All Stories

  1. State of the Early Career Profession in Space Physics and Aeronomy: Climatological Survey Results
  2. Compressive Structures in the Foreshock of Collisionless Shocks
  3. Automated Identification of Foreshock Transients
  4. Multipoint analysis of interplanetary shocks with 6-point observatories around Sun-Earth L
  5. Solar Magnetic Configuration Control over Radiation Belt Electrons
  6. Universal energy limits of radiation belts in planetary and brown dwarf magnetospheric systems
  7. Relationship Between Magnetosheath ULF Waves and Ground‐Based Pc3‐4 Waves: A Statistical Study
  8. Energy Partition at a Collisionless Supercritical Quasi‐Parallel Shock
  9. Statistical Characteristics of Stormtime Bursty Bulk Flows
  10. State of the Early Career Profession in Space Physics and Aeronomy: Climatological Survey Results
  11. Reconstructing the Geometry of a Hot Flow Anomaly With Bounding Jets in Magnetosheath
  12. The Correlation Function for Magnetic Field Fluctuations at Ion Dissipation Scales in the Solar Wind
  13. Stormtime Magnetospheric Processes Associated With the Dawnside Current Wedge
  14. The Correlation Function for Magnetic Field Fluctuations at Ion Dissipation Scales in the Solar Wind
  15. Energy Conversion and Exchange in a Magnetosheath Jet
  16. A Comparison of Modeled and Observed Dayside Bow Shock Locations in 8 Years of MMS Data
  17. Automated Bow Shock Identification and Multi‐Spacecraft Timing Using Magnetospheric Multiscale (MMS) Observations
  18. On the Spatial Relationship Between the Aurora and Relativistic Electron Precipitation During a Storm‐Time Substorm
  19. Statistical Relationship Between Foreshock ULF Wave Power and Ground‐Based Pc3‐4 Wave Power
  20. Fermi Acceleration of Electrons at Earth's Bow Shock Due To Current Sheet Interaction
  21. The Correlation Function for Magnetic Field Fluctuations at Ion Dissipation Scales in the Solar Wind
  22. Role of ULF Waves in Reforming the Martian Bow Shock
  23. Automated Classification of MESSENGER Plasma Observations via Unsupervised Transfer Learning
  24. Multipoint observations of an atypical coronal mass ejection from Earth to Mars informed by early Europa Clipper data
  25. Interplay Between a Foreshock Bubble and a Hot Flow Anomaly Forming Along the Same Rotational Discontinuity
  26. Control of Solar Wind on Magnetic Field Fluctuations in the Subsolar Magnetosheath
  27. Ground Magnetic Response to an Extraordinary IMF BY Flip During the May 2024 Storm: Travel Time From the Magnetosheath to Dayside High Latitudes
  28. What is the relationship between the aurora and relativistic electron precipitation during a storm-time substorm?
  29. Morphology of magnetic holes: Methodology and case studies
  30. Magnetosheath Jet‐Triggered ULF Waves: Energy Deposition in the Ionosphere
  31. Magnetosheath Restructuring by Shock-Discontinuity Interaction
  32. Revealing an unexpectedly low electron injection threshold via reinforced shock acceleration
  33. Understanding stormtime geospace as a complex, coupled system: Recent progress from the Center for Geospace Storms
  34. Morphology of magnetic holes: Methodology and case studies
  35. Multimission Observations of Relativistic Electrons and High-speed Jets Linked to Shock-generated Transients
  36. Evaluating the magnetic and plasma flux transport in the plasma sheet during geomagnetic storms using MMS
  37. Heliophysics Applications on Education and Research using Cloud Computing
  38. Hot Flow Anomalies Delimiting Traveling Foreshocks
  39. Magnetosheath jets at jupiter and across the solar system
  40. Solar Wind Structures Impacting the Plasma Stability and Ion Energy Distribution Downstream of the Terrestrial Bow Shock
