Spherically Polarized Alfv'en Waves and the Gosling Boost

arXiv:2608.05091 · astro-ph.SR, physics.plasm-ph · Submitted 2026-08-05 · Read on arXiv

Yuliang Ding, Marco Velli, Zesen Huang, Chen Shi, Lorenzo Matteini, Nikos Sioulas, Stuart D. Bale, Anna Tenerani, Mingzhe Liu

astro-ph.SR, physics.plasm-ph

Submitted: 2026-08-05

Comments: 12 pages, 6 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Anisotropy — 4× in this paper · explained in 3 episodes
• Alignment — 3× in this paper · explained in 1 episode
• Parker Solar Probe — 3× in this paper
• Trace — 2× in this paper · explained in 2 episodes
• Analyzer — 1× in this paper · explained in 1 episode
• Anti-correlation — 1× in this paper · explained in 3 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• alpha — 1× in this paper · explained in 1 episode

Sources

• Quantifying the Energy Budget in the Solar Wind from 13.3-100 Solar Radii
• Solitary Alfv'en Waves
• Radial Evolution of Near-Sun Magnetic Switchbacks Alfvenicity, Occurrence Rate, and Size

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