view Observations
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- Evaluating Solar Wind Forecast Using Magnetic Maps That Include Helioseismic Far-Side Information
- Witnessing Magnetic Reconnection in Tangled Superpenumbral Fibrils Around a Sunspot
- Wide-Field Image Restoration of G-Band and Ca ii K Images Containing Large and Complex Active Regions
- Helioseismic Constraints: Past, Current, and Future Observations
- Understanding the secular variability of solar irradiance: the potential of Ca II K observations
- Validating DIRECD: Statistical Evaluation of Coronal Mass Ejections Direction Estimates from Coronal Dimmings
- Atmospheric Gravity Waves Modulated by the Magnetic Field Configuration
- Magnetic Dip Found in a Quiescent Prominence Foot via Observation and Simulation
- Observational Evidence Linking Loop Length and Thermal-Nonthermal Peak Timing in Solar Flares
- Back reaction of the untwisting solar corona scars sunspots
- Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager
- A new facility for airborne solar astronomy: NASA's WB-57 at the 2017 total solar eclipse
- Solar Observation with MeerKAT: Demonstration of Technical Readiness and Initial Science Highlight
- Nonthermal X-Ray Emission Associated with Supra-arcade Downflows in the Late Decay Phase of a Solar Flare
- Kinematics and Untwisting Motion of an Intriguing Jet-like Prominence Eruption
- High-Resolution Modeling of Coronae and Winds in Solar-Type Stars with Varying Rotation Rates. I. X-Ray Coronae
- Sun-as-a-star Analysis of the Solar Eruption Source Region Using Ha Spectroscopic Observations of CHASE
- Extreme Ultraviolet Wave and Quasi-periodic Pulsations during an eruptive M-class Flare
- On the analysis of eruptive events with non-radial evolution
- The Solar Orbiter mission -- Science overview
- A Multimodal Tiered Magnetic Polarity Inversion Features Dataset for Space Weather Forecasting
- The Kinematical Behavior of Solar Eruptive Filaments Affected by the Poloidal Magnetic Field
- An intense geomagnetic storm originated from stealth Coronal Mass Ejection: remote and in situ observations by near radially aligned spacecraft
- Observations of Flare Induced Doppler Shifts in the Si~iii 1206 \textrmÅ line
- Formation of a Coronal Hole by a quiet-Sun Filament Eruption
- CoSEE-Cat: A Comprehensive Solar Energetic Electron event Catalogue obtained from combined in situ and remote-sensing observations from Solar Orbiter -- Catalogue description and first statistical results
- The Role of Far-side Magnetic Structures in Modeling 2024 Solar Eclipse
- Identification of Nonlinear Damping of Transverse Loop Oscillations by KHI-induced Turbulence
- Modeling of AR 12760 with GX Simulator and Evidence for the Extended Transition Region in Peripheral Active Region Loops
- COCONUT: A coronal model with an energy decomposition strategy
- Early Evolution of the Cavity and Core of a Coronal Mass Ejection in the Inner Corona
- Size Distributions of Arcsecond-Scale Properties of Solar Flare Ribbons
- Self-Consistent Heating of the Magnetically Closed Solar Corona: Generation of Nanoflares, Thermodynamic Response of the Plasma and Observational Signatures
- SuryaBench: Benchmark Dataset for Advancing Machine Learning in Heliophysics and Space Weather Prediction
- Period Increase and Amplitude Distribution of Kink Oscillation of Coronal Loop
- Automatic detection of Ellerman bombs in the Hα line
- A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842. II. Dynamics of the Solar Eruption Associated with the X9.0 Solar Flare
- SARD: A YOLOv8-Based System for Solar Active Region Detection with SDO/HMI Magnetograms
- Coronal dimmings and what they tell us about solar and stellar coronal mass ejections
- Pivot of the Emerging Bipolar Magnetic Region in the Birth of Sigmoidal Solar Active Regions
