activity
20192025
most citedParker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum

158 citations · 688 across the 26 of their papers we have counts for

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Showing 2023Show all

11 papers · 1 filter

astro-ph.SR2023

Properties of an interplanetary shock observed at 0.07 and 0.7 Astronomical Units by Parker Solar Probe and Solar Orbiter

D. Trotta, A. Larosa, G. Nicolaou +23

The Parker Solar Probe (PSP) and Solar Orbiter (SolO) missions opened a new observational window in the inner heliosphere, which is finally accessible to direct measurements. On Se…

physics.space-ph2023

Coherent deflection pattern and associated temperature enhancements in the near-Sun solar wind

R. Laker, T. S. Horbury, L. D. Woodham +2

Measurements of transverse magnetic field and velocity components from Parker Solar Probe have revealed a coherent quasi-periodic pattern in the near-Sun solar wind. As well as bei…

physics.space-ph2023

Estimates of Proton and Electron Heating Rates Extended to the Near-Sun Environment

R. Bandyopadhyay, C. M. Meyer, W. H. Matthaeus +11

A central problem of space plasma physics is how protons and electrons are heated in a turbulent, magnetized plasma. The differential heating of charged species due to dissipation…

astro-ph.SR2023

Development of a structured, turbulent solar wind as a result of interchange reconnection

J. F. Drake, S. D. Bale, M. Swisdak +2

The role of interchange reconnection as a drive mechanism for the solar wind is explored by solving the global magnetic-field-aligned equations describing wind acceleration. Bounda…

astro-ph.SR2023★ 32 cited

Quantifying the Energy Budget in the Solar Wind from 13.3-100 Solar Radii

J. S. Halekas, S. D. Bale, M. Berthomier +10

A variety of energy sources, ranging from dynamic processes like magnetic reconnection and waves to quasi-steady terms like the plasma pressure, may contribute to the acceleration…

astro-ph.SR2023★ 26 cited

The Evolution of the 1/f Range Within a Single Fast-Solar-Wind Stream Between 17.4 and 45.7 Solar Radii

Nooshin Davis, B. D. G. Chandran, T. A. Bowen +7

The power spectrum of magnetic-field fluctuations in the fast solar wind ($V_{\rm SW}> 500 \mbox{ km} \mbox{ s}^{-1}$) at magnetohydrodynamic (MHD) scales is characterized by two d…