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 …
Scaling laws for the energy transfer in space plasma turbulence
R Marino, L Sorriso-Valvo - Physics Reports, 2023 - Elsevier
One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …
A solar source of Alfvénic magnetic field switchbacks: in situ remnants of magnetic funnels on supergranulation scales
A Solar Source of Alfvénic Magnetic Field Switchbacks: In Situ Remnants of Magnetic Funnels
on Supergranulation Scales - IOPscience This site uses cookies. By continuing to use this site …
on Supergranulation Scales - IOPscience This site uses cookies. By continuing to use this site …
[HTML][HTML] Turbulence-driven magnetic reconnection and the magnetic correlation length: Observations from Magnetospheric Multiscale in Earth's magnetosheath
Turbulent plasmas generate a multitude of thin current structures that can be sites for
magnetic reconnection. The Magnetospheric Multiscale (MMS) mission has recently …
magnetic reconnection. The Magnetospheric Multiscale (MMS) mission has recently …
Isotropization and evolution of energy-containing eddies in solar wind turbulence: Parker solar probe, helios 1, ace, wind, and voyager 1
We examine the radial evolution of correlation lengths perpendicular (${\lambda} _
{C}^{\perp} $) and parallel (${\lambda} _ {C}^{\parallel} $) to the magnetic-field direction …
{C}^{\perp} $) and parallel (${\lambda} _ {C}^{\parallel} $) to the magnetic-field direction …
Mesoscale structure in the solar wind
NM Viall, CE DeForest, L Kepko - Frontiers in Astronomy and Space …, 2021 - frontiersin.org
Structures in the solar wind result from two basic mechanisms: structures injected or
imposed directly by the Sun, and structures formed through processing en route as the solar …
imposed directly by the Sun, and structures formed through processing en route as the solar …
Turbulence Properties of Interplanetary Coronal Mass Ejections in the Inner Heliosphere: Dependence on Proton Beta and Flux Rope Structure
SW Good, OK Rantala, ASM Jylhä… - The Astrophysical …, 2023 - iopscience.iop.org
Interplanetary coronal mass ejections (ICMEs) have low proton beta across a broad range of
heliocentric distances and a magnetic flux rope structure at large scales, making them a …
heliocentric distances and a magnetic flux rope structure at large scales, making them a …
Magnetic field intermittency in the solar wind: Parker solar probe and SolO observations ranging from the alfvén region up to 1 AU
Abstract Parker Solar Probe (PSP) and SolO data are utilized to investigate magnetic field
intermittency in the solar wind (SW). Small-scale intermittency (20− 100 di) is observed to …
intermittency in the solar wind (SW). Small-scale intermittency (20− 100 di) is observed to …
Exploring the solar wind from its source on the corona into the inner heliosphere during the first Solar Orbiter–Parker Solar Probe quadrature
D Telloni, V Andretta, E Antonucci… - The Astrophysical …, 2021 - iopscience.iop.org
This Letter addresses the first Solar Orbiter (SO)–Parker Solar Probe (PSP) quadrature,
occurring on 2021 January 18 to investigate the evolution of solar wind from the extended …
occurring on 2021 January 18 to investigate the evolution of solar wind from the extended …
Intermittency in the expanding solar wind: Observations from parker solar probe (0.16 au), helios 1 (0.3–1 au), and voyager 1 (1–10 au)
We examine statistics of magnetic-field vector components to explore how intermittency
evolves from near-Sun plasma to radial distances as large as 10 au. Statistics entering the …
evolves from near-Sun plasma to radial distances as large as 10 au. Statistics entering the …