Parker solar probe: Four years of discoveries at solar cycle minimum
Abstract Launched on 12 Aug. 2018, NASA's Parker Solar Probe had completed 13 of its
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …
scheduled 24 orbits around the Sun by Nov. 2022. The mission's primary science goal is to …
Turbulence in the outer heliosphere
The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their
interaction is governed by complex physical processes and creates heliospheric regions …
interaction is governed by complex physical processes and creates heliospheric regions …
In Situ Signature of Cyclotron Resonant Heating in the Solar Wind
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; …
and energy transfer in astrophysical environments such as the solar corona and wind; …
On the violation of the zeroth law of turbulence in space plasmas
The zeroth law of turbulence states that, for fixed energy input into large-scale motions, the
statistical steady state of a turbulent system is independent of microphysical dissipation …
statistical steady state of a turbulent system is independent of microphysical dissipation …
Constraining ion-scale heating and spectral energy transfer in observations of plasma turbulence
We perform a statistical study of the turbulent power spectrum at inertial and kinetic scales
observed during the first perihelion encounter of the Parker Solar Probe. We find that often …
observed during the first perihelion encounter of the Parker Solar Probe. We find that often …
Mediation of collisionless turbulent dissipation through cyclotron resonance
The dissipation of turbulence in astrophysical systems is fundamental to energy transfer and
heating in environments ranging from the solar wind and corona to accretion disks and the …
heating in environments ranging from the solar wind and corona to accretion disks and the …
The radial variation of the solar wind turbulence spectra near the kinetic break scale from Parker Solar Probe measurements
In this study we examine the radial dependence of the inertial and dissipation range indices,
as well as the spectral break separating the inertial and dissipation range in power density …
as well as the spectral break separating the inertial and dissipation range in power density …
Strong perpendicular velocity-space diffusion in proton beams observed by parker solar probe
JL Verniero, BDG Chandran, DE Larson… - The Astrophysical …, 2022 - iopscience.iop.org
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 …
beams associated with coherent, circularly polarized, ion-scale waves observed by PSP's …
Inferred linear stability of parker solar Probe observations using one-and two-component proton distributions
The hot and diffuse nature of the Sun's extended atmosphere allows it to persist in non-
equilibrium states for long enough that wave–particle instabilities can arise and modify the …
equilibrium states for long enough that wave–particle instabilities can arise and modify the …
Coherent events at ion scales in the inner heliosphere: Parker solar probe observations during the first encounter
Abstract The Parker Solar Probe mission has shown the ubiquitous presence of strong
magnetic field deflections, namely switchbacks, during its first perihelion where it was …
magnetic field deflections, namely switchbacks, during its first perihelion where it was …