Parker Solar Probe Enters the Magnetically Dominated Solar Corona
The high temperatures and strong magnetic fields of the solar corona form streams of solar
wind that expand through the Solar System into interstellar space. At 09: 33 UT on 28 April …
wind that expand through the Solar System into interstellar space. At 09: 33 UT on 28 April …
The transport and evolution of MHD turbulence throughout the heliosphere: models and observations
A detailed study of solar wind turbulence throughout the heliosphere in both the upwind and
downwind directions is presented. We use an incompressible magnetohydrodynamic (MHD) …
downwind directions is presented. We use an incompressible magnetohydrodynamic (MHD) …
[HTML][HTML] The solar orbiter mission-science overview
D Müller, OCS Cyr, I Zouganelis, HR Gilbert… - Astronomy & …, 2020 - aanda.org
Aims. Solar Orbiter, the first mission of ESA's Cosmic Vision 2015–2025 programme and a
mission of international collaboration between ESA and NASA, will explore the Sun and …
mission of international collaboration between ESA and NASA, will explore the Sun and …
Solar radio emissions and ultralight dark matter
Ultralight axions and dark photons are well-motivated dark matter candidates. Inside the
plasma, once the mass of ultralight dark matter candidates equals the plasma frequency …
plasma, once the mass of ultralight dark matter candidates equals the plasma frequency …
Near-Sun In Situ and Remote-sensing Observations of a Coronal Mass Ejection and its Effect on the Heliospheric Current Sheet
During the thirteenth encounter of the Parker Solar Probe (PSP) mission, the spacecraft
traveled through a topologically complex interplanetary coronal mass ejection (ICME) …
traveled through a topologically complex interplanetary coronal mass ejection (ICME) …
Sub-alfvénic solar wind observed by the parker solar probe: Characterization of turbulence, anisotropy, intermittency, and switchback
In the lower solar coronal regions where the magnetic field is dominant, the Alfvén speed is
much higher than the wind speed. In contrast, the near-Earth solar wind is strongly super …
much higher than the wind speed. In contrast, the near-Earth solar wind is strongly super …
Prediction and Verification of Parker Solar Probe Solar Wind Sources at 13.3 R⊙
Drawing connections between heliospheric spacecraft and solar wind sources is a vital step
in understanding the evolution of the solar corona into the solar wind and contextualizing in …
in understanding the evolution of the solar corona into the solar wind and contextualizing in …
Occurrence and evolution of switchbacks in the inner heliosphere: Parker solar probe observations
Since its launch in 2018, the Parker Solar Probe (PSP) mission revealed the presence of
numerous fascinating phenomena occurring closer to the Sun, such as the presence of …
numerous fascinating phenomena occurring closer to the Sun, such as the presence of …
On the generation and evolution of switchbacks and the morphology of the Alfvénic transition: low Mach-number boundary layers
We investigate the generation and evolution of switchbacks (SBs), the nature of the sub-
Alfvénic wind observed by the Parker Solar Probe (PSP), and the morphology of the Alfvénic …
Alfvénic wind observed by the Parker Solar Probe (PSP), and the morphology of the Alfvénic …
Switchbacks: Statistical properties and deviations from Alfvénicity
Context. Parker Solar Probe's first solar encounter has revealed the presence of sudden
magnetic field deflections in the slow Alfvénic solar wind. These structures, which are often …
magnetic field deflections in the slow Alfvénic solar wind. These structures, which are often …