activity
20152026
most citedThe Solar Probe Cup on Parker Solar Probe

218 citations · 817 across the 21 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

12 papers · 1 filter

astro-ph.SR2026

Strong Prevalence of Hammerhead Velocity Distributions Close to the Heliospheric Current Sheet

Srijan Bharati Das, Jaye L. Verniero, Samuel T. Badman +13

The solar wind undergoes non-adiabatic heating as it travels away from the Sun. The velocity phase space distribution of non-equilibrium ions in the solar wind indicate a source of…

astro-ph.SR2026

Solar Wind Heating Near the Sun: A Radial Evolution Approach

Yogesh, Leon Ofman, Kristopher Klein +19

Characterizing the plasma state in the near-Sun environment is essential to constrain the mechanisms that heat and accelerate the solar wind. In this study, we use Parker Solar Pro…

astro-ph.SR2026

Conversion Layer Controls the Evolution of Magnetic Deflections Near the Alfven Surface

Dominic Payne, Mojtaba Akhavan-Tafti, Joshua Goodwill +10

We examine the statistics of Alfvenic deflections in both sub-Alfvenic and super-Alfvenic solar wind with particular focus on a common parameter that underlies the definition of sw…

astro-ph.SR2025

Tracing a Multi-Temperature Quiescent Prominence's Thermodynamic Evolution from Sun to Earth

Callie A. García, Yeimy J. Rivera, Samuel T. Badman +5

Solar prominences are cool, dense stable structures routinely observed in the corona. Prominences are often ejected from the Sun via coronal mass ejections (CMEs). However, they ar…

astro-ph.SR2025

Evidence of Interaction between Ion-Scale Waves and Ion Velocity Distributions in the Solar Wind

Yogesh, Leon Ofman, Scott A Boardsen +9

Recent in situ observations from Parker Solar Probe (PSP) near perihelia reveal ion beams, temperature anisotropies, and kinetic wave activity. These features are likely linked to…

astro-ph.SR2025★ 4 cited

Helium Abundance Periods Observed by the Solar Probe Cup on Parker Solar Probe: Encounters 1-14

Madisen Johnson, Yeimy J. Rivera, Tatiana Niembro +7

Parker Solar Probe is a mission designed to explore properties of the solar wind closer than ever before. Detailed particle observations from the Solar Probe Cup (SPC) have primari…

astro-ph.SR2024

Mixed Source Region Signatures Inside Magnetic Switchback Patches Inferred by Heavy Ion Diagnostics

Yeimy J. Rivera, Samuel T. Badman, Michael L. Stevens +13

Since Parker Solar Probe's (Parker's) first perihelion pass at the Sun, large amplitude Alfvén waves grouped in patches have been observed near the Sun throughout the mission. Seve…

astro-ph.SR2024★ 77 cited

In situ observations of large amplitude Alfvén waves heating and accelerating the solar wind

Yeimy J. Rivera, Samuel T. Badman, Michael L. Stevens +16

After leaving the Sun's corona, the solar wind continues to accelerate and cools, but more slowly than expected for a freely expanding adiabatic gas. We use in situ measurements fr…

astro-ph.SR2024★ 11 cited

Near subsonic solar wind outflow from an active region

Tamar Ervin, Stuart D. Bale, Samuel T. Badman +10

During Parker Solar Probe (Parker) Encounter 15 (E15), we observe an 18-hour period of near subsonic ( 1) and sub-Alfvénic (SA), <<< 1, slow speed…

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…

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.SR2020★ 111 cited

Parker Solar Probe In-Situ Observations of Magnetic Reconnection Exhausts During Encounter 1

T. D. Phan, S. D. Bale, J. P. Eastwood +23

Magnetic reconnection in current sheets converts magnetic energy into particle energy. The process may play an important role in the acceleration and heating of the solar wind clos…