All Stories

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