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 …
Coronal heating by MHD waves
The heating of the solar chromosphere and corona to the observed high temperatures, imply
the presence of ongoing heating that balances the strong radiative and thermal conduction …
the presence of ongoing heating that balances the strong radiative and thermal conduction …
In-situ switchback formation in the expanding solar wind
J Squire, BDG Chandran… - The Astrophysical Journal …, 2020 - iopscience.iop.org
Recent near-Sun solar-wind observations from Parker Solar Probe have found a highly
dynamic magnetic environment, permeated by abrupt radial-field reversals, or" switchbacks." …
dynamic magnetic environment, permeated by abrupt radial-field reversals, or" switchbacks." …
The evolution and role of solar wind turbulence in the inner heliosphere
The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere - IOPscience This
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site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …
Turbulence in the sub-Alfvénic solar wind
Abstract The Parker Solar Probe (PSP) entered a region of sub-Alfvénic solar wind during
encounter 8, and we present the first detailed analysis of low-frequency turbulence …
encounter 8, and we present the first detailed analysis of low-frequency turbulence …
Turbulent generation of magnetic switchbacks in the Alfvénic solar wind
M Shoda, BDG Chandran… - The Astrophysical …, 2021 - iopscience.iop.org
One of the most important early results from the Parker Solar Probe (PSP) is the ubiquitous
presence of magnetic switchbacks, whose origin is under debate. Using a three-dimensional …
presence of magnetic switchbacks, whose origin is under debate. Using a three-dimensional …
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; …
MHD turbulence: a biased review
AA Schekochihin - Journal of Plasma Physics, 2022 - cambridge.org
This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …
developments of the last few years in the context of the canonical time line (from Kolmogorov …
Magnetohydrodynamic waves in open coronal structures
D Banerjee, S Krishna Prasad, V Pant… - Space Science …, 2021 - Springer
Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …
Cross helicity reversals in magnetic switchbacks
We consider 2D joint distributions of normalized residual energy, σ r (s, t), and cross helicity,
σ c (s, t), during one day of Parker Solar Probe's (PSP's) first encounter as a function of …
σ c (s, t), during one day of Parker Solar Probe's (PSP's) first encounter as a function of …