All Stories

  1. Evaluating the magnetic and plasma flux transport in the plasma sheet during geomagnetic storms using MMS
  2. Heliophysics Applications on Education and Research using Cloud Computing
  3. Hot Flow Anomalies Delimiting Traveling Foreshocks
  4. Magnetosheath jets at jupiter and across the solar system
  5. Solar Wind Structures Impacting the Plasma Stability and Ion Energy Distribution Downstream of the Terrestrial Bow Shock
  6. How do relativistic electrons form at shocks?
  7. Revealing an Unexpectedly Low Electron Injection Threshold via Reinforced Shock Acceleration
  8. Automated Classification of MESSENGER Plasma Observations via Unsupervised Transfer Learning
  9. On the Formation of Super-Alfvénic Flows Downstream of Collisionless Shocks
  10. Plasma Sheet Magnetic Flux Transport During Geomagnetic Storms
  11. Classifying 8 Years of MMS Dayside Plasma Regions via Unsupervised Machine Learning
  12. Temporal Evolution of O+ Population in the Near‐Earth Plasma Sheet During Geomagnetic Storms as Observed by the Magnetospheric Multiscale Mission
  13. The Effect of Fast Solar Wind on Ion Distribution Downstream of Earth’s Bow Shock
  14. Electron Acceleration at Earth's Bow Shock Due to Stochastic Shock Drift Acceleration
  15. Magnetosheath jets at Jupiter and across the solar system
  16. Velocity of magnetic holes in the solar wind from Cluster multipoint measurements
  17. MMS Observation of Two‐Step Electron Acceleration at Earth's Bow Shock
  18. Electron acceleration mechanisms at Earth’s quasi-perpendicular bow shock
  19. Morphology case study of magnetic holes in the pristine solar wind
  20. Velocity distribution functions and non‐Maxwellianity of magnetosheath jets using MMS
  21. Velocity of magnetic holes in the solar wind from cluster multipoint measurements
  22. Solar wind magnetic holes can cross the bow shock and enter the magnetosheath
  23. Dynamics of Earth's bow shock under near-radial interplanetary magnetic field conditions
  24. On Magnetosheath Jet Kinetic Structure and Plasma Properties
  25. Solar wind magnetic holes can cross the bow shock and enter the magnetosheath
  26. Solar wind magnetic holes can cross the bow shock and enter the magnetosheath
  27. Electron Kinetic Entropy across Quasi-Perpendicular Shocks
  28. Morphology of magnetic holes in the pristine solar wind
  29. Electron Kinetic Entropy Generation at Quasi-perpendicular Collisionless Shocks: Dependence on Shock Parameters
  30. High-speed Magnetosheath Jet Generation due to Shock Reformation
  31. On the Generation of Pi2 Pulsations due to Plasma Flow Patterns Around Magnetosheath Jets
  32. Causes of jets in the quasi-perpendicular magnetosheath
  33. Author Correction: Downstream high-speed plasma jet generation as a direct consequence of shock reformation
  34. How solar wind particles slip through Earth's magnetic field
  35. Downstream Super-magnetosonic Plasma Jet Generation as a Direct Consequence of Shock Reformation
  36. Classifying the Magnetosheath Behind the Quasi‐Parallel and Quasi‐Perpendicular Bow Shock by Local Measurements
  37. Solar wind magnetic holes can cross the bow shock and enter the magnetosheath
  38. On the Generation of Pi2 Pulsations due to Plasma Flow Patterns Around Magnetosheath Jets
  39. Causes of Jets in the Quasi‐Perpendicular Magnetosheath
  40. On the generation of Pi2 pulsations due to plasma flow patterns around magnetosheath jets
  41. Magnetosheath jet evolution as a function of lifetime: global hybrid-Vlasov simulations compared to MMS observations
  42. Fast Plasma Flows Downstream of the Bow Shock Using MMS: Correlations and Generation Mechanisms
  43. Magnetosheath jet evolution as a function of lifetime: Global hybrid-Vlasov simulations compared to MMS observations
  44. Solar Energetic Particle Event occurrence prediction using Solar Flare Soft X-ray measurements and Machine Learning
  45. Classifying Magnetosheath Jets Using MMS: Statistical Properties
  46. Helium in the Earth's foreshock: a global Vlasiator survey
  47. Classifying Magnetosheath Jets using MMS - Statistical Properties
  48. Magnetosheath jet evolution as a function of lifetime: Global hybrid-Vlasov simulations compared to MMS observations
  49. Supplementary material to "Magnetosheath jet evolution as a function of lifetime: Global hybrid-Vlasov simulations compared to MMS observations"
  50. Classification of Magnetosheath Jets Using Neural Networks and High Resolution OMNI (HRO) Data
  51. Classifying Magnetosheath Jets using MMS - Statistical Properties
  52. Current sheets and waves inside magnetosheath jets
  53. First Evidence of Flux Transfer Events Caused by Mangetosheath Jets
  54. Current Sheet Statistics in the Magnetosheath
  55. Classifying Magnetosheath Jets using MMS - Statistical Properties