activity
20182026
most citedOn the transmission of turbulent structures across the Earth's Bow Shock

35 citations · 188 across the 35 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

15 papers · 1 filter

astro-ph.SR2026

Averaging Effects on the Solar Wind Alfven Mach Number: Implications for Switchbacks and Alfven Transition

Joshua Goodwill, Subash Adhikari, Francesco Pecora +10

Averaging techniques in solar wind measurements have been a longstanding subject of debate. Using Parker Solar Probe (PSP) observations from encounters 1 to 19, we investigate how…

astro-ph.SR2025

Characterization of the Trans-Alfvénic Region Using Observations from Parker Solar Probe

Subash Adhikari, Riddhi Bandyopadhyay, Joshua Goodwill +14

Close to Earth the solar wind is usually super-Alfvénic, i.e. the speed of the solar wind is much larger than the Alfvén speed. However, in the lower coronal regions, the solar win…

astro-ph.SR2025★ 9 cited

Polarimeter to Unify the Corona and Heliosphere (PUNCH)

Craig E. DeForest, Sarah E. Gibson, Ronnie Killough +74

The Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a NASA Small Explorer to determine the cross-scale processes that unify the solar corona and heliosphere. PUN…

astro-ph.SR2025★ 3 cited

Interplanetary magnetic correlation and low-frequency spectrum over many solar rotations

Jiaming Wang, Francesco Pecora, Rohit Chhiber +2

Fluctuations and structure across a wide range of spatial and temporal scales are frequently studied in the solar wind. The properties of the low-frequency fluctuations are of rele…

astro-ph.SR2025★ 4 cited

The effect of turbulence on the angular momentum of the solar wind

Rohit Chhiber, Arcadi Usmanov, William H. Matthaeus +1

The transfer of a star's angular momentum to its atmosphere is a topic of considerable and wide-ranging interest in astrophysics. This letter considers the effect of kinetic and ma…

astro-ph.SR2024★ 7 cited

Observed Fluctuation Enhancement and Departure from WKB Theory in Sub-Alfvénic Solar Wind

David Ruffolo, Panisara Thepthong, Peera Pongkitiwanichakul +12

Using Parker Solar Probe data from orbits 8 through 17, we examine fluctuation amplitudes throughout the critical region where the solar wind flow speed approaches and then exceeds…

astro-ph.SR2024

Noise in the Heliosphere: A Target for PUNCH Science

Jiaming Wang, William H. Matthaeus, Rohit Chhiber +4

We present a broad review of 1/f noise observations in the heliosphere, and discuss and complement the theoretical background of generic 1/f models as relevant to NASA's PUNCH miss…

astro-ph.SR2024★ 1 cited

Parker Solar Probe Observations of Energetic Particles in the Flank of a Coronal Mass Ejection Close to the Sun

N. A. Schwadron, Stuart D. Bale, J. Bonnell +32

We present an event observed by Parker Solar Probe at 0.2 au on March 2, 2022 in which imaging and \emph{in situ} measurements coincide. During this event, PSP passed through…

astro-ph.SR2024

The Alfvén Transition Zone observed by the Parker Solar Probe in Young Solar Wind -- Global Properties and Model Comparisons

Rohit Chhiber, Francesco Pecora, Arcadi V Usmanov +6

The transition from subAlfvénic to superAlfvénic flow in the solar atmosphere is examined by means of Parker Solar Probe (PSP) measurements during solar encounters 8 to 14. Around…

astro-ph.SR2023

The eruption of a magnetic flux rope observed by \textit{Solar Orbiter} and \textit{Parker Solar Probe}

David M. Long, Lucie M. Green, Francesco Pecora +11

Magnetic flux ropes are a key component of coronal mass ejections, forming the core of these eruptive phenomena. However, determining whether a flux rope is present prior to erupti…

astro-ph.SR2023★ 11 cited

Compressible Turbulence in the Near-Sun Solar Wind: Parker Solar Probe's First Eight Perihelia

Manuel Enrique Cuesta, Rohit Chhiber, Xiangrong Fu +10

Many questions remain about the compressibility of solar wind turbulence with respect to its origins and properties. Low plasma beta (ratio of thermal to magnetic pressure) environ…

astro-ph.SR2022

Isotropization and Evolution of Energy-Containing Eddies in Solar Wind Turbulence: Parker Solar Probe, Helios 1, ACE, WIND, and Voyager 1

Manuel Enrique Cuesta, Rohit Chhiber, Sohom Roy +6

We examine the radial evolution of correlation lengths perpendicular (\(λ_C^{\perp}\)) and parallel (\(λ_C^{\parallel}\)) to the magnetic-field direction, computed from solar wind…

astro-ph.SR2022

Magnetic Switchback Occurrence Rates in the Inner Heliosphere: Parker Solar Probe and 1 au

Francesco Pecora, William H. Matthaeus, Leonardo Primavera +4

The subject of switchbacks, defined either as large angular deflections or polarity reversals of the magnetic field, has generated substantial interest in the space physics communi…

astro-ph.SR2021★ 23 cited

Parker Solar Probe Observations of Helical Structures as Boundaries for Energetic Particles

F. Pecora, S. Servidio, A. Greco +15

Energetic particle transport in the interplanetary medium is known to be affected by magnetic structures. It has been demonstrated for solar energetic particles in near-Earth orbit…

astro-ph.SR2021

Current sheets, plasmoids and flux ropes in the heliosphere. Part II: Theoretical aspects

O. Pezzi, F. Pecora, J. le Roux +13

Our understanding of processes occurring in the heliosphere historically began with reduced dimensionality - one-dimensional (1D) and two-dimensional (2D) sketches and models, whic…