  41. How do relativistic electrons form at shocks?
  42. Revealing an Unexpectedly Low Electron Injection Threshold via Reinforced Shock Acceleration
  43. Automated Classification of MESSENGER Plasma Observations via Unsupervised Transfer Learning
  44. On the Formation of Super-Alfvénic Flows Downstream of Collisionless Shocks
  45. Plasma Sheet Magnetic Flux Transport During Geomagnetic Storms
  46. Classifying 8 Years of MMS Dayside Plasma Regions via Unsupervised Machine Learning
  47. Temporal Evolution of O+ Population in the Near‐Earth Plasma Sheet During Geomagnetic Storms as Observed by the Magnetospheric Multiscale Mission
  48. The Effect of Fast Solar Wind on Ion Distribution Downstream of Earth’s Bow Shock
  49. Electron Acceleration at Earth's Bow Shock Due to Stochastic Shock Drift Acceleration
  50. Magnetosheath jets at Jupiter and across the solar system
  51. Velocity of magnetic holes in the solar wind from Cluster multipoint measurements
  52. MMS Observation of Two‐Step Electron Acceleration at Earth's Bow Shock
  53. Electron acceleration mechanisms at Earth’s quasi-perpendicular bow shock
  54. Morphology case study of magnetic holes in the pristine solar wind
  55. Velocity distribution functions and non‐Maxwellianity of magnetosheath jets using MMS
  56. Velocity of magnetic holes in the solar wind from cluster multipoint measurements
  57. Solar wind magnetic holes can cross the bow shock and enter the magnetosheath
  58. Dynamics of Earth's bow shock under near-radial interplanetary magnetic field conditions
  59. On Magnetosheath Jet Kinetic Structure and Plasma Properties
  60. Solar wind magnetic holes can cross the bow shock and enter the magnetosheath
  61. Solar wind magnetic holes can cross the bow shock and enter the magnetosheath
  62. Electron Kinetic Entropy across Quasi-Perpendicular Shocks
  63. Morphology of magnetic holes in the pristine solar wind
  64. Electron Kinetic Entropy Generation at Quasi-perpendicular Collisionless Shocks: Dependence on Shock Parameters
  65. High-speed Magnetosheath Jet Generation due to Shock Reformation
  66. On the Generation of Pi2 Pulsations due to Plasma Flow Patterns Around Magnetosheath Jets
  67. Causes of jets in the quasi-perpendicular magnetosheath
  68. Author Correction: Downstream high-speed plasma jet generation as a direct consequence of shock reformation
  69. How solar wind particles slip through Earth's magnetic field
  70. Electron kinetic entropy across quasi-perpendicular 1 shocks
  71. Downstream Super-magnetosonic Plasma Jet Generation as a Direct Consequence of Shock Reformation
  72. Classifying the Magnetosheath Behind the Quasi‐Parallel and Quasi‐Perpendicular Bow Shock by Local Measurements
  73. Solar wind magnetic holes can cross the bow shock and enter the magnetosheath
  74. On the Generation of Pi2 Pulsations due to Plasma Flow Patterns Around Magnetosheath Jets
  75. Causes of Jets in the Quasi‐Perpendicular Magnetosheath
  76. On the generation of Pi2 pulsations due to plasma flow patterns around magnetosheath jets
  77. Magnetosheath jet evolution as a function of lifetime: global hybrid-Vlasov simulations compared to MMS observations
  78. Fast Plasma Flows Downstream of the Bow Shock Using MMS: Correlations and Generation Mechanisms
  79. Magnetosheath jet evolution as a function of lifetime: Global hybrid-Vlasov simulations compared to MMS observations
  80. Solar Energetic Particle Event occurrence prediction using Solar Flare Soft X-ray measurements and Machine Learning
  81. Classifying Magnetosheath Jets Using MMS: Statistical Properties
  82. Helium in the Earth's foreshock: a global Vlasiator survey
  83. Classifying Magnetosheath Jets using MMS - Statistical Properties
  84. Magnetosheath jet evolution as a function of lifetime: Global hybrid-Vlasov simulations compared to MMS observations
  85. Supplementary material to "Magnetosheath jet evolution as a function of lifetime: Global hybrid-Vlasov simulations compared to MMS observations"
  86. Classification of Magnetosheath Jets Using Neural Networks and High Resolution OMNI (HRO) Data
  87. Classifying Magnetosheath Jets using MMS - Statistical Properties
  88. Current sheets and waves inside magnetosheath jets
  89. First Evidence of Flux Transfer Events Caused by Mangetosheath Jets
  90. Current Sheet Statistics in the Magnetosheath
  91. Classifying Magnetosheath Jets using MMS - Statistical Properties