[HTML][HTML] HUXt—An open source, computationally efficient reduced-physics solar wind model, written in Python
HUXt is an open source numerical model of the solar wind written in Python. It is based on
the solution of the 1D inviscid Burger's equation. This reduced-physics approach produces …
the solution of the 1D inviscid Burger's equation. This reduced-physics approach produces …
A statistical evaluation of ballistic backmapping for the slow solar wind: The interplay of solar wind acceleration and corotation
Mapping solar wind plasma back to its source is often achieved using the 'two-step ballistic
backmapping'method. Solar wind observations are mapped through the heliosphere to the …
backmapping'method. Solar wind observations are mapped through the heliosphere to the …
The evolution of inverted magnetic fields through the inner heliosphere
Local inversions are often observed in the heliospheric magnetic field (HMF), but their
origins and evolution are not yet fully understood. Parker Solar Probe has recently observed …
origins and evolution are not yet fully understood. Parker Solar Probe has recently observed …
Constraints on solar wind density and velocity based on coronal tomography and parker solar probe measurements
Previous work has established an empirical relationship between densities gained from
coronal rotational tomography near the ecliptic plane with solar wind outflow speeds at …
coronal rotational tomography near the ecliptic plane with solar wind outflow speeds at …
The impact of sudden commencements on ground magnetic field variability: Immediate and delayed consequences
Abstract We examine how Sudden Commencements (SCs) and Storm Sudden
Commencements (SSCs) influence the occurrence of high rates of change of the magnetic …
Commencements (SSCs) influence the occurrence of high rates of change of the magnetic …
Predicting solar wind streams from the inner-heliosphere to Earth via shifted operator inference
Solar wind conditions are predominantly predicted via three-dimensional numerical
magnetohydrodynamic (MHD) models. Despite their ability to produce highly accurate …
magnetohydrodynamic (MHD) models. Despite their ability to produce highly accurate …
[HTML][HTML] Unifying the validation of ambient solar wind models
MA Reiss, K Muglach, R Mullinix… - Advances in Space …, 2023 - Elsevier
Progress in space weather research and awareness needs community-wide strategies and
procedures to evaluate our modeling assets. Here we present the activities of the Ambient …
procedures to evaluate our modeling assets. Here we present the activities of the Ambient …
Drag‐based CME modeling with heliospheric images incorporating frontal deformation: ELEvoHI 2.0
J Hinterreiter, T Amerstorfer, M Temmer… - Space …, 2021 - Wiley Online Library
The evolution and propagation of coronal mass ejections (CMEs) in interplanetary space is
still not well understood. As a consequence, accurate arrival time and arrival speed …
still not well understood. As a consequence, accurate arrival time and arrival speed …
Improving solar wind forecasting using data assimilation
Data Assimilation (DA) has enabled huge improvements in the skill of terrestrial operational
weather forecasting. In this study, we use a variational DA scheme with a computationally …
weather forecasting. In this study, we use a variational DA scheme with a computationally …
Effect of a magnetospheric compression on Jovian radio emissions: In situ case study using Juno data
CK Louis, CM Jackman, G Hospodarsky… - Journal of …, 2023 - Wiley Online Library
During its polar orbits around Jupiter, Juno often crosses the boundaries of the Jovian
magnetosphere (namely the magnetopause and bow shock). From the boundary locations …
magnetosphere (namely the magnetopause and bow shock). From the boundary locations …