activity
20192025
most citedInterchange reconnection as the source of the fast solar wind within coronal holes

115 citations · 692 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.SR2025★ 1 cited

Multi-spacecraft Measurements of the Evolving Geometry of the Solar Alfvén Surface Over Half a Solar Cycle

Samuel T. Badman, Michael L. Stevens, Stuart D. Bale +18

The geometry of a star's Alfvén surface determines stellar angular momentum loss, separates a causally distinct 'corona' and stellar wind, and potentially affects exoplanetary habi…

physics.space-ph2024

Ion-Scale Solitary Structures in the Solar Wind Observed by Solar Orbiter and Parker Solar Probe

Yufei Yang, Timothy S. Horbury, Domenico Trotta +12

We investigate a class of ion-scale magnetic solitary structures in the solar wind, characterized by distinct magnetic field enhancements and bipolar rotations over spatial scales…

astro-ph.SR2023

Proton and Alpha Driven Instabilities in an Ion Cyclotron Wave Event

Michael D. McManus, Kristopher G. Klein, Davin Larson +8

Ion scale wave events or "wave storms" in the solar wind are characterised by enhancements in magnetic field fluctuations as well as coherent magnetic field polarisation signatures…

astro-ph.SR2023★ 14 cited

Are Switchback boundaries observed by Parker Solar Probe closed?

Nina Bizien, Thierry Dudok de Wit, Clara Froment +7

Switchbacks are sudden and large deflections in the magnetic field that Parker Solar Probe frequently observes in the inner heliosphere. Their ubiquitous occurrence has prompted nu…

physics.space-ph2023★ 12 cited

The Temperature, Electron, and Pressure Characteristics of Switchbacks: Parker Solar Probe Observations

Jia Huang, Justin C. Kasper, Davin E. Larson +19

Parker Solar Probe (PSP) observes unexpectedly prevalent switchbacks, which are rapid magnetic field reversals that last from seconds to hours, in the inner heliosphere, posing new…

astro-ph.SR2023★ 35 cited

New Observations of Solar Wind 1/f Turbulence Spectrum from Parker Solar Probe

Zesen Huang, Nikos Sioulas, Chen Shi +22

The trace magnetic power spectrum in the solar wind is known to be characterized by a double power law at scales much larger than the proton gyro-radius, with flatter spectral expo…

physics.space-ph2023★ 18 cited

Parker Solar Probe Observations of High Plasma Beta Solar Wind from Streamer Belt

Jia Huang, J. C. Kasper, Davin E. Larson +23

In general, slow solar wind from the streamer belt forms a high plasma beta equatorial plasma sheet around the heliospheric current sheet (HCS) crossing, namely the heliospheric pl…

physics.space-ph2023★ 25 cited

The Structure and Origin of Switchbacks: Parker Solar Probe Observations

Jia Huang, J. C. Kasper, L. A. Fisk +25

Switchbacks are rapid magnetic field reversals that last from seconds to hours. Current Parker Solar Probe (PSP) observations pose many open questions in regard to the nature of sw…

physics.space-ph2023★ 25 cited

On the evolution of the Anisotropic Scaling of Magnetohydrodynamic Turbulence in the Inner Heliosphere

Nikos Sioulas, Marco Velli, Zesen Huang +19

We analyze a merged Parker Solar Probe () and Solar Orbiter () dataset covering heliocentric distances to investigate…

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…

astro-ph.SR2022★ 115 cited

Interchange reconnection as the source of the fast solar wind within coronal holes

S. D. Bale, J. F. Drake, M. D. McManus +13

The fast solar wind that fills the heliosphere originates from deep within regions of open magnetic field on the Sun called coronal holes. The energy source responsible for acceler…

astro-ph.SR2022★ 45 cited

The Radial Evolution of the Solar Wind as Organized by Electron Distribution Parameters

J. S. Halekas, P. Whittlesey, D. E. Larson +9

We utilize observations from the Parker Solar Probe (PSP) to study the radial evolution of the solar wind in the inner heliosphere. We analyze electron velocity distribution functi…

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★ 17 cited

Density And Velocity Fluctuations of Alpha Particles in Magnetic Switchbacks

M. D. McManus, J. L. Verniero, S. D. Bale +9

Magnetic switchbacks, or sudden reversals in the magnetic field's radial direction, are one of the more striking observations of Parker Solar Probe (PSP) thus far in its mission. W…

astro-ph.SR2021★ 68 cited

The In Situ Signature of Cyclotron Resonant Heating

Trevor A. Bowen, Benjmin D. G. Chandran, Jonathan Squire +9

The dissipation of magnetized turbulence is an important paradigm for describing heating and energy transfer in astrophysical environments such as the solar corona and wind; howeve…

astro-ph.SR2021★ 22 cited

Suprathermal Ion Energy spectra and Anisotropies near the Heliospheric Current Sheet crossing observed by the Parker Solar Probe during Encounter 7

M. I. Desai, D. G. Mitchell, D. J. McComas +31

We present observations of >10-100 keV/nucleon suprathermal (ST) H, He, O, and Fe ions associated with crossings of the heliospheric current sheet (HCS) at radial distances <0.1 au…

astro-ph.SR2021★ 58 cited

Strong perpendicular velocity-space in proton beams observed by Parker Solar Probe

J. L. Verniero, B. D. G. Chandran, D. E. Larson +16

The SWEAP instrument suite on Parker Solar Probe (PSP) has detected numerous proton beams associated with coherent, circularly polarized, ion-scale waves observed by PSP's FIELDS i…

astro-ph.SR2021★ 41 cited

Direct evidence for magnetic reconnection at the boundaries of magnetic switchbacks with Parker Solar Probe

C. Froment, V. Krasnoselskikh, T. Dudok de Wit +20

Parker Solar Probe's first encounters with the Sun revealed the presence of ubiquitous localised magnetic deflections in the inner heliosphere; these structures, often called switc…

astro-ph.SR2020★ 13 cited

The Contribution of Alpha Particles to the Solar Wind Angular Momentum Flux in the Inner Heliosphere

Adam J. Finley, Michael D. McManus, Sean P. Matt +14

An accurate assessment of the Sun's angular momentum (AM) loss rate is an independent constraint for models that describe the rotation evolution of Sun-like stars. In-situ measurem…

physics.space-ph2020★ 22 cited

Wave-particle energy transfer directly observed in an ion cyclotron wave

Daniel Vech, Mihailo M. Martinovic, Kristopher G. Klein +21

Context. The first studies with Parker Solar Probe (PSP) data have made significant progress toward the understanding of the fundamental properties of ion cyclotron waves in the in…

astro-ph.SR2020★ 59 cited

Sunward propagating whistler waves collocated with localized magnetic field holes in the solar wind: Parker Solar Probe observations at 35.7 Sun radii

O. V. Agapitov, T. Dudok de Wit, F. S. Mozer +21

Observations by the Parker Solar Probe mission of the solar wind at about 35.7 solar radii reveal the existence of whistler wave packets with frequencies below 0.1 f/fce (20-80 Hz…

physics.space-ph2019★ 37 cited

Plasma Waves near the Electron Cyclotron Frequency in the near-Sun Solar Wind

David M. Malaspina, Jasper Halekas, Laura Bercic +17

Data from the first two orbits of the Sun by Parker Solar Probe reveal that the solar wind sunward of 50 solar radii is replete with plasma waves and instabilities. One of the most…