- Understanding the Magnetic Field and Plasma-β along Umbral Fan Loops Traced Using 3 Minute Slow Waves
- 3D fast-mode Wave Propagation from Corona to Chromosphere: Triggering Mechanism for 3D Oscillations of filaments
- A Center-Median Filtering Method for Detection of Temporal Variation in Coronal Images
- Waiting Time Distribution of Supra-Arcade Downflows
- Responses of a Coronal Hole to a Fast Flare-Driven Coronal Wave
- High-resolution Observations of a C9.3 White-light Flare and Its Impact on the Solar Photosphere
- LOCNES: a solar telescope to study stellar activity in the near infrared
- Ion-rich acceleration during an eruptive flux rope event in a multiple null-point configuration
- Observation and Modeling of Small Spatial Structures of Solar Radio Noise Storms using the uGMRT
- Dynamics of Reconnection Nanojets in Eruptive and Confined Solar Flares
- High-frequency magnetohydrodynamic waves with substantial energy in the solar polar corona
- Two Cases of Non-Radial Filament Eruption and Associated CME Deflection
- EUV Wave and Coronal Seismology
- Avalanching together: A model for sympathetic flaring
- Dynamics of Subsurface Flows in Solar Active Regions During the May 2024 Storm
- Earth-affecting Solar Transients: A Review of Progresses in Solar Cycle 24
- Characterizing the Observational Properties of the Sun's High-latitude m=1 Inertial Mode
- Counter-Streaming Velocities in a Quiescent Filament
- Systematic non-thermal velocity increase preceding soft X-ray flare onset: A large-scale Hinode/EIS study
- Prominence material observed by SoloHI beyond 0.5au
- Intense Hard X-ray Emissions in C-class Flares: A Statistical Study with ASO-S/HXI Data
- Photospheric magnetic field variations accompanying the 2011 June 7 eruptive event
- A Novel Fine Spectral Structure of Solar Radio Bursts with Periodic Beaded Stripes Observed by CBSm of CMP-II
- The Observations of Magnetic Reconnection During the Interaction Process of Two Active Region Filaments
- Quantifying Suppression of Solar Surface Magnetic Flux Advection with Increasing Field Strength
- Structure and dynamics of erupting solar prominences using the Rolling Hough Transform: Toward a feature-oriented classification
- Numerical simulation of oscillatory magnetic reconnection modulated by solar convective motions
- Relationship between prominence eruptions and coronal mass ejections during solar cycle 24
- Ensemble Modeling of the Solar Wind Flow with Boundary Conditions Governed by Synchronic Photospheric Magnetograms. I. Multi-point Validation in the Inner Heliosphere
- Falling Threads During Solar Filament Eruptions
- Long-Duration Nonthermal Motions in the Supra-Arcade and Loop-Top Region During an Eruptive Solar Flare
- Inferring the magnetic field asymmetry of solar flares from the degree of polarisation at millimetre wavelengths
- How Reconnection-Unfavored Magnetic Flux Emergence Suppresses Solar Filament Eruptions
- Deciphering the Formation and Dynamics of Double-decker Filament Through Component Magnetic Reconnection
- Oscillatory magnetic reconnection at a coronal bright point
- Quantifying Chromosphere Response to Flare Energy Release Using AIA Observations in 1600~Å and 304~Å Passbands
- Reconstructing solar irradiance from historical Ca II K observations. I. Method and its validation
- Recurrent Jetlets Associated with the Disappearance of a Satellite Spot
- Observations of a New Form of Partial Filament Eruption
- PINN ME: A Physics-Informed Neural Network Framework for Accurate Milne-Eddington Inversions of Solar Magnetic Fields
- Solar polarimetry through the K i lines at 770 nm
- DARK POST-FLARE LOOPS OBSERVED BY THE SOLAR DYNAMICS OBSERVATORY
- The Role of Reconnection at Magnetic Separators in Complex Solar Flare Ribbons
- Multi-Viewpoint Observation of a Failed Prominence Eruption on the Sun
