Dependence of the Solar Wind Plasma Density on Moderate- and Extremely High-Geomagnetic Activity Elucidated by Potential Learning

Documenti analoghi

• The Quasi-Radial Field-line Tracing (QRaFT): an Adaptive Segmentation of the Open-Flux Solar Corona
  di: Uritsky, Vadim M., et al.
  Pubblicazione: (2025)
• A Point-cloud Clustering & Tracking Algorithm for Radar Interferometry
  di: Ivarsen, Magnus F, et al.
  Pubblicazione: (2024)
• Multi-Point Gradient Estimation in Turbulence
  di: Broeren, Theodore, et al.
  Pubblicazione: (2024)
• Medium-scale thermospheric gravity waves in the high-resolution Whole Atmosphere Model: Seasonal, local time, and longitudinal variations
  di: Malhotra, Garima, et al.
  Pubblicazione: (2024)
• Reconstruction of Polarization Properties of Whistler Waves From Two Magnetic and Two Electric Field Components: Application to Parker Solar Probe Measurements
  di: Colomban, L., et al.
  Pubblicazione: (2024)