All Stories

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