- Quasiperiodic Slipping Motion of Flare Ribbon Fine Structures Anchored in a Sunspot Light Bridge
- A new view of the solar interface region from the Interface Region Imaging Spectrograph (IRIS)
- Installation of solar chromospheric telescope at the Indian Astronomical Observatory, Merak
- Space weather: the solar perspective -- an update to Schwenn (2006)
- Revisiting Approaches to Stellar White-Light Flare Energy Based on Spatiotemporally Resolved Solar Observations
- Energetics and Emission in a Simulated Solar Flare Initialised by a Non-Force Free Magnetic Field
- Observations of a Twin Pair of Atypical Solar Flares and a Magnetic-reconnection Scenario
- Few Made It Out: A Multi-Messenger Study of an In Situ Solar Energetic Electron Event Driven by a Solar Jet
- Power-law Indices of EUV Intensity Power Spectrum in Flaring Coronal Active Regions
- ON THE MAGNETISM AND DYNAMICS OF PROMINENCE LEGS HOSTING TORNADOES
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- LOCNES: Low Cost NIR Extended Solar Telescope
- Optimization of Photospheric Electric Field Estimates for Accurate Retrieval of Total Magnetic Energy Injection
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- Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona
- Energy Evolution from the Chromosphere to the Heliosphere in the 2021 October 28 Solar Eruption
- Coronal Mass Ejection and Heliospheric Current Sheet Interaction Causing a Long-Duration Magnetic Field Sector Transition
- Reconnection nanojets in an erupting solar filament with unprecedented high speeds
- Operational Solar Flare Forecasting System Using an Explainable Large Language Model
- Quasiperiodic Pulsations and Three-dimensional Magnetic Reconnection during 2022 March 31 Flare Observed by IRIS and STIX
- The Non-Eruptive Reconfiguration of a Quiescent Filament After a Nearby Active Region Emergence
- SPECTROSCOPIC DIAGNOSTICS OF SOLAR MAGNETIC FLUX ROPES USING IRON FORBIDDEN LINE
- Kelvin-Helmholtz instability in coronal mass ejecta in the lower corona
- Prospects of Solar Magnetometry—From Ground and in Space
- EXTREMELY LARGE EUV LATE PHASE OF SOLAR FLARES
- Sigmoid Formation, Filament Destabilization, and Initiation of Weak Flare by Tether-Cutting Reconnection
- EMERGING DIMMINGS OF ACTIVE REGIONS OBSERVED BY THE SOLAR DYNAMICS OBSERVATORY
- PROPAGATION OF THE 2014 JANUARY 7 CME AND RESULTING GEOMAGNETIC NON-EVENT
- CORONAL RESPONSE TO AN EUV WAVE FROM DEM ANALYSIS
- Supergranular-scale magnetic flux emergence beneath an unstable filament
- Analysis of Solar Flare and Sunspots on 4th Jan 2025 and Their Effects on Space Weather
- Multiwavelength Studies of MHD Waves in the Solar Chromosphere
- Improved methods for determining the kinematics of coronal mass ejections and coronal waves
- Giant quiescent solar filament observed with high-resolution spectroscopy
- EUV Irradiance Observations from SDO/EVE as a Diagnostic of Solar Flares
- The Relationship between the Kinematics of Coronal Mass Ejections and the Brightness of the Corona
- Spectral Irradiance Variability in Lyman-Alpha Emission During Solar Flares
- ALEXIS: Recreating the X-Ray Emission from the Full Solar Disk as a Linear Combination of Discrete Regions in the Extreme Ultraviolet and Soft X-Rays
- Spectroscopic and imaging observations of small-scale reconnection events
- Observational study on the fine structure and dynamics of a solar jet. II. Energy release process revealed by spectral analysis
- Correlated Spatiotemporal Evolution of Extreme-Ultraviolet Ribbons and Hard X-rays in a Solar Flare
- Statistical analysis of the onset temperature of solar flares in 2010–2011
- Coronal Magnetic Structure of Earthbound CMEs and In Situ Comparison
- Detection and analysis of white-light emission in solar flares through light curve diagnostics
- Long-Period Oscillations of Sunspots Observed by SOHO/MDI
