The Dual Nature of Solar Wind Structuring: Resonant Standing Waves and Laval Nozzle Dynamics in Coronal Streamers
Olena Podladchikova
TL;DR
This paper resolves the puzzle of periodic density structures in the solar wind by proposing a dual-mechanism framework for coronal streamers. It combines a magnetohydrodynamic resonator model, where standing slow waves establish global PDS with discrete periods $P_n^{\text{res}} = \frac{2L}{n c_s}$, and a Laval nozzle model, where overexpanded geometry drives local oscillations with periods $P_n^{\text{nozzle}} = \frac{L_{\text{over}}}{v_{\text{SW}}} \cdot k_n$. The work shows that resonant dynamics dominate PDS formation across ~85% of streamers, while nozzle oscillations operate in ~35% to generate shock diamonds and vortices, producing a coherent, hierarchical view of solar wind structuring with implications for astrophysical plasma flows. Overall, the dual-mechanism framework resolves longstanding questions about PDS coherence, persistence to 1 AU with minimal energy loss, and the interplay between global and local flow processes in coronal streamers.
Abstract
Periodic Density Structures (PDS) observed in white-light coronagraphs represent a fundamental challenge to conventional solar wind paradigms. Through systematic analysis of multi-instrument observations and theoretical modeling, we demonstrate that coronal streamers operate as dual-nature systems: magnetohydrodynamic resonators that establish global periodicity through standing waves (122, 61, 41 minutes) and Laval nozzles that generate local flow structures through shock-driven oscillations (93, 47, 31, 23 minutes). The resonant mechanism dominates PDS formation, explaining their universal occurrence across 85\% of streamers, coherence over 10+ cycles, and persistence to 1 AU with only 0.1\% energy loss. Nozzle oscillations, while limited to 35\% of overexpanded streamers and maintaining only 1-2 cycle coherence, play crucial secondary roles in vortex formation and provide the essential converging-diverging geometry for supersonic solar wind acceleration. This dual-mechanism framework resolves longstanding puzzles in solar wind structuring while revealing the hierarchical organization of standing-wave and flow processes in astrophysical plasmas.
