A generalized method for estimating solar wind speeds and densities using spectral broadening for a Kolmogorov turbulence spectrum

Documenti analoghi

• On the estimation of solar wind velocity under varying solar activity conditions using Akatsuki measurements
  di: Aggarwal, Keshav, et al.
  Pubblicazione: (2025)
• A turbulence index independent framework for deriving solar wind speed and coronal electron density from radio spectral broadening
  di: Aggarwal, Keshav, et al.
  Pubblicazione: (2026)
• A robust empirical relationship between speed and turbulence energy in the near-Earth solar wind
  di: Chhiber, Rohit, et al.
  Pubblicazione: (2025)
• Evolution of MHD turbulence in the expanding solar wind: residual energy and intermittency
  di: Shi, Chen, et al.
  Pubblicazione: (2023)
• Insights into Solar Wind Flow Speeds from the Coronal Radio occultation Experiment: Findings from the Indian Mars Orbiter Mission
  di: Aggarwal, Keshav, et al.
  Pubblicazione: (2025)