- The chromospheric component of coronal bright points. Coronal and chromospheric responses to magnetic-flux emergence
- A SOLAR CORONAL JET EVENT TRIGGERS A CORONAL MASS EJECTION
- Diagnosing a Solar Flaring Core with Bidirectional Quasi-periodic Fast Propagating Magnetoacoustic Waves
- Mapping solar magnetic fields from the photosphere to the base of the corona
- Recurrent coronal jets observed by SDO/AIA
- The Energetics of White-light Flares Observed bySDO/HMI andRHESSI
- Flare Expansion to a Magnetic Rope Accompanied by Rare Radio Bursts
- Understanding the Origins of Problem Geomagnetic Storms Associated with “Stealth” Coronal Mass Ejections
- The need for new techniques to identify the high-frequency MHD waves of an oscillating coronal loop
- Formation of a Solar Filament by Magnetic Reconnection, Associated Chromospheric Evaporation, and Subsequent Coronal Condensation
- Stellar X-rays and magnetic activity in 3D MHD coronal models
- THE FORMATION AND EARLY EVOLUTION OF A CORONAL MASS EJECTION AND ITS ASSOCIATED SHOCK WAVE ON 2014 JANUARY 8
- Nonlinear Force-Free Modeling of the Corona in Spherical Coordinates
- Block-induced Complex Structures Building the Flare-productive Solar Active Region 12673
- The Coronal Monsoon: Thermal Nonequilibrium Revealed by Periodic Coronal Rain
- CNN-Based Deep Learning Model for Solar Wind Forecasting
- DETERMINING HEATING RATES IN RECONNECTION FORMED FLARE LOOPS OF THE M8.0 FLARE ON 2005 MAY 13
- Interaction of Two Active Region Filaments Observed by NVST and SDO
- Pre-eruption Splitting of the Double-decker Structure in a Solar Filament
- Oscillations and Mass Draining that Lead to a Sympathetic Eruption of a Quiescent Filament
- Measuring stellar magnetic helicity density
- Understanding the Plasma and Magnetic Field Evolution of a Filament Using Observations and Nonlinear Force-free Field Modeling
- TIME-DEPENDENT SUPPRESSION OF OSCILLATORY POWER IN EVOLVING SOLAR MAGNETIC FIELDS
- Prominence instability and CMEs triggered by massive coronal rain in the solar atmosphere
- Study on Precursor Activity of the X1.6 Flare in the Great AR 12192 with SDO, IRIS, and Hinode
- Flux rope breaking and formation of a rotating blowout jet
- Partial Eruption, Confinement, and Twist Buildup and Release of a Double-decker Filament
- Height-Dependent Slow Magnetoacoustic Wave Amplitude and Energy Flux in Sunspot Atmospheres
- A New Formation Mechanism of Counterstreaming Mass Flows in Filaments and the Doppler Bullseye Pattern in Prominences
- Observation of solar coronal heating powered by magneto-acoustic oscillations in a moss region
- The Drivers of Active Region Outflows into the Slow Solar Wind
- Electric Current Evolution at the Footpoints of Solar Eruptions
- Active-region Tilt Angles from White-light Images and Magnetograms: The Role of Magnetic Tongues
- ULTRA-NARROW NEGATIVE FLARE FRONT OBSERVED IN HELIUM-10830 Å USING THE 1.6 m NEW SOLAR TELESCOPE
- Large-amplitude Longitudinal Oscillations Triggered by the Merging of Two Solar Filaments: Observations and Magnetic Field Analysis
- Observation of a Large-scale Quasi-circular Secondary Ribbon Associated with Successive Flares and a Halo CME
- An Extreme-ultraviolet Wave Generating Upward Secondary Waves in a Streamer-like Solar Structure
- IRIS Observations of Short-term Variability in Moss Associated with Transient Hot Coronal Loops
- Characteristics of Chromospheric Oscillation Periods in Magnetic Bright Points (MBPs)
- ABOVE-THE-LOOP-TOP OSCILLATION AND QUASI-PERIODIC CORONAL WAVE GENERATION IN SOLAR FLARES
- LOFAR Observations of a Jet-driven Piston Shock in the Low Solar Corona
- Direct Observations of Different Sunspot Waves Influenced by Umbral Flashes
- A New Magnetic Parameter of Active Regions Distinguishing Large Eruptive and Confined Solar Flares
- Magnetohydrodynamic Modeling of Solar Coronal Dynamics with an Initial Non-force-free Magnetic Field
- Spatial and Temporal Analysis of 3 minute Oscillations in the Chromosphere Associated with the X2.2 Solar Flare on 2011 February 15
- The Interface Region Imaging Spectrograph (IRIS)
- Deep Flare Net (DeFN) Model for Solar Flare Prediction
- REFLECTION OF PROPAGATING SLOW MAGNETO-ACOUSTIC WAVES IN HOT CORONAL LOOPS: MULTI-INSTRUMENT OBSERVATIONS AND NUMERICAL MODELING
- Filament Activation in Response to Magnetic Flux Emergence and Cancellation in Filament Channels
- The magnetic helicity density patterns from non-axisymmetric solar dynamo
- Recovering the unsigned photospheric magnetic field from Ca II K observations
- Abnormal oscillation modes in a waning light bridge
- IRIS Observations of Magnetic Interactions in the Solar Atmosphere between Preexisting and Emerging Magnetic Fields. I. Overall Evolution
- A Statistical Study of Propagating MHD Kink Waves in the Quiescent Corona
- Multi-Scale Gaussian Normalization for Solar Image Processing
- Coronal Elemental Abundances in Solar Emerging Flux Regions
- A SOLAR FLARE DISTURBING A LIGHT WALL ABOVE A SUNSPOT LIGHT BRIDGE
- Impulsive coronal heating during the interaction of surface magnetic fields in the lower solar atmosphere
- Relation of Coronal Rain Originating from Coronal Condensations to Interchange Magnetic Reconnection
- Observations of a Quasi-periodic, Fast-Propagating Magnetosonic Wave in Multiple Wavelengths and Its Interaction with Other Magnetic Structures
- Evolution of a streamer-blowout CME as observed by imagers on Parker Solar Probe and the Solar Terrestrial Relations Observatory
- HOOKED FLARE RIBBONS AND FLUX-ROPE-RELATED QSL FOOTPRINTS
- The active region source of a type III radio storm observed by Parker Solar Probe during encounter 2
- The solar wind from a stellar perspective
- Sympathetic Eruptions of Two Filaments with an Identifiable Causal Link Observed by the Solar Dynamics Observatory
- The Observational Uncertainty of Coronal Hole Boundaries in Automated Detection Schemes
- Estimation of the Physical Parameters of a CME at High Coronal Heights Using Low-frequency Radio Observations
- Plasma flows and magnetic field interplay during the formation of a pore
- Active Region Photospheric Magnetic Properties Derived from Line-of-Sight and Radial Fields
- Recurrent Two-sided Loop Jets Caused By Magnetic Reconnection between Erupting Minifilaments and a nearby Large Filament
- TEMPORAL EVOLUTION AND SPATIAL DISTRIBUTION OF WHITE-LIGHT FLARE KERNELS IN A SOLAR FLARE
- Determining the Intrinsic CME Flux Rope Type Using Remote-sensing Solar Disk Observations
- Microflare Heating of a Solar Active Region Observed with NuSTAR, Hinode/XRT, and SDO/AIA
- Flux Erosion of Magnetic Clouds by Reconnection With the Sun's Open Flux
- Observations of the Formation, Development, and Structure of a Current Sheet in an Eruptive Solar Flare
- NONLINEAR FORCE-FREE FIELD MODELING OF THE SOLAR MAGNETIC CARPET AND COMPARISON WITHSDO/HMI ANDSUNRISE/IMAX OBSERVATIONS
- On Solar Recurrent Coronal Jets: Coronal Geysers as Sources of Electron Beams and Interplanetary Type-III Radio Bursts
- Chromospheric Heating due to Cancellation of Quiet Sun Internetwork Fields
- Bypassing the static input size of neural networks in flare forecasting by using spatial pyramid pooling
- Effect of Transport Coefficients on Excitation of Flare-induced Standing Slow-mode Waves in Coronal Loops
- Solar Flare Prediction Model with Three Machine-learning Algorithms using Ultraviolet Brightening and Vector Magnetograms
- Multiwavelength Signatures of Episodic Null Point Reconnection in a Quadrupolar Magnetic Configuration and the Cause of Failed Flux Rope Eruption
- The Width Distribution of Loops and Strands in the Solar Corona—Are We Hitting Rock Bottom?
- Observation and modelling of solar jets
- Stereoscopic Observations of an Erupting Mini-filament-driven Two-sided-loop Jet and the Applications for Diagnosing a Filament Magnetic Field
- Network Jets as the Driver of Counter-streaming Flows in a Solar Filament/Filament Channel
- Measuring three-dimensional shapes of stable solar prominences using stereoscopic observations from SDO and STEREO
- Sequential ejections of plasma blobs due to unbraiding of tangled loops in the solar atmosphere
- Quasi‐Periodic Pulsations in Ionospheric TEC Synchronized With Solar Flare EUV Emission
- Detection of Opposite Magnetic Polarity in a Light Bridge: Its Emergence and Cancellation in Association with LB Fan-shaped Jets
- X-class Flare on 2023 December 31 Observed by the Solar Ultraviolet Imaging Telescope on Board Aditya-L1
- Connecting solar flare hard X-ray spectra to in situ electron spectra
- Magnetically coupled atmosphere, fast sausage MHD waves, and forced magnetic field reconnection during the SOL2014-09-10T17:45 flare
- Homologous White Light Solar Flares Driven by Photospheric Shear Motions
- OSCILLATION OF NEWLY FORMED LOOPS AFTER MAGNETIC RECONNECTION IN THE SOLAR CHROMOSPHERE
- RESOLVING THE FAN-SPINE RECONNECTION GEOMETRY OF A SMALL-SCALE CHROMOSPHERIC JET EVENT WITH THE NEW SOLAR TELESCOPE
- Probing progression of heating through the lower flare atmosphere via high-cadence IRIS spectroscopy
- A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842 I. Dynamics of the Solar Eruption Associated with the X7.1 Solar Flare
- Observational Evidence of a Flux Rope within a Sunspot Umbra
- The role of partial ionization effects in the chromosphere. [europepmc]
- Multi-Scale Gaussian Normalization for Solar Image Processing. [europepmc]
- On Flare-CME Characteristics from Sun to Earth Combining Remote-Sensing Image Data with In Situ Measurements Supported by Modeling. [europepmc]
- Formation and dynamics of a solar eruptive flux tube. [europepmc]
- Observing Kelvin-Helmholtz instability in solar blowout jet. [europepmc]
- Solar UV and X-ray spectral diagnostics. [europepmc]
- On-Orbit Performance of the Helioseismic and Magnetic Imager Instrument onboard the Solar Dynamics Observatory . [europepmc]
- Flare-productive active regions. [europepmc]
- CME-HSS Interaction and Characteristics Tracked from Sun to Earth. [europepmc]
- Magnetism, dynamo action and the solar-stellar connection. [europepmc]
- On-Disc Observations of Flux Rope Formation Prior to Its Eruption. [europepmc]
- The ELFIN Mission. [europepmc]
- Solar Coronal Jets: Observations, Theory, and Modeling. [europepmc]
- Accurately constraining velocity information from spectral imaging observations using machine learning techniques. [europepmc]
- An overall view of temperature oscillations in the solar chromosphere with ALMA. [europepmc]
- Magnetoacoustic wave energy dissipation in the atmosphere of solar pores. [europepmc]
- Spectropolarimetric fluctuations in a sunspot chromosphere. [europepmc]
- Design and Performance of the ICON EUV Spectrograph. [europepmc]
- Understanding the Origins of Problem Geomagnetic Storms Associated with "Stealth" Coronal Mass Ejections. [europepmc]
- On a limitation of Zeeman polarimetry and imperfect instrumentation in representing solar magnetic fields with weaker polarization signal. [europepmc]
- Defining the Middle Corona. [europepmc]
- Solar active region magnetogram image dataset for studies of space weather. [europepmc]
- Multi-source connectivity as the driver of solar wind variability in the heliosphere. [europepmc]
- On the Instrumental Discrepancies in Lyman-Alpha Observations of Solar Flares. [europepmc]
- Combined Surface Flux Transport and Helioseismic Far-Side Active Region Model (FARM). [europepmc]
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