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20102024
most citedThe Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere

270 citations · 3.9k across the 80 of their papers we have counts for

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Showing 2022Show all

7 papers · 1 filter

physics.space-ph2022★ 60 cited

Space Plasma Physics: A Review

Bruce T. Tsurutani, Gary P. Zank, Veerle J. Sterken +13

Owing to the ever-present solar wind, our vast solar system is full of plasmas. The turbulent solar wind, together with sporadic solar eruptions, introduces various space plasma pr…

astro-ph.SR2022★ 31 cited

Magnetic field spectral evolution in the inner heliosphere

Nikos Sioulas, Zesen Huang, Chen Shi +23

Parker Solar Probe and Solar Orbiter data are used to investigate the radial evolution of magnetic turbulence between au. The spectrum is studied as…

physics.space-ph2022★ 1 cited

Correlation between bandwidth and frequency of plasmaspheric hiss uncovered with unsupervised machine learning

Daniel Vech, David M. Malaspina, Alexander Drozdov +1

Previous statistical studies of plasmaspheric hiss investigated the averaged shape of the magnetic field power spectra at various points in the magnetosphere. However, this approac…

astro-ph.SR2022★ 34 cited

Patches of magnetic switchbacks and their origins

Chen Shi, Olga Panasenco, Marco Velli +18

Parker Solar Probe (PSP) has shown that the solar wind in the inner heliosphere is characterized by the quasi omni-presence of magnetic switchbacks ("switchback" hereinafter), loca…

astro-ph.SR2022★ 9 cited

Parker Solar Probe observations of near- harmonics emissions in the near-Sun solar wind and their dependence on the magnetic field direction

Sabrina F. Tigik, Andris Vaivads, David M. Malaspina +1

Wave emissions at frequencies near electron gyrofrequency harmonics are observed at small heliocentric distances below about 40 solar radii and are known to occur in regions with q…

physics.space-ph2022★ 67 cited

Sub-Alfvenic Solar Wind observed by PSP: Characterization of Turbulence, Anisotropy, Intermittency, and Switchback

R. Bandyopadhyay, W. H. Matthaeus, D. J. McComas +18

In the lower solar coronal regions where the magnetic field is dominant, the Alfven speed is much higher than the wind speed. In contrast, the near-Earth solar wind is strongly sup…