Ensemble Forecasts of Solar Wind Connectivity to 1 Rs Using ADAPT‐WSA
Abstract The solar wind which arrives at any location in the solar system is, in principle, relatable to the outflow of solar plasma from a single source location. This source location, itself usually being part of a larger coronal hole, is traceable to 1 RS along the Sun's magnetic field, in w...
Saved in:
Main Authors: | D. E. daSilva, S. Wallace, C. N. Arge, S. Jones |
---|---|
Format: | Article |
Language: | English |
Published: |
Wiley
2023-10-01
|
Series: | Space Weather |
Subjects: | |
Online Access: | https://doi.org/10.1029/2023SW003554 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
A Parametric Study of Performance of Two Solar Wind Velocity Forecasting Models During 2006–2011
by: Sandeep Kumar, et al.
Published: (2022-09-01) -
Radial Evolution of MHD Turbulence Anisotropy in Low Mach Number Solar Wind
by: Xingyu Zhu, et al.
Published: (2025-01-01) -
An Empirical Relationship Between Coronal Density and Solar Wind Velocity in the Middle Corona With Applications to Space Weather
by: Kaine A. Bunting, et al.
Published: (2023-03-01) -
Data Assimilative Optimization of WSA Source Surface and Interface Radii using Particle Filtering
by: Grant David Meadors, et al.
Published: (2020-05-01) -
Adapting Ensemble‐Calibration Techniques to Probabilistic Solar‐Wind Forecasting
by: N. O. Edward‐Inatimi, et al.
Published: (2024-12-01)