-
1
Are Switchback Boundaries Observed by Parker Solar Probe Closed?
Published 2023-01-01“…Switchbacks are sudden and large deflections in the magnetic field that Parker Solar Probe frequently observes in the inner heliosphere. …”
Get full text
Article -
2
The Structure and Origin of Switchbacks: Parker Solar Probe Observations
Published 2023-01-01“…Switchbacks are rapid magnetic field reversals that last from seconds to hours. Current Parker Solar Probe (PSP) observations pose many open questions in regard to the nature of switchbacks. …”
Get full text
Article -
3
The Temperature, Electron, and Pressure Characteristics of Switchbacks: Parker Solar Probe Observations
Published 2023-01-01“…Parker Solar Probe observes unexpectedly prevalent switchbacks, which are rapid magnetic field reversals that last from seconds to hours, in the inner heliosphere, posing new challenges to understanding their nature, origin, and evolution. …”
Get full text
Article -
4
Occurrence and Evolution of Switchbacks in the Inner Heliosphere: Parker Solar Probe Observations
Published 2023-01-01“…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 ubiquitous switchbacks (SBs). …”
Get full text
Article -
5
Theory of Magnetic Switchbacks Fully Supported by Parker Solar Probe Observations
Published 2023-01-01“…First seen sporadically in the 1970s in Mariner and Helios data, switchbacks were later observed by the Ulysses spacecraft beyond 1 au and have been recently discovered to be a typical component of solar wind fluctuations in the inner heliosphere by the Parker Solar Probe spacecraft. While switchbacks are now well understood to be spherically polarized Alfvén waves thanks to Parker Solar Probe observations, their formation has been an intriguing and unsolved puzzle. …”
Get full text
Article -
6
Dispersive Suprathermal Ion Events Observed by the Parker Solar Probe Mission
Published 2023-01-01“…During Encounter 11, Parker Solar Probe observed a low-energy dispersive ions event of solar origin. …”
Get full text
Article -
7
A Living Catalog of Parker Solar Probe IS⊙IS Energetic Particle Enhancements
Published 2023-01-01“…The Integrated Science Investigation of the Sun (IS⊙IS) on board the Parker Solar Probe is a suite of energetic particle detectors covering the energy range ∼20 keV–200 MeV nuc ^−1 . …”
Get full text
Article -
8
Self-Organization through the Inner Heliosphere: Insights from Parker Solar Probe
Published 2021-02-01Subjects: Get full text
Article -
9
Alpha-to-proton Temperature Ratio Distributions Using Parker Solar Probe Measurements
Published 2024-01-01“…The distributions of the temperature excess of alphas to protons ( ε ) were studied using Parker Solar Probe measurements for Encounters 2 through 14. …”
Get full text
Article -
10
Heating and Acceleration of the Solar Wind by Ion Acoustic Waves—Parker Solar Probe
Published 2024-01-01Get full text
Article -
11
Radial Evolution of the Near-Sun Solar Wind: Parker Solar Probe Observations
Published 2024-01-01“…A statistical study of the radial evolution of the solar wind within 0.3 au is shown in this Letter based on Parker Solar Probe observations. We show the radial distribution of the main solar wind parameters, including the solar wind speed V _sw , magnetic field ∣ B ∣, the number density of electrons N _e , protons N _p , and α particles N _α , and the temperature of protons T _p and α particles T _α . …”
Get full text
Article -
12
Can the Parker Solar Probe Detect a CME-flare Current Sheet?
Published 2023-01-01“…However, the detailed physical properties and fine structures of the CS are still unknown, since there is no relevant information obtained via in situ detections. The Parker Solar Probe (PSP) may provide us with such information should it traverse a CS in an eruption. …”
Get full text
Article -
13
Scale and Time Dependence of Alfvénicity in the Solar Wind as Observed by the Parker Solar Probe
Published 2024-01-01“…Alfvénicity is a well-known property, common in the solar wind, characterized by a high correlation between magnetic and velocity fluctuations. Data from the Parker Solar Probe (PSP) enable the study of this property closer to the Sun than ever before, as well as in the sub-Alfvénic solar wind. …”
Get full text
Article -
14
The Eruption of a Magnetic Flux Rope Observed by Solar Orbiter and Parker Solar Probe
Published 2023-01-01“…The erupting flux rope then passed over the Parker Solar Probe spacecraft during its encounter (13), enabling in situ diagnostics of the structure. …”
Get full text
Article -
15
Parker Solar Probe Observations of Magnetic Reconnection Exhausts in Quiescent Plasmas near the Sun
Published 2024-01-01“…Parker Solar Probe observations are analyzed for the presence of reconnection exhausts across current sheets (CSs) within R < 0.26 au during encounters 4–11. …”
Get full text
Article -
16
Nature, Generation, and Dissipation of Alfvénic Kinks/Switchbacks Observed by Parker Solar Probe and WIND
Published 2023-01-01“…The discovery of very prominent magnetic kinks/switchbacks in the solar wind within 0.3 au has become a scientific highlight of the Parker Solar Probe (PSP) mission. This discovery points at the promising impact of small-scale solar activity on the inner heliosphere. …”
Get full text
Article -
17
A Dust Detection Database for the Inner Heliosphere Using the Parker Solar Probe Spacecraft
Published 2023-01-01“…A database of in situ dust impact detections made by the Parker Solar Probe spacecraft is created to facilitate studies of interplanetary dust dynamics in the inner heliosphere. …”
Get full text
Article -
18
A Coronal Mass Ejection Impacting Parker Solar Probe at 14 Solar Radii
Published 2024-01-01“…Until recently, a wide spatial gap existed between the two regions, which prevented us from disentangling the spatial and temporal evolution of CMEs. NASA’s Parker Solar Probe (PSP) has imaged multiple CMEs since its launch in 2018, but these events either intercepted the spacecraft far from the corona or completely missed it. …”
Get full text
Article -
19
A prominence eruption from the Sun to the Parker Solar Probe with multi-spacecraft observations
Published 2023-08-01Subjects: Get full text
Article -
20
Parker Solar Probe Observations of High Plasma β Solar Wind from the Streamer Belt
Published 2023-01-01“…In general, slow solar wind from the streamer belt forms a high plasma β equatorial plasma sheet around the heliospheric current sheet (HCS) crossing, namely, the heliospheric plasma sheet (HPS). Current Parker Solar Probe (PSP) observations show that the HCS crossings near the Sun could be full or partial current sheet (PCS) crossings, and they share some common features but also have different properties. …”
Get full text
Article