Origins of the ambient solar wind: implications for space weather
SR Cranmer, SE Gibson, P Riley - Space Science Reviews, 2017 - Springer
The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …
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 …
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
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …
site uses cookies. By continuing to use this site you agree to our use of cookies. To find out …
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 …
The role of Alfvén wave dynamics on the large-scale properties of the solar wind: comparing an MHD simulation with Parker solar probe E1 data
Abstract During Parker Solar Probe's first orbit, the solar wind plasma was observed in situ
closer than ever before, the perihelion on 2018 November 6 revealing a flow that is …
closer than ever before, the perihelion on 2018 November 6 revealing a flow that is …
Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal heating
B De Pontieu, P Testa, J Martínez-Sykora… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The Multi-slit Solar Explorer (MUSE) is a proposed mission composed of a multislit
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
Reflection-driven magnetohydrodynamic turbulence in the solar atmosphere and solar wind
BDG Chandran, JC Perez - Journal of Plasma Physics, 2019 - cambridge.org
We present three-dimensional direct numerical simulations and an analytic model of
reflection-driven magnetohydrodynamic (MHD) turbulence in the solar wind. Our simulations …
reflection-driven magnetohydrodynamic (MHD) turbulence in the solar wind. Our simulations …
Evolution of large-amplitude Alfvén waves and generation of switchbacks in the expanding solar wind
Abstract Motivated by recent Parker Solar Probe (PSP) observations of" switchbacks"(abrupt,
large-amplitude reversals in the radial magnetic field, which exhibit Alfvénic correlations) …
large-amplitude reversals in the radial magnetic field, which exhibit Alfvénic correlations) …
A self-consistent model of the coronal heating and solar wind acceleration including compressible and incompressible heating processes
We propose a novel one-dimensional model that includes both shock and turbulence
heating and qualify how these processes contribute to heating the corona and driving the …
heating and qualify how these processes contribute to heating the corona and driving the …
Parametric instability, inverse cascade and the range of solar-wind turbulence
BDG Chandran - Journal of plasma physics, 2018 - cambridge.org
Parametric instability, inverse cascade and the 1/f range of solar-wind turbulence Page 1 J. Plasma
Phys. (2018), vol. 84, 905840106 c Cambridge University Press 2018 This is an Open Access …
Phys. (2018), vol. 84, 905840106 c Cambridge University Press 2018 This is an Open Access …