Simulations show high-speed solar wind streams evolve via interactions and 3D flows, making them non-parcel-preserving and location-dependent in their observed properties.
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Stellar winds from young weak-lined T Tauri stars compress exoplanet magnetospheres to sizes significantly smaller than Earth's, with sizes increasing as stellar activity decays with age.
citing papers explorer
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MHD simulations on the large-scale propagation of high-speed solar wind streams
Simulations show high-speed solar wind streams evolve via interactions and 3D flows, making them non-parcel-preserving and location-dependent in their observed properties.
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Interaction between Winds from Weak-lined T Tauri Stars with Exoplanetary Magnetospheres
Stellar winds from young weak-lined T Tauri stars compress exoplanet magnetospheres to sizes significantly smaller than Earth's, with sizes increasing as stellar activity decays with age.