All Stories

  1. 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
  2. Acceleration of Solar Eruptions via Enhanced Torus Instability Driven by Small-scale Flux Emergence
  3. 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
  4. A Magnetohydrodynamics Simulation of Coronal Mass Ejections in the Upper Corona at 2.5R⊙ ≤ r ≤ 19R⊙
  5. Are Electric-field-driven Magnetohydrodynamic Simulations of the Solar Corona Sensitive to the Initial Condition?
  6. Boundary Treatment for the Subsonic/Alfvénic Inner Boundary at 2.5 R ⊙ in a Time-dependent 3D Magnetohydrodynamics Solar Wind Simulation Model
  7. A new time-dependent three-dimensional magnetohydrodynamics (MHD) simulation model for the trans-sonic/Alfvenic solar wind from 2.5Rs
  8. An Evolution and Eruption of the Coronal Magnetic Field through a Data-driven MHD Simulation
  9. A Comparative Study of Solar Active Region 12371 with Data-constrained and Data-driven Magnetohydrodynamic Simulations
  10. The Nonpotentiality of Steady-state Coronal Magnetic Field Derived with Time-relaxation Magnetohydrodynamics Simulations Using Helioseismic and Magnetic Imager Three-component Magnetic Field Data
  11. An Electric-field-driven Global Coronal Magnetohydrodynamics Simulation Model Using Helioseismic and Magnetic Imager Vector-magnetic-field Synoptic Map Data
  12. Optimization of parameters of CME initiation in the MHD simulation suite
  13. Coupling a Global Heliospheric Magnetohydrodynamic Model to a Magnetofrictional Model of the Low Corona
  14. The Coronal Global Evolutionary Model: Using HMI Vector Magnetogram and Doppler Data to Determine Coronal Magnetic Field Evolution
  15. Comparative Study of Data-driven Solar Coronal Field Models Using a Flux Emergence Simulation as a Ground-truth Data Set
  16. Parametric Study of ICME Properties Related to Space Weather Disturbances via a Series of Three-Dimensional MHD Simulations
  17. The Role of a Tiny Brightening in a Huge Geoeffective Solar Eruption Leading to the St. Patrick’s Day Storm
  18. Magnetohydrodynamic Simulations for Solar Active Regions using Time-series Data of Surface Plasma Flow and Electric Field Inferred from Helioseismic Magnetic Imager Vector Magnetic Field Measurements
  19. Prospective White-light Imaging and In Situ Measurements of Quiescent Large-scale Solar-wind Streams from the Parker Solar Probe and Solar Orbiter
  20. Erratum: “An MHD Simulation of Solar Active Region 11158 Driven with Time-dependent Electric Field Determined from HMI Vector Magnetic Field Measurement Data” (2018, ApJ, 855, 11)
  21. An MHD Simulation of Solar Active Region 11158 Driven with a Time-dependent Electric Field Determined from HMI Vector Magnetic Field Measurement Data
  22. Prospective Out-of-ecliptic White-light Imaging of Coronal Mass Ejections Traveling through the Corona and Heliosphere
  23. Prospective Out-of-ecliptic White-light Imaging of Interplanetary Corotating Interaction Regions at Solar Maximum
  24. Relation Between Coronal Hole Areas and Solar Wind Speeds Derived from Interplanetary Scintillation Measurements
  25. Vector Magnetic Field Synoptic Charts from the Helioseismic and Magnetic Imager (HMI)
  26. Exploration of solar photospheric magnetic field data sets using the UCSD tomography
  27. LONG-TERM TREND OF SOLAR CORONAL HOLE DISTRIBUTION FROM 1975 TO 2014
  28. MHD-IPS analysis of relationship among solar wind density, temperature, and flow speed
  29. STRUCTURE AND STABILITY OF MAGNETIC FIELDS IN SOLAR ACTIVE REGION 12192 BASED ON NONLINEAR FORCE-FREE FIELD MODELING
  30. Comparison of potential field solutions for Carrington Rotation 2144
  31. The Coronal Global Evolutionary Model: Using HMI Vector Magnetogram and Doppler Data to Model the Buildup of Free Magnetic Energy in the Solar Corona
  32. The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Magnetohydrodynamics Simulation Module for the Global Solar Corona
  33. MAGNETOHYDRODYNAMIC SIMULATION OF THE X2.2 SOLAR FLARE ON 2011 FEBRUARY 15. II. DYNAMICS CONNECTING THE SOLAR FLARE AND THE CORONAL MASS EJECTION
  34. STATISTICAL ANALYSIS OF THE HORIZONTAL DIVERGENT FLOW IN EMERGING SOLAR ACTIVE REGIONS
  35. MAGNETOHYDRODYNAMIC SIMULATION OF THE X2.2 SOLAR FLARE ON 2011 FEBRUARY 15. I. COMPARISON WITH THE OBSERVATIONS
  36. The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches
  37. The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Overview and Performance
  38. MAGNETIC HELICITY IN EMERGING SOLAR ACTIVE REGIONS
  39. The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Optimization of the Spectral Line Inversion Code
  40. MHD analysis of the velocity oscillations in the outer heliosphere
  41. An MHD simulation model of time‐dependent global solar corona with temporally varying solar‐surface magnetic field maps
  42. MAGNETIC STRUCTURE PRODUCING X- AND M-CLASS SOLAR FLARES IN SOLAR ACTIVE REGION 11158
  43. Properties of High-Frequency Wave Power Halos Around Active Regions: An Analysis of Multi-height Data from HMI and AIA Onboard SDO
  44. A NON-RADIAL ERUPTION IN A QUADRUPOLAR MAGNETIC CONFIGURATION WITH A CORONAL NULL
  45. An MHD simulation model of time-dependent co-rotating solar wind
  46. DETECTION OF THE HORIZONTAL DIVERGENT FLOW PRIOR TO THE SOLAR FLUX EMERGENCE
  47. Comparison of Line-of-Sight Magnetograms Taken by the Solar Dynamics Observatory/Helioseismic and Magnetic Imager and Solar and Heliospheric Observatory/Michelson Doppler Imager
  48. EVOLUTION OF MAGNETIC FIELD AND ENERGY IN A MAJOR ERUPTIVE ACTIVE REGION BASED ONSDO/HMI OBSERVATION
  49. The MHD simulation of the inner heliosphere over 9 years using the observation-based time-varying boundary data
  50. A New Method for Polar Field Interpolation
  51. Non‐dipolar solar wind structure observed in the cycle 23/24 minimum
  52. Validation of Two MHD Models of the Solar Corona with Rotational Tomography
  53. MHD simulations of the global solar corona around the Halloween event in 2003 using the synchronic frame format of the solar photospheric magnetic field
  54. IPS tomographic observations of 3D solar wind structure
  55. MHD simulation of two successive interplanetary disturbances driven by cone-model parameters in IPS-based solar wind
  56. The 2003 October–November Fast Halo Coronal Mass Ejections and the Large‐Scale Magnetic Field Structures
  57. Three-Dimensional Magnetohydrodynamic Simulation of a Global Solar Corona Using a Temperature Distribution Map Obtained fromSOHOEIT Measurements
  58. Magnetohydrodynamic Simulations of the Solar Corona and Solar Wind Using a Boundary Treatment to Limit Solar Wind Mass Flux
  59. Fast solar wind after the rapid acceleration
  60. Polar low-speed solar wind reappeared at the solar activity maximum of cycle 23
  61. MHD tomography using interplanetary scintillation measurement
  62